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  • Other Sources  (6,912)
  • CITATION GEO-LEO  (6,726)
  • Bibliography of Trans-Basin Floods in Germany  (186)
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  • 1
    Publication Date: 2024-02-29
    Description: In dieser Abschrift der Bergordnung wurden zur besseren Übersicht noch einmal die 23 Paragrafen der Kremnitzer Bergordnung von 1492 aufgeführt. Im Jahr 1504 wurden drei Paragrafen hinzugefügt. Im Jahr 1537 erließ Oberkammergrafen Bernhard Behem weitere 21 Paragrafen. Der Bergmeister wurde hier zur obersten Amtsperson im Revier erklärt und entsprechend vereidigt. Beschrieben wurden ausführlich seine Rechte und Pflichten.
    Description: source
    Keywords: Slowakei ; Ungarn ; Kremnitz/Kremnica ; Silberbergbau ; Bergordnung
    Language: German
    Type: doc-type:book , updatedVersion
    Format: 20
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  • 2
    Publication Date: 2024-02-21
    Description: Diese Bergordnung, erlassen im Jahr 1520, wiederholt die 103 Paragrafen der Annaberger Bergordnung aus dem Jahr 1509 sowie die dort aufgeführten Eide. Zusätzlich wurden ihr weitere 32 Paragrafen hinzugefügt, die in der Zeit zwischen 1510 und 1519 erlassen wurden. Mit dem Druck der neuen Bergordnung wollte man den Text der alten Bergordnung und die inzwischen erlassenen Paragrafen in einem Buch zusammenfassen. Obwohl auch in den neuen Paragrafen immer wieder Bezug auf Annaberg genommen wurde, war es aber schon in der Einleitung deutlich, dass diese Bergordnung für die gesamte Grafschaft Sachsen Gültigkeit hatte. Ausgenommen, waren auch hier die Bergwerke in Freiberg.
    Description: source
    Keywords: Herzog Georg von Sachsen ; Annaberg ; Freiberg ; Dresden ; Sachsen ; Silberbergbau ; Bergordnung
    Language: German
    Type: doc-type:book , updatedVersion
    Format: 47
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  • 3
    Publication Date: 2024-02-07
    Description: Diese Bergordnung für Schemnitz/Banská Štiavnica wurde im Jahr 1513 veröffentlicht. Sie wiederholt die Bergordnung von Schemnitz aus dem Jahr 1466. Danach werden neun weitere Artikel hinzugefügt. Sie präzisieren die Rechte der einzelnen Gruben beim Anschaaren von zwei Gängen und das Prozedere der Vermessung dieser Gänge.
    Description: source
    Keywords: König Bela IV. von Ungarn ; König Vladislav II. von Böhmen und Ungarn ; Slowakei ; Ungarn ; Schemnitz/Banská Štiavnica ; Silberbergbau ; Bergordnung
    Language: German
    Type: doc-type:book , updatedVersion
    Format: 11
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  • 4
    Publication Date: 2024-01-04
    Description: Um das Jahr 1540 erließen die Herren zu Franckenstein und die Herren von Heusenstamm eine Bergordnung für die Bergwerke in Espa im Taunus. Als Vorlage für diese Bergordnung diente eine Abschrift der Bergordnung der Grafen von Hohnstein vom 3. Februar 1528 für die Bergwerke in der Grafschaft Lauterberg. Es wurden aber nicht alle Paragrafen übernommen. Es fehlen eine Abschlusserklärung mit den Anwendungsbestimmungen sowie ein Datum zum Erlass dieser Bergordnung. Wahrscheinlich handelt es sich bei dieser Bergordnung um einen unveröffentlichten Entwurf. Eine weitere Bergordnung für dieses Gebiet ist aber nicht bekannt.
    Description: source
    Keywords: Herren zu Frankenstein ; Herren zu Heusenstamm ; Espa (Langgöns) ; Silberbergbau ; Bergordnung
    Language: German
    Type: doc-type:book , updatedVersion
    Format: 21
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  • 5
    Publication Date: 2024-01-11
    Description: Im Jahr 1529 erließ Herzog Georg von Sachsen eine neue Bergordnung für die Bergwerke in Freiberg. Im Gegensatz zum Erzgebirge, wo die 1509 erlassene Annaberger Bergordnung allgemeine Gültigkeit erlangt hatte, beharrte der Rat zu Freiberg auf ein in Teilen eigenständiges Bergrecht für die Stadt. Die Freiberger Bergordnung wurde vom Rat zu Freiberg gemeinsam mit den Gewerken im Beisein von Herzog Georg erstellt. In den 38 Artikeln wurde im Wesentlichen der Inhalt der Annaberger Bergordnung wiederholt. Neu für Freiberg war die Abrechnung und Austeilung sowie Veranschlagung der Zubuße in einem festgesetzten Zeitraum. Im Gegensatz zur Abrechnung in vier Quartalen, wie es im Erzgebirge seit 1476 Vorschrift war, erfolgte diese in Freiberg zu drei Terminen im Jahr. Weiterhin wurde darauf verwiesen, dass die Freiberger Bergbeamten die Eide analog der Annaberger Bergordnung leisten sollten.
    Description: source
    Keywords: Herzog Georg von Sachsen ; Freiberg ; Annaberg ; Silberbergbau ; Sachsen ; Bergordnung
    Language: German
    Type: doc-type:book , updatedVersion
    Format: 11
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  • 6
    Publication Date: 2024-01-18
    Description: Die Bergordnung für Schemnitz/Banská Štiavnica wurde im Jahr 1466 als Anhang zum Stadtrecht im Stadtbuch (1432 begonnen) niedergeschrieben. Von den 59 Paragrafen waren nur die Paragrafen 42 bis 59 für das das Bergrecht relevant. Die Entstehungszeit der Bergordnung geht auf die Regierungszeit König Béla IV. (1235-1270) zurück. Nach der Einleitung durch König Béla IV. beschreiben die Geschworenen der Stadt die Verleihung von Gruben, die Rechte und Pflichten beim Betrieb der Bergwerke, das Stollenrecht und die Vermessung der Gruben. Im Gegensatz zu späteren Bergordnungen wurden hier nicht aufgetretene Fehlentwicklungen geregelt, sondern bereits klare gesetzliche Regelungen für den Bergbau vorgegeben.
    Description: source
    Keywords: König Béla IV. von Ungarn ; Slowakei ; Ungarn ; Schemnitz/Banská Štiavnica ; Iglau/Jihlava ; Silberbergbau ; Bergordnung
    Language: German
    Type: doc-type:book , updatedVersion
    Format: 9
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  • 7
    Publication Date: 2024-01-28
    Description: Diese im Jahr 1536 neu verfasste Bergordnung für Freiberg, erlassen von Herzog Georg von Sachsen wiederholt die 38 Artikel der Bergordnung von 1529. Zwischen 1530 und 1536 wird sie um vier weitere Artikel, unterteilt in 24 Absätze und einen Nachsatz, erweitert. Aus den angefügten Artikeln geht hervor, das die Bergordnung von 1529 nur widerwillig umgesetzt wurde. Die alte Bergordnung wird präzisiert, ein Hüttenraiter eingeführt und der Freiberger Rat mit Nachdruck aufgefordert die Durchsetzung der Bergordnung streng zu befolgen.
    Description: source
    Keywords: Herzog Georg von Sachsen ; Freiberg ; Annaberg ; Silberbergbau ; Sachsen ; Bergordnung
    Language: German
    Type: doc-type:book , updatedVersion
    Format: 16
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  • 8
    Publication Date: 2024-03-22
    Description: Obwohl die Wettiner das Gebiet um Berggießhübel und Gottleuba schon 1405 übernommen haben, wurde erst 1516 eine Bergordnung für den dortigen Eisenerzbergbau erlassen. In den vier Paragrafen geht es um Zustand der Bergwerke, das ordentliche Vermessen der Gruben und die Zahlung des Zehnten. Weiterhin soll der offensichtlich dauerhafte Streit zwischen den Gewerken und den Hammermeistern um Menge und Qualität des Eisensteins beendet werden.
    Description: source
    Keywords: Herzog Georg von Sachsen ; Freiberg ; Pirna ; Berggießhübel ; Bad Gottleuba ; Eger/Cheb ; Sachsen ; Eisenerzbergbau ; Bergordnung
    Language: German
    Type: doc-type:book , updatedVersion
    Format: 5
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  • 9
    Publication Date: 2024-04-03
    Description: In der Bohrung Moosburg 4 wurden die Nichtkarbonate (HCl-Unlösliches; 45 Proben) der Karbonatgesteine vom Malm Alpha (Unteres Oxfordium) bis zum Malm Zeta (Oberes Tithonium) röntgendiffraktometrisch untersucht. Ziel war es, die bestehende lithostratigraphische Untergliederung genauer mineralogisch und tonmineralogisch zu untermauern, um diese in Malm-Bohrungen des Molasse-Untergrundes besser belegen zu können. Die Kombination von mineralogischen und tonmineralogischen röntgenographischen Untersuchungen der Nichtkarbonate ermöglichen es, unter Bezug zum Gamma-Log der Bohrung Moosburg SC4 eine Untergliederung in neun Einheiten (I – IX) zu definieren. Diese entspricht vom Malm Alpha bis Malm Zeta 3 weitgehend der lithostratigraphischen Unterteilung, wie sie von Meyer (1994) dokumentiert wird. Die von Meyer (1994) vorgenommene Positionierung des Malm Zeta 4-5 und die der als Purbeck definierten Schichtfolge müssen dagegen revidiert werden. Die Malm/ Purbeck-Grenze ist um 99 m ins Hangende zu legen. Damit entspricht der dort im Malm analysierte Bereich dem Untertithon und dem Obertithon. Karbonatgesteine des Purbeck wurden in der vorliegenden Studie nicht untersucht. Die Zuordnung der Einheiten I-VI zu den lithostratigraphischen Einheiten von Meyer (1994) ist gut. Es ist nur der obere Teil der Bohrung Moosburg 4 als Unteres und als Oberes Tithon neu zu definieren. Allgemein kann festgestellt werden, dass eine lithostratigraphische Untergliederung des Malm auf der Basis mineralogisch/tonmineralogischer Analysen der Nichtkarbonate erstellt werden kann. Diese Methode kann daher auch in neuen Bohrungen im Molassebecken zur Untergliederung der oberjurassischen Schichtfolge erfolgreich angewendet werden.
    Description: research
    Keywords: Ober-Jura ; Tonmineral-Stratigraphie ; Mineralostratigraphie
    Language: German
    Type: doc-type:article
    Format: 21
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  • 10
    Publication Date: 2024-04-03
    Description: Bergordnung für St. Joachimsthal, vom 2. August 1518. Basis dieser Bergordnung bildet die Bergordnungen für St. Annaberg vom 5. Februar 1509. Die 103 Paragraphen der Annaberger Bergordnung wurden fast wortwörtlich übernommen. Es wurde der gesamte Bergwerksbetrieb, die Arbeit der Schmelzhütten und das Gericht in St. Joachimsthal geregelt. Auch die Eide der Bergbeamten wurden übernommen. In weiteren drei Paragraphen wurden die Entlohnung der Bergleute sowie die Lohnfortzahlung und das Arztgeld nach Arbeitsunfällen aufgeführt.
    Description: source
    Keywords: Graf Stefan Schlick zu Passaun ; Konradsgrün ; Joachimsthal/Jáchymov ; Annaberg ; Marienberg ; Schneeberg ; Silberbergbau ; Böhmen ; Bergordnung
    Language: German
    Type: doc-type:book , updatedVersion
    Format: 39
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  • 11
    Publication Date: 2024-04-03
    Description: Tiefgreifende Hangbewegungen stellen neben Muren und Lawinen, welche durch Faktoren wie Extremniederschlagsereignisse und Unterschneidungsvorgänge entstehen, eine akute Gefahr für die Bevölkerung und die Infrastruktur im alpinen Raum dar (Moser 2013). Talzuschübe, oder auch DSGSD für Deep-seated Gravitational Slope Deformation (Crosta et al. 2013), sind großflächige und tiefgreifende Hangbewegungen im alpinen Raum. Im Rahmen dieser Untersuchungen erfolgte eine ingenieurgeologische Aufnahme des Dürnbachtals bei Neukirchen am Großvenediger mit der Erstellung von Hangprofilen und der Aufnahme des Trennflächengefüges. Weiter wurde der Einfluss der beidseitigen Talzuschübe auf den Wildbach und das Murereignis nach einem Starkniederschlagsereignis am 28.07.2022 analysiert. Zuletzt wurde eine Abschätzung des Gefahrenpotentials des Dürnbachs für den Ort Neukirchen am Großvenediger erstellt.
    Description: research
    Keywords: Talzuschub ; counterscarps ; Massenbewegung ; Murgang ; Starkniederschlag ; Salzburger Land ; Österreich
    Language: German
    Type: doc-type:article
    Format: 41
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  • 12
    Publication Date: 2024-04-19
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Heavy‐mineral suites are used widely in sandstone provenance and are key when connecting source and sink. When characterizing provenance related signatures, it is essential to understand the different factors that may influence a particular heavy‐mineral assemblage for example, chemical weathering or diagenetic processes. Hydrodynamics, causing size‐density sorting, exert major control on the distribution of heavy minerals. Here, we highlight the effect of grain‐size inheritance, essentially the absence of certain grain sizes within a specific heavy‐mineral species, on two distinct types of sediments. Modern deposits from a high‐energy beach in NW Denmark give an analog for heavily reworked sediment, primarily controlled by hydrodynamic processes. In contrast, three Palaeogene turbidite successions in the Eastern Alps were sampled, presenting a more complex history that includes diagenesis. All samples were processed for their heavy‐mineral compositions using Raman spectroscopy, and several techniques applied to determine the effect of grain‐size inheritance. Results show that (a) even within the hydrodynamically well‐sorted beach and placer deposits, evidence of grain‐size inheritance is apparent, and (b) turbidites of variable heavy‐mineral composition show strong effects of grain‐size inheritance for several mineral species. Moreover, considerable intersample contrasts within single turbidite beds are observed. We enforce the importance of understanding grain‐size inheritance, as well as other processes effecting size‐density relations in clastic sediment that go well beyond purely hydrodynamic control of intrasample heavy‐mineral variability.〈/p〉
    Description: Plain Language Summary: Heavy minerals are commonly found within sediments and sedimentary rocks and can tell us from which source regions the sediment may have originated. However, it is important to understand that the type, size, and abundance of particular heavy minerals can change depending on factors such as environmental conditions. The size, shape, and density of the heavy minerals also limits when and where they will settle and/or stay. A lack of big or small grains of a particular heavy mineral in the source rocks dictates the size of the minerals deposited; this is known as grain‐size inheritance. Using both ancient and modern sediment, we are looking for traces of grain‐size inheritance. Surprisingly, in all samples investigated we noted effects of grain‐size inheritance, for different heavy‐mineral types. The modern beach sediments, as expected, show more impact of hydraulic processes, but inherited grain sizes are still apparent. Within the ancient examples, grain‐size inheritance is more obvious, with further variations even observed between samples collected from the same area. Having identified this control on grain size, we can highlight the importance of understanding this effect when analyzing clastic sediments.〈/p〉
    Description: Key Points: 〈list list-type="bullet"〉 〈list-item〉 〈p xml:lang="en"〉Understanding factors that can modify a heavy‐mineral assemblage is fundamental in provenance analysis〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉Heavy minerals of two distinct sedimentary environments were analyzed and compared to their “ideal” hydrodynamically sorted compositions〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉Several heavy‐mineral species of modern and ancient settings were identified to be influenced by grain‐size inheritance from the source〈/p〉〈/list-item〉 〈/list〉 〈/p〉
    Description: https://doi.org/10.25625/MVUIJQ
    Keywords: ddc:552.5 ; heavy minerals ; provenance ; grain‐size inheritance ; hydrodynamics ; diagenesis
    Language: English
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  • 13
    Publication Date: 2024-04-19
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉The Ismenius Lacus region of Mars has a diverse geological history, and we present the first high‐resolution map of Deuteronilus Cavus (36.2°N; 14.0°E, ∼120 km diameter) in the fretted terrain south of the dichotomy boundary. Strong evidence suggests a volcanic origin of the regional plains, based on the ∼50 m thick volcanic bed underlying 180–300 m of sublimation residue associated with Amazonian plateau glaciation. Pervasive external volcanic flooding, internal erosional modification, and enlargement of a pre‐existing crater by up to 175%–200% resulted in the cavus' present shape. The phyllosilicates detected within Deuteronilus Cavus could be primary materials associated with the surficial aqueous activity, subsurface alteration products excavated by impacts, or a combination of both. We observe branching fluvial channels that are more recent than the traditional valley networks and may be related to fretted terrain resurfacing during the waning period of a high‐obliquity glaciation phase. This is consistent with our interpretation of the ∼600 m thick lobate and lineated deposits, which are remnants of receding glaciers. The glacial ice, protected by a 15–20 m insulating layer of debris cover, is of significant interest for future landing missions because of its potential to preserve biological and climatological signatures, to provide a critical test of Amazonian plateau glaciation, and to be used for in situ resource utilization. With our detailed geological mapping, we improved our understanding of the geological evolution and climatic conditions in the enigmatic fretted terrain near the dichotomy boundary.〈/p〉
    Description: Plain Language Summary: The ∼120 km long Deuteronilus Cavus was initiated by an impact event. The resulting impact crater was modified by glacial erosional and fluvial processes, leading to the enlargement of 175%–200% of the pre‐existing crater. In addition, we find strong evidence for recent glaciation (〈1 Ga) that left 180–300 m of sublimation residue on the plateau superimposed on a ∼50 m thick volcanic bed, suggesting a volcanic origin of the regional plains. During the waning period of a high‐glacial phase, the meltwater ponded on the surface of the cavus, altered surface rocks to produce phyllosilicates, formed channels (now observed as inverted sinuous ridges), and locally distributed branched fluvial channels that are more recent than the traditional valley networks. Glacial landforms still contain up to 600 m of remnant ice from the retreating glaciers at the end of the last glacial period. The relatively pure ice, protected by a 15–20 m insulating layer of debris cover, is critical for future landing missions because of its potential to preserve biological and climatological signatures and to be used for in situ resource utilization. Overall, this research enhances our understanding of the geological evolution and climatic history of Mars.〈/p〉
    Description: Key Points: 〈list list-type="bullet"〉 〈list-item〉 〈p xml:lang="en"〉We have produced the first high‐resolution map of Deuteronilus Cavus in the fretted terrain south of the Martian dichotomy boundary〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉The region records a complex erosional and depositional history, including fluvial and glacial processes in the Amazonian period〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉This study provides a framework for exploration of high‐obliquity mid‐latitude plateau glaciation〈/p〉〈/list-item〉 〈/list〉 〈/p〉
    Description: Deutsches Zentrum für Luft‐ und Raumfahrt http://dx.doi.org/10.13039/501100002946
    Description: https://doi.org/10.5281/zenodo.8205276
    Description: https://doi.org/10.17189/1520332
    Description: https://doi.org/10.17189/1520266
    Description: https://doi.org/10.17189/1520303
    Description: https://doi.org/10.5270/esa-pm8ptbq
    Keywords: ddc:523 ; Mars ; Deuteronilus Cavus ; geological mapping ; glaciation
    Language: English
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  • 14
    Publication Date: 2024-04-20
    Description: Im Zusammenhang mit der Neuordnung der Bergverwaltung fand auch in Berggießhübel eine Besichtigung der Bergwerke statt. Aufgrund der festgestellten Unregelmäßigkeiten wurde eine neue Bergordnung erlassen. In 11 Paragrafen wurde eine ordentliche Rechnungslegung festgelegt, die Hammerherren zur pünktlichen Bezahlung des Eisensteins aufgefordert und eine strenge Kontrolle der Arbeitszeit angeordnet. Weiterhin erhielten Gewerken eine Steuererleichterung beim Stollnvortrieb.
    Description: source
    Keywords: Herzog Moritz von Sachsen ; Dresden ; Pirna ; Berggießhübel ; Gottleuba ; Sachsen ; Eisenerzbergbau ; Bergordnung
    Language: German
    Type: doc-type:book , updatedVersion
    Format: 7
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  • 15
    Publication Date: 2023-01-05
    Description: Nachdem sich Herzog Georg von Sachsen mit den Problemen des Bergbaus auf dem Aldenberg und Geising auseinandergesetzt hatte, erlies er am 11. November 1489 eine Ordnung für die dortigen Bergwerke. In den acht Artikeln dieser Ordnung wurden die Entlohnung der Bergleute sowie die Pflichten der Hutleute, Mühlmeister, Schmelzer und die Strafen bei Zuwiderhandlung festgelegt. Weiterhin wurde eine Vereidigung der Hutleute, Mühlenmeister und Schmelzer befohlen.
    Description: source
    Keywords: Herzog Georg von Sachsen ; Herzog Albrecht von Sachsen ; Hans von Bärenstein zu Ottendorf ; Altenberg ; Geising ; Zinnbergbau ; Sachsen ; Bergordnung
    Language: German
    Type: doc-type:book , updatedVersion
    Format: 6
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  • 16
    Publication Date: 2023-01-11
    Description: Diese Bergordnung wurde am 7. Januar 1474 für die Bergwerke in Schwaz von Herzog Siegmund von Österreich erlassen. Mit dem ab 1470 stark ansteigenden Bergbauaktivitäten kam es gleichzeitig zu zahlreichen Missständen bei der Dienstdurchführung der Hutleute sowie zu offensichtlich chaotischen Zuständen bei der Vermessung der Grubenfelder. In 16 Paragrafen wurden deshalb die Rechte der Gruben an ihren Feldern, das ordentliche Vermessen der Grubenfelder und das Verhalten bei Durchschlägen beschrieben sowie die Zuständigkeiten der Hutleute klar benannt. In einem später eingefügten Zusatz wurde das Fällen von Bäumen im gesamten Bergbaubezirk verboten.
    Description: source
    Keywords: Herzog Siegmund von Österreich ; Österreich ; Tirol ; Schwaz ; Freundsberg, Burg ; Schlitters ; Innsbruck ; Silberbergbau ; Bergordnung
    Language: German
    Type: doc-type:book , updatedVersion
    Format: 7
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  • 17
    Publication Date: 2023-01-20
    Description: Die Entstehung dieser als Bergweistum bezeichnete Bergordnung von Graf Egino IV. für die Bergwerke auf dem Diesselmut am 30. Juni 1372 ist auf die unklaren Rechtsverhältnisse beim Silberbergbau im Breisgau zur damaligen Zeit zurückzuführen. In einem Frage- und Antwortspiel mit 10 namentlich genannten Bergverständigen klärte Graf Egino IV. seine Rechtsansprüche am Silberbergbau.
    Description: source
    Keywords: Graf Egino IV. von Freiburg ; Breisgau ; Freiburg im Breisgau ; Kloster St. Trudpert ; Todtnau ; Silberbergbau ; Bergordnung
    Language: German
    Type: doc-type:book , updatedVersion
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  • 18
    Publication Date: 2023-06-21
    Description: Volcanic inflation and deflation often precede eruptions and can lead to seismic velocity changes (dv/v $dv/v$) in the subsurface. Recently, interferometry on the coda of ambient noise‐cross‐correlation functions yielded encouraging results in detecting these changes at active volcanoes. Here, we analyze seismic data recorded at the Klyuchevskoy Volcanic Group in Kamchatka, Russia, between summer of 2015 and summer of 2016 to study signals related to volcanic activity. However, ubiquitous volcanic tremors introduce distortions in the noise wavefield that cause artifacts in the dv/v $dv/v$ estimates masking the impact of physical mechanisms. To avoid such instabilities, we propose a new technique called time‐segmented passive image interferometry. In this technique, we employ a hierarchical clustering algorithm to find periods in which the wavefield can be considered stationary. For these periods, we perform separate noise interferometry studies. To further increase the temporal resolution of our results, we use an AI‐driven approach to find stations with similar dv/v $dv/v$ responses and apply a spatial stack. The impacts of snow load and precipitation dominate the resulting dv/v $dv/v$ time series, as we demonstrate with the help of a simple model. In February 2016, we observe an abrupt velocity drop due to the M7.2 Zhupanov earthquake. Shortly after, we register a gradual velocity increase of about 0.3% at Bezymianny Volcano coinciding with surface deformation observed using remote sensing techniques. We suggest that the inflation of a shallow reservoir related to the beginning of Bezymianny's 2016/2017 eruptive cycle could have caused this local velocity increase and a decorrelation of the correlation function coda.
    Description: Plain Language Summary: Before eruptions, volcanoes inflate due to the rising magma from below. Previous studies have found that these deformations can lead to small changes in the properties of the surrounding rock. We use passive image interferometry, a method that relies on the omnipresent background vibration of the Earth—mostly induced by the oceans, to measure these changes at the Klyuchevskoy Volcanic Group in Kamchatka, Russia. However, in Kamchatka, this background noise is masked and distorted by small earthquakes and tremors originating from the volcanoes themselves. We combine machine learning techniques with established monitoring methods to find times when these tremors remain similar. Afterward, we use data from these time periods in the conventional way to observe changes in the soil and the rock. Our results show that rain‐ and snowfall and the thickness of the snow cover exert the strongest influence on the properties of the rocks. Additionally, we found that a large magnitude 7.2 earthquake, which struck Kamchatka during our study, caused a slight weakening of the rocks due to microstructural damage. We register changes shortly before an eruption and suggest a connection to the beginning of an eruptive cycle in 2016.
    Description: Key Points: Fluctuating noise conditions lead to distortions in noise interferometry studies, which we avoid with the help of machine learning. The seismic velocity on Kamchatka is affected by numerous mechanisms, amongst them environmental, tectonic, and volcanic events. We observe a velocity increase at Bezymianny during February 2016 and link it to the beginning of the eruptive cycle.
    Description: German Research Foundation
    Description: https://doi.org/10.14470/K47560642124
    Description: https://doi.org/10.24381/cds.e2161bac
    Description: https://doi.org/10.5880/GFZ.2.4.2022.002
    Description: https://doi.org/10.5281/zenodo.7481934
    Keywords: ddc:551 ; seismology ; volcano monitoring ; machine learning ; ambient noise ; seismic velocity change ; time varying earth structure
    Language: English
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  • 19
    Publication Date: 2023-06-21
    Description: We provide an updated estimate of the annual‐mean, seasonal cycle and interannual variability of the transports and properties of the Weddell Sea Bottom Water (WSBW) plume in the northwestern Weddell Sea. For this we used a densely instrumented mooring array deployed across the continental slope between January 2017 and January 2019. We found that the annual‐mean WSBW transport is 3.4 ± 1.5 Sv, corresponding to a cross‐section area of 35 km2 and a maximum thickness of 203 m. The annual mean transport‐weighted properties of WSBW are −0.99°C (Θ), 34.803 g/kg (SA) and 28.44 kg/m3 (γn). The WSBW is characterized by 3 bottom‐intensified velocity cores, which display seasonal variations in flow speed and transport different varieties of WSBW. The seasonal peak of WSBW transport and density is reached in May (4.7 Sv, 28.443 kg m−3) while the minimum values are observed in February (2.8 Sv, 28.435 kg m−3). The coldest WSBW is found between March and May, and the warmest between August and October. The density decrease of WSBW observed in the austral autumn of 2018 can be explained by warmer ambient waters being entrained during the formation of WSBW. This was enabled by the weakening of the along‐shore winds associated with a positive Southern Annular Mode index, reinforced by a La Niña event in early 2018. The synchronous decrease of total WSBW transport and volume between September 2018 and February 2019 indicates a reduction in the export of the dense precursors of WSBW from the Weddell Sea continental shelf.
    Description: Plain Language Summary: The Meridional Overturning Circulation (MOC) redistributes heat and carbon dioxide in the world ocean. Thus, it plays an important role in the regulation of our planet's climate. The Weddell Sea is the main contributor to the deep branch of the MOC in the Southern Hemisphere. Despite the importance of this contribution, uncertainties still remain associated to the plume of dense waters transported along the continental slope of the Weddell Sea. To reduce these uncertainties, we analyzed the most densely instrumented mooring array deployed across the continental slope in the northwestern Weddell Sea. We found that this plume flows faster close to the seafloor and that it presents important seasonal and interannual variability. The Weddell Sea Bottom Water interannual variability is influenced by changes in the along‐shore winds driven by the phase of two important climate modes, the Southern Annular Mode and the El Niño‐Southern Oscillation, but also by changes in the export of the dense precursors of WSBW in its formation areas. Increasing our knowledge on the along‐slope plume variability and properties is important to better understand the causes behind the variability of the MOC observed further downstream.
    Description: Key Points: The Weddell Sea Bottom Water (WSBW) plume presents 3 velocity cores and a clear seasonal cycle, with maximum transports and densities in May and minimum in February. A +SAM, reinforced by a ‐ENSO, favors the warming of WSBW via a wind‐driven warming of the ambient waters entrained during its formation. We observed a marked decrease in WSBW density and transports between September 2018 and February 2019 compared to the previous year.
    Description: EU Horizon 2020 Research and Innovation Program
    Description: German Research Foundation
    Description: Alfred Wegener Institute Helmholtz‐Center
    Description: https://doi.org/10.5281/zenodo.7500163
    Keywords: ddc:551.46 ; Weddell Sea ; WSBW ; Meridional Overturning Circulation ; SAM ; ENSO ; deep‐water plume
    Language: English
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  • 20
    Publication Date: 2023-06-21
    Description: Fossil spinicaudatan taxonomy heavily relies on carapace features (size, shape, ornamentation) and palaeontologists have greatly refined methods to study and describe carapace variability. Whether carapace features alone are sufficient for distinguishing between species of a single genus has remained untested. In our study, we tested common palaeontological methods on 481 individuals of the extant Australian genus Ozestheria that have been previously assigned to ten species based on genetic analysis. All species are morphologically distinct based on geometric morphometrics (p ≤ 0.001), but they occupy overlapping regions in Ozestheria morphospace. Linear discriminant analysis of Fourier shape coefficients reaches a mean model performance of 93.8% correctly classified individuals over all possible 45 pairwise species comparisons. This can be further increased by combining the size and shape datasets. Nine of the ten examined species are clearly sexually dimorphic but male and female morphologies strongly overlap within species with little influence on model performance. Ornamentation is commonly species‐diagnostic; seven ornamentation types are distinguished of which six are species‐specific while one is shared by four species. A transformation of main ornamental features (e.g. from punctate to smooth) can occur among closely related species suggesting short evolutionary timescales. Our overall results support the taxonomic value of carapace features, which should also receive greater attention in the taxonomy of extant species. The extensive variation in carapace shape and ornamentation is noteworthy and several species would probably have been assigned to different genera or families if these had been fossils, bearing implications for the systematics of fossil Spinicaudata.
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: https://doi.org/10.5061/dryad.fbg79cnxs
    Keywords: ddc:565 ; clam‐shrimp carapace ; morphometrics ; species delimitation ; Spinicaudata ; Ozestheria ; Australia
    Language: English
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  • 21
    Publication Date: 2023-06-21
    Description: Groundwater abstraction and drainage are considered to be the main drivers for the salinization of low‐lying coastal groundwater systems, while the role of past boundary conditions is less clear. In this study, 3‐D paleo‐hydrogeological variable‐density groundwater flow and salt transport modeling (“paleo‐modeling”) is applied to reconstruct the evolution of groundwater salinities during the Holocene, that is, the last 9,000 years, in Northwestern Germany. Novel aspects of this study include the consideration of highly resolved time‐variant boundary conditions in a 3‐D paleo‐modeling framework, for example, sea‐level rise, surface elevation and coastline changes, development of drainage networks and groundwater abstraction, as well as the quantification of isolated processes impacting salinization. Results show that salinization was a function of sea‐level rise from 9000 BP until 1300 CE. The creation of the dike line ∼1300 CE set the starting point for increasing anthropogenic control of the hydro(geo)logical system: changes in surface elevation and drainage of low‐lying marshes have become main drivers for salinization after 1600 CE when peat was artificially degenerated. Moreover, changes in the dike line caused by storm floods impacted the salinities. Model results for 2020 CE match well with present‐day salinity observations. Yet, salinization will continue in the future, as the hydro(geo)logical system has not reached an equilibrium. The presented paleo‐modeling framework can be viewed as a blueprint for similar low‐lying coastal groundwater systems, influenced by marine transgression and human development. Thereby, it enables the reconstruction of meaningful present‐day salinity distributions, serving as a vital basis for modeling future groundwater systems in a changing climate.
    Description: Key Points: Salinization of a low‐lying coastal groundwater system during the Holocene, that is, 9000 BP until present‐day, was investigated. Sea‐level rise and the evolution of paleogeography were major controls on groundwater salinization during most of the time. Surface elevation changes due to land cultivation, as well as the development of drainage networks, control salinization since ∼1600 CE.
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: Bundesministerium für Bildung und Forschung http://dx.doi.org/10.13039/501100002347
    Description: https://doi.org/10.5281/zenodo.7633381
    Keywords: ddc:551.49 ; saltwater intrusion ; variable‐density groundwater flow ; salt transport ; sea‐level rise ; parameter estimation ; iMOD‐WQ
    Language: English
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  • 22
    Publication Date: 2023-06-21
    Description: Measurements of kinetic energy in vortical and divergent fluctuations in the mesosphere and lower thermosphere can be used to study stratified turbulence (ST) and gravity waves. This can be done using horizontal correlation functions of the fluctuating component of velocity. This study introduces a novel method for estimating these correlation functions using radars that observe Doppler shifts of ionized specular meteor trails. The technique solves the correlation functions directly on a longitudinal‐transverse‐up coordinate system, assuming axial symmetry. This procedure is more efficient and leads to smaller uncertainties than a previous approach. The new technique is applied to a year‐long data set from a multistatic specular meteor radar network in Germany, to study the annual variability of kinetic energy within turbulent fluctuations at 87–93 km of altitude. In monthly averages, the kinetic energy is found to be nearly equipartitioned between vortical and divergent modes. Turbulent fluctuations maximize during the winter months with approximately 25% more energy in these months than at other times. The horizontal correlation functions are in agreement with the inertial subrange of ST, exhibiting a 2/3 power law in the horizontal lag direction, with an outermost scale of ST to be about 380 km. This suggests that horizontal correlation functions could be used to estimate turbulent energy transfer rates.
    Description: Plain Language Summary: Flows exhibit a phenomenon called turbulence, which transfers energy from large scales into smaller scales. This effect is important to quantify the energy budget of the Earth's upper atmosphere. The range of length scales where this phenomenon occurs is called the inertial subrange of turbulence. The classical theory of isotropic turbulence predicts that this energy transfer occurs on length scales smaller than ∼100 m, at 60–110 km altitude. Recent work has shown that horizontal velocity fluctuations can extend the inertial subrange to length scales of up to hundreds of kilometers horizontally. This type of turbulence is called stratified turbulence (ST). So far no comprehensive study has been made to experimentally examine ST in the mesosphere and lower thermosphere (MLT) region on horizontal mesoscales. This study introduces a method for doing so by measuring how the wind fluctuations are correlated as a function of horizontal separation. This is achieved by using meteor radar measurements. The technique is applied to a year‐long data set over Germany. It is found that the MLT wind fluctuations are compatible with ST theory. The introduced method could potentially be used for routinely measuring how kinetic energy flows from large‐scale to small‐scale atmospheric fluctuations.
    Description: Key Points: A more efficient estimator for horizontal correlation functions is introduced. The rotational and divergent correlation functions of mesosphere and lower thermosphere wind fluctuations are found to be balanced at horizontal mesoscales. Horizontal correlations of wind fluctuations follow a 2/3‐power law for horizontal separations of up to 300–400 km.
    Description: Bundesministerium für Bildung und Forschung http://dx.doi.org/10.13039/501100002347
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: French Ministry of Foreign and European Affairs
    Description: Leibniz SAW project FORMOSA
    Keywords: ddc:551.5 ; mesosphere ; lower thermosphere ; wind fluctuations
    Language: English
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  • 23
    Publication Date: 2023-06-19
    Description: Geochemical analyses of carbonate minerals yield multiple parameters which can be used to estimate the temperature and water composition at which they formed. Analysis of fluid trapped in minerals is a potentially powerful tool to reconstruct paleotemperatures as well as diagenetic and hydrothermal processes, as these could represent the parent fluid. Internal fluids play important roles during the alteration of carbonate fossils, lowering energetic barriers associated with resetting of clumped isotopes, as well as mediating the transport of elements during diagenesis. Here, we explore the behavior of the ∆47–∆48 “dual‐clumped” isotope thermometer during fluid‐carbonate interaction and demonstrate that it is highly sensitive to the water/carbonate ratio, behaving as a linear system in “rock buffered” alteration, and as a decoupled system in water‐dominated systems due to non‐linear mixing effects in ∆48. Dry heating experiments show that the extrapolated “heated” end‐member is indistinguishable from the predicted ∆47 and ∆48 value expected for the experimental temperature. Furthermore, we evaluate two common laboratory sampling methods for their ability to thermally alter samples. We find that the temperature of the commonly used crushing cells used to vapourize water for fluid inclusion δ18O analyses is insufficient to cause fluid‐carbonate oxygen isotope exchange, demonstrating its suitability for analyses of fluid inclusions in carbonates. We also find that belemnites sampled with a hand‐drill yield significantly warmer paleotemperatures than those sampled with mortar and pestle. We conclude that thermally‐driven internal fluid‐carbonate exchange occurs indistinguishably from isotopic equilibrium, limited by the extent to which internal water and carbonate can react.
    Description: Plain Language Summary: Carbonate minerals contain multiple, independent, chemical and isotopic parameters which can be used to calculate the temperature at which the mineral formed. If these proxies agree with one another, it has been confidently assumed that the temperature is indeed genuine. Here, we investigate three such parameters and show how they record kinetic processes during mineral formation, as well as thermally‐driven processes which may alter a climate record. We find that this method could potentially be used to study the kinetic factors at play during biomineralization, even if the “true” temperature is unknown. We also find that some thermal processes result in all three parameters agreeing with one another. Because thermal alteration poses a potential dilemma for climate researchers, we investigate two common laboratory preparation techniques that involve heating a sample before analysis: drilling and heating sample for fluid inclusion analysis. We find that the heat of a drill is sufficient to facilitate these reactions, and potentially imparts a warm bias onto paleotemperatures, however the apparatus used for analyzing fluid inclusions does not appear to significantly alter the material. We conclude our approach using fluid inclusion analysis and dual‐clumped isotopes has the potential to resolve many ambiguities in interpreting climate records.
    Description: Key Points: We explore the behavior of dual‐clumped and fluid‐inclusion isotope paleothermometers during thermal alteration. Different conditions during diagenesis may result in discrepant paleotemperature estimates, which may be used to identify altered records. Hand‐drilling belemnites produces sufficient heat to reset paleotemperatures, but the heat during analysis of fluid inclusions does not.
    Description: DFG
    Description: https://doi.org/10.5281/zenodo.7565557
    Keywords: ddc:551.9 ; diagenesis ; clumped isotopes ; fluid inclusions ; numerical modeling
    Language: English
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  • 24
    Publication Date: 2023-06-19
    Description: Energetic particle acceleration and energization in planetary magnetotails are often associated with dipolarization fronts characterized by a rapid increase of the meridional component of the magnetic field. Despite many studies of dipolarization events in Earth's magnetotail, Jupiter’s magnetotail provides an almost ideal environment to study high‐energetic ion acceleration by dipolarization fronts because of its large spatial scales and plasma composition of heavy and light ions. In this study, we focus on the response of different high‐energetic ion intensities (H, He, S, and O) to prominent magnetic dipolarization fronts inside the Jovian magnetotail. We investigate if ion energization and acceleration are present in the observations around the identified dipolarization fronts. Therefore, we present a statistical study of 87 dipolarization front signatures, which are identified in the magnetometer data of the Juno spacecraft from July 2016 to July 2021. For the ion intensity analysis, we use the energetic particle observations from the Jupiter Energetic Particle Detector Instrument. Our statistical study reveals that less than half of the identified events are accompanied by an increase of the ion intensities, while most of the other events show no significant change in the ion intensity dynamics. In about 40% of the events located in the dawn sector a significant decrease of the energy spectral index is detected indicating ion acceleration by the dipolarization fronts.
    Description: Key Points: Eighty‐seven prominent dipolarization front signatures are observed in the MAG data during Juno's prime mission during 21:00–05:30 local time. Less than half of the identified events are accompanied by an increase of the ion intensities. In 40% of the events observed on the dawn side a significant decrease of the energy spectral index indicates ion acceleration by the fronts.
    Description: Volkswagen Foundation http://dx.doi.org/10.13039/501100001663
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: https://doi.org/10.17189/1519711
    Description: https://doi.org/10.17189/1519713
    Keywords: ddc:523 ; Juno ; Jovian magnetotail ; energetic ions ; dipolarization fronts ; JEDI
    Language: English
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  • 25
    Publication Date: 2023-07-04
    Description: The recent diversification of macromolecular crystallographic experiments including the use of pink beams, convergent electron diffraction and serial snapshot crystallography has shown the limitations of using the Laue equations for diffraction prediction. This article gives a computationally efficient way of calculating approximate crystal diffraction patterns given varying distributions of the incoming beam, crystal shapes and other potentially hidden parameters. This approach models each pixel of a diffraction pattern and improves data processing of integrated peak intensities by enabling the correction of partially recorded reflections. The fundamental idea is to express the distributions as weighted sums of Gaussian functions. The approach is demonstrated on serial femtosecond crystallography data sets, showing a significant decrease in the required number of patterns to refine a structure to a given error.
    Description: Reflection position, size and shape prediction and partiality estimation of crystal diffraction by integrating using a Gaussian basis are described.
    Keywords: ddc:548 ; partiality estimation ; diffraction prediction ; merging ; serial snapshot crystallography
    Language: English
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  • 26
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    ARGE GMIT, Bonn
    Publication Date: 2023-07-04
    Description: Die Ausgabe der Geowissenschaftlichen Mitteilungen vom Juni 2022 enthält die Themenblöcke: GEOfokus:Mariengraben - Am Puls der tiefen Erde, GEOaktiv (Wirtschaft, Beruf, Forschung und Lehre), GEOlobby (Gesellschaften, Verbände, Institutionen), GEOreport (Geowissenschaftliche Öffentlichkeitsarbeit, Tagungsberichte, Ausstellungen, Exkursionen, Publikationen), GEOszene (Würdigungen, Nachrufe).
    Description: DFG, SUB Göttingen
    Description: journal
    Keywords: ddc:550 ; GMIT
    Language: German
    Type: doc-type:book , publishedVersion
    Format: 124
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  • 27
    Publication Date: 2023-07-04
    Description: The Andean Plateau of north‐western Argentina (Puna) at a mean elevation of ca. 4.2 km constitutes the southern continuation of the Altiplano; it is a compressional basin‐and‐range province comprising fault‐bounded, high‐elevation mountain ranges and largely internally drained basins with often thick sedimentary and volcaniclastic fill. Growing sedimentological and structural evidence supports the notion that the north‐western Argentine Andes between 22° and 26°S developed from an initial extensive broken‐foreland system that extended across the present‐day eastern Andean flank during the early to middle Eocene. However, compelling evidence of the tectonic history of this region is still missing. Here, we present new apatite fission track and zircon (U–Th)/He thermochronological data and U–Pb zircon ages from intercalated volcanic ash deposits from the Pastos Chicos Basin (23.5°S, 66.5°W) to constrain basin formation and the timing of major crustal deformation in the northern Puna. Inverse thermal modeling of the thermochronological data provides further temporal constraints on the late Cenozoic cooling history of the crust in this region and, by inference, on the timing of upper‐crustal shortening, range uplift, and basin formation in the northern sector of the present‐day Puna Plateau. Specifically, we argue for plateau‐wide distributed deformation in the Eocene between 23° and 24°S, followed by spatially disparate and diachronous deformation (Oligocene to Pliocene).
    Description: Plain Language Summary: The Argentine Puna Plateau is a mountainous region in the Central Andes of South America. It is the result of the tectonic convergence between the oceanic Nazca Plate and the continental South American Plate. However, the detailed tectonic evolution of this region is yet unknown. We present new thermochronologic data from the Puna Plateau that allow inferences about crustal deformation and mountain range uplift. Combined with previous studies, our results suggest deformation distributed over the entire plateau during the Eocene. Thereafter, local deformation occurred spatially non‐systematic, possibly related to zones of weakness in the crust.
    Description: Key Points: Thermal modeling of apatite fission track and (U‐Th)/He zircon data from the Pastos Chicos Basin shows Oligo‐Miocene onset of exhumation. Regional compilation of spatio‐temporal deformation at 23°–24°S suggests out‐of‐sequence deformation related to basement heterogeneities. Mio‐Pliocene U–Pb zircon ages of volcanic ash deposits refine the chronostratigraphy of the Pastos Chicos Basin.
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: Brandenburg Ministry of Sciences, Research and Cultural Affairs, Germany
    Description: Blaustein Fund
    Description: Fulbright Foundation
    Description: France‐Stanford Center for Interdisciplinary Studies
    Description: https://doi.org/10.6084/m9.figshare.20209865.v1
    Keywords: ddc:551.8 ; Puna Plateau ; NW Argentina ; thermochronology ; U–Pb zircon geochronology ; mountain range uplift ; Tectonics
    Language: English
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  • 28
    Publication Date: 2023-06-20
    Description: Thin sections of three Palaeozoic bryozoans reveal fossilized soft tissues that show the position of organic cuticle and internal structures such as the membranous sac and gut. The fossilization occurred apparently due to fast burial under anoxic conditions. The position of a membranous sac in the Permian trepostome Rhombotrypella superangustata is indicative of a progressive polypide cycle. The position of the polypide in the Ordovician Graptodictya delicata behind the superior and interior hemisepta suggests a protective function of the hemisepta.
    Keywords: ddc:564 ; morphology ; Bryozoa ; fossilization ; Palaeozoic
    Language: English
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  • 29
    Publication Date: 2023-06-20
    Description: Whether Archean tectonics were horizontally or vertically dominated is controversially discussed because arguments bear on the kinematics and thermal state of the Archean mantle and constrain the mode of formation of the earliest continental crust. Highly deformed strata of Archean greenstone belts figure prominently in this debate because they record long periods of time and multiple deformation phases. Among the best‐preserved greenstone belts counts the Barberton Greenstone Belt (BGB) of southern Africa. Geological mapping of part of the southern BGB in Eswatini (Swaziland), combined with U‐Pb zircon dating, shows that the region preserves a tightly re‐folded imbricate thrust stack in which metavolcanic and ‐volcaniclastic strata of the Onverwacht Group, deposited at 3.34–3.29 Ga, have been thrust on top of ca. 3.22 Ga siliciclastic strata of the Moodies Group. The structurally highest element, the Malolotsha Syncline, forms a tectonic klippe of substantial size and is 〉1,450 m thick. Forward modeling of a balanced cross section indicates that this thrust stack was part of a northwestward‐verging orogen along the southern margin of the BGB and records a minimum horizontal displacement of 33 km perpendicular to its present‐day faulted, ductily strained and multiply metamorphosed margin. Because conglomerate clasts indicate a significantly higher degree of prolate strain which extends further into the BGB than at its northern margin, late‐stage tectonic architecture of the BGB may be highly asymmetrical. Our study documents that the BGB, and perhaps other Archean greenstone belts, preserves a complex array of both vertically‐ and horizontally‐dominated deformation styles that have interfered with each other at small regional and short temporal scales.
    Description: Plain Language Summary: Worldwide, only a few regions exist where ancient rock strata document how earth cooled, surface strata deformed, and continents grew. It is debated whether vertical movements dominated (akin to a lava lamp) and when major horizontal motions (as they dominate Earth today) began; certainly, there was also overlap between these regimes. Radiometric age dating of zircons extracted from strata along the southern margin of one of the best‐preserved ancient regions in southern Africa, the Barberton Greenstone Belt in Eswatini, show that older strata were thrust there over younger strata for at least 33 km distance subhorizontally. Then they were shingled, and then folded. The results show that even at a time when Earth's oldest continents were just forming, significant horizontal displacements existed already.
    Description: Key Points: U‐Pb zircon dating and geological mapping confirm a folded thrust‐stack along part of the southern margin of the Archean Barberton Greenstone Belt (BGB). Forward modeling of a balanced cross‐section indicates 〉33 km of horizontal shortening toward the northwest. Vertically‐ and horizontally‐dominated tectonics interfered with each other in the BGB and may have done so in other Archean greenstone belts as well.
    Description: Friedrich‐Schiller‐University Jena
    Description: https://doi.org/10.5880/fidgeo.2022.037
    Keywords: ddc:551.8 ; Greenstone Belt ; Archean ; Eswatini ; Klippe ; Barberton ; Swaziland
    Language: English
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  • 30
    Publication Date: 2023-06-12
    Description: Soils and landscapes are bridges of space and time, as they simultaneously and authentically show essential aspects that were previously separated by time and space (such as cultural and activity-related aspects from past and present) to the trained observer - albeit only in excerpts. Therefore, this article presents a series of impact indicators for soil changes, starting with extreme (anthropogenic) interventions and ending with equally extreme ("natural") events. An essential difference to specifically planning-relevant or human ecological concepts, which, for example, specify land use/load categories, is that the following impact indicators perceive soils as a phenomenon in themselves and do not define them through attributed functions. Particular attention is focused on their changeability and vital development potential, as well as on their property as a sphere of penetration of living and material things, with emphasis on the noetic effect. The intervention or event spaces on the earth's surface can be differentiated quantitatively through the type, strength, and duration of the phenomena. The intensity of all processes can be described by amplitude (the strength of the interventions/events) and frequency (the repetition rate of the interventions/events) and can be specifically identified and quantified by, for example, material inputs or outputs per unit of time. For the first time, there would be a system for measuring the ecological quality of anthropogenic land use, which could serve as an "alert system for the external technological culture," and could help us become aware of our "inner" culture.
    Description: research
    Keywords: ddc:550 ; Boden ; Landschaft ; Bodendegeneration ; Deutschland ; Anthropogene Bodenveränderung
    Language: German
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  • 31
    Publication Date: 2023-04-01
    Description: Diese Im Stadtbuch von Göllnitz (Gelnica) unter dem Jahr 1498 eingetragene Stollenordnung für Göllnitz geht auf eine ältere Stollenordnung zurück. Sie wurde anlässlich einer am 5. Oktober 1498 auf Antrag des Kanzlers des Königreiches Ungarn, dem Erzbischof von Gran (Esztergom), Tamás Bakócz (Thomas) in Göllnitz, stattfindenden Verhandlung in das Stadtbuch eingetragen. In dieser Verhandlung ging es um die Klärung eines Rechtsstreites zum Stollenrecht, der Verleihung von Fundgruben samt Stollen sowie der Vermessung der Gruben und Maaßen. Der Rechtsstreit war zwischen Gewerken aus Rosenau (Rožňava) und dem Rat der Bergstadt Rosenau entflammt.
    Description: source
    Keywords: Ungarn ; Slowakei ; Göllnitz/Gelnica ; Zips/Spiš ; Schemnitz/Baňská Štiavnica ; Kremnitz/Kremnica ; Rosenau/Rožňava ; Gran/Esztergom ; Iglau/Jihlava ; Tamás Bakócz (Erzbischof) ; Stephan Zápolya (Oberkammergraf) ; Stollenordnung ; Silberbergbau
    Language: German
    Type: doc-type:book , updatedVersion
    Format: 6
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  • 32
    Publication Date: 2023-04-03
    Description: Digitale Gelände-Modelle (DGM) erstellt aus Laserscan-Daten und Daten der Persistent Scatterer Interferometrie (PSI) bieten Datengrundlagen zur Analyse von großflächigen Bodenbewegungen im cm- und mm-Bereich. Es besteht ein Bedarf an geeigneten Verarbeitungs- und Interpretationswerkzeugen für diese Datenquellen, um sie der breiten Öffentlichkeit zur Nutzung zur Verfügung zu stellen. Die dafür notwendigen Arbeiten werden innerhalb des Umwelt 4.0 – Projektes, Cluster I – „Nutzung digitaler Geländemodelle und Copernicus-Daten“, durchgeführt, welches vom Hessischen Landesamt für Naturschutz, Umwelt und Geologie in Kooperation mit der TU Darmstadt durchgeführt und von der Hessischen Ministerin für Digitale Strategie und Entwicklung gefördert wird. Um automatisch Bewegungs-Hot-Spots in Hessen zu detektieren, werden mittels eines erstellten GIS-Tools Gebiete, die detektierbare Setzungen (Geschwindigkeit 〈 - 2 mm/a) oder Hebungen (Geschwindigkeit 〉 2 mm/a) aufweisen und in denen möglichst viele Persistent Scatterer Bewegungsgeschwindigkeiten aufweisen, ermittelt. Je stärker eine Bodenbewegung ist und je mehr Persistent Scatterer diese Bodenbewegung anzeigen, desto stärker wird dieser Bereich hervorgehoben. Zur Analyse der Bewegungsursachen werden die Zeitreihen mittels Fitting untersucht und des Weiteren mit möglichen Bewegungsursachen der Region verglichen. Um die räumlichen Lücken der Persistent Scatterer Daten in unbebauten Regionen zu füllen, wird an zwei unterschiedlichen Lösungen gearbeitet. Zum einen werden Differenzenkarten aus Digitalen Geländemodellen, die zu unterschiedlichen Zeitpunkten aufgenommen wurden, erstellt. Zum anderen soll das Small Baseline Subset (SBAS)-Verfahren Anwendung finden. Der hier beschriebene Workflow liefert verschiedene Bewegungs-Hot-Spots in Hessen. Anhand von Fallbeispielen werden erste Ergebnisse des Projektes vorgestellt. Die räumliche Fusion der PSI-Daten mit Differenzenkarten und SBAS-Daten ist im weiteren Projektverlauf vorgesehen.
    Description: Hessische Ministerin für Digitale Strategie und Entwicklung
    Description: poster
    Keywords: Fernerkundung ; Sentinel-1 ; Radarinterferometrie ; Laserscan ; Bodenbewegung ; Hessen
    Language: German
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  • 33
    Publication Date: 2023-04-17
    Description: Diese Bergordnung für Kremnitz (Kremnica) wurde am 26. November 1492 auf Initiative des Oberkammergrafen Peter Schaider (hoher Beamter im Königreich Ungarn) sowie des königlichen Bergmeisters und Steigers Niclas Czor in das Stadtbuch von Kremnitz eingetragen. Hintergrund dafür waren wahrscheinlich zunehmende Probleme bei der Einhaltung der gültigen Rechtsnormen des Bergbaus. Beschrieben wurden die Aufnahme von Fundgruben sowie deren Rechte, die Maße des Grubenfeldes die Anforderungen an Schächte und Schürfe und die technische Ausstattung eines Göpels. Bei allen genannten Punkten wurde immer wieder auf altes Recht und Gewohnheit verwiesen.
    Description: source
    Keywords: Slowakei ; Ungarn ; Kremnitz/Kremnica ; Iglau/Jihlava ; Freiberg ; Silberbergbau ; Bergordnung
    Language: German
    Type: doc-type:book , updatedVersion
    Format: 15
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  • 34
    Publication Date: 2023-04-19
    Description: Induced seismicity during mine flooding is the focus of the FloodRisk project. One of the study areas is the Ruhr area, which is characterised by centuries of intensive coal mining. After the closure of the last mines, controlled flooding began. Within the FloodRisk project, we investigate ground uplift, stress changes due to pore pressure changes and the reactivation potential of faults to explain induced seismicity. We concentrate on the seismicity monitoring and geomechanics of the Haus Aden catchment, for which we investigate the relationship between water rise, tectonic stress and induced seismicity. The monitoring of seismicity is based on a network of up to 30 short-period seismic stations installed by the Ruhr University in the area of the former "Bergwerk Ost", which exhibited the highest seismicity in the Ruhr area during active mining. The stations cover an area of about 160 km 2 and are spaced between 0.5 and 3.5 km apart. They allow continuous monitoring of seismicity. Since 2019, more than 2200 induced events have been localised. A prerequisite for the interpretation of seismicity is a detailed localisation of the events. The relative localisation of the induced earthquakes has significantly reduced the location uncertainty and allowed the spatial and temporal evolution of earthquake clusters due to the rise in mine water levels to be studied. The resulting pattern of seismicity was compared with known underground structures. This comparison indicates that most of the events occur approximately 300 m below the main pillars between the longwall panels in the already flooded deepest level of the mine. A generic FE numerical model was developed for a section of the Heinrich Robert mine based on the geometry of the pillars, shafts and longwall panels. The stress data for model calibration are based on a compilation of the regional stress state in the eastern Ruhr area. For this purpose, hydraulic fracture tests carried out in the mines to minimise rock bursts were re-evaluated and compared with stress orientations derived from independent sources such as borehole fractures and earthquake source mechanisms. Using this 3D numerical approach, we conclude that there is increased vertical stress within and below the pillars as a result of stress arching. As the horizontal stress changes below the mine levels are small, this results in increasing differential stresses that can lead to the observed events below the mine level when the mine water level rises.
    Description: Bundesministerium für Bildung und Forschung
    Description: poster
    Keywords: induced seismicity ; post mining ; mine water rise ; numerical stress model ; stress arching ; failure potential
    Language: English
    Type: doc-type:conferenceObject
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  • 35
    Publication Date: 2023-04-22
    Description: Dieser als Freiberger Bergrecht B oder Jüngeres Freiberger Bergrecht bezeichneter Gesetzestext, ist wahrscheinlich nach der Chemnitzer Teilung vom 13. November 1382 entstanden. In 43 Paragrafen wurde das zu dieser Zeit gültige Bergrecht niedergeschrieben. Das Bergrecht ist eine Mischung aus dem Freiberger Bergrecht A und der deutschen Version des Iglauer Bergrechtes. Die Entstehungszeit der verwendeten Variante des Iglauer Bergrechtes ist allerdings unbekannt.
    Description: source
    Keywords: Wilhelm I. Markgraf von Meißen ; Balthasar Landgraf von Thüringen ; Friedrich I. Herzog von Sachsen ; Wilhelm II. Herzog von Sachsen ; Georg Herzog von Sachsen ; Freiberg ; Iglau/Jihlava ; Silberbergbau ; Bergrecht
    Language: German
    Type: doc-type:book , updatedVersion
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  • 36
    Publication Date: 2023-06-16
    Description: The angular momentum of the Earth‐Moon system was initially dominated by Earth's rotation with a short solar day of around 5 hr duration. Since then, Earth gradually transferred angular momentum through tidal friction to the orbit of the Moon, resulting in an increasing orbital radius and a deceleration of Earth's rotation. Geologic observations of tidal deposits can be used to verify and constrain models of lunar orbital evolution. In this work we reexamine the oldest tidal record suitable for analysis from the Moodies Group, South Africa, with an age of 3.22 billion years. Time frequency analysis of the series of thicknesses of the sandstone‐shale layers yields a periodicity of 15.0 layers, taking into account the possibility of missing laminae. Assuming a mixed tidal system, the duration of two neap‐spring‐neap cycles was 30.0 lunar days for dominant semidiurnal or 30.0 sidereal days for dominant diurnal tides. We derive the relationship between this observation and the past Earth‐Moon distance and re‐visit related published work. We find that the Earth‐Moon distance 3.2 billion years ago was about 70% of today's value. The Archean solar day was around 13 hr long. The ratio of solar to lunar tide‐raising torque controls the leakage of angular momentum from the Earth‐Moon system, but deviation from the assumed ratio of 0.211 results in only moderate changes. A duration of a postulated 21‐hr atmospheric resonance shorter than 200 million years would be consistent with our observation; it would significantly alter the Earth‐Moon distance.
    Description: Plain Language Summary: After its formation 4.5 billion years ago, the Moon circled Earth in a low orbit while Earth rotated faster than today around its axis. In the course of time, the Moon gradually evolved to a higher orbit while the rotation of Earth slowed due to the frictional effect of tides. Theoretical models can describe the evolution of the distance between Earth and the Moon with time until today. Counting the thickness of thin sandstone‐shale couplets of known age, which are layered due to tides, can constrain these models. In this work we reexamine the oldest of these geological records in the Moodies Group of South Africa, with an age of 3.2 billion years. The thickness of layers changes with a periodicity of 15 layers which is assumed to originate from varying strengths of currents between successive spring tides. Kepler's third law and the law of conservation of angular momentum allow us to derive the parameters of the lunar orbit from this measurement. According to our analysis, the Earth‐Moon distance was around 70% of today's value 3.2 billion years ago. The faster rotation rate of Earth resulted in a length of day of around 13 hr.
    Description: Key Points: Time frequency analysis yields 30.0 layers per two neap‐spring‐neap cycles, taking missing laminae in the tidal record into account. Earth‐Moon distance of ca. 70% of today's value 3.2 billion years ago results in a solar day of 13 hr duration. Duration of 21‐hr atmospheric resonance for 〈200 million years is consistent with our observation, alters estimate of Earth‐Moon distance.
    Keywords: ddc:523 ; Earth‐Moon system ; lunar orbital evolution ; tidal friction ; Moodies Group ; tidal deposits ; time‐frequency analysis
    Language: English
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  • 37
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    Unknown
    ARGE GMIT, Bonn
    Publication Date: 2023-10-16
    Description: Die Ausgabe der Geowissenschaftlichen Mitteilungen vom September 2023 enthält die Themenblöcke: GEOfokus: Unterbindung förderinduzierter Salzwasseraufstiege in Trinkwasserbrunnen, GEOaktiv (Wirtschaft, Beruf, Forschung und Lehre), GEOlobby (Gesellschaften, Verbände, Institutionen), GEOreport (Geowissenschaftliche Öffentlichkeitsarbeit, Tagungsberichte, Ausstellungen, Exkursionen, Publikationen), GEOszene (Würdigungen, Nachrufe).
    Description: journal
    Keywords: ddc:550 ; GMIT
    Language: German
    Type: doc-type:book , publishedVersion
    Format: 112
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  • 38
    Publication Date: 2023-10-26
    Description: Ocean turbulent mixing is a key process affecting the uptake and redistribution of heat, carbon, nutrients, oxygen and other dissolved gasses. Vertical turbulent diffusivity sets the rates of water mass transformations and ocean mixing, and is intrinsically an average quantity over process time scales. Estimates based on microstructure profiling, however, are typically obtained as averages over individual profiles. How representative such averaged diffusivities are, remains unexplored in the quiescent Arctic Ocean. Here, we compare upper ocean vertical diffusivities in winter, derived from the 7Be tracer‐based approach to those estimated from direct turbulence measurements during the year‐long Multidisciplinary drifting Observatory for the Study of Arctic Climate (MOSAiC) expedition, 2019–2020. We found that diffusivity estimates from both methods agree within their respective measurement uncertainties. Diffusivity estimates obtained from dissipation rate profiles are sensitive to the averaging method applied, and the processing and analysis of similar data sets must take this sensitivity into account. Our findings indicate low characteristic diffusivities around 10〈sup〉−6〈/sup〉 m〈sup〉2〈/sup〉 s〈sup〉−1〈/sup〉 and correspondingly low vertical heat fluxes.
    Description: Plain Language Summary: Ocean turbulent mixing plays an important role in the uptake and redistribution of heat, carbon, nutrients, oxygen and other properties. For example, this process delivers nutrients to the sunlit surface ocean where they are utilized to produce plants (phytoplankton) for the ecosystem food web. However, strong changes in density within the upper Arctic Ocean hinder vertical transport of nutrients, such that nutrient fluxes are generally smaller than those observed elsewhere in the world ocean. Furthermore, low vertical transport rates isolate the surface ocean from heat input from below which helps protect the ice from melting. Here, we compare the strength of upper ocean mixing, an important parameter for the calculation of vertical transport, derived from two independent methods during the MOSAiC (Multidisciplinary drifting Observatory for the Study of Arctic Climate) ice drift experiment, 2019–2020. This comparison allows us to better quantify the vertical diffusivity, and in turn also the vertical transport of for example, heat and nutrients in the ocean.
    Description: Key Points: Arctic Ocean vertical diffusivity (K〈sub〉z〈/sub〉) in the upper halocline in winter is O(10〈sup〉−6〈/sup〉) m〈sup〉2〈/sup〉 s〈sup〉−1〈/sup〉. Diffusivity estimates from 〈sup〉7〈/sup〉Be measurements and ocean microstructure profiling agree within a factor of 2. K〈sub〉z〈/sub〉 estimates from turbulent dissipation rate profiles are sensitive to the averaging method.
    Description: Bundesministerium für Bildung und Forschung http://dx.doi.org/10.13039/501100002347
    Description: Research Council of Norway
    Description: National Science Foundation http://dx.doi.org/10.13039/100000001
    Description: https://doi.org/10.1594/PANGAEA.939816
    Description: https://doi.org/10.26008/1912/bco-dmo.861596.1
    Keywords: ddc:551.46 ; Arctic Ocean ; vertical mixing ; halocline ; winter ; turbulent diffusivity ; microstructure profiling
    Language: English
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  • 39
    Publication Date: 2023-10-26
    Description: Earth's core‐mantle boundary (CMB) shows a complex structure with various seismic anomalies such as the large low shear‐wave velocity provinces (LLSVPs) and ultra‐low velocity zones (ULVZs). As these structures are possibly induced by chemically distinct material forming a layer above the CMB, models of mantle convection made ad hoc assumptions to simulate the dynamics of this layer. In particular, density and mass were prescribed. Both conditions are critical for the dynamics but hardly constrained. Core‐mantle interaction is considered as one possible origin for this dense layer. For example, diffusion‐controlled enrichment of iron has been proposed. We here apply a chemical gradient between the mantle and the denser core to analyze the penetration of dense material into the mantle. As such, we employ 2D Cartesian models where a thermochemical layer at the base of the mantle develops self‐consistently by a diffusive chemical influx. Our simulations indicate that chemical diffusion is strongly affected by the convective mantle flow. This convection‐assisted diffusion yields a compositional influx mainly in the areas where slabs spread over the bottom boundary and sweep dense material aside to form accumulations with rising plumes atop. Like for a prescribed dense layer this process leads to chemically distinct piles, which are typically smaller (therefore more suited to explain ULVZs) but more persistent due to the constant chemical influx. Combining the influx scenario with the primordial layer can possibly explain the simultaneous existence of LLSVPs and ULVZs along with the observation of a core‐like isotopic composition in the mantle.
    Description: Plain Language Summary: The core‐mantle boundary (CMB) shows a complex structure. Seismologists have observed features that are possibly denser than their surroundings. These structures form from a dense layer above the CMB. Therefore typical mantle convection models have assumed an initial dense basal layer. The thickness and density of this prescribed layer are crucial but hardly constrained. Here we investigate core‐mantle interaction as one possible origin for this layer and employ 2D Cartesian models of mantle convection that consider a diffusive chemical gradient between the iron‐rich core and the silicate mantle. Our simulations show that the diffusive influx is coupled to the convective mantle flow. Convection‐assisted diffusion gives a larger influx beneath slabs spreading over the CMB. Additionally, as in the models with a prescribed layer, the rising plumes pull dense material up and form piles. In this study, however, the constant chemical influx leads to piles existing for longer times. The piles are typically smaller but can maybe in combination with a primordial layer explain different seismologically observed structures and the presence of core material in the mantle.
    Description: Key Points: We analyze convection‐assisted core‐mantle interaction in thermochemical mantle convection models. Dense material penetrates into the mantle as a result of a basal diffusive chemical influx, where penetration is promoted by convection. Small piles form with some of the dense core material being entrained by plumes.
    Description: Deutsche Forschungsgemeinschaft
    Description: https://doi.org/10.1080/03091929608208968
    Description: https://doi.org/10.1002/2015GC005807
    Description: https://doi.org/10.35003/JENO4T
    Keywords: ddc:551.1 ; core‐mantle interaction ; mantle convection ; LLSVPs ; ULVZs
    Language: English
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  • 40
    Publication Date: 2023-10-26
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Planetary impacts have shaped the surfaces and interiors of planets. They were particularly critical in the last stage of planetary accretion, as they have eventually formed terrestrial planets. During these large supersonic collisions, shock waves melted the impactor and the target, and formed silicate magma oceans. Because the propagation of shock waves and the melting is faster than the excavation of an impact crater, the cratering stage can be considered as a purely hydrodynamic process. Here, we use both laboratory impact experiments in water and numerical simulations to investigate the crater dimensions resulting from the impact of a liquid impactor onto a liquid target. We show that our numerical models reproduce the laboratory experiments at subsonic impact velocities. We then explore the effect of both the Froude number, which is the ratio of the impactor kinetic energy to gravity, and the Mach number, which is the ratio of the impact speed to the sound speed. We vary these two parameters independently in impact simulations, going from subsonic to supersonic conditions. We obtain a new scaling law for the crater dimensions that describes the transition from subsonic to supersonic impacts. Our results indicate that the transition between these two regimes results from a change in the partitioning of the impactor kinetic energy into potential energy in the crater and internal energy. Finally, our scaling suggests that, in the limit of large Mach numbers, the crater depth depends only on the sound velocity and gravity, and is independent of the impact speed.〈/p〉
    Description: Plain Language Summary: Planetary formation involved a large number of very energetic collisions. Such impacts generated shock waves which led to widespread melting and the formation of magma oceans. Understanding the dynamics of impacts into magma oceans is of great importance as these collisions set the initial temperature and composition of terrestrial planets and satellites. Laboratory experiments and numerical simulations have been used to investigate large impacts. However, each approach has pros and cons. Liquid impact experiments can produce the small scales responsible for the mixing between the impactor and the target, but they fail to reproduce shock waves and supersonic speeds. In contrast, current numerical simulations reach supersonic conditions but produce a limited amount of turbulence and mixing. In this study, we bridge the gap between these two methods and improve our understanding of the effect of the impact velocity on the cratering process. Using the code iSALE, we numerically reproduce water impact experiments at low subsonic velocities. We then explore supersonic conditions in impact simulations. We obtain a new scaling law predicting the crater depth in more realistic impact conditions and show that it is limited only by the sound speed for large impact velocities.〈/p〉
    Description: Key Points: 〈list list-type="bullet"〉 〈list-item〉 〈p xml:lang="en"〉The shock physics code iSALE is successfully benchmarked against subsonic water impact experiments〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉A scaling law is proposed for the crater depth as a function of the Mach and Froude numbers which are varied as independent parameters〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉In the limit of high Mach numbers, our scaling suggests that the maximum crater depth is controlled by the sound velocity and gravity, but not by the impact speed〈/p〉〈/list-item〉 〈/list〉 〈/p〉
    Description: DFG
    Description: EPSRC
    Description: National Aeronautics and Space Administration
    Description: NSF Physics Frontier Center
    Description: Programme National de Planétologie
    Description: CNES
    Description: Alfred P. Sloan Foundation
    Description: https://isale-code.github.io/
    Keywords: ddc:523 ; impact cratering ; pi‐scaling ; magma ocean ; scaling laws ; fluid dynamics
    Language: English
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  • 41
    Publication Date: 2023-10-26
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Atmospheric gravity waves play an important role in driving the dynamics of the Mesosphere and Lower Thermosphere and the basic structure of this region is determined by momentum deposition of these waves. Mesospheric bores are a type of non‐linear response that cause the amplification of gravity wave, due to trapping, that is characterized by a propagating step‐like jump followed by undulating waves. They require a stable layer or duct to travel horizontally with little attenuation thereby capable of transporting wave energy and momentum over larger distances. We present a prominent bright undular bore event observed in the mesospheric O(〈sup〉1〈/sup〉S), O〈sub〉2〈/sub〉, and OH emission layers on 16 March 2021 over Germany. A striking feature of this observation is the capture of bore's rapid dissipation around the center of the imager's field of view. The vertical temperature profile obtained from the satellite data indicates the presence of temperature inversion layer which acted as a thermal duct for the bore propagation. In addition, we have performed idealized two dimensional direct numerical simulations (DNS) of Navier‐Stokes equations under Boussinesq approximation. The DNS results reproduce many important characteristics of the observed airglow event like the nonlinear wave‐steepening, number of trailing waves, and its dissipation by implementing a thermal duct and a wave‐like perturbation. Furthermore, the DNS results also indicate that the duct width and amplitude of the initial perturbation have a considerable effect on the bore morphology.〈/p〉
    Description: Key Points: 〈list list-type="bullet"〉 〈list-item〉 〈p xml:lang="en"〉Observation of a mesospheric bright bore event that dissipated within the field of view〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉The duct that enabled the bore propagation was near the O(〈sup〉1〈/sup〉S) emission layer based on the observational data〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉The majority of the observed features are reproduced with idealized 2D direct numerical simulations using Boussinesq approximation〈/p〉〈/list-item〉 〈/list〉 〈/p〉
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: Alexander von Humboldt‐Stiftung http://dx.doi.org/10.13039/100005156
    Description: https://doi.org/10.22000/809
    Description: http://sirius.bu.edu/data/
    Description: http://saber.gats-inc.com/coin.php
    Keywords: ddc:551.5 ; bores ; direct numerical simulations ; gravity waves ; inversion layers
    Language: English
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  • 42
    Publication Date: 2023-10-24
    Description: Small stress changes such as those from sea level fluctuations can be large enough to trigger earthquakes. If small and large earthquakes initiate similarly, high‐resolution catalogs with low detection thresholds are best suited to illuminate such processes. Below the Sea of Marmara section of the North Anatolian Fault, a segment of ≈ $\approx $150 km is late in its seismic cycle. We generated high‐resolution seismicity catalogs for a hydrothermal region in the eastern Sea of Marmara employing AI‐based and template matching techniques to investigate the link between sea level fluctuations and seismicity over 6 months. All high resolution catalogs show that local seismicity rates are larger during time periods shortly after local minima of sea level, when it is already rising. Local strainmeters indicate that seismicity is promoted when the ratio of differential to areal strain is the largest. The strain changes from sea level variations, on the order of 30–300 nstrain, are sufficient to promote seismicity.
    Description: Plain Language Summary: Quasi‐periodic phenomena are a natural probe to test how the Earth's responses to a certain stress perturbation. High‐resolution catalogs with low detection thresholds may provide a new opportunity to look for this type of earthquake triggering. A segment of 150 km below the Sea of Marmara section of the North Anatolian Fault is late in its seismic cycle. Here, we generated high‐resolution seismicity catalogs for 6 months covering a hydrothermal region south of Istanbul in the eastern Sea of Marmara including seismicity up to MW 4.5. For first time in this region, we document a strong effect of the Sea of Marmara water level changes on the local seismicity. Both high‐resolution catalogs show that local seismicity rates are significantly larger during time periods shortly after local minima on sea level, when the sea level is rising. The available local instrumentation provided an estimate of the strain changes that were sufficient to promote seismicity. If such small stress perturbations from sea level changes are enough to trigger seismicity, it may suggest that the region is very close to failure.
    Description: Key Points: We generated enhanced seismicity catalogs to investigate the potential link between sea level change and seismicity in a hydrothermal region. Higher seismicity rates from the entire and declustered catalogs are observed during time periods when sea level is rising. Strain estimates from local strainmeters show that seismicity was promoted during reduced normal and enhanced shear strain conditions.
    Description: Helmholtz Association http://dx.doi.org/10.13039/501100009318
    Description: Alexander von Humboldt‐Stiftung http://dx.doi.org/10.13039/100005156
    Description: National Science Foundation http://dx.doi.org/10.13039/100000001
    Description: National Aeronautics and Space Administration http://dx.doi.org/10.13039/100000104
    Description: VW momentum
    Description: https://tdvms.afad.gov.tr/
    Description: http://www.koeri.boun.edu.tr/sismo/2/earthquake-catalog/
    Description: https://www.unavco.org/data/strain-seismic/bsm-data/bsm-data.html
    Keywords: ddc:551.22 ; seismicity catalog ; sea level change ; hydrothermal region ; strain ; strainmeter ; solid Earth tides
    Language: English
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  • 43
    Publication Date: 2023-10-24
    Description: Trends in flood magnitudes vary across the conterminous USA (CONUS). There have been attempts to identify what controls these regionally varying trends, but these attempts were limited to certain—for example, climatic—variables or to smaller regions, using different methods and datasets each time. Here we attribute the trends in annual maximum streamflow for 4,390 gauging stations across the CONUS in the period 1960–2010, while using a novel combination of methods and an unprecedented variety of potential controlling variables to allow large‐scale comparisons and minimize biases. Using process‐based flood classification and complex networks, we find 10 distinct clusters of catchments with similar flood behavior. We compile a set of 31 hydro‐climatological and land use variables as predictors for 10 separate Random Forest models, allowing us to find the main controls the flood magnitude trends for each cluster. By using Accumulated Local Effect plots, we can understand how these controls influence the trends in the flood magnitude. We show that hydro‐climatologic changes and land use are of similar importance for flood magnitude trends across the CONUS. Static land use variables are more important than their trends, suggesting that land use is able to attenuate (forested areas) or amplify (urbanized areas) the effects of climatic changes on flood magnitudes. For some variables, we find opposing effects in different regions, showing that flood trend controls are highly dependent on regional characteristics and that our novel approach is necessary to attribute flood magnitude trends reliably at the continental scale while maintaining sensitivity to regional controls.
    Description: Key Points: A wide variety of controls are necessary to explain flood magnitude trends across the United States between 1960 and 2010. Climatic changes and land cover conditions are of similar importance for flood magnitude trends at the regional scale. Controls on flood trends can have highly nonlinear effects and can have opposing effects in different hydro‐climatological subregions.
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: USACE Water Institute
    Description: Bundesministerium für Bildung und Forschung http://dx.doi.org/10.13039/501100002347
    Description: https://nwis.waterdata.usgs.gov/usa/nwis/peak
    Description: https://water.usgs.gov/GIS/metadata/usgswrd/XML/streamgagebasins.xml
    Description: https://psl.noaa.gov/
    Description: https://www.sciencebase.gov/catalog/item/59692a64e4b0d1f9f05fbd39
    Keywords: ddc:551.48 ; annual maximum flood ; magnitude trends ; drivers ; Random Forest ; clustering ; climate change
    Language: English
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  • 44
    Publication Date: 2023-10-24
    Description: 〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉In a reconnaissance study, we investigated the potential of γ‐ray induced production of 〈sup〉38〈/sup〉Ar〈sub〉K〈/sub〉 from 〈sup〉39〈/sup〉K for geochronological applications. For this purpose, various age monitors commonly in use for the established 〈sup〉40〈/sup〉Ar/〈sup〉39〈/sup〉Ar‐method were co‐irradiated for 60 h at 17.6 MeV maximum energy in the ELBE facility, Dresden‐Rossendorf, Germany. Because the available energy was low, total production of 〈sup〉38〈/sup〉Ar〈sub〉K〈/sub〉 was depressed, leading to low 〈italic toggle="no"〉J〈/italic〉〈sub〉38〈/sub〉‐values of (2.1–4.1) × 10〈sup〉‐6〈/sup〉 and hence resulted in only minor 〈sup〉38〈/sup〉Ar excess when compared with atmospheric 〈sup〉38〈/sup〉Ar〈sub〉/〈/sub〉〈sup〉36〈/sup〉Ar ratios. In spite of these restrictions, ages of younger monitors could be reproduced within error, whereas older age reference materials showed discrepancies due to the low production rate. We observed Ca‐derived contributions on 〈sup〉36〈/sup〉Ar in analysed CaF〈sub〉2〈/sub〉 reference materials, and calculated a limit for Ca‐interference on 〈sup〉38〈/sup〉Ar〈sub〉Ca〈/sub〉 of (〈sup〉38〈/sup〉Ar/〈sup〉36〈/sup〉Ar)〈sub〉Ca〈/sub〉 = 0.07 ± 0.03 (1〈italic toggle="no"〉s〈/italic〉). In addition, we investigated a potential recoil redistribution of 〈sup〉38〈/sup〉Ar by stepwise heating experiments, but could not quantify this further because of concurring processes. More work at higher photon energies is necessary to resolve other open issues, in particular the potential of utilising 〈sup〉40〈/sup〉Ar/〈sup〉37〈/sup〉Ar ratios for age determination and the possibility of 〈sup〉42〈/sup〉Ar production from 〈sup〉44〈/sup〉Ca, which would allow correction for Ca‐interference reactions on other Ar isotopes. This would be a pre‐requisite for dating extra‐terrestrial rocks.〈/p〉
    Description: Klaus‐Tschira‐Stiftung gGmbH
    Keywords: ddc:550.724 ; geochronology ; γ‐irradiation ; 40Ar/39Ar dating ; age spectra ; isochrons
    Language: English
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  • 45
    Publication Date: 2023-10-24
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Evapotranspiration of urban street trees is essential in mitigating urban heat islands due to its cooling effect. However, current shifts in rainfall and temperature regimes towards drier and hotter periods in Central Europe have caused substantial water stress for street trees. Quantifying and subsequently managing these changing dynamics as well as estimating evapotranspiration and water availability is necessary but at the same time extremely challenging in urban environments. Both dynamics are influenced by soil sealing and complex shading patterns of the surrounding street canyon, which vary on a small spatial scale as a function of the canyon layout and orientation. In the present study, the diurnal patterns of six typical urban shading types for street trees were derived by considering a large set of street orientations, widths and tree positions within the street canyon. A shading model was integrated into a hydrological urban tree model to assess the impact of those shading types on diurnal patterns of radiation and evapotranspiration rates calculated using the Penman–Monteith approach and the resulting soil moisture conditions for several vegetation seasons and water‐supply scenarios. The modelling results showed that the six shading patterns significantly influenced the simulated hourly, daily and seasonal potential and actual evapotranspiration rates and water availability. Shaded trees have a substantially reduced, simulated water stress period, regardless of initial water supply, and are able to provide a longer‐lasting cooling function during dry periods due to higher evapotranspiration rates later in the summer season.〈/p〉
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: Federal Ministry for the Environment, Nature Conservation, Nuclear Safety and Consumer Protection http://dx.doi.org/10.13039/501100013549
    Keywords: ddc:577.2 ; diffuse radiation ; direct radiation ; evapotranspiration (ET) ; global radiation ; shading ; urban environment ; urban trees ; water stress
    Language: English
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  • 46
    Publication Date: 2023-10-24
    Description: Similar to other research fields, new knowledge in the Earth System Sciences is increasingly produced by computational research. However, the reproducibility of this type of research has been shown to be very limited, and its efficiency and quality need to be improved. Reproducibility requires researchers to publish both their research outcome in the form of a paper and their research workflows, software and data so that other researchers can reproduce the findings without any further support still years later. Efficient and high-quality computational research requires skills beyond programming as well as the capacity for software maintenance. Inspired by a best-practice example from the Netherlands, we provide 15 recommendations for universities, research funders and the scientific community who wish to support the development of sustainable high-quality computational research in Germany. They relate to the training and support of researchers by universities and other research organizations and to research funding. Of particular importance are options for establishing institutional support by research software engineers who are employed in permanent positions, funding of research software as research infrastructure as well as approaches for increasing the scientific merit that is achieved by producing sustainable research software and providing reproducible research output.
    Description: Deutsche Forschungsgemeinschaft, Rundgespräch DO 737/22-1
    Description: report
    Language: English
    Type: doc-type:book
    Format: 10
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  • 47
    Publication Date: 2023-10-24
    Description: 〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Complex functional materials play a crucial role in a broad range of energy‐related applications and in general for materials science. Revealing the structural mechanisms is challenging due to highly correlated coexisting phases and microstructures, especially for 〈italic〉in situ〈/italic〉 or 〈italic〉operando〈/italic〉 investigations. Since the grain sizes influence the properties, these microstructural features further complicate investigations at synchrotrons due to the limitations of illuminated sample volumes. In this study, it is demonstrated that such complex functional materials with highly correlated coexisting phases can be investigated under 〈italic〉in situ〈/italic〉 conditions with neutron diffraction. For large grain sizes, these experiments are valuable methods to reveal the structural mechanisms. For an example of 〈italic〉in situ〈/italic〉 experiments on barium titanate with an applied electric field, details of the electric‐field‐induced phase transformation depending on grain size and frequency are revealed. The results uncover the strain mechanisms in barium titanate and elucidate the complex interplay of stresses in relation to grain sizes as well as domain‐wall densities and mobilities.〈/p〉
    Description: 〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉This work reports 〈italic〉in situ〈/italic〉 neutron diffraction experiments on a broad range of grain sizes of barium titanate. The study reveals the grain‐size‐dependent strain mechanisms and shows the competitiveness of neutron diffraction with high‐resolution synchrotron diffraction.〈boxed-text position="anchor" content-type="graphic" xml:lang="en"〉〈graphic position="anchor" id="jats-graphic-1" xlink:href="urn:x-wiley:16005767:jcr2vb5054:jcr2vb5054-fig-0001"〉 〈alt-text〉image〈/alt-text〉 〈/graphic〉〈/boxed-text〉〈/p〉
    Keywords: ddc:550.724 ; ddc:548 ; neutron diffraction ; in situ ; applied electric fields ; barium titanate ; strain mechanisms ; grain sizes ; complex functional materials ; microstructures ; coexisting phases
    Language: English
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  • 48
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    Institut für Geographie und Geologie der Universität Greifswald
    Publication Date: 2023-11-25
    Description: Dieser Sammelband umfasst verschiedene Arbeiten zum Thema Tauchsport und dessen Einfluss auf marine Ökosysteme. Aus verschiedenen interdisziplinären Perspektiven setzen sich die Autor*innen des Bandes mit dem Nutzen des Tauchsports für einen verbesserten marinen Artenschutz auseinander.
    Description: Der Druck dieser Publikation wurde aus dem Teilprojekt Fragmentierte Transformation des Interdisziplinären Forschungszentrums Ostseeraum finanziert.
    Description: Tauchtourismus in marinen Schutzgebieten als nachhaltige Meeresnutzung – Eine Fallstudie in den ägyptischen Northern Red Sea Islands5 ; A matter of affection? – The role of SCUBA divers’ emotions and nature affiliation in divers’ site-specific and everyday behaviour concerning coral reef conservation37 ; Perspektiven des Tauchens als Beitrag zu einer Ocean Literacy – Ergebnisse einer Fallstudie am Roten Meer (Soma Bay, Ägypten)64 ;
    Description: research
    Keywords: Tauchen ; Nachhaltigkeit ; Ocean Literacy ; Meeresschutz ; Ägypten
    Language: German
    Type: doc-type:book
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  • 49
    Publication Date: 2023-12-05
    Description: Cloud ice particle effective radius in atmospheric models is usually parametrized. A widely‐used parametrization comprises a strong dependence on the temperature. Utilizing available satellite‐based estimates of both cloud ice particle effective radius and cloud‐top temperature we evaluate if a similar temperature‐dependence exists in these observations. We find that for very low cloud‐top temperatures the modeled cloud ice particle effective radius generally agrees on average with satellite observations. For high sub‐zero temperatures however, the modeled cloud ice particle effective radius becomes very large, which is not seen in the satellite observations. We conclude that the investigated parametrization for the cloud ice particle effective radius, and parametrizations with a similar temperature dependence, likely produce systematic biases at the cloud top. Supporting previous studies, our findings suggest that the vertical structure of clouds should be taken into account as factor in potential future updates of the parametrizations for cloud ice particle effective radius.
    Description: Plain Language Summary: Atmospheric models are often used to diagnose and predict the atmospheric state including clouds. One very important property of clouds that consist of ice particles is the cloud ice particle effective radius. This ice effective radius is based on assumptions about the size and shapes of the ice particles in clouds, and thus parametrized, and is one of the important variables needed for calculating the effect of clouds on electromagnetic radiation, in particular on the solar radiation that enters the Earth's atmosphere. In our study we found that the parametrized ice effective radius agrees well on average and global scale with the ice effective radius inferred from satellite observations for cold clouds. However, we also found that for warmer ice clouds the parametrized ice effective radius is much higher than in satellite observations. Our study suggests that parametrizations of the ice effective radius used in atmospheric models show potential for improvements.
    Description: Key Points: Comparisons of modeled cloud ice particle effective radius with satellite observations are presented. For very low cloud temperatures the modeled cloud ice particle effective radius agrees on average with satellite observations. Modeled large cloud ice particle effective radii for high sub‐zero temperatures are not found in satellite observations.
    Description: European Space Agency http://dx.doi.org/10.13039/501100000844
    Description: https://doi.org/10.5281/zenodo.7445152
    Description: https://doi.org/10.5676/DWD/ESA_Cloud_cci/AVHRR-PM/V003
    Description: https://doi.org/10.5676/EUM_SAF_CM/CLARA_AVHRR/V002
    Description: http://doi.org/10.5067/MODIS/MYD06_L2.NRT.061
    Keywords: ddc:551.5 ; clouds ; ice particle effective radius ; parametrization ; model ; satellite observations
    Language: English
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  • 50
    Publication Date: 2023-12-05
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉This manuscript presents a study of oceanic diurnal warm layers (DWLs) in kilometer‐scale global coupled simulations and their impact on atmospheric convection in the tropics. With the implementation of thin vertical levels in the ocean, DWLs are directly resolved, and sea surface temperature (SST) fluctuations of up to several Kelvin appear in regions with low wind and high solar radiation. The increase of SST during the day causes an abrupt afternoon increase of atmospheric moisture due to enhanced latent heat flux (LHF), followed by an increase in cloud cover (CC) and cloud liquid water (CLW). However, although the diurnal SST amplitude is even exaggerated in comparison to reanalysis, this effect only lasts for 5–6 hr and leads to an absolute difference of 1% for CC and 0.01 kg m〈sup〉−2〈/sup〉 for CLW. This can be explained by the fact that the low wind over the SST anomalies dampens their potential effect on the LHF and hence clouds. All in all, the impact of DWLs on convective CC is found to be negligible in the tropical mean.〈/p〉
    Description: Plain Language Summary: The diurnal fluctuations of sea surface temperature (SST) have been extensively studied for the last decades, but the assessment of the importance of this phenomenon for atmospheric convection on the global scale has come within reach only very recently, thanks to the development of simulations with a horizontal resolution of O(1 km). In this manuscript we show that we can indeed observe an impact of SST fluctuations on moisture in the atmosphere. However, the impact on the amount of clouds in the tropics is found to be short‐lived and its magnitude negligible on average.〈/p〉
    Description: Key Points: 〈list list-type="bullet"〉 〈list-item〉 〈p xml:lang="en"〉diurnal warm layers (DWLs) increase atmospheric moisture〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉The increase of cloud cover (CC) following the formation of a DWL is immediate and only lasts for several hours〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉The magnitude of the CC increase is small and has no discernible influence on the global mean〈/p〉〈/list-item〉 〈/list〉 〈/p〉
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: https://gotm.net/
    Description: https://hdl.handle.net/21.11116/0000-000C-1447-E
    Keywords: ddc:551 ; diurnal warm layers (DWLs) ; atmospheric moisture ; cloud cover ; convection
    Language: English
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  • 51
    Publication Date: 2023-12-05
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Unlike actual rainfall, the spatial extent of rainfall maps is often determined by administrative and political boundaries. Similarly, data from commercial microwave links (CMLs) is usually acquired on a national basis and exchange among countries is limited. Up to now, this has prohibited the generation of transboundary CML‐based rainfall maps despite the great extension of networks across the world. We present CML based transboundary rainfall maps for the first time, using independent CML data sets from Germany and the Czech Republic. We show that straightforward algorithms used for quality control strongly reduce anomalies in the results. We find that, after quality control, CML‐based rainfall maps can be generated via joint and consistent processing, and that these maps allow to seamlessly visualize rainfall events traversing the German‐Czech border. This demonstrates that quality control represents a crucial step for large‐scale (e.g., continental) CML‐based rainfall estimation.〈/p〉
    Description: Plain Language Summary: Rainfall maps are usually based on gauge observations on the ground or radar. They are crucial for predicting or reconstructing flooding events. Commercial microwave links are special kinds of rainfall sensors. Their actual purpose is the signal propagation within a cellular network. However, since the signal is attenuated when it rains, they can also be exploited for rainfall estimation. To estimate rainfall from the observed attenuation requires careful data processing. Algorithms for that are usually adjusted to national data sets with their specific characteristics. In this study, we use, for the first time, two independent data sets of commercial microwave links (from Germany and the Czech Republic) with the aim of generating transboundary rainfall maps. As the data sets vary in many respects, several algorithms need to be adjusted and extended to allow processing them consistently. We show that it is possible to create meaningful rainfall maps of rain events that traverse the border between Germany and the Czech Republic. This can be considered a major step toward seamless rainfall maps on even larger, that is, continental scale.〈/p〉
    Description: Key Points: 〈list list-type="bullet"〉 〈list-item〉 〈p xml:lang="en"〉Transboundary rainfall maps based on independent networks of commercial microwave links (CMLs) are generated for the first time〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉German and Czech data sets of CMLs differ significantly with respect to network characteristics〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉Quality control is important for heterogeneous data of CMLs〈/p〉〈/list-item〉 〈/list〉 〈/p〉
    Description: German Research Foundation
    Description: Czech Science Foundation
    Description: https://doi.org/10.5281/zenodo.4810169
    Description: https://doi.org/10.5281/zenodo.7973736
    Description: https://opendata.dwd.de/climate_environment/CDC
    Keywords: ddc:551.6 ; transboundary rainfall maps ; commercial microwave links ; quantitative precipitation estimation ; data quality control
    Language: English
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  • 52
    Publication Date: 2023-12-05
    Description: An important aspect of rainfall estimation is to accurately capture extreme events. Commercial microwave links (CMLs) can complement weather radar and rain gauge data by estimating path‐averaged rainfall intensities near ground. Our aim with this paper was to investigate attenuation induced complete loss of signal (blackout) in the CML data. This effect can occur during heavy rain events and leads to missing extreme values. We analyzed 3 years of attenuation data from 4,000 CMLs in Germany and compared it to a weather radar derived attenuation climatology covering 20 years. We observed that the average CML experiences 8.5 times more blackouts than we would have expected from the radar derived climatology. Blackouts did occur more often for longer CMLs (e.g., 〉10 km) despite their increased dynamic range. Therefore, both the hydrometeorological community and network providers can consider our analysis to develop mitigation measures.
    Description: Plain Language Summary: Commercial microwave links (CMLs) are used to transmit information between towers of cellphone networks. If there is rainfall along the transmission path, the signal level is attenuated. By comparing the transmitted and received signal levels, the average rainfall intensity along the path can be estimated. If the attenuation is too strong, no signal is received, no information can be transmitted and no rainfall estimate is available. This is unfavorable both for network stability and rainfall estimation. In this study, we investigated the frequency of such blackouts in Germany. How many blackouts per year are observed in a 3 year CML data set covering around 4,000 link paths and how many are expected from 20 years of weather radar data? We observed that the average CML experiences 8.5 times more blackouts than we would have expected from the radar derived climatology. Blackouts did occur more often for long CMLs, which was an unexpected finding. While only one percent of the annual rainfall amount is missed during blackouts, the probability that a blackout occurs was very high for high rain rates. Both, the hydrometeorological community and network providers can consider our analysis to develop mitigation measures.
    Description: Key Points: Complete loss of commercial microwave link (CML) signals during heavy rain leads to missing rainfall extremes. Magnitude of observed blackouts exceeds climatologically expected values. Unexpectedly, longer CMLs experience more blackouts.
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: Helmholtz Association http://dx.doi.org/10.13039/501100009318
    Description: Bundesministerium für Bildung und Forschung http://dx.doi.org/10.13039/501100002347
    Description: Karlsruhe Institute of Technology http://dx.doi.org/10.13039/100009133
    Description: https://doi.org/10.5281/zenodo.7245440
    Description: https://github.com/pycomlink/pycomlink/blob/12fc302539851b19f7656cf7e2438c0ddbaa48bf/notebooks/Blackout%20gap%20detection%20examples.ipynb
    Description: https://doi.org/10.5281/zenodo.6337557
    Description: https://doi.org/10.5676/DWD/RADKLIM_YW_V2017.002
    Keywords: ddc:551.6 ; commercial microwave links ; rainfall ; opportunistic sensing ; weather radar ; rainfall extremes ; precipitation
    Language: English
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  • 53
    Publication Date: 2023-12-05
    Description: The Arctic is warming much faster than the global average. This is known as Arctic Amplification and is caused by feedbacks in the local climate system. In this study, we explore a previously proposed hypothesis that an associated wind feedback in the Barents Sea could play an important role by increasing the warm water inflow into the Barents Sea. We find that the strong recent decrease in Barents Sea winter sea ice cover causes enhanced ocean‐atmosphere heat flux and a local air temperature increase, thus a reduction in sea level pressure and a local cyclonic wind anomaly with eastward winds in the Barents Sea Opening. By investigating various reanalysis products and performing high‐resolution perturbation experiments with the ocean and sea ice model FESOM2.1, we studied the impact of cyclonic atmospheric circulation changes on the warm Atlantic Water import into the Arctic via the Barents Sea and Fram Strait. We found that the observed wind changes do not significantly affect the warm water transport into the Barents Sea, which rejects the wind‐feedback hypothesis. At the same time, the cyclonic wind anomalies in the Barents Sea increase the amount of Atlantic Water recirculating westwards in Fram Strait by a downslope shift of the West Spitsbergen Current, and thus reduce Atlantic Water reaching the Arctic basin via Fram Strait. The resulting warm‐water anomaly in the Greenland Sea Gyre drives a local anticyclonic circulation anomaly.
    Description: Plain Language Summary: The Barents Sea has been experiencing a rapid decrease in its winter sea ice extent during the last 30 years. The loss of sea ice creates new areas where, in winter, the relatively warm ocean loses heat to the cold atmosphere. As warm air rises, the warming reduces the sea level air pressure, changing the atmospheric circulation to develop a local anticlockwise wind system centered over the northern Barents Sea. The associated eastward winds in the Barents Sea Opening and southeastward winds in Fram Strait affect how warm water from the North Atlantic moves toward the Arctic. There has been a long debate on whether this wind anomaly can increase the warm Atlantic Water transport into the Barents Sea and thus cause a positive feedback mechanism for further reducing the sea ice through melting. We find that the observed atmospheric circulation changes have no significant impact on the Barents Sea warm water inflow and thus reject the wind feedback as a strong player in contributing to Arctic Amplification. However, strong anomalous southeastward winds in Fram Strait and the northern Nordic Seas cause a southward shift of the warm Atlantic Water recirculation and reduce its flow toward the Arctic.
    Description: Key Points: A hypothesis that a wind feedback contributes to Arctic Amplification is rejected by performing dedicated wind perturbation simulations. Winter sea ice retreat in the northern Barents Sea causes anomalous cyclonic winds by locally enhancing ocean heat loss. Anomalous cyclonic winds result in less Atlantic Water transport through Fram Strait.
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: North‐German Supercomputing Alliance
    Description: https://github.com/FESOM/fesom2
    Description: https://doi.org/10.7265/N5K072F8
    Description: https://doi.org/10.5065/D6HH6H41
    Description: https://doi.org/10.5065/D6WH2N0S
    Description: https://github.com/FESOM/pyfesom2
    Description: https://doi.org/10.5281/zenodo.7458143
    Keywords: ddc:551 ; Barents Sea ; Arctic Amplification ; feedback ; Atlantic water ; modeling ; Fram Strait
    Language: English
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  • 54
    Publication Date: 2023-12-04
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Knowledge of the shock behavior of planetary materials is essential to interpret shock metamorphism documented in rocks at hypervelocity impact structures on Earth, in meteorites, and in samples retrieved in space missions. Although our understanding of shock metamorphism has improved considerably within the last decades, the effects of friction and plastic deformation on shock metamorphism of complex, polycrystalline, non‐porous rocks are poorly constrained. Here, we report on shock‐recovery experiments in which natural granite was dynamically compressed to 0.5–18 GPa by singular, hemispherically decaying shock fronts. We then combine petrographic observations of shocked samples that retained their pre‐impact stratigraphy with distributions of peak pressures, temperatures, and volumetric strain rates obtained from numerical modeling to systematically investigate progressive shock metamorphism of granite. We find that the progressive shock metamorphism of granite observed here is mainly consistent with current classification schemes. However, we also find that intense shear deformation during shock compression and release causes the formation of highly localized melt veins at peak pressures as low as 6 GPa, which is an order of magnitude lower than currently thought. We also find that melt veins formed in quartz grains compressed to >10–12 GPa contain the high‐pressure silica polymorph stishovite. Our results illustrate the significance of shear and plastic deformation during hypervelocity impact and bear on our understanding of how melt veins containing high‐pressure polymorphs form in moderately shocked terrestrial impactites or meteorites.〈/p〉
    Description: Plain Language Summary: When asteroids, comets, or smaller fragments thereof impact the solid surfaces of planets, moons, or other asteroids, the rocks they strike undergo sudden and irreversible changes while an impact crater forms. These material changes are called shock metamorphism and result from the extremely high pressures, temperatures, and deformation rates caused by the impact. However, the role of rapid shear deformation on impact heating and shock metamorphism is poorly understood. Using a novel experimental setup, we performed shock‐wave experiments with granite, a naturally occurring rock, that allows us to study the role of extreme deformation rates during impact‐crater formation. Furthermore, our experimental setup allows us to avoid several pitfalls such as excavation and ejection of shocked material from a growing impact crater or multiple reflections of shock waves at sample containers that typically plagued previous experiments. We find that intense shear deformation during crater formation results in significant but highly localized heating. This additional heating causes melting of granite at shock pressures as low as 6 GPa, which is about 10 times less than currently thought. Our findings may explain how thin melt veins often observed in shock‐metamorphosed meteorites or rocks sampled from terrestrial impact craters have formed.〈/p〉
    Description: Key Points: 〈list list-type="bullet"〉 〈list-item〉 〈p xml:lang="en"〉We performed shock recovery experiments with granite and spherically decaying compressive waves; numerical models constrain peak pressures〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉Shocked granite samples are found to retain pre‐impact stratigraphy and to document shock‐stage transitions between 〈0.5 and ∼18 GPa〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉Shear‐induced melting of granite at bulk peak pressures as low as 6 GPa; stishovite nucleated as a liquidus phase in melt veins at >10 GPa〈/p〉〈/list-item〉 〈/list〉 〈/p〉
    Description: Japan Society for the Promotion of Science
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Keywords: ddc:https://isale-code.github.io/terms-of-use.html ; ddc:https://doi.org/10.5281/zenodo.7881492 ; ddc:552 ; shock metamorphism ; granite ; stishovite ; melt vein ; shock recovery ; numerical modeling
    Language: English
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  • 55
    Publication Date: 2023-12-04
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉The lunar regolith breccia Dhofar 1769, which was found in 2012 as a single 125 g piece in the Zufar desert area of Oman, contains a relatively large, dark‐colored impact melt breccia embedded in a fine‐grained clastic matrix. The internal texture of the fragment indicates the repeated melt breccia formation on the lunar surface, their repeated brecciation, and mixing in second, third, and fourth generations of brecciated rock types. The chemical and mineralogical data reveal the incorporation of a feldspar‐rich subophitic crystalline melt within a feldspar‐rich microporphyritic crystalline melt breccia. This lithic paragenesis itself is embedded within a mafic, crystalline melt breccia. The entire breccia with the three different impact melts has been finally incorporated into the whole rock breccia. The three impact melts are mixtures of different source rocks and impact projectiles, based on the obtained minor and trace element compositions (in particular of Ni and the rare earth elements [REE]) of the impact melt lithologies. For all processes of impact melt formation, additional steps of their brecciation and re‐lithification require a minimum number of seven impact processes.〈/p〉
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Keywords: ddc:552 ; Dhofar 1769 ; lunar regolith breccia ; impact melt formation ; brecciation ; re-lithification ; impact processes
    Language: English
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  • 56
    Publication Date: 2023-11-20
    Description: Trong bối cảnh đó, Sổ tay về Nhà ở Xanh và Sống Lành mạnh đã được xây dựng với sự hỗ trợ của dự án CAMaRSEC do Chính phủ Đức tài trợ. Với nỗ lực truyền bá các khái niệm và thực hành về nhà ở bền vững và sống lành mạnh cho công chúng, Sổ tay sử dụng ngôn ngữ “không chuyên môn” và “dễ hiểu”, hiệu ứng hình ảnh phù hợp và thiết kế thân thiện với người đọc. Đối tượng chính của Sổ tay là tầng lớp trung lưu tại các đô thị phát triển nhanh chóng (được gọi là “người tiêu dùng mới”), cơ quan chính quyền các cấp, doanh nghiệp, đặc biệt là các công ty trong ngành xây dựng, kiến trúc sư, giáo viên, sinh viên và tất cả các đối tượng quan tâm đến Nhà ở Xanh và Cuộc sống Lành mạnh. Nội dung tuân theo cách tiếp cận toàn diện đa ngành, cung cấp các hướng dẫn thiết thực để lập kế hoạch, thiết kế, xây dựng, vận hành và bảo trì, các khía cạnh hành vi và nhà ở bền vững để cải thiện hiệu quả năng lượng và cuộc sống lành mạnh. Nội dung cuốn sách tập trung vào loại hình nhà chung cư cao tầng, là loại hình nhà có tốc độ phát triển nhanh nhất tại Việt Nam, nhưng các nguyên tắc và giải pháp được giới thiệu cũng có thể áp dụng cho các loại hình nhà ở khác tại Việt Nam.
    Description: BMBF (Bundesministerium für Bildung und Forschung)
    Description: lecture
    Type: doc-type:book , publishedVersion
    Format: 130
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  • 57
    Publication Date: 2023-11-24
    Description: This study investigates the impact of increased global warming on heat stress changes and the potential number of people exposed to heat risks over Africa. For this purpose a heat index has been computed based on an ensemble‐mean of high‐resolution regional climate model simulations from the Coordinated Output for Regional Evaluations embedded in the COordinated Regional Climate Downscaling EXperiment, under two Representative Concentration Pathways (RCPs) scenarios (RCP2.6 and RCP8.5), combined with projections of population growth developed based on the Shared Socioeconomic Pathways (SSPs) scenarios (SSP1 and SSP5). Results show that by the late 21st century, the increased global warming is expected to induce a 12‐fold increase in the area extent affected by heat stress of high‐risk level. This would result in an increase of about 10%–30% in the number of days with high‐risk heat conditions, as well as about 6%–20% in their magnitude throughout the seasonal cycle over West, Central, and North‐East Africa. Therefore, and because of the lack of adaptation and mitigation policies, the exacerbation of ambient heat conditions could contribute to the exposure of about 2–8.5 million person‐events to heat stress of high‐risk level over Burkina Faso, Ghana, Niger, and Nigeria. Furthermore, it was found that the interaction effect between the climate change and population growth seems to be the most dominant in explaining the total changes in exposure due to moderate and high heat‐related risks over all subregions of the African continent.
    Description: Plain Language Summary: This study investigates the impact of increased global warming on heat stress changes and the potential number of persons likely to be exposed to heat risks over Africa. Results show that by the end of the 21st century, the increased global warming is expected to induce a 12‐fold increase in the total area affected by dangerous heat conditions over the continent. This would result in an increase of about 10%–30% in the number of days with these heat conditions, as well as about 6%–20% in their magnitude throughout the seasonal cycle over West, Central and North‐East Africa. Therefore, because of the lack of adaptation and mitigation policies, the exacerbation of ambient heat conditions could contribute to the exposure of about 2–8.5 million person‐events to heat stress of high‐risk level over Burkina Faso, Ghana, Niger, and Nigeria. Since these heat events would be partly driven by interactions effects between climate change and population growth, efficient measures allowing not only to mitigate the increased greenhouse gas emissions, but also the effects of high heat on the human body must be urgently implemented on the affected countries' scale, in order to significantly decrease the vulnerability of their populations to potential heat‐related health problems.
    Description: Key Points: Increased global warming induces more spatially and temporally widespread extreme heat events over West, Central and North‐East Africa. Populations of some West African countries are projected to be particularly exposed to moderate and high heat conditions. Change in population exposure to dangerous heat categories is mainly driven by the interaction effect between climate and population growth.
    Description: Deutscher Akademischer Austauschdienst http://dx.doi.org/10.13039/501100001655
    Description: Projekt DEAL
    Description: https://esg-dn1.nsc.liu.se/search/cordex/
    Description: https://esgf-data.dkrz.de/projects/esgf-dkrz/
    Description: https://www.isimip.org/gettingstarted/details/31
    Description: https://sedac.ciesin.columbia.edu/data/set/popdynamics-1-8th-pop-base-year-projection-ssp-2000-2100-rev01/data-download
    Description: https://cds.climate.copernicus.eu/cdsapp#!/dataset/reanalysis-era5-single-levels?tab=form
    Keywords: ddc:551.6 ; Africa ; climate change ; heat stress index ; global warming
    Language: English
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  • 58
    Publication Date: 2023-11-24
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉In this study, a new multilayer urban canopy parameterization for high‐resolution (∼1 km) atmospheric models using the nudging approach to represent the impacts of urban canopies on airflow is presented. In our parameterization, a nudging term is added to the momentum equations and a source term to the turbulent kinetic energy equation to account for building effects. The challenge of this parameterization lies in defining appropriate values for the nudging coefficient and the weighting function used to reflect canopy effects. Values of both are derived and the parameterization developed is implemented and tested for idealized cases in the Mesoscale Transport and Stream model (METRAS). Comparison data are taken from obstacle‐resolving microscale model results. Results show that the parameterization using the nudging approach can simulate aerodynamic effects induced within the canopy by obstacles well, in terms of reduction of wind speeds and production of additional turbulent kinetic energy. Thus, models with existing nudging can use this approach as an efficient and effective method to parameterize dynamic urban canopy effects.〈/p〉
    Description: 〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉In this study, a new multilayer urban canopy parameterization for high‐resolution (∼1 km) atmospheric models using the nudging approach to represent the impacts of urban canopies on airflow is presented. Results show that the parameterization developed can simulate aerodynamic effects induced within the canopy by obstacles well, in terms of reduction of wind speeds and production of additional turbulent kinetic energy. Models with existing nudging can use this approach as an efficient and effective method to parameterize dynamic urban canopy effects. 〈boxed-text position="anchor" id="qj4524-blkfxd-0001" content-type="graphic" xml:lang="en"〉〈graphic position="anchor" id="jats-graphic-1" xlink:href="urn:x-wiley:00359009:media:qj4524:qj4524-toc-0001"〉 〈/graphic〉 〈/boxed-text〉〈/p〉
    Description: Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany's Excellence Strategy‐EXC 2037 'CLICCS‐Climate, Climatic Change, and Society'
    Keywords: ddc:551.6 ; canopy parameterization ; evaluation ; nudging ; numerical modelling ; urban boundary layer ; urban canopy parameterization
    Language: English
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  • 59
    Publication Date: 2023-11-24
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Uplift of the Tian Shan range modified regional climate during Cenozoic aridification in Central Asia. This study presents facies analyses and Neogene oxygen and carbon isotopic records from magnetostratigraphically dated terrestrial sedimentary sections on the southern side of the intermontane Issyk‐Kul basin in the Kyrgyz Tian Shan and 〈sup〉26〈/sup〉Al/〈sup〉10〈/sup〉Be isochron burial ages from the southern and eastern sides of the basin. The δ〈sup〉18〈/sup〉O and δ〈sup〉13〈/sup〉C data show a positive ca. 2‰ shift in values between ca. 8 and 7 Ma and a change from a negative to a positive trend. This change is attributed to the upwind growth of the Kyrgyz, Kungey and Trans Ili (Zaili) ranges, which diverted the westerlies, thereby changing the Issyk‐Kul basin from a windward to a leeward position, enhancing aridification and establishing the modern‐day spring and summer precipitation regime within the basin. Two 4 to 5 Ma 〈sup〉26〈/sup〉Al/〈sup〉10〈/sup〉Be isochron burial ages constrain the onset of Sharpyl Dak deposition on the eastern side of the basin; southward paleocurrent directions there suggest the eastward growth of the Kungey range in the Pliocene. Increased subsidence on the southern side of the basin and local tectonically induced river system reorganization led to the commencement of lake formation at ca. 5 Ma, followed by a ca. 2 Ma local depositional hiatus. The transition from sandstones of the Chu sedimentary group to conglomerates of the Sharpyl Dak group, marking a change from fluvial‐alluvial deposits to a proximal alluvial fan, is dated at 2.6–2.8 Ma by 〈sup〉26〈/sup〉Al/〈sup〉10〈/sup〉Be isochron burial dating on the southern side of the basin, driven either by tectonics or Northern Hemisphere glaciation. This study concludes that the late Miocene–Pliocene northward growth of Tian Shan significantly altered environmental conditions within the range, preventing the moisture‐bearing westerlies from reaching the intermontane Issyk‐Kul basin and promoting lake formation and expansion.〈/p〉
    Description: 〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉The late Miocene–Pliocene northward growth of Tian Shan created an orographic barrier that diverted the moisture‐bearing westerlies and enhanced aridification in the Issyk‐Kul basin. Reorganization of the river systems and enhanced subsidence led to the formation of an internally drained lake in Pliocene. The transition from sandstone to conglomerate (Sharpyl Dak group) deposition, linked to a change in climate and/or tectonic activity, occurred diachronously within the basin.〈boxed-text position="anchor" content-type="graphic" id="bre12751-blkfxd-0001" xml:lang="en"〉〈graphic position="anchor" id="jats-graphic-1" xlink:href="urn:x-wiley:0950091X:bre12751:bre12751-toc-0001"〉 〈/graphic〉〈/boxed-text〉〈/p〉
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: University of Wollongong http://dx.doi.org/10.13039/501100001777
    Keywords: ddc:551 ; Cenozoic aridification ; Central Asia ; cosmogenic 26Al/10Be ; tectonic uplift ; westerlies ; δ18O and δ13C stable isotopes
    Language: English
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  • 60
    Publication Date: 2023-11-24
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉The inherent complexity of underground mining requires highly selective ore extraction and adaptive mine planning. Repeated geological face mapping and reinterpretation throughout mine life is therefore routine in underground mines. Hyperspectral imaging (HSI) has successfully been applied to enhance geological mapping in surface mining environments, but remains a largely unexplored opportunity in underground operations due to challenges associated with illumination, wet surfaces and data corrections. In this study, we propose a workflow that paves the way for the operational use of HSI in active underground mines. In a laboratory set‐up, we evaluated different hyperspectral sensors and lighting set‐ups as well as the effect of surface moisture. We then acquired hyperspectral data in an underground mine of the Zinnwald/Cínovec Sn‐W‐Li greisen‐type deposit in Germany. These data were corrected for illumination effects, back‐projected into three dimensions and then used to map mineral abundance and estimate Li content across the mine face. We validated the results with handheld laser‐induced breakdown spectroscopy. Despite remaining challenges, we hope this study will help establish hyperspectral sensors in the extractive industry as a means to increase the volume and efficiency of raw material supply, advance digitalisation, and reduce the environmental footprint and other risks associated with underground mining.〈/p〉
    Description: 〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉This study proposes a workflow for using hyperspectral imaging for geological mapping in underground mining. The authors evaluated sensors and lighting set‐ups in a lab and acquired data in a German underground mine. The corrected data were used to map mineral abundance and estimate Li content, validated with laser‐induced breakdown spectroscopy. Despite challenges, this study aims to establish hyperspectral sensors in the extractive industry to increase raw material supply, advance digitalisation, and reduce environmental impact and mining risks.〈boxed-text position="anchor" content-type="graphic" id="phor12457-blkfxd-0001" xml:lang="en"〉〈graphic position="anchor" id="jats-graphic-1" xlink:href="urn:x-wiley:0031868X:media:phor12457:phor12457-toc-0001"〉 〈/graphic〉〈/boxed-text〉〈/p〉
    Description: https://doi.org/10.14278/rodare.2078
    Description: https://tinyurl.com/Zinnwald
    Keywords: ddc:622.1 ; hyperspectral ; lithium ; mineral mapping ; point cloud ; underground mining
    Language: English
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  • 61
    Publication Date: 2023-11-23
    Description: Based on inferences from proxy records the Miocene (23.03–5.33 Ma) was a time of amplified polar warmth compared to today. However, it remains a challenge to simulate a warm Miocene climate and pronounced polar warmth at reconstructed Miocene CO〈sub〉2〈/sub〉 concentrations. Using a state‐of‐the‐art Earth‐System‐Model, we implement a high‐resolution paleobathymetry and simulate Miocene climate at different atmospheric CO〈sub〉2〈/sub〉 concentrations. We estimate global mean surface warming of +3.1°C relative to the preindustrial at a CO〈sub〉2〈/sub〉 level of 450 ppm. An increase of atmospheric CO〈sub〉2〈/sub〉 from 280 to 450 ppm provides an individual warming of ∼1.4°C, which is as strong as all other Miocene forcing contributions combined. Substantial changes in surface albedo are vital to explain Miocene surface warming. Simulated surface temperatures fit well with proxy reconstructions at low‐ to mid‐latitudes. The high latitude cooling bias becomes less pronounced for higher atmospheric CO〈sub〉2〈/sub〉 concentrations. At such CO〈sub〉2〈/sub〉 levels simulated Miocene climate shows a reduced polar amplification, linked to a breakdown of seasonality in the Arctic Ocean. A pronounced warming in boreal fall is detected for a CO〈sub〉2〈/sub〉 increase from 280 to 450 ppm, in comparison to weaker warming for CO〈sub〉2〈/sub〉 changes from 450 to 720 ppm. Moreover, a pronounced warming in winter is detected for a CO〈sub〉2〈/sub〉 increase from 450 to 720 ppm, in contrast to a moderate summer temperature increase, which is accompanied by a strong sea‐ice concentration decline that promotes cloud formation in summer via enhanced moisture availability. As a consequence planetary albedo increases and dampens the temperature response to CO〈sub〉2〈/sub〉 forcing at a warmer Miocene background climate.
    Description: Key Points: At a CO〈sub〉2〈/sub〉 level of 450 ppm, a Miocene simulation shows a global mean surface warming of +3.1°C relative to the preindustrial state. Atmospheric CO〈sub〉2〈/sub〉 increase from 280 to 450 ppm causes a warming of ∼1.4°C, which is as strong as all other forcing factors combined. At higher atmospheric CO〈sub〉2〈/sub〉 levels, the Miocene climate shows a reduced polar amplification linked to a breakdown of seasonality in the Arctic.
    Description: Alfred Wegener Institute
    Description: Helmholtz Centre for Polar and Marine Research
    Description: https://doi.org/10.1594/PANGAEA.943430
    Description: https://github.com/FESOM/fesom2/
    Description: https://mpimet.mpg.de/en/science/modeling-with-icon/code-avilability
    Keywords: atmospheric CO2 ; Miocene ; Miocene temperature change ; polar amplification ; climate modeling ; Miocene bathymetry
    Language: English
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  • 62
    Publication Date: 2023-11-23
    Description: The climatologies of the stratopause height and temperature in the UA‐ICON model are examined by comparing them to 17‐years (2005–2021) of Microwave Limb Sounder (MLS) observations. In addition, the elevated stratopause (ES) event occurrence, their main characteristics, and driving mechanisms in the UA‐ICON model are examined using three 30‐year time‐slice experiments. While UA‐ICON reasonably simulates the large‐scale stratopause properties similar to MLS observations, at polar latitudes in the Southern Hemisphere the stratopause is ∼8 K warmer and ∼3 km higher than observed. A time lag of about two months also exists in the occurrence of the tropical semiannual oscillation of the stratopause compared to the observations. ES events occur in ∼20% of the boreal winters, after major sudden stratospheric warmings (SSWs). Compared to the SSWs not followed by ES events (SSW‐only), the ES events are associated with the persistent tropospheric forcing and prolonged anomalies of the stratospheric jet. Our modeling results suggest that the contributions of both gravity waves (GW)s and resolved waves are important in explaining the enhanced residual circulation following ES events compared to the SSW‐only events but their contributions vary through the lifetime of ES events. We emphasize the role of the resolved wave drag in the ES formation as in the sensitivity test when the non‐orographic GW drag is absent, the anomalously enhanced resolved wave forcing in the mesosphere gives rise to the formation of the elevated stratopause at about 85 km.
    Description: Plain Language Summary: Using 17 years (2005–2021) of Microwave Limb Sounder (MLS) observations, we show negative (cooling stratopause temperatures and decreasing stratopause heights) trends in most regions and seasons. The largest negative trend in the stratopause temperature (by considering all regions and all seasons) is found in the Southern Hemisphere (SH)'s polar region during austral spring. The seasonal average of cooling rates is comparable in the mid‐latitudes of Northern Hemisphere and SH. In the UA‐ICON simulations, the elevated stratopause events (ESEs) occur after major sudden stratospheric warmings (SSWs). ESEs frequency is 2 events per decade in UA‐ICON simulations. Our results show that the wind reversal is stronger and long‐lasting in the ESEs compared to SSW‐only events. In addition, the easterlies extend to the mesosphere in the composites of ESEs, but the reversed winds are limited to below 60 km in the case of SSW‐only events. We show that the non‐orographic gravity wave drag induces anomalous residual circulation after SSW that causes the ESEs. We also show that the ESEs form even in the absence of non‐orographic gravity wave drag. In this case, the anomalous residual circulation is due to the anomalously enhanced resolved wave forcing in the mesosphere that gives rise to the formation of the ESEs at about 85 km.
    Description: Key Points: The largest stratopause trend is found in the Southern Hemisphere polar region during austral springbased on Microwave Limb Sounder observations. The suppression of gravity waves in UA‐ICON reveals the importance of resolvedwaves and their ability to compensate missing drag. In the polar regions, the simulated stratopause is too warm and the tropical semi‐annual oscillation is about two months out of phase.
    Description: Deutsche Forschungsgemeinschaft
    Description: Transregional Collaborative Research Centre
    Description: GACR
    Description: MS‐GWaves
    Description: https://code.mpimet.mpg.de/projects/iconpublic
    Description: https://doi.org/10.26050/WDCC/UAICON_timesl_ctrl
    Description: https://doi.org/10.26050/WDCC/UAICON_timesl_nonon
    Description: https://doi.org/10.26050/WDCC/UAICON_timesl_nosso
    Keywords: ddc:551.5 ; gravity waves ; elevated stratopause ; middle atmosphere
    Language: English
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  • 63
    Publication Date: 2023-11-23
    Description: Offshore meteoric groundwater (OMG) has long been hypothesized to be a driver of seafloor geomorphic processes in continental margins worldwide. Testing this hypothesis has been challenging because of our limited understanding of the distribution and rate of OMG flow and seepage, and their efficacy as erosive/destabilizing agents. Here we carry out numerical simulations of groundwater flow and slope stability using conceptual models and evolving stratigraphy—for passive siliciclastic and carbonate margin cases—to assess whether OMG and its evolution during a late Quaternary glacial cycle can generate the pore pressures required to trigger mechanical instabilities on the seafloor. Conceptual model results show that mechanical instabilities using OMG flow are most likely to occur in the outer shelf to upper slope, at or shortly before the Last Glacial Maximum sea‐level lowstand. Models with evolving stratigraphy show that OMG flow is a key driver of pore pressure development and instability in the carbonate margin case. In the siliciclastic margin case, OMG flow plays a secondary role in preconditioning the slope to failure. The higher degree of spatial/stratigraphic heterogeneity of carbonate margins, lower shear strengths of their sediments, and limited generation of overpressures by sediment loading may explain the higher susceptibility of carbonate margins, in comparison to siliciclastic margins, to mechanical instability by OMG flow. OMG likely played a more significant role in carbonate margin geomorphology (e.g., Bahamas, Maldives) than currently thought.
    Description: Plain Language Summary: The flow of fresh to brackish groundwater has been proposed as an important process shaping the seafloor. However, we still have a poor understanding of how groundwater behaves in the sub‐seafloor and whether it can erode seafloor sediments. In this study, we test this hypothesis by using conceptual and realistic numerical models of two common types of seafloor margins—siliciclastic and carbonate—to assess the role of groundwater in making the seafloor susceptible to erosion. We show that the flow of groundwater offshore could have driven seafloor erosion close to the shelf break during the Last Ice Age, when sea level was lower than at present. Carbonate margins are more susceptible to this type of failure than siliciclastic margins. This may be explained by the higher variability in sediment properties across carbonate margins as well as the lower strength of their sediments. Groundwater has likely played an important role in shaping the seafloor in carbonate margins, and it may be responsible for landforms such as canyons, scars, and depressions in the Bahamas and the Maldives.
    Description: Key Points: Offshore meteoric groundwater (OMG) flow can drive mechanical instabilities in the outer shelf to upper slope. Such instabilities occur at, or shortly after, the Last Glacial Maximum sea‐level lowstand. Carbonate margins are more susceptible to mechanical instability by OMG than siliciclastic margins.
    Description: European Research Council http://dx.doi.org/10.13039/501100000781
    Description: National Science Foundation http://dx.doi.org/10.13039/100000001
    Description: https://doi.org/10.5281/zenodo.7094202
    Description: https://www.rocscience.com/software/slide2
    Description: https://figshare.com/s/5336d42d19ef771d4ad8
    Description: https://figshare.com/s/5027cd5ca22a7e96b3d1
    Keywords: ddc:551.3 ; offshore groundwater ; mechanical instability ; continental margins ; seafloor geomorphology ; siliciclastic ; carbonate
    Language: English
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  • 64
    Publication Date: 2023-11-23
    Description: In this work, we introduce a method for constraining the optical scattering models of natural ice crystals based on in‐situ measurements. Specifically the measured angular scattering functions for ice crystals can be used to compute a set of the asymmetry parameter (g) and the corresponding complexity parameter (C〈sub〉p〈/sub〉). It is demonstrated that the g‐C〈sub〉p〈/sub〉 relation can give valuable information on the morphology of ice crystal. The validity of the methods is shown from theoretical perspectives and the geometric‐optics ray‐tracing simulations. As an application, we investigate rimed ice crystals from in‐situ measurements and found that (a) the C〈sub〉p〈/sub〉 parameter is very well correlated with the surface riming degree and (b) only those models with both roughness and internal scattering can explain the observed g‐C〈sub〉p〈/sub〉 relation for rimed particles.
    Description: Plain Language Summary: Light scattering models of ice crystals are important for remote sensing and climate studies. Yet, many physical parameters, such as shape, aspect ratio, and inhomogeneity of the ice crystal can impose significant uncertainty in the single‐scattering properties predicted by light scattering models. To reduce such uncertainty and constrain the physical parameters in modeling, we introduce a novel method by analyzing the in‐situ measurement of the phase functions of ice crystals. We demonstrate the validity and usefulness of the method using both geometric ray‐tracing simulations and a case study on rimed crystals from two campaigns.
    Description: Key Points: A method is developed for analyzing in‐situ polar nephelometer measurements, aiming for constraining the light scattering models for natural ice crystal. Validity of the method is demonstrated by geometric‐optics ray‐tracing simulations and in‐situ measurements. A case study of rimed crystals measured in‐situ during two aircraft field campaigns using the Particle Habit Imaging and Polar Scattering probe is presented.
    Description: Helmholtz Association's Initiative and Networking Fund
    Description: https://doi.org/10.1594/PANGAEA.902611
    Description: https://doi.org/10.5065/D6639NKQ
    Description: https://zenodo.org/badge/latestdoi/440147565
    Keywords: ddc:551.5 ; light scattering ; ice crystals
    Language: English
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  • 65
    Publication Date: 2023-11-23
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Breadcrust bombs formed during Vulcanian eruptions are assumed to originate from the shallow plug or dome. Their rim to core texture reflects the competition between cooling and degassing timescales, which results in a dense crust with isolated vesicles contrasting with a highly vesicular vesicle network in the interior. Due to relatively fast quenching, the crust can shed light on pre‐ and syn‐eruptive conditions prior to or during fragmentation, whereas the interior allows us to explore post‐fragmentation vesiculation. Investigation of pre‐ to post‐fragmentation processes in breadcrust bombs from the 1999 Vulcanian activity at Guagua Pichincha, Ecuador, via 2D and 3D textural analysis reveals a complex vesiculation history, with multiple, spatially localized nucleation and growth events. Large vesicles (Type 1), present in low number density in the crust, are interpreted as pre‐eruptive bubbles formed by outgassing and collapse of a permeable bubble network during ascent or stalling in the plug. Haloes of small, syn‐fragmentation vesicles (Type 2), distributed about large vesicles, are formed by pressurization and enrichment of volatiles in these haloes. The nature of the pressurization process in the plug is discussed in light of seismicity and ground deformation signals, and previous textural and chemical studies. A third population (Type 3) of post‐fragmentation small vesicles appears in the interior of the bomb, and growth and coalescence of Type 2 and 3 vesicles causes the transition from isolated to interconnected bubble network in the interior. We model the evolution of viscosity, bubble growth rate, diffusion timescales, bubble radius and porosity during fragmentation and cooling. These models reveal that thermal quenching dominates in the crust whereas the interior undergoes a viscosity quench caused by degassing, and that the transition from crust to interior corresponds to the onset of percolation and development of permeability in the bubble network.〈/p〉
    Description: Plain Language Summary: Breadcrust bombs are volcanic ejecta formed during explosive volcanic eruptions by rapid cooling of the exterior (the crust) and slow cooling of the interior that causes gas loss, bubble growth and cracking of the exterior. The rapidly cooled crust preserves characteristics of the magma prior to explosion. We study here the variations in porosity and vesicle properties from crust to interior in breadcrust bombs from the Guagua Pichincha volcano in Ecuador. Our results shed light on the pre‐eruptive conditions in the magma prior to explosive activity, and on the post‐fragmentation evolution of the bomb interior by bubble formation.〈/p〉
    Description: Key Points: 〈list list-type="bullet"〉 〈list-item〉 〈p xml:lang="en"〉Vesicle textures in breadcrust bombs correlate with pre‐ to post‐fragmentation degassing processes during Vulcanian eruptions〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉Large isolated vesicles preserved in the crust record a pre‐eruptive episode of outgassing and pressurization prior to fragmentation〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉Small vesicles provide insights into post‐fragmentation onset of permeability from the crust to the interior〈/p〉〈/list-item〉 〈/list〉 〈/p〉
    Description: ERC
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: Alexander von Humboldt‐Stiftung http://dx.doi.org/10.13039/100005156
    Description: National Science Foundation
    Description: German Research Foundation
    Description: https://doi.org/10.26022/IEDA/112846
    Keywords: ddc:552 ; breadcrust bombs ; Vulcanian eruptions ; vesicle number density ; vesiculation ; bubble nucleation ; fragmentation
    Language: English
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  • 66
    Publication Date: 2023-11-23
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Spectral induced polarization (SIP) laboratory measurements on water‐saturated rocks show a strong correlation between the electrical polarization strength and the inner surface area of rocks. We investigate the influence of inner surface roughness on the SIP response by simulating the frequency‐dependent complex conductivity of micro‐scale rock models. Starting with smooth grain models, we introduce surface roughness using two different approaches: increasing the surface roughness in a fractal‐like manner, and creating random surface structures, resulting in more natural‐looking surfaces. We find that surface roughness has two distinct effects on the SIP response: (a) a shift in the position and magnitude of the primary relaxation frequency to lower frequencies and lower magnitudes, respectively, and (b) the formation of secondary polarizations above the polarization frequency of the primary polarization. We also compare the relaxation time and normalized chargeability obtained by Debye decomposition and the imaginary conductivity at 1 Hz of our models with mechanistic models and empirical relations. We point out the congruences and offer explanations for the discrepancies between our models and the empirical observations. We conclude that the results of our study are applicable to real rocks and that the SIP method has the potential to detect inner surface roughness. However, the SIP method it not able to discriminate between signals from rough particles and a distribution of smooth particles.〈/p〉
    Description: Plain Language Summary: The spectral induced polarization method measures the electrical conductivity of the subsurface at depths of investigation ranging from a few dm to several 100 m. The potential of the method to detect mineral resources, contamination, microbial activity, etc. makes it a promising tool for today's environmental challenges. However, due to the complexity of the underlying physical and chemical processes the interpretation of SIP measurements often remains qualitative. Mathematical and mechanistic models used to describe the processes are usually simplified with respect to geometry, chemistry, and physical properties. In this study, we use computer simulations to investigate the surfaces of spherical particles (grains). After simulating the SIP response of models with smooth and rough surfaces, we analyze the influence of surface roughness on the SIP response. We find that surface roughness causes distinct changes in the SIP response compared to the smooth grain. However, we also find that this introduces an ambiguity in the interpretation of SIP data.〈/p〉
    Description: Key Points: 〈list list-type="bullet"〉 〈list-item〉 〈p xml:lang="en"〉Inner surface roughness of rocks has substantial impact on spectral induced polarization response〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉Surface roughness shifts the primary polarization peak to lower frequencies〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉Surface roughness causes additional polarizations above the primary peak frequency〈/p〉〈/list-item〉 〈/list〉 〈/p〉
    Description: https://doi.org/10.5281/ZENODO.7049722
    Keywords: ddc:550 ; SIP ; surface ; roughness
    Language: English
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  • 67
    Publication Date: 2023-11-30
    Description: DFG, SUB Göttingen
    Description: research
    Keywords: Meereis ; Elektromagnetik
    Language: German
    Type: doc-type:article
    Format: 5
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  • 68
    Publication Date: 2023-02-26
    Description: Am 24. April 1503 erließ Herzog Georg von Sachsen eine neue Bergordnung für die Bergwerke in Altenberg und Geising. In der Einleitung begründete er den Erlass der neuen Bergordnung damit, dass vor allem die Hutleute, Mühlmeister, Schmelzer und Steiger sich nicht an die 1491 erlassene Ordnung hielten. Die Festlegung der Regeln für den Bergbau in dieser Bergordnung erfolgte in 21 Artikeln. So wurden die Hutleute, Mühlmeister und Schmelzer zum Eid gegenüber dem Bergmeister verpflichtet. Neben der Aufzählung der Plichten der Steiger wurde die Arbeitszeit der Mühlmeister und die Höhe des wöchentlichen Biergeldes für die Schmelzer geregelt. Die Einwohner von Geising und des Geisinggrundes durften nur noch bis abends 9 Uhr Bier und Wein ausschenken. Die Zinnhändler wurden ermahnt, gekauftes Zinn pünktlich zu bezahlen und die festgesetzten Preise einzuhalten.
    Description: source
    Keywords: Herzog Georg von Sachsen ; Graupen/Krupka ; Altenberg ; Geising ; Zinnbergbau ; Sachsen ; Bergordnung
    Language: German
    Type: doc-type:book , updatedVersion
    Format: 7
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  • 69
    Publication Date: 2023-03-21
    Description: DFG
    Description: Bei bodenkundlichen und geologischen Untersuchungen werden ground-penetrating radar (GPR)-Reflexionsdaten routinemäßig zur Erkundung des oberflächennahen Untergrundes verwendet. Da Torfgebiete einen wichtigen Teil des globalen Klimasystems darstellen, besteht ein zunehmendes Interesse daran, Torfablagerungen detaillierter zu untersuchen und zu charakterisieren. Bis heute konzentriert sich die Anwendung von GPR in Mooren auf die Erfassung von 2D Daten entlang ausgewählter Profile, häufig mit dem Ziel, Modelle der Torfmächtigkeit und -stratigraphie abzuleiten. Wir stellen eine 3D GPR-Fallstudie aus einem Moorgebiet im Nordosten Deutschlands vor, in welcher wir unter Verwendung moderner Aufzeichnungs-, Bearbeitungs- und Interpretationsstrategien ein detailliertes 3D Modell des untersuchten Torfkörpers entwickeln. Unsere Ergebnisse zeigen erhebliche Schwankungen in der Torfmächtigkeit einschließlich einer markanten, kreisförmigen Vertiefungsstruktur. Wir kommen zu dem Schluss, dass solche Strukturen mittels 2D GPR-Aufzeichnungsstrategien nicht zuverlässig hätten abgebildet werden können. Somit unterstreichen unsere Ergebnisse den Nutzen von 3D GPRStrategien, um ein tieferes Verständnis von Torfablagerungen und ihren Eigenschaften zu etablieren.
    Description: poster
    Language: German
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  • 70
    Publication Date: 2023-03-21
    Description: Two mysterious moons whirl around Mars. Despite the many missions to the planet, not a single one has focused on its satellites — or, rather, not a single successful one. Three previous Martian moon explorers, launched by Russia or the Soviet Union, all failed. Now Japan is trying its luck with a high-risk venture that aims to grab rocks from the larger Martian moon and bring them to Earth for laboratory analysis. “It’s a very scary mission,” says Tomohiro Usui of the Japan Aerospace Exploration Agency (JAXA) in Sagamihara. The spacecraft’s daunting tasks will include multiple touchdowns on a heavily cratered world. The chief goal is to settle a debate over the origin of the moons (1). Did the Red Planet steal them from the asteroid belt, or did they form after an asteroid smashed into Mars? The answer carries implications for satellites elsewhere and perhaps even for the origin of water on Earth.
    Description: report
    Keywords: ddc:520 ; Mars ; Monde ; moons
    Language: English
    Type: doc-type:article , publishedVersion
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  • 71
    Publication Date: 2023-03-21
    Description: Gas exchange between the atmosphere and ocean interior profoundly impacts global climate and biogeochemistry. However, our understanding of the relevant physical processes remains limited by a scarcity of direct observations. Dissolved noble gases in the deep ocean are powerful tracers of physical air-sea interaction due to their chemical and biological inertness, yet their isotope ratios have remained underexplored. Here, we present high-precision noble gas isotope and elemental ratios from the deep North Atlantic (~32°N, 64°W) to evaluate gas exchange parameterizations using an ocean circulation model. The unprecedented precision of these data reveal deep-ocean undersaturation of heavy noble gases and isotopes resulting from cooling-driven air-to-sea gas transport associated with deep convection in the northern high lati-tudes. Our data also imply an underappreciated and large role for bubble-mediated gas exchange in the global air-sea transfer of sparingly soluble gases, including O2, N2, and SF6. Using noble gases to validate the physical representation of air-sea gas exchange in a model also provides a unique opportunity to distinguish physical from biogeochemical signals. As a case study, we compare dissolved N2/Ar measurements in the deep North Atlantic to physics-only model predictions, revealing excess N2 from benthic denitrification in older deep waters (below 2.9 km). These data indicate that the rate of fixed N removal in the deep Northeastern Atlantic is at least three times higher than the global deep-ocean mean, suggesting tight coupling with organic carbon export and raising potential future implications for the marine N cycle.
    Description: NSF, UK NERC, University of Oxford Advanced Research Computing facility
    Description: https://www.bco-dmo.org/project/887496
    Description: research
    Keywords: ddc:551 ; gas exchange ; nitrogen cycle ; overturning circulation ; air-sea interaction ; noble gases
    Language: English
    Type: doc-type:article , publishedVersion
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  • 72
    Publication Date: 2023-03-20
    Description: Geophysical sensing methods such as magnetics, electromagnetics and ground penetrating radar are the essential methods for the detection of unexploded ordnances (UXO) in the subsurface. Apart from a precise localization of buried ammunition remnants, a reliable discrimination of anomaly signatures caused by UXO and Non-UXO bodies is one of the currently most challenging tasks in the field of explosive ordnance clearance. Therefore, we exploit different phase-based edge detectors to evaluate their applicability for improving the detection performance and especially for distinguishing buried objects by the anomaly signature they cause. In the present poster, we apply our new approach on synthetic magnetic data for spherical and elliptical object geometries. Furthermore, we compare the synthetic cases to real magnetic survey data collected from a test site at SENSYS GmbH in Bad Saarow.
    Description: poster
    Keywords: edge detection ; UXO ; magnetics
    Language: English
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  • 73
    Publication Date: 2023-03-24
    Description: The AdriaArray project addresses fundamental questions related to the geodynamics and the deformation and stress field of the Adriatic plate in south-eastern Europe. The observational basis of AdriaArray is a recently formed seismic broadband array that joins newly deployed temporary and existing permanent stations all over the entire Adriatic plate. Here, we report on the deployment of temporary stations by Ruhr-University Bochum (RUB) in Greece and Northern Macedonia. This contribution enhances the local networks by 35 new temporary stations and upgrades the instruments at 17 permanent sites. Most of these sites are equipped with broadband instruments from the German DSEBRA array which were previously installed within the scope of the AlpArray project. Deployment started with 37 stations in Greece at the end of September / beginning of October 2022 in cooperation with partners from the universities of Thessaloniki, Athens and Patras, as well the National Observatory of Athens (NOA). The deployment of stations in North Macedonia is planned for February 2023 in cooperation with the Seismological Observatory of the University of Skopje. All stations are supplied with mobile routers for live-streaming of waveform data and for monitoring the state-of-health of the stations. Data is streamed in near real-time to servers of the Seismological Observatory of the RUB and to the EIDA node of NOA. The FDSN network code 1Y is assigned to the temporary stations, while the upgraded permanent stations remain a part of their original networks. The newly deployed stations in Greece were able to register data of the still ongoing seismic series of Evia which started in November 2022. We present examples of the recorded seismograms from these events and estimate the quality of the stations by calculating probability power spectral densities (PPSD) to ensure that the stations meet the quality requirements of the AdriaArray project. First results of the calculated PPSDs illustrate the overall performance of these stations and help to identify problematic stations for which alternative sites have to be scouted.
    Description: poster
    Language: English
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  • 74
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    ARGE GMIT, Bonn
    In:  ARGE GMIT
    Publication Date: 2023-03-27
    Description: Die Ausgabe der Geowissenschaftlichen Mitteilungen vom September 2022 enthält die Themenblöcke: GEOfokus: Zwischen Scylla und Charybdis - Die Rolle von Recycling und Primärrohstoffen am Beispiel von Kupfer und Lithium, GEOaktiv (Wirtschaft, Beruf, Forschung und Lehre), GEOlobby (Gesellschaften, Verbände, Institutionen), GEOreport (Geowissenschaftliche Öffentlichkeitsarbeit, Tagungsberichte, Ausstellungen, Exkursionen, Publikationen), GEOszene (Würdigungen, Nachrufe).
    Description: journal
    Keywords: ddc:550 ; GMIT
    Language: German
    Type: doc-type:book , publishedVersion
    Format: 124
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  • 75
    Publication Date: 2023-07-18
    Description: Methane seeps are typified by the formation of authigenic carbonates, many of which exhibit corrosion surfaces and secondary porosity believed to be caused by microbial carbonate dissolution. Aerobic methane oxidation and sulfur oxidation are two processes capable of inducing carbonate corrosion at methane seeps. Although the potential of aerobic methanotrophy to dissolve carbonate was confirmed in laboratory experiments, this process has not been studied in the environment to date. Here, we report on a carbonate corrosion experiment carried out in the REGAB Pockmark, Gabon‐Congo‐Angola passive margin, in which marble cubes were deployed for 2.5 years at two sites (CAB‐B and CAB‐C) with apparent active methane seepage and one site (CAB‐D) without methane seepage. Marble cubes exposed to active seepage (experiment CAB‐C) were found to be affected by a new type of microbioerosion. Based on 16〈italic toggle="no"〉S r〈/italic〉RNA gene analysis, the biofilms adhering to the bioeroded marble mostly consisted of aerobic methanotrophic bacteria, predominantly belonging to the uncultured Hyd24‐01 clade. The presence of abundant 〈sup〉13〈/sup〉C‐depleted lipid biomarkers including fatty acids (〈italic toggle="no"〉n〈/italic〉‐C〈sub〉16:1ω8c〈/sub〉, 〈italic toggle="no"〉n〈/italic〉‐C〈sub〉18:1ω8c〈/sub〉, 〈italic toggle="no"〉n〈/italic〉‐C〈sub〉16:1ω5t〈/sub〉), various 4‐mono‐ and 4,4‐dimethyl sterols, and diplopterol agrees with the dominance of aerobic methanotrophs in the CAB‐C biofilms. Among the lipids of aerobic methanotrophs, the uncommon 4α‐methylcholest‐8(14)‐en‐3β,25‐diol is interpreted to be a specific biomarker for the Hyd24‐01 clade. The combination of textural, genetic, and organic geochemical evidence suggests that aerobic methanotrophs are the main drivers of carbonate dissolution observed in the CAB‐C experiment at the REGAB pockmark.〈/p〉
    Description: Deutscher Akademischer Austauschdienst http://dx.doi.org/10.13039/501100001655
    Keywords: ddc:550 ; carbonate ; corrosion ; lipid biomarker ; methane seep ; methanotrophic bacteria ; microbioerosion
    Language: English
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  • 76
    Publication Date: 2023-08-12
    Description: Trying to impart concepts and practices of sustainable housing and health to the public, the Handbook aims to apply a “non-expert” and “easy-to-understand” language, adequate visual effects, and user-friendly design. The Handbook’s main target groups are the rapidly developing urban middle classes (the so-called “new consumers”) with their sharply rising ecological footprint, agencies of government at all levels, businesses, especially companies in the construction industry, architects, teachers, students, and all others interested in green housing and healthy living. The content follows a multi-disciplinary holistic approach, providing practical guidelines for planning, designing, constructing, operating, and maintaining sustainable housing and behavioral dimensions to improve energy efficiency and healthy living. While the book content might focus on the most rapidly developed housing typology in Vietnam, high-rise residential buildings, the principles and solutions introduced are applicable to all other types of housing in Vietnam.
    Description: BMBF
    Description: lecture
    Keywords: "Green Housing" ; "Healthy Living" ; "Sustainable Building" ; "Sustainable Lifestyles" ; "Sustainable Buildings" ; Handbook ; "Energy-Saving" ; "Household Waste Management" ; "Renewable Energy" ; "Water-Saving" ; "Building Envelope" ; "Thermal Comfort" ; "New consumers"
    Language: English
    Type: doc-type:book , publishedVersion
    Format: 130
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  • 77
    Publication Date: 2023-08-24
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Polarity reversals and excursions are the most significant geomagnetic field changes generated in the liquid outer core of the Earth, therefore studying them helps understand geodynamo processes. This study examines the Matuyama‐Brunhes (MB) reversal using a new reconstruction of the global geomagnetic field based on paleomagnetic data, termed Global Geomagnetic Field Model for the MB reversal (GGFMB). GGFMB covers 900–700 ka, including late Matuyama and early Brunhes. This allows us to also investigate the Kamikatsura excursion (ca. 888 ka). The model is based on 38 high‐quality paleomagnetic sediment records with age control mostly independent of the magnetic signal. GGFMB suggests that the MB reversal began about ∼799 ka, when non‐dipole field components increased and the axial dipole component decreased. The transitional fields first appeared on Earth's surface in the high‐latitude southern hemisphere and equatorial regions. The minimum dipole strength was reached around 780 ka and the axial dipole changed sign. After ∼10 Kyr, the field stabilized in the normal polarity of the early Brunhes. The MB reversal lasted ∼29 Kyr (from 799 to 770 ka) and had slower rate of dipole decay than recovery as well as lower dipole moment for several millennia before than after the reversal. According to GGFMB, the dipole moment during the Kamikatsura excursion was approximately half that of the current field and it was a regional excursion observed only over eastern Asia and North America. Our sediment data collection is heavily biased toward the northern hemisphere, thus more southern hemisphere records are needed to demonstrate GGFMB's robustness in this region.〈/p〉
    Description: Plain Language Summary: The Earth's magnetic field originates deep inside the planet and extends far into space, and it has undergone significant direction and intensity changes throughout geological history. The most extreme magnetic field changes are reversals, when the field changes its polarity and global field intensity reaches a minimum. We reconstruct the global geomagnetic field evolution over the time interval 900,000 to 700,000 years ago. The information about the magnetic field variations comes from the paleomagnetic signal recovered from sediment drill cores from locations all over the globe, and with good constraints on the ages of the material. Our model includes the Matuyama‐Brunhes field reversal, which occurred ∼780,000 years ago. It provides a global view of this drastic field change, indicating, for example, that the recovery of the global field intensity was much faster than its decay and the average global field strength was lower for several millennia before than after the polarity change. Our model suggests that the reversal started at ∼799 ka, the actual polarity change of the axial dipole field occurred at ∼780 ka, and a stable normal polarity was reached at ∼770 ka. The whole process of the reversal therefore took ∼29,000 years.〈/p〉
    Description: Key Points: A global geomagnetic field model for 900–700 ka is presented, including the Matuyama‐Brunhes (MB) reversal and Kamikatsura excursion. The mid‐point of the Matuyama‐Brunhes reversal is at 780 ka, with an overall duration of nearly 30 Kyr. The dipole field decays from moderate dipole moment in the late Matuyama and recovers quickly to higher values in the early Brunhes.
    Description: Helmholtz‐Zentrum Potsdam ‐ Deutsches GeoForschungsZentrum GFZ http://dx.doi.org/10.13039/501100010956
    Description: https://earthref.org/ERDA/2548/
    Description: https://earthref.org/ERDA/2548/
    Keywords: ddc:538.7 ; geomagnetic field model ; Matuyama-Brunhes (MB) reversal ; Kamikatsura excursion
    Language: English
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  • 78
    Publication Date: 2023-08-24
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Loess deposits are widespread in the Quaternary, but relatively rare in older geological records. This disparity is commonly linked to the unique climate conditions of the Quaternary, but those cannot fully explain the scarcity of loess in older records. Instead, we propose that the poor preservation of loess also plays an essential role. To test this hypothesis, we assess the preservation potential of loess by quantifying its modern‐day distribution in active sedimentary basins. This analysis shows that on the global scale only 20% of loess occurs in basins of which the majority is in a foreland setting. This could be due to nearby silt‐producing mountains and the effects of rain shadow aridity. The other 80% is ultimately either eroded or reworked and therefore poorly preserved in the long term. This conclusion implies that loess deposits may have been more common in pre‐Quaternary periods, despite being less abundant in the geological record.〈/p〉
    Description: Hessisches Ministerium für Wissenschaft und Kunst http://dx.doi.org/10.13039/501100003495
    Keywords: ddc:551.3 ; loess ; preservation ; geological record
    Language: English
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  • 79
    Publication Date: 2023-09-12
    Description: Two data evaluation concepts for X‐ray stress analysis based on energy‐dispersive diffraction on polycrystalline materials with cubic crystal structure, almost random crystallographic texture and strong single‐crystal elastic anisotropy are subjected to comparative assessment. The aim is the study of the residual stress state in hard‐to‐reach measurement points, for which the sin2ψ method is not applicable due to beam shadowing at larger sample tilting. This makes the approaches attractive for stress analysis in engineering parts with complex shapes, for example. Both approaches are based on the assumption of a biaxial stress state within the irradiated sample volume. They exploit in different ways the elastic anisotropy of individual crystallites acting at the microscopic scale and the anisotropy imposed on the material by the near‐surface stress state at the macroscopic scale. They therefore complement each other, in terms of both their preconditions and their results. The first approach is based on the evaluation of strain differences, which makes it less sensitive to variations in the strain‐free lattice parameter a0. Since it assumes a homogeneous stress state within the irradiated sample volume, it provides an average value of the in‐plane stresses. The second approach exploits the sensitivity of the lattice strain to changes in a0. Consequently, it assumes a homogeneous chemical composition but provides a stress profile within the information depth. Experimental examples from different fields in materials science, namely shot peening of austenitic steel and in situ stress analysis during welding, are presented to demonstrate the suitability of the proposed methods.
    Description: The single‐crystal elastic anisotropy and the anisotropy of the near‐surface (residual) stress state of polycrystalline materials with random texture are exploited in energy‐dispersive X‐ray stress analysis to study samples under constrained measurement conditions.
    Keywords: ddc:548 ; X‐ray stress analysis ; energy‐dispersive diffraction ; polycrystalline materials ; single‐crystal elastic anisotropy
    Language: English
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  • 80
    Publication Date: 2023-09-12
    Description: Studies of host rock deformation around magmatic intrusions usually focus on the development of stresses directly related to the intrusion process. This is done either by considering an inflating region that represents the intruding body, or by considering multiphase deformation. Thermal processes, especially volume changes caused by thermal expansion are typically ignored. We show that thermal stresses around upper crustal magma bodies are likely to be significant and sufficient to create an extensive fracture network around the magma body by brittle yielding. At the same time, cooling induces decompression within the intrusion, which can promote the appearance of a volatile phase. Volatile phases and the development of a fracture network around the inclusion may thus be the processes that control magmatic‐hydrothermal alteration around intrusions. This suggests that thermal stresses likely play an important role in the development of magmatic systems. To quantify the magnitude of thermal stresses around cooling intrusions, we present a fully compressible 2D visco‐elasto‐plastic thermo‐mechanical numerical model. We utilize a finite difference staggered grid discretization and a graphics processing unit based pseudo‐transient solver. First, we present purely thermo‐elastic solutions, then we include the effects of viscous relaxation and plastic yielding. The dominant deformation mechanism in our models is determined in a self‐consistent manner, by taking into account stress, pressure, and temperature conditions. Using experimentally determined flow laws, the resulting thermal stresses can be comparable to or even exceed the confining pressure. This suggests that thermal stresses alone could result in the development of a fracture network around magmatic bodies.
    Description: Plain Language Summary: Quantifying the stresses that magma bodies exert on the surrounding rocks is an important part of understanding mechanical processes that control the evolution of magmatic systems and volcanic eruptions. Previous analytical or numerical models typically describe the mechanical response to changes in magma volume due to intrusion or extraction of magma. However, volume changes related to thermal expansion/contraction around a cooling magma body are often neglected. Here, we develop a new software which runs on modern graphics processing unit machines, to quantity the effect of this process. The results show that stresses due to thermal expansion/contraction are significant, and often large enough to fracture the rocks nearby the magma body. Such fracture networks may form permeable pathways for the magma or for fluids such as water and CO〈sub〉2〈/sub〉, thus influencing the evolution of magmatic and hydrothermal systems. Finally we show that cooling and shrinking of magma bodies causes significant decompression which can influence the chemical evolution of the magma during crystallization and devolatilization.
    Description: Key Points: We present a numerical quantification of the effect of thermal stresses in visco‐elasto‐plastic rock with tensile and dilatant shear failure. The pressure drop in thermally contracting upper crustal magma bodies can exceed 100 MPa, potentially triggering devolatilization. Thermal cracking can create an extensive fracture network around an upper crustal magma body.
    Description: European Research Council http://dx.doi.org/10.13039/501100000781
    Description: https://zenodo.org/record/6958273
    Description: https://doi.org/10.5281/zenodo.6958273
    Keywords: ddc:551.8 ; magmatic intrusions ; host rock deformation ; thermal stress ; numerical quantification
    Language: English
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  • 81
    Publication Date: 2023-09-12
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Chloromethane (CH〈sub〉3〈/sub〉Cl) is the most abundant natural chlorinated organic compound in the atmosphere playing an important role in catalyzing stratospheric ozone loss. Vegetation emits the largest amounts of CH〈sub〉3〈/sub〉Cl to the atmosphere but its source strength is highly uncertain leading also to large uncertainties in the global budget of CH〈sub〉3〈/sub〉Cl. Triple‐element stable isotope analysis may help to reduce uncertainties because it provides additional process‐level information compared to conventional quantification methods. In this study we performed experiments to obtain a first triple‐elemental isotopic fingerprint (〈sup〉2〈/sup〉H, 〈sup〉13〈/sup〉C, 〈sup〉37〈/sup〉Cl) of CH〈sub〉3〈/sub〉Cl emitted by a relevant plant species (royal fern, 〈italic〉Osmunda regalis〈/italic〉). Isotopic values of all three elements showed considerable differences compared to isotopic values of industrially manufactured CH〈sub〉3〈/sub〉Cl which bodes well for future applications to distinguish individual sources. Isotopic analysis of potential precursors (rain, methoxy groups) of CH〈sub〉3〈/sub〉Cl in plants revealed no measurable change of hydrogen and chlorine isotopic ratios during formation which may provide a simpler route to estimate the isotopic composition of CH〈sub〉3〈/sub〉Cl emissions. Plant degradation experiments of CH〈sub〉3〈/sub〉Cl were carried out with club moss (〈italic〉Selaginella kraussiana〈/italic〉) revealing significant isotopic fractionation for all three elements. The fractionation pattern characterized by epsilon and lambda is inconsistent with known biotic dechlorination reactions indicating a yet unreported biotic degradation mechanism for CH〈sub〉3〈/sub〉Cl. Overall, this study provides first insights into the triple‐elemental isotopic fingerprint of plant emissions and degradation. The results may represent important input data for future isotope‐based models to improve global budget estimates of CH〈sub〉3〈/sub〉Cl and to explore the yet unknown degradation pathways.〈/p〉
    Description: Plain Language Summary: Chloromethane is the most abundant chlorinated organic compound in the atmosphere. It contributes to the destruction of the ozone layer that protects us from skin cancer and genetic damage. Currently, we do not have a good understanding of the sources and removal processes of chloromethane in the atmosphere. In this paper, we use a technique that takes advantage of the different varieties of a chemical element. These so‐called isotopes behave differently during chemical reactions that lead to individual isotopic fingerprints depending on the source or removal process. We used isotopic fingerprints of all three chemical elements in chloromethane and showed that chloromethane produced by a plant (royal fern) differs substantially from chloromethane manufactured by industry. Other plant species such as club moss are able to remove chloromethane from the atmosphere but it is often not clear how this occurs. Isotopic analysis revealed that the studied club moss uses a unique, thus far unknown, way to break down chloromethane. This study demonstrates how information extracted from isotopic fingerprints will help to improve our understanding of sources and removal processes of chloromethane in the atmosphere. It can help to better predict how ozone destruction in the stratosphere affects us in the future.〈/p〉
    Description: Key Points: First triple‐element isotopic characterization of plant CH〈sub〉3〈/sub〉Cl emission and degradation. Plant degradation experiments suggest another yet unknown transformation pathway. Important input data for future isotope based models to improve understanding of global CH〈sub〉3〈/sub〉Cl budget.
    Description: Helmholtz Association http://dx.doi.org/10.13039/501100009318
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: https://doi.org/10.48758/ufz.13388
    Keywords: ddc:551.9 ; CH3Cl ; ozone depletion ; isotopes ; plant emissions ; halogens
    Language: English
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  • 82
    Publication Date: 2023-07-20
    Description: The seismic activity of a planet can be described by the corner magnitude, events larger than which are extremely unlikely, and the seismic moment rate, the long‐term average of annual seismic moment release. Marsquake S1222a proves large enough to be representative of the global activity of Mars and places observational constraints on the moment rate. The magnitude‐frequency distribution of relevant Marsquakes indicates a $b$‐value of 1.06. The moment rate is likely between $1.55\times {10}^{15}\mathrm{N}\mathrm{m}/\mathrm{a}$ and $1.97\times {10}^{18}\mathrm{N}\mathrm{m}/\mathrm{a}$, with a marginal distribution peaking at $4.9\times {10}^{16}\mathrm{N}\mathrm{m}/\mathrm{a}$. Comparing this with pre‐InSight estimations shows that these tended to overestimate the moment rate, and that 30% or more of the tectonic deformation may occur silently, whereas the seismicity is probably restricted to localized centers rather than spread over the entire planet.
    Description: Plain Language Summary: The seismic moment rate is a measure for how fast quakes accumulate deformation of the planet's rigid outer layer, the lithosphere. In the past decades, several models for the deformation rate of Mars were developed either from the traces quakes leave on the surface, or from mathematical models of how quickly the planet's interior cools down and shrinks. The large marsquake that occurred on the 4th of May 2022 now allows a statistical estimation of the deformation accumulated on Mars per year, and thus to confront these models with reality. It turns out that, although there is a considerable overlap, the models published prior to InSight tend to overestimate the seismic moment rate, and hence the ongoing deformation on Mars. Possible explanations are that 30% or more of the deformation occurs silently, that is, without causing quakes, or that not the entire planet is seismically active but only specific regions.
    Description: Key Points: A single large marsquake suffices to constrain the global seismic moment rate. Pre‐InSight estimations tended to overestimate the moment rate. Either a significant part of the ongoing deformation occurs silent, or seismic activity is restricted to some activity centers, or both.
    Description: Eidgenössische Technische Hochschule Zürich http://dx.doi.org/10.13039/501100003006
    Description: National Aeronautics and Space Administration http://dx.doi.org/10.13039/100000104
    Description: UK Space Agency http://dx.doi.org/10.13039/100011690
    Description: Deutsches Zentrum für Luft‐ und Raumfahrt http://dx.doi.org/10.13039/501100002946
    Description: Insight SFI Research Centre for Data Analytics http://dx.doi.org/10.13039/501100021525
    Description: http://dx.doi.org/10.18715/SEIS.INSIGHT.XB_2016
    Description: http://doi.org/10.17189/1517570
    Keywords: ddc:523 ; Mars ; InSight ; seismic moment rate ; S1222a
    Language: English
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  • 83
    Publication Date: 2023-07-20
    Description: A pseudosymmetric description of the crystal lattice derived from a single wide‐angle Kikuchi pattern can have several causes. The small size (〈15%) of the sector covered by an electron backscatter diffraction pattern, the limited precision of the projection centre position and the Kikuchi band definition are crucial. Inherent pseudosymmetries of the crystal lattice and/or structure also pose a challenge in the analysis of Kikuchi patterns. To eliminate experimental errors as much as possible, simulated Kikuchi patterns of 350 phases have been analysed using the software CALM [Nolze et al. (2021). J. Appl. Cryst.54, 1012–1022] in order to estimate the frequency of and reasons for pseudosymmetric crystal lattice descriptions. Misinterpretations occur in particular when the atomic scattering factors of non‐equivalent positions are too similar and reciprocal‐lattice points are systematically missing. As an example, a pseudosymmetry prediction depending on the elements involved is discussed for binary AB compounds with B1 and B2 structure types. However, since this is impossible for more complicated phases, this approach cannot be directly applied to compounds of arbitrary composition and structure.
    Description: Distinguishing between actual and apparent pseudosymmetry in electron backscatter diffraction patterns is nearly impossible, even for simulated patterns. However, the resulting lattice is always a superlattice as long as the signal is not a superposition of multiple patterns.
    Keywords: ddc:548 ; Bravais lattices ; pseudosymmetry ; lattice point density ; ordered/disordered structures ; lattice distortion ; electron backscatter diffraction ; backscattered Kikuchi diffraction patterns ; lattice parameters ; Funk transform
    Language: English
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  • 84
    Publication Date: 2023-07-20
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉The dryness of the stratosphere is the result of air entering through the cold tropical tropopause layer (TTL). However, our understanding of the moisture flux partitioning into water vapor and frozen hydrometeors is incomplete. This raises concerns regarding the ability of General Circulation Models to accurately predict changes in stratospheric water vapor following perturbations in the radiative budget due to volcanic aerosol or stratospheric geoengineering. We present the first results using a global storm‐resolving model investigating the sensitivity of moisture fluxes within the TTL to an additional heating source. We address the question how the partitioning of moisture fluxes into water vapor and frozen hydrometeors changes under perturbations. The analysis reveals the resilience of the TTL, keeping the flux partitioning constant even at an average cold‐point warming exceeding 8 K. In the control and perturbed simulations, water vapor contributes around 80% of the moisture entering the stratosphere.〈/p〉
    Description: Plain Language Summary: The stratosphere is a dry region since moisture entering it from below has to pass the cold‐point, a temperature minimum between troposphere and stratosphere. The low temperatures lead to ice formation and sedimentation of moisture. Frozen moisture within clouds rising above the cold‐point tropopause can pass this temperature barrier and be injected into the stratosphere, where temperatures increase again, promoting the melting and sublimation of ice crystals. However, little is known about the sensitivity of the split of moisture entering the stratosphere into frozen and non‐frozen moisture, especially under external influences, like heating by volcanic aerosol or stratospheric geoengineering efforts. Convective parameterizations in conventional simulations can lead to biases. The emerging km‐scale simulations, which explicitly resolve the physical processes, offer the unique possibility to study moisture fluxes under external forcing while circumventing the downsides of parameterizations. Here, the sensitivity of the moisture flux partitioning into non‐frozen and frozen components to an additional heating source is studied for the first time in global storm‐resolving simulations. The analysis reveals an unaltered flux partitioning even at an average cold‐point warming exceeding 8 K. In the control and perturbed simulations, water vapor contributes around 80% of the moisture entering the stratosphere.〈/p〉
    Description: Key Points:Water vapor dominates the stratospheric moisture budget with a contribution of around 80% in global storm‐resolving simulation. The partitioning of stratospheric moisture fluxes into vapor and frozen hydrometeors remains stable under large temperature perturbations.
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: Bundesministerium für Bildung und Forschung http://dx.doi.org/10.13039/501100002347
    Description: Fueglistaler Group
    Keywords: ddc:551.5 ; stratospheric water vapor ; tropopause ; perturbation ; moisture budget ; geoengineering ; volcano
    Language: English
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  • 85
    Publication Date: 2023-07-20
    Description: The subduction of bathymetric highs, such as aseismic ridges, leads to far‐reaching changes in the dynamics of subduction zones with increased plate coupling and deformation in the upper plate. Subduction of the submarine Carnegie Ridge on the Nazca Plate has fundamentally impacted late Cenozoic magmatism and tectonic activity in the northern Andes. However, the timing of onset of Carnegie Ridge subduction has been a matter of debate. Time‐temperature inverse modeling of new thermochronological data from the Western Cordillera of Ecuador reveals two phases of cooling separated by isothermal conditions. The first cooling phase postdates early and middle Miocene magmatism in the Western Cordillera and is attributed to post‐magmatic thermal relaxation. The second cooling phase started after 6 Ma. Inferred to record the onset of tectonically controlled rock uplift and exhumation in the Western Cordillera, this phase is coeval with the last cooling phase recorded in the Eastern Cordillera. Based on these findings, we suggest that the onset of subduction of the Carnegie Ridge at ∼6–5 Ma increased plate coupling at the subduction interface, promoting shortening, regional rock uplift, and exhumation in the northern Andes. Overall, our results highlight the essential role of bathymetric highs in driving regional upper‐plate deformation at non‐collisional convergent plate margins.
    Description: Plain Language Summary: Topographic growth and morphology of the Andes have been influenced by subduction processes, tectonic inheritance, and climate. Here, we investigate the role of subduction of high topography on the ocean floor in driving deformation in the upper plate at the Nazca‐South America ocean‐continent plate margin. The subduction of the Carnegie Ridge, a linear, topographically high sector on the Nazca Plate, has impacted magmatism and deformation processes in the Ecuadorian Andes. However, the timing of onset of ridge subduction is debated. We employed radioisotopic dating techniques to evaluate the uplift of the Andes. These techniques record the cooling of rocks as mountain ranges are uplifted and eroded. The thermal histories of rocks from the Western Cordillera in Ecuador reveal two distinct cooling phases. The first cooling phase occurred shortly after Miocene magmatic bodies were emplaced in the Western Cordillera. The second cooling phase began at ∼6–5 Ma, coeval with the last cooling phase in the Eastern Cordillera. We attribute this cooling phase to the onset of uplift and erosion in the Western Cordillera. Based on these findings, we suggest that the onset of subduction of the Carnegie Ridge increased plate coupling and promoted shortening and rock uplift in the northern Andes.
    Description: Key Points: Thermochronological data reveal two cooling phases in the Western Cordillera of Ecuador, during the Miocene and after 6 Ma. The onset of cooling at 6 Ma was associated with shortening, rock uplift, and exhumation in the Western Cordillera. Mio‐Pliocene exhumation was related to stronger coupling of the subduction interface due to the initial subduction of the Carnegie Ridge.
    Description: Deutscher Akademischer Austauschdienst http://dx.doi.org/10.13039/501100001655
    Description: Potsdam University Graduate School
    Description: Yachay Tech University
    Description: Arizona LaserChron Center
    Description: https://zenodo.org/record/7311529#Y4YTYYLMITU
    Keywords: ddc:551.8 ; aseismic ridge subduction ; topographic growth ; zircon U‐Pb geochronology ; apatite and zircon (U‐Th)/He and apatite fission‐track thermochronology ; Carnegie ridge ; northern Andes
    Language: English
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  • 86
    Publication Date: 2023-07-20
    Description: Knowledge of lithospheric structure is essential for understanding the impact of continental collision and oceanic subduction on surface tectonic configurations. Full‐waveform tomographic images reveal lateral heterogeneities and anisotropy of the lithosphere and asthenosphere in Asia. Estimating lithospheric thickness from seismic velocity reductions at depth exhibits large variations underneath different tectonic units. The thickest cratonic roots are present beneath the Sichuan, Ordos, and Tarim basins and central India. Radial anisotropy signatures of 11 representative tectonic provinces uncover the different nature and geodynamic processes of their respective past and present deformation. The large‐scale continental lithospheric deformation is characterized by low‐velocity anomalies from the Himalayan Orogen to the Baikal rift zone in central Asia, coupled with the post‐collision thickening of the crust. The horizontal low‐velocity layer of ∼100–300 km depth extent below the lithosphere points toward the existence of the asthenosphere beneath East and Southeast Asia, with heterogeneous anisotropy indicative of channel flows.
    Description: Plain Language Summary: The lithospheric plates, like mosaics of the Earth’s surface, are moving coherently over the weaker, convecting asthenosphere. The lithospheric structure and thickness dictated by mantle dynamics play a first‐order role in understanding the active tectonics and morphological evolution of the Asian region. Here, the latest high‐resolution full‐waveform tomographic model, SinoScope 1.0, is employed to investigate the seismic structure and dynamics of the lithosphere and asthenosphere from a seismological perspective. The lithospheric thickness of known various geological units and cratonic blocks is retrieved with large variability. The observed anisotropic signatures within the lithosphere and asthenosphere provide important constraints on the deformation state and history of different tectonic provinces. The India‐Eurasia collision primarily induced large‐scale lithospheric deformation and thickening of the crust in the west of the North‐South Gravity Lineament. The narrow low‐velocity layer below the lithosphere lies beneath East and Southeast Asia and is bounded by subduction trenches and cratonic blocks, which provides seismic evidence for the low‐viscosity asthenosphere that partially decouples plates from mantle flow beneath and allows plate tectonics to work above. The lithospheric thinning and extension, intensive magmatism, and mineralization are potentially associated with the strong interaction between the lithosphere and asthenospheric flow in the eastern Asian margin.
    Description: Key Points: Full‐waveform tomographic images reveal lateral heterogeneities and anisotropy in the lithosphere and asthenosphere beneath the Asian region. India‐Eurasia collision induced large‐scale low‐velocity anomaly and crustal thickening spanning from the Himalayas to the Baikal rift zone. Asthenosphere in East and SE Asia exhibits strong vsh, 〉 vsv, and partially decouples lithosphere, bounded by subduction trench and cratonic keels.
    Description: China Scholarship Council http://dx.doi.org/10.13039/501100004543
    Description: National Natural Science Foundation of China http://dx.doi.org/10.13039/501100001809
    Description: Korea Meteorological Administration Research and Development Program http://dx.doi.org/10.13039/501100003629
    Description: National Research Foundation of Korea http://dx.doi.org/10.13039/501100003725
    Keywords: ddc:551.1 ; Asia ; seismic structure ; lithosphere dynamics ; asthenosphere dynamics
    Language: English
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  • 87
    Publication Date: 2023-07-27
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Results from the Cassini‐Huygens space mission at Enceladus revealed a substantial inventory of organic species embedded in plume and E ring ice grains originating from a global subsurface and putative habitable ocean. Compositional analysis by the Cosmic Dust Analyzer indicated the presence of aromatic species and constrained some structural features, although their exact nature remains unclear. As indicated by many studies, among other organic species, low‐mass aromatics likely played a role in the emergence of life on Earth and may be linked to potential prebiotic or biogenic chemistry on icy moons. Here, we study the behavior of single‐ringed aromatic compounds—benzoic acid and two isomeric derivatives, 2,3‐dihydroxybenzoic acid and 2,5‐dihydroxybenzoic acid—using Laser‐Induced Liquid Beam Ion Desorption (LILBID), an analogue setup to simulate the impact ionization mass spectra of ice grains in space. These compounds share common structural features but also exhibit differences in functional groups and substituent positions. We investigate the fragmentation behavior and spectral appearance of each molecule over three simulated impact velocities, in both positive and negative ion modes. Parent compounds can be distinguished easily from their derivatives due to various spectral differences, including the (de)protonated molecular ion peaks appearing at different 〈italic〉m〈/italic〉/〈italic〉z〈/italic〉 values. We conclude that distinction between structural isomers in LILBID is more challenging, but some insights can be revealed by considering intermolecular bonding regimes. This work will guide future investigations into elucidating the composition of isomeric biosignatures in ice grains, relevant for future space missions to Enceladus and Europa.〈/p〉
    Description: Plain Language Summary: The Cassini‐Huygens space mission discovered a plume at Enceladus that ejects gases and frozen ice grains originating from an ocean of liquid water below its icy shell. In these ice grains, a range of interesting organic molecules were discovered by Cassini's Cosmic Dust Analyzer mass spectrometer. Organic molecules are important in the search for life beyond Earth as they form the basis of all known Earth life, and active biology elsewhere would likely have a discernible effect on the local inventory of organic species. One class of organic, with a ring structure of carbon atoms, called aromatics, were discovered in the plume. We investigate the spectral appearance of one example of aromatic compound, benzoic acid, as well as two similar compounds with additional chemical groups attached to the aromatic ring. The two similar compounds have the same mass and general structure, but slightly different arrangements of the additional groups, known as isomers. We find that it is simple to distinguish mass spectral features between benzoic acid and its related compounds, but more difficult to explain the differences between the isomers. This work will assist the analysis of mass spectrometry data from future habitability‐investigating space missions to ocean‐bearing icy moons.〈/p〉
    Description: Key Points: Cassini revealed a variety of organic compounds including clear evidence of aromatics in the plume of Enceladus. Identifying mass spectral features of isomeric organics enhances our ability to assess the astrobiological potential of Enceladus/Europa. Parent aromatic compounds can be easily distinguished from their derivatives in ice grains with impact ionization mass spectrometry.
    Description: European Research Council Consolidator
    Description: http://dx.doi.org/10.17169/refubium-37960
    Description: https://lilbid-db.planet.fu-berlin.de/
    Keywords: ddc:523 ; mass spectrometry ; LILBID and impact ionization ; aromatics and isomeric derivatives ; Enceladus and Europa ; space missions ; habitability
    Language: English
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  • 88
    Publication Date: 2023-07-27
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉The Radiation Assessment Detector (RAD) on board the Mars Science Laboratory's Curiosity rover has been monitoring the surface radiation environment on Mars for just over 10 years. It has been found by Wimmer‐Schweingruber et al. (2015, 〈ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1002/2015gl066664"〉https://doi.org/10.1002/2015gl066664〈/ext-link〉) that within the narrow view cone of RAD, the directionality of the radiation field is close to but not completely isotropic. In order to better understand the directionality of the surface radiation over a wide range of zenith angles (〈italic〉θ〈/italic〉), we perform a three‐dimensional Geant4 Monte Carlo simulation to derive the 〈italic〉θ〈/italic〉‐dependence of the surface dose rate. The results show that galactic cosmic ray protons, coming in at 〈italic〉θ〈/italic〉 ∼ 74° make the greatest contribution to the surface dose. For helium ions, this angle is at around 46°. This is a consequence of the increasing column depth at larger zenith angles and the complex interplay of the destruction of primary and the creation of secondary particles as the primary cosmic ray interacts with the Martian atmosphere. We also compared the simulated results with the RAD measurements and found a reasonable agreement. Our results are important for future human exploration of Mars, for instance, to estimate the effectiveness of radiation shielding of a given geometry or for optimizing the radiation shielding design of a Martian habitat.〈/p〉
    Description: Plain Language Summary: Space agencies and private companies are working to place humans on the surface of Mars. Astronauts would be exposed to a different and considerably harsher radiation environment on Mars than humans are on Earth. Space radiation is largely determined by galactic cosmic rays, which have sufficient energy to reach the Martian surface. Thus, a better understanding of the radiation on the surface of Mars is needed. The shielding provided by the atmosphere increases with the zenith angle, and it also causes an increase in the creation of secondary particles. To better understand this, we perform a Geant4 Monte Carlo simulation to derive the dependence of the surface dose rate on the zenith angle 〈italic〉θ〈/italic〉. The results show that the radiation dose on the surface of Mars depends on the incoming angle of the primary radiation. Moreover, the radiation dose rate is significantly modulated by solar activity, and the Mars surface dose rate differs by about 50% between solar maximum and minimum periods. We validate our simulation by comparing the dose measured by the Mars Science Laboratory Radiation Assessment Detector and find good agreement.〈/p〉
    Description: Key Points: We model the downward radiation dose on the surface of Mars and find that it only depends weakly on the zenith angle. The surface dose rate depends on solar modulation, and weaker modulation results in higher dose rate for each.The local topographical features influence the Martian surface radiation.
    Description: Deutsches Zentrum für Luft‐und Raumfahrt http://dx.doi.org/10.13039/501100002946
    Description: Jet Propulsion Laboratory http://dx.doi.org/10.13039/100006196
    Description: Strategic Priority Program of CAS
    Description: National Natural Science Foundation of China http://dx.doi.org/10.13039/501100001809
    Description: Civil Aerospace Technologies
    Description: NASA Johnson Space Center
    Description: https://doi.org/10.17189/1519761
    Description: https://doi.org/10.17189/1519760
    Description: https://doi.org/10.17189/1523028
    Description: https://doi.org/10.5281/zenodo.7257306
    Keywords: ddc:523 ; space radiation ; Mars exploration ; MSL mission ; zenith angle
    Language: English
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  • 89
    Publication Date: 2023-07-27
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉The composition of basaltic melts in equilibrium with the mantle can be determined for several Martian meteorites and in‐situ rover analyses. We use the melting model MAGMARS to reproduce these primary melts and estimate the bulk composition and temperature of the mantle regions from which they originated. We find that most mantle sources are depleted in CaO and Al〈sub〉2〈/sub〉O〈sub〉3〈/sub〉 relative to models of the bulk silicate Mars and likely represent melting residues or magma ocean cumulates. The concentrations of Na〈sub〉2〈/sub〉O, K〈sub〉2〈/sub〉O, P〈sub〉2〈/sub〉O〈sub〉5〈/sub〉, and TiO〈sub〉2〈/sub〉 are variable and often less depleted, pointing to the re‐fertilization of the sources by fluids and low‐degree melts, or the incorporation of residual trapped melts during the crystallization of the magma ocean. The mantle potential temperatures of the sources are 1400–1500°C, regardless of the time at which they melted and within the range of the most recent predictions from thermochemical evolution models.〈/p〉
    Description: Plain Language Summary: Martian meteorites and rocks analyzed by rovers are witnesses of magmatic processes on Mars. Some of the basaltic specimens among them have been classified as “primitive” as they are closely related to the melts that form in the mantle and feature high MgO/FeO. They record important properties of the mantle of Mars. We use the mantle melting model MAGMARS to constrain the temperature and composition of the mantle source regions from which primitive basalts originated. We find that the mantle compositions were low in CaO and Al〈sub〉2〈/sub〉O〈sub〉3〈/sub〉, either because they melted on several occasions, or because these components were locked in deeper layers of the mantle when it solidified from the bottom up (early magma ocean). Several mantle sources are comparatively rich in Na〈sub〉2〈/sub〉O, K〈sub〉2〈/sub〉O, P〈sub〉2〈/sub〉O〈sub〉5〈/sub〉, and TiO〈sub〉2〈/sub〉. These components were either subsequently added to the mantle sources by fluids and low‐degree melts or can be explained by the trapping of melts during the progressive crystallization of the magma ocean. The temperature of the mantle sources projected to surface conditions for easier comparison (potential temperature) was 1400–1500°C, regardless of the time at which they melted, and is within the range of recent predictions from planetary‐scale models of interior dynamics.〈/p〉
    Description: Key Points: Basalts that sampled discrete mantle regions throughout Mars's history provide information about the mantle composition and temperature. The mantle potential temperature of primitive basalts appears constant (1400–1500ºC), yet is likely not representative of the average mantle. Incompatible element concentrations in the mantle vary due to magma ocean crystallization, partial melting, and metasomatism.
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: Deutsches Zentrum für Luft‐ und Raumfahrt http://dx.doi.org/10.13039/501100002946
    Description: https://doi.org/10.5281/zenodo.7949084
    Keywords: ddc:552 ; Martian magmatism ; mantle melting ; Mars interior structure ; depleted mantle ; metasomatism ; secular cooling
    Language: English
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  • 90
    Publication Date: 2023-07-27
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Rockwall erosion by rockfall is largely controlled by frost weathering in high alpine environments. As alpine rock types are characterized by crack‐dominated porosity and high rock strength, frost cracking observations from low strength and grain supported pore‐space rocks cannot be transferred. Here, we conducted laboratory experiments on Wetterstein limestone samples with different initial crack density and saturation to test their influence on frost cracking efficacy. We exposed rocks to real‐rockwall freezing conditions and monitored acoustic emissions as a proxy for cracking. To differentiate triggers of observed cracking, we modeled ice pressure and thermal stresses. Our results show initial full saturation is not a singular prerequisite for frost cracking. We also observe higher cracking rates in less‐fractured rock. Finally, we find that the temperature threshold for frost cracking in alpine rocks falls below −7°C. Thus, colder, north‐exposed rock faces in the Alps likely experience more frost cracking than southern‐facing counterparts.〈/p〉
    Description: Plain Language Summary: Freezing results in the formation of ice that exerts stresses on fracture walls and draws in additional moisture to supply further growth and break down rocks, a process termed frost cracking. Frost cracking drives much erosion and rockfall in alpine environments. Here we test hypotheses from prior work about how frost cracking is impacted by saturation and rock properties. We exposed rock samples of different strength and saturation to identical freezing conditions in laboratory experiments. We monitored rock temperature and acoustic emissions (AE), assuming frost cracking produces the recorded AE hits. We find that initial full saturation is not required for frost cracking, as water transport is enhanced by fractures in alpine rocks. Furthermore, rock with initial higher short‐term strength showed more frost cracking because, we infer, of stiffness properties that make these rocks more brittle compared to lower strength rocks. Frost cracking occurred at a wide range of temperatures below freezing and was highest between −9 and −7°C. We thus conclude that frost cracking is most impacted by temperature and rock short‐term strength. In Alpine environments, this may result in more frost cracking and rockfall on colder north‐facing rockwalls than warmer southern exposures.〈/p〉
    Description: Key Points: Initial saturation levels do not limit the efficacy of ice segregation in fractured alpine rocks. Rock initial crack density impacts rock stiffness and thermal properties and thus frost cracking efficacy. The “frost cracking window” temperature range is dependent on rock strength and crack‐controlled porosity in alpine rocks.
    Description: German Reserach Foundation
    Description: https://doi.org/10.6084/m9.figshare.23584686
    Keywords: ddc:551.3 ; frost weathering ; frost cracking ; periglacial processes ; rock weathering ; thermal stress ; acoustic emission
    Language: English
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  • 91
    Publication Date: 2023-07-27
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉In this paper we describe a method to compute spatial scales for images acquired by NASA's Mars Curiosity rover (Mars Science Laboratory, MSL). The method is based on the assumption that the rover stands on an infinite plane that may have any orientation with respect to the local gravity vector. While not new, it is the first time that this method is systematically applied to Martian images acquired by a lander. A continuously run software pipeline processes the images acquired by the rover within a 20 m radius, adds approximate scalebars to the raw images, and generates, whenever possible, rectified (warped) versions of those images. The products of this software pipeline and the chemical compositions of relevant rover science targets from NASA's Planetary Data System archive, are made available to the public via the Approximate Scale for Images and Chemistry website, which has been developed in collaboration with the Planetary Data System Analyst's Notebook for the MSL mission. Hyperlinks connect the two resources.〈/p〉
    Description: Plain Language Summary: We developed a software pipeline that calculates the spatial scale of images acquired by NASA's Mars Curiosity rover. The software pipeline is linked to a new website: the Approximate Scale for Images and Chemistry, in which the scalebar products are paired with information about the shape, size, color, and chemical composition of the imaged site, obtained by the rover suite of instruments. The images mimic the vantage point of human eyes and are therefore well‐suited to inspire field geologists (including those mainly working on Earth) to interpret Martian geologic features.〈/p〉
    Description: Key Points: A systematic method to generate approximate scalebars for obliquely acquired Martian landscape images was developed. A newly created Approximate Scale for Images and Chemistry (ASIC) website links images, color, spatial scale, and chemistry, as returned by NASA's Curiosity rover in Gale crater. The ASIC website is complementary and strongly linked to the Analyst's Notebook, the data resource for Martian/lunar landed missions.
    Description: Deutsche Forschungsgemeinschaft
    Description: Project DEAL
    Description: https://asic.mps.mpg.de/
    Description: https://an.rsl.wustl.edu/msl/
    Description: http://pds-geosciences.wustl.edu/msl/msl-m-chemcam-libs-4_5-rdr-v1/mslccm_1xxx/data/moc/
    Description: http://pds-geosciences.wustl.edu/msl/msl-m-chemcam-libs-4_5-rdr-v1/mslccm_1xxx/extras/rmi_mosaics/
    Description: http://pds-geosciences.wustl.edu/msl/msl-m-chemcam-libs-4_5-rdr-v1/mslccm_1xxx/extras/rmi_contours_in_mcam_images/
    Description: http://pds-geosciences.wustl.edu/msl/msl-m-apxs-4_5-rdr-v1/mslapx_1xxx/extras/
    Keywords: ddc:523 ; Mars ; Curiosity rover ; images ; spatial scale ; science targets ; chemistry
    Language: English
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  • 92
    Publication Date: 2023-07-28
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉The Lagrangian representation of fluid flows offers a natural perspective to study many kinds of physical mechanisms. By contrast, the Eulerian representation is more convenient from a diagnostic point of view. This article attempts to combine elements of both worlds by proposing an Eulerian method that allows one to extract Lagrangian information about the atmospheric flow. The method is based on the offline advection of passive tracer fields and includes a relaxation term. The latter device allows one to run the integration in a continuous fashion without the need for reinitialization. As a result one obtains accumulated Lagrangian information, for example, about the recent parcel displacement or the recent parcel‐based diabatic heating, at each point of an Eulerian grid at any time step. The method is implemented with a pseudospectral algorithm suitable for gridded global atmospheric data and compared with the more traditional trajectory method. The method's utility is demonstrated on the basis of a few examples, which relate to cloud formation and the development of temperature anomalies. The examples highlight that the method provides a convenient diagnostic of parcel‐based changes, paving an intuitive way to explore the physical processes involved. Due to its gridpoint‐based nature, the proposed method can be applied to large data sets in a straightforward and computationally efficient manner, suggesting that the method is particularly useful for climatological analyses.〈/p〉
    Description: 〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉The Lagrangian representation of fluid flows offers the most natural perspective to study many kinds of physical mechanisms; by contrast, the Eulerian representation is more convenient from a diagnostic point of view. This article attempts to combine elements of both worlds by proposing an Eulerian method that allows one to extract Lagrangian information about the atmospheric flow. The method enables one to easily produce a sequence of maps showing accumulated Lagrangian changes. 〈boxed-text position="anchor" id="qj4453-blkfxd-0001" content-type="graphic" xml:lang="en"〉〈graphic position="anchor" id="jats-graphic-1" xlink:href="urn:x-wiley:00359009:media:qj4453:qj4453-toc-0001"〉 〈/boxed-text〉〈/p〉
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Keywords: ddc:551.5 ; air‐parcel approach ; atmospheric fluid dynamics ; atmospheric transport ; Eulerian tracer technique ; Lagrangian analysis ; Lagrangian tracking ; synoptic‐scale meteorology ; trajectories
    Language: English
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  • 93
    Publication Date: 2023-07-21
    Description: Oceanic circulation and mass‐field variability play important roles in exciting Earth's wobbles and length‐of‐day changes (ΔΛ), on time scales from days to several years. Modern descriptions of these effects employ oceanic angular momentum (OAM) series from numerical forward models or ocean state estimates, but nothing is known about how ocean reanalyses with sequential data assimilation (DA) would fare in that context. Here, we compute daily OAM series from three 1/4° global ocean reanalyses that are based on the same hydrodynamic core and input data (e.g., altimetry, Argo) but different DA schemes. Comparisons are carried out (a) among the reanalyses, (b) with an established ocean state estimate, and (c) with Earth rotation data, all focusing on the period 2006–2015. The reanalyses generally provide credible OAM estimates across a range of frequencies, although differences in amplitude spectra indicate a sensitivity to the adopted DA scheme. For periods less than 120 days, the reanalysis‐based OAM series explain ∼40%–50% and ∼30%–40% of the atmosphere‐corrected equatorial and axial geodetic excitation, similar to what is achieved with the state estimate. We find mixed performance of the reanalyses in seasonal excitation budgets, with some questionable mean ocean mass changes affecting the annual cycle in ΔΛ. Modeled excitations at interannual frequencies are more uncertain compared to OAM series from the state estimate and show hints of DA artifacts in one case. If users are to choose any of the tested reanalyses for rotation research, our study points to the Ocean Reanalysis System 5 as the most sensible choice.
    Description: Key Points: We evaluate three ocean reanalyses for their skill in explaining Earth rotation variations on different time scales from 2006 to 2015. For periods 〈120 days, reanalyses explain 40%–50% of atmosphere‐reduced polar motion excitation variance, similar to an ocean state estimate. Reanalyses show mixed skill in seasonal excitation budgets and, in one case, hints of data assimilation artifacts at interannual periods.
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: https://resources.marine.copernicus.eu/product-detail/GLOBAL_REANALYSIS_PHY_001_031/INFORMATION
    Description: https://isdc.gfz-potsdam.de/ggfc-oceans/oam/
    Description: https://www.ncei.noaa.gov/access/metadata/landing-page/bin/iso?id=gov.noaa.ngdc.mgg.dem:316
    Description: https://podaac-tools.jpl.nasa.gov/drive/files/GeodeticsGravity/tellus/L3/mascon/RL06/JPL/v02/CRI/netcdf
    Description: https://keof.jpl.nasa.gov/combinations/
    Keywords: ddc:550 ; Earth rotation ; ocean angular momentum ; ocean reanalysis ; data assimilation
    Language: English
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  • 94
    Publication Date: 2023-07-21
    Description: A band width determination using the first derivative of the band profile systematically underestimates the true Bragg angle. Corrections are proposed to compensate for the resulting offset Δa/a of the mean lattice parameters derived from as many Kikuchi band widths as possible. For dynamically simulated Kikuchi patterns, Δa/a can reach up to 8% for phases with a high mean atomic number Z, whereas for much more common low‐Z materials the offset decreases linearly. A predicted offset Δa/a = f(Z) is therefore proposed, which also includes the unit‐cell volume and thus takes into account the packing density of the scatterers in the material. Since Z is not always available for unknown phases, its substitution by Zmax, i.e. the atomic number of the heaviest element in the compound, is still acceptable for an approximate correction. For simulated Kikuchi patterns the offset‐corrected lattice parameter deviation is Δa/a 〈 1.5%. The lattice parameter ratios, and the angles α, β and γ between the basis vectors, are not affected at all.
    Description: Automatically determined band widths in simulated backscatter Kikuchi patterns exhibit differences from the double Bragg angles that correlate with the scatterer density. Corrections are proposed to compensate for this.
    Keywords: ddc:548 ; mean atomic number ; Kikuchi patterns ; lattice parameters ; automated Bragg angle determination ; lattice parameter determination ; dynamical theory of electron diffraction ; electron backscatter diffraction ; Funk transform
    Language: English
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  • 95
    Publication Date: 2023-07-21
    Description: The presence of the Etendeka flood basalts in northwestern Namibia is taken as evidence for the activity of the Tristan da Cunha mantle plume during the continental breakup between Africa and South America. We investigate seismic anisotropy beneath NW Namibia by splitting analysis of core‐refracted teleseismic shear waves (XKS phases) to probe mantle flow and lithospheric deformation related to the tectonic history of the region. We present the results of the joint splitting analysis of XKS data collected from 34 onshore stations and 12 ocean‐bottom seismometers. The fast polarization directions (FPDs) are consistent with a model that combines the effects of lithospheric deformation and large‐scale mantle flow due to the NE motion of the African plate. The dominantly NNW‐SSE‐oriented FPDs in the northern part are likely caused by shallow lithospheric structures. Our observations do not show any strong evidence of a pervasive effect of the Tristan da Cunha mantle plume.
    Description: Plain Language Summary: The geology of Northwest Namibia is characterized by the presence of flood basalts, originating from magma sourced in the Earth's mantle. The source magma of these flood basalts was produced during the passage of the African plate over a mantle plume, more than 80 million years ago, contemporaneous with the onset of the breakup of the South American plate from the African plate. The role of the mantle plume in the continental breakup can be examined by a seismological technique named shear wave splitting analysis. The mantle flow induces direction‐dependent physical properties, that is, seismic anisotropy, which causes a shear wave to split into two different components traveling at different speeds. The leading component is polarized in a direction representing the direction of the flow in the earth's mantle. Except for the northern part, the polarization direction of the fast shear wave is consistent with the model of mantle flow caused by the NE motion of the African plate and deformations in the lithosphere. The results of our study do not show any direct evidence for the direct impact of the mantle plume on the mantle beneath our region of study.
    Description: Key Points: Upper mantle anisotropy beneath NW Namibia is a combined effect of the present‐day motion of the African Plate and lithospheric structures. No significant direct effect of the Tristan da Cunha mantle plume is observed in shear wave splitting measurements. Localized shearing in the lithosphere and crustal underplating are likely the main causes of the lateral variations in seismic anisotropy.
    Description: https://doi.org/10.14470/KP6443475642
    Description: https://doi.org/10.14470/1N134371
    Description: https://doi.org/10.7914/SN/IU
    Description: https://doi.org/10.18715/SKS_SPLITTING_DATABASE
    Description: https://www.geophysik.uni-frankfurt.de/64002762/Software
    Keywords: ddc:551.1 ; seismic anisotropy ; Tristan da Cunha mantle plume ; Namibia ; lithospheric shearing ; continental breakup ; shear wave splitting
    Language: English
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  • 96
    Publication Date: 2023-07-21
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Heat flow across oceanic transform faults (TFs) and fracture zones (FZs) has rarely been studied in detail, despite these features representing distinct thermal boundaries within the oceanic lithosphere. Here, we present heat flow measurements across the St Paul fracture zone (SPFZ) in the equatorial Atlantic Ocean, from 48 Ma crust in the south to 71 Ma in the north. To the north of the FZ we find a basal heat flow of 63 mWm〈sup〉−2〈/sup〉, and to the south a basal heat flow of 79 mWm〈sup〉−2〈/sup〉, both in agreement with plate cooling models. However, within the SPFZ we find a heat flow of 83 mWm〈sup〉−2〈/sup〉, greater than the values of the adjacent crust and 10–15 mWm〈sup〉−2〈/sup〉 higher than predicted from conductive cooling models, suggesting that the thermal structure of the FZ has been modified. Evidence from seismic and sub‐bottom profiler data indicate recent active deformation within the SPFZ, potentially driven by lithospheric flexure across the FZ or temporal changes in TF configuration. We propose that this deformation may enable fluid circulation and heat advection within the basement, creating the seafloor heat flow anomaly within the FZ. These findings suggest that FZs may remain important zones predisposed to host deformation and fluid flow in the oceanic lithosphere, despite not being active plate boundaries.〈/p〉
    Description: Key Points: A high heat flow anomaly of 10–15 mWm〈sup〉−2〈/sup〉 is observed in the St Paul fracture zone compared to the adjacent oceanic crust. The heat flow anomaly is likely due to tectonically driven fluid flow but thermal rejuvenation at the transform fault could also contribute. Fracture zones may act as high permeability pathways for fluid flow, and form and evolve differently to standard oceanic lithosphere.
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: FP7 Ideas: European Research Council http://dx.doi.org/10.13039/100011199
    Description: https://doi.pangaea.de/10.1594/PANGAEA.950419
    Description: https://doi.pangaea.de/10.1594/PANGAEA.950420
    Keywords: ddc:551 ; fracture zone ; heat flow ; oceanic crust ; St Paul ; fluid flow ; lithosphere
    Language: English
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  • 97
    Publication Date: 2023-07-21
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Parameterised by the Love number 〈italic〉k〈/italic〉〈sub〉2〈/sub〉 and the tidal quality factor 〈italic〉Q〈/italic〉, and inferred from lunar laser ranging (LLR), tidal dissipation in the Moon follows an unexpected frequency dependence often interpreted as evidence for a highly dissipative, melt‐bearing layer encompassing the core‐mantle boundary. Within this, more or less standard interpretation, the basal layer's viscosity is required to be of order 10〈sup〉15〈/sup〉–10〈sup〉16〈/sup〉 Pa s and its outer radius is predicted to extend to the zone of deep moonquakes. While the reconciliation of those predictions with the mechanical properties of rocks might be challenging, alternative lunar interior models without the basal layer are said to be unable to fit the frequency dependence of tidal 〈italic〉Q〈/italic〉. The purpose of our paper is to illustrate under what conditions the frequency‐dependence of lunar tidal 〈italic〉Q〈/italic〉 can be interpreted without the need for deep‐seated partial melt. Devising a simplified lunar model, in which the mantle is described by the Sundberg‐Cooper rheology, we predict the relaxation strength and characteristic timescale of elastically accommodated grain boundary sliding in the mantle that would give rise to the desired frequency dependence. Along with developing this alternative model, we test the traditional model with a basal partial melt; and we show that the two models cannot be distinguished from each other by the available selenodetic measurements. Additional insight into the nature of lunar tidal dissipation can be gained either by measurements of higher‐degree Love numbers and quality factors or by farside lunar seismology.〈/p〉
    Description: Plain Language Summary: As the Moon raises ocean tides on the Earth, the Earth itself gives rise to periodic deformation of the Moon. Precise measurements of lunar shape and motion can reveal those deformations and even relate them to our natural satellite's interior structure. In this work, we discuss two interpretations of those measurements. According to the first one, the lunar interior is hot and a small part of it might have melted, forming a thick layer of weak material buried more than 1,000 km deep under the lunar surface. According to the second one, there is no such layer, and the measured deformation can be explained by the behavior of solid rocks at relatively low temperatures. We show that the two possibilities cannot be distinguished from each other by the existing data.〈/p〉
    Description: Key Points: A lunar mantle governed by the Andrade model fits selenodetic constraints only with a very weak frequency dependence of tidal dissipation. We seek the parameters of two more complex models that may explain the anomalous frequency dependence of tidal 〈italic〉Q〈/italic〉 measured by lunar laser ranging. Both a dissipative basal layer and elastically accommodated grain‐boundary sliding in the deep mantle can result in the same tidal response.
    Description: Czech Science Foundation
    Description: https://doi.org/10.5281/zenodo.7788121
    Keywords: ddc:523 ; Moon ; tidal dissipation ; interior structure
    Language: English
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  • 98
    Publication Date: 2023-07-21
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Hydroxyl defects in nominally anhydrous minerals (NAMs) were potential carriers of water in the early Solar System and might have contributed to the accretion of terrestrial water. To better understand this, we have conducted a nanoscale secondary ion mass spectrometry survey of water contents in olivine and orthopyroxene from a set of equilibrated ordinary chondrites of the L and LL groups (Baszkówka, Bensour, Kheneg Ljouâd, and Tuxtuac) and several ultramafic achondrites (Zakłodzie, Dhofar 125, Northwest Africa [NWA] 4969, NWA 6693, and NWA 7317). For calibration, we used terrestrial olivine and orthopyroxene with H〈sub〉2〈/sub〉O contents determined by Fourier transform infrared. Our 99.7% (~3SD) detection limits are 3.6–5.4 ppmw H〈sub〉2〈/sub〉O for olivine and 7.7–10.9 ppmw H〈sub〉2〈/sub〉O for orthopyroxene. None of the meteoritic samples studied consistently shows water contents above the detection limits. A few exceptions slightly above the detection limits are suspected of terrestrial contamination by ferric oxyhydroxides. If the meteorite samples investigated accreted in the presence of small amounts of water ice, the upper limits of water contents provided by our survey suggest that the retention of hydrogen during thermal metamorphism and differentiation was ineffective. We suggest that loss occurred through combinations of low internal pressures, high permeability along grain boundaries, and speciation of hydrogen into reduced compounds such as H〈sub〉2〈/sub〉 and methane, which are less soluble in NAMs than in water.〈/p〉
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: Europlanet 2020 RI
    Keywords: ddc:549 ; chondrites ; achondrites ; olivine ; orthopyroxene ; water contents
    Language: English
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  • 99
    Publication Date: 2023-07-21
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Due to the complexity of 2D magnetic anomaly maps north of 18°S and the sparsity of seismic data, the tectonic evolution of the northern Lau Basin has not yet been unraveled. We use a multi‐method approach to reconstruct the formation of the basin at ∼16°S by compiling seismic, magnetic, gravimetric and geochemical data along a 185 km‐long crustal transect. We identified a crustal zonation which preserves the level of subduction input at the time of the crust's formation. Paired with the seafloor magnetization, the crustal zonation enabled us to qualitatively approximate the dynamic spreading history of the region. Further assessment of the recent tectonic activity and the degree of tectonic overprinting visible in the crust both suggest a complex tectonic history including a dynamically moving spreading center and the reorganizing of the local magma supply. Comparing the compiled data sets has revealed substantial differences in the opening mechanisms of the two arms of the Overlapping Spreading Center (OSC) that is made up by the northernmost tip of the Fonualei Rift and Spreading Center in the east and the southernmost segment of the Mangatolu Triple Junction in the west. The observed transition from a predominantly tectonic opening mechanism at the eastern OSC arm to a magmatic opening mechanism at the western OSC arm coincides with an equally sharp transition from and strongly subduction influenced crust to a crust with virtually no subduction input. The degree of subduction input alters the geochemical composition, as well as the lithospheric stress response.〈/p〉
    Description: Plain Language Summary: The opening of back‐arc basins is often described as analogy to mid‐ocean ridge spreading, where the only difference is the force driving the extension. However, the northern Lau Basin is a prime example for the shortcomings of this analogy since its crust preserves an image of its complex tectonic history. The complexity results from the short‐lived nature of zones of active rifting and spreading in the northern Lau Basin, which is very different from the temporally and spatially steady nature of spreading centers at mid‐ocean ridges. The analysis of different methods (wide angle seismic data using ocean bottom seismometers, multi‐channel seismic, magnetic, gravity, and geochemical data) has led us to conclude that the Lau Basin's crust at 15°30–17°20′S was formed by a dynamically changing, both in regard of magma composition and position, extensional system that consists of the Fonualei Rift and Spreading Center and the Mangatolu Triple Junction. Nevertheless, the crustal zonation, formed by the varying subduction influence during its formation, is still preserved and affects the stress response of the crust and thus the present‐day tectonic behavior.〈/p〉
    Description: Key Points: Oceanic crust in the north‐eastern Lau Basin formed at the now reorganized FRSC‐MTJ system. The position and the opening mechanisms of back‐arc basin spreading center's change more dynamically than at mid‐ocean ridges. Different opening mechanisms at the southern Mangatolu Triple Junction and northern Fonualei Rift Spreading Center despite their proximity.
    Description: German Ministry of Science and Education
    Description: GEOMAR Helmholtz Centre for Ocean Research Kiel
    Description: Federal Institute for Geosciences and Natural Resources
    Description: https://doi.org/10.1594/PANGAEA.945716
    Description: https://doi.org/10.1594/PANGAEA.945716
    Keywords: ddc:551.1 ; Lau Basin ; back‐arc basins ; multi‐disciplinary approach ; crustal evolution ; traveltime tomography ; extension dynamics
    Language: English
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  • 100
    Publication Date: 2023-07-21
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉The Red Sea is an ideal location for studying rifting processes, offering a young and active intra‐continental rift at the final stages of breakup. We explore the 3D lithospheric structure of the Red Sea by analyzing the gravity response of four end‐member models of rift architecture, including two end‐member types margin architecture Type I—narrow margins and exhumed lithospheric mantle, and Type II—(ultra)wide margins and removal of lithospheric mantle. Additionally, we test two options for the distribution of the oceanic crust (a) limited, that is, confined only to regions of magnetic stripes, and (b) extended, that is, available in vast areas within the basin. South of latitude 23°N, our results suggest the presence of ultrawide margins and limited oceanic crust. North of this latitude, the model of exhumed mantle and limited oceanic crust has minimized residuals compared to the observed gravity field, and agrees with a previously published regional tomographic model. Additionally, we find evidence for the presence of a high‐density body along the southern Arabian coast, probably associated with magmatic underplating. We discuss the lithospheric structure of the Red Sea with respect to the nearby Afar plume, agreeing that the close proximity of the central‐southern regions to the plume promoted a reduction in the strength of the lithosphere, and led to the development of ultrawide margins in these areas.〈/p〉
    Description: Plain Language Summary: The Red Sea is a young example of continental break‐up, a process in which a continent disintegrate into smaller pieces and an ocean is formed between them. We explore the sub‐surface structure of the Red Sea, down to 140 km, aiming to better understand the mechanisms that allowed the Arabian plate to separate from Africa ∼23 million years ago. We examine the gravity response of four end‐member models of rift structures and compare them to the gravity signal measured in this region. We find that the sub‐surface structure in the central‐southern region is different than in the northern regions. Toward the south, the crust is thin and stretched, the lithospheric mantle is absent, and the asthenosphere is rising in a wide region. In the north the lithospheric mantle is exhumed and the asthenosphere is rising in narrow regions below the center of the basin. We discuss the reasons for these differences and support the possibility that the Afar Plume, currently located to the south of the Red Sea, had a thermal weakening effect on the central‐southern regions of the Red Sea, which allowed the lithosphere to deform more easily, having direct implications in the present‐day architecture of the Red Sea.〈/p〉
    Description: Key Points: Gravity modeling in the Red Sea suggests a contrasting rift architecture in the central‐southern regions and in the northern regions. In the central‐southern regions, ultrawide margins and thinned continental crust are underlaid by a broad asthenosphere upwelling. In the northern regions, we infer exhumed mantle lithosphere and a narrow asthenosphere upwelling.
    Description: Minerva Foundation http://dx.doi.org/10.13039/501100001658
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: http://icgem.gfz-potsdam.de/calcgrid
    Description: https://www.gebco.net/data_and_products/gridded_bathymetry_data/#global
    Description: https://ngdc.noaa.gov/mgg/sedthick/
    Description: https://ds.iris.edu/ds/products/emc-af2019/
    Description: https://zenodo.org/record/5771863#.Y6gmBHZBzfs
    Description: https://zenodo.org/record/4482096#.Y6gnPHZBzfs
    Description: https://igmas.git-pages.gfz-potsdam.de/igmas-pages/
    Keywords: ddc:551.1 ; Red Sea ; gravity anomaly ; passive margins ; rifting ; Afro Arabian rift ; Sediment thickness
    Language: English
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