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  • GFZ, Helmholtz-Zentrum  (111)
  • Univ. Berlin  (46)
  • Univ. Hamburg  (44)
  • English  (117)
  • German  (84)
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  • 2020-2023
  • 2010-2014  (201)
  • 2010  (201)
  • 1
    facet.materialart.
    Unknown
    Univ. Hamburg
    Publication Date: 2020-10-07
    Description: The main topic of this work is the introduction of time dependence into PHOENIX. This has been achieved for both the radiation field and the matter in the SN Ia model atmosphere. First, time dependence in the radiative transfer equation has been implemented. Two discretization schemes have been used for the implementation of the time derivative. Test calculations have been performed to confirm the correctness of the implementations. The radiation time scale computed with the time dependent radiative transfer is comparable to a simple analytic approach. Perturbations of the inner boundary condition of the atmosphere move through the whole atmosphere. For instance, an atmosphere with a sinusoidally varying inner light bulb leads to an atmosphere where the luminosity varies sinusoidally everywhere. For the next extension of time dependence for the matter, a simple hydrodynamical solver has been implemented. It computes the changes in the energy of an SN Ia atmosphere by considering the homologous expansion, energy transport and the deposition of energy by g -ray emission due to the radioactive decay of 56Ni and 56Co. Test calculations verified that each part of the solver works correctly. The energy deposition heats the atmosphere and increases the observed luminosity, whereas the adiabatic e expansion cools the atmosphere. The energy transport always pushes the temperature structure of the atmosphere towards the radiative equilibrium state ...
    Description: thesis
    Keywords: 523 ; THI 000 ; THU 162 ; Helligkeit von Sternen {Astronomie} ; Supernovae {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 107 S.
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  • 2
    Publication Date: 2021-03-29
    Description: This work focuses on the distribution of atomic hydrogen in the exosphere of Saturns̉ moon Titan. This work is based on measurements performed by the Hydrogen Deuterium Absorption Cell (HDAC) aboard the Cassini spacecraft, that should directly determine the D/H ratio from the UV emission of atomic hydrogen and deuterium at 121.567 and 121.533 nm, respectively. HDAC measurements were performed on December 26, 2005 during the ninth Titan flyby of the Cassini orbiter. Unfortunately the amount of deuterium in the absorption cell could not be determined. Thus, the purpose, HDAC was designed for could not be achieved. For this reason, HDAC has performed measurements only once. However, the amount of atomic hydrogen in the absorption cell is well known, hence the data using only the hydrogen cell can be used in order to investigate Titans̉ exosphere. This work aims at simulating the HDAC measurements performed in order to investigate Titan’s exosphere, e.g. to determine the distribution of atomic hydrogen. A model of Titan’s exosphere including atomic hydrogen and methane has been developed and the transfer of solar radiation is calculated in order to simulate the HDAC measurements. The radiative transfer is solved using the Monte Carlo method. For the exospheric model, two different atomic hydrogen density distributions were applied, which determine the distribution in the exosphere by different approaches. Density profiles calculated by both models mainly differ in the lower exosphere ...
    Description: thesis
    Keywords: 523 ; TGG 655 ; Saturnmonde {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 171 S.
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  • 3
    Publication Date: 2021-03-29
    Description: Spectro-astrometry is a technique to obtain information about the structure of an astronomical source on sub-diffraction limited spatial scales down to milli- or micro-arcseconds. The method exploits the shift of the photocentre of a structured source over emission/absorption lines in its spectral energy distribution. Sub-diffraction limited resolution can be achieved because the method only uses wavelength-differential information of longslit spectra. Although spectro-astrometry has already been devised by Bailey (1998) and some studies have been performed to date on different astronomic targets, so far, no systematic analysis of the potential of this technique has been undertaken. The aim of this work was to analyse the potential of the method, develop the tools to exploit this potential and write the software which is needed to perform the analysis procedure. To verify the practical feasibility, observations were done with the VLT/CRIRES facility to demonstrate the capabilities of the method with respect to detecting structures on giant star surfaces. All steps of data reduction were analysed with respect to their influence on the spectro-astrometric quantities and a new method for bad pixel detection was devised and implemented ...
    Description: thesis
    Keywords: 523 ; THT 600 ; THK 000 ; THT 400 ; Riesensterne {Astronomie} ; Spektren und Spektroskopie von Sternen {Astronomie} ; Kalte Sterne {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 109 S.
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  • 4
    facet.materialart.
    Unknown
    Univ. Hamburg
    Publication Date: 2021-03-29
    Description: This thesis deals with the high-energy emission from young stellar objects, which are on the one hand still actively accreting from their disk, and on the other hand are no longer deeply obscured by their natal cloud. Stars of spectral type B and A are called Herbig Ae/Be (HAeBe) stars in this stage, all stars of later spectral type are termed classical T Tauri stars (CTTS); strictly speaking both types are defined by spectroscopic signatures, which are equivalent to the evolutionary stage described above. In this thesis CTTS and HAeBes are studied through high-resolution X-ray and UV spectroscopy and through detailed physical simulations. Spectroscopic X-ray data is reduced and presented for two targets: The CTTS V4046 Sgr was observed with Chandra for 100 ks, using a high-resolution grating spectrometer. The lightcurve contains one flare and the He-like triplets of Si XIII, Ne IX and O VII indicate high densities in the X-ray emitting regions. The second target is the HAeBe HD 163296, which was observed with XMM-Newton for 130 ks. The lightcurve shows only moderate variability, the elemental abundance follows a pattern, that is usual for active stars. The He-like triplet of O VII exhibits line ratios similar to coronal sources, indicating that neither a high density nor a strong UV-field is present in the region of the X-ray emission ...
    Description: thesis
    Keywords: 523 ; THP 000 ; Thermodynamische Vorgänge in Sternen {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 84 S.
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  • 5
    Publication Date: 2021-03-29
    Description: This thesis discusses dust formation in binary systems, in particular for binary systems consisting of a Mira like star and a brown dwarf. A Mira-like star is an intermediate mass star in a late stage of their stellar evolution on the Asymptotic Giant Branch (AGB), and a brown dwarf, is a sub-stellar object with a mass below that necessary to maintain hydrogen-burning nuclear fusion reactions in their cores. In their radial pulsating elevated convective atmospheres, Mira-stars often develop strong stellar winds, which are driven by radiation pressure on the dust and lead to a substantial mass-loss of the star. Stellar winds are of central importance for the development of medium-heavy-AGB stars. Also, they are a reliable source for the production of dust particles and heavy elements for the interstellar medium and the chemical evolution of galaxies. In fact, most stars are in binary or multiple star systems.For a complete description of the processes of dust formation in binary star systems it is necessary to study the perturbative influence of a second star in the vicinity of a AGB-star with a strong stellar wind. This endeavour is embedded in a long standing tradition of scientific investigation of dust formation at the Zentrum für Astronomie und Astrophysik (ZAA) at the Technical University of Berlin...
    Description: thesis
    Keywords: 523 ; THT 900 ; TII 900 ; Doppelsterne {Astronomie} ; Interstellarer Staub {Astronomie: Interstellare Materie}
    Language: English
    Type: monograph , publishedVersion
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  • 6
    Publication Date: 2021-03-29
    Description: Many stars evolve not alone but along one or more companions. While the evolution of single isolated stars is well predicted by theoretical calculations, close binary systems with their interactions are on the one hand far more difficult to handle, but on the other hand well constrained in their masses and sizes. One mechanism thought to produce such close binaries is the Common Envelope Evolution (CEE). Especially young post CEE binaries show great temperature differences between both components of about a factor 10 at a separation of just a few solar radii. This work focuses on close binary systems with a hot primary component (e.g. a subdwarf O-type star (sdO)) and a much cooler secondary component (e.g. a main-sequence star), which is heavily influenced by external radiation originating from the first. The technique to include external radiation into the stellar atmosphere code PHOENIX, i.e., the deviation of the outer boundary condition and the change in the temperature correction method, is described in detail. To concentrate on the irradiation effect, other difficulties such as asymmetric effects due to tear-drop shaped stars, ongoing mass accretion or shadows of a circumbinary disc, are avoided by selecting pre-cataclysmic variables (pre CVs) out of the class of close binaries as laboratory. The total eclipsing binary system UU~Sagittae is used as an example for massive irradiation and observed spectral features in the optical are fitted ...
    Description: thesis
    Keywords: 523 ; THK 000 ; THT 900 ; Spektren und Spektroskopie von Sternen {Astronomie} ; Doppelsterne {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 100 S.
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  • 7
    Publication Date: 2021-03-29
    Description: The first extrasolar planet 51 Peg b around the G-type star has been reported in 1995. The planet with few Jupiter masses orbiting its star very closely was detected by measurement of the oscillation in the radial velocity of the host star. In 1999 the first transit, when the planet is eclipsing the host star, of the extrasolar planet HD209458 b was observed with a small ground based photometric telescope. Ever since, new planets in distant systems are continuously being detected with new high precision instruments from the ground and from space. The department of Extrasolar Planets and Atmospheres at Deutsches Zentrum für Luft- und Raumfahrt, Berlin (DLR) is involved in the detection and characterization of extrasolar planets, through participation in the CoRoT space mission. Furthermore, two ground based photometric telescope systems are operated as a ground based support for the space mission CoRoT, dedicated to asteroseismology and to extrasolar planet search with the help of the transit method. The BEST project consists of two small aperture wide field-of-view photometric telescopes devoted to the search for transiting Jupiter-sized extrasolar planets and to the characterization of variable stars in CoRoT target fields...
    Description: thesis
    Keywords: 523 ; THX 100 ; TJ 900 ; TCE 220 ; Detektionsmethoden {Astronomie: Extrasolare Planetensysteme} ; Einzelne Weltraumprojekte ; Bodenständige UV-, Optische und Infrarotteleskope {Astronomische Instrumente}
    Language: English
    Type: monograph , publishedVersion
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  • 8
    Publication Date: 2021-03-29
    Description: Das Antarctic Muon And Neutrino Detector Array (AMANDA) ist ein Cherenkov Detektor, der sich im Gletscher der Antarktis am Südpol befindet. Wir präsentieren die Analyse von Daten, die in den Jahren 2000 bis 2004 gesammelt wurden, die einer effektiven Detektorlaufzeit von 1001 Tagen entsprechen. Die Suche zielt auf den Nachweis von elektomagnetische und hadronische Teilchenschauern, so gennante Kaskaden, die durch Elektron- und Tauneutrinowechselwirkung produziert werden können. Die hadronischen Kaskaden können auch über neutrale Ströme Wechselwirkung von Neutrinos aller Arten produziert werden. Der Kaskadenkanal hat einige Vorteile in der Suche nach einem diffusen Fluss von astrophysikalischen Neutrinos. Durch die gute Energieauflösung des AMANDA Detektors kann man zwischen einem harten astrophysikalische Spektrum und einem weichen atmosphärischen Spektrum unterscheiden. Außerdem ist der atmosphärischen Elektronneutrinos Fluss um eine Gößenordnung kleiner als der atmosphärische Myonneutrinofluss. Der Untergrund von atmosphärischem Myonen aus Luftschauern kann unterdrückt werden, weil diese als Spuren im Detektor erscheinen und leicht zu identifizieren sind...
    Description: thesis
    Keywords: 539.7215 ; 523 ; 550 ; TBN 000 ; TCE 500 ; Neutrino-Astronomie ; Sonstige Instrumente {Astronomische Instrumente}
    Language: English
    Type: monograph , publishedVersion
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  • 9
    facet.materialart.
    Unknown
    Univ. Berlin
    Publication Date: 2021-03-29
    Description: Magnetic cataclysmic variables, also called AM Her stars or 'polars', are close binaries with mass transfer (accretion), consisting of a late-type main-sequence star (commonly called secondary)and a more massive white dwarf with a strong magnetic field. The late-type star is losing mass to the white dwarf. The overflowing matter firstly follows a ballistic trajectory and is then captured by the magnetic field of the white dwarf and guided along the field lines onto the white dwarf. The released gravitational energy is radiated away in all wavelength ranges from infra-red to X-ray. The observed light of an AM Her system is composed of the contributions from the stellar components and the contributions of the accretion column and the accretion region on the white dwarf. The last two components are not only depending on the actual mass transfer rate but also from the spatial orientation of the magnetic field. Since the white dwarf is locked in synchronous rotation, this leads to emission that varies with orbital phase. The decomposition of the observed light from an AM Her system makes it possible to analyse the different components within this system...
    Description: thesis
    Keywords: 523 ; THK 000 ; Spektren und Spektroskopie von Sternen {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 140 S.
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  • 10
    Publication Date: 2021-03-29
    Description: The term "stellar activity" summarizes a number of phenomena on the stellar surface and in the stellar atmosphere. The origin of many of these phenomena are changes in the structure of the stellar magnetic field. While it is possible to directly observe different forms of activity on the Sun in great detail, this remains impossible for other stars. However, by analyzing the spectra of these stars, information about their activity can be obtained. This thesis addresses two aspects of activity: First, the X-ray emission from the positions of A-type stars and a possible mechanism to produce these X-rays and second, the chromospheric activity in the spectral range from late A- to late K-type stars. Since the dynamo, which is responsible for the activity of solar-like stars, emerges in the range of late A- to early F-type stars, this spectral range is of special interest for the understanding of the activity phenomena. To study the X-ray activity of A-type stars, their optical positions as given in the Bright Star Catalogue were compared with the positions of the X-ray sources listed in the ROSAT catalogs. The matching criteria for the ROSAT All-Sky Survey data were 90 arcseconds, 36 arcseconds for the pointing observations with the PSPC and 18 arcseconds for HRI data. Those stars which could be associated with X-ray sources were tested for indications of hidden late-type companions. Variations in the radial velocity, the proper motion, and the light curve were interpreted as signs for binarity...
    Description: thesis
    Keywords: 523 ; THP 000 ; THN 400 ; Thermodynamische Vorgänge in Sternen {Astronomie} ; Sternatmosphären {Astronomie}
    Language: English
    Type: monograph , publishedVersion
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  • 11
    Publication Date: 2021-03-29
    Description: Die Natur der dunklen Materie ist nach wie vor ungeklart und stellt eine der fundamentalsten Fragen der aktuellen Kosmologie dar. In vielen verschiedenen Experimenten wird versucht, diese Teilchen, die sogenannten WIMPs (aus dem Englischen: Weakly Interacting Massive Particles), nachzuweisen. In einigen Modellen der dunklen Materie wird vorhergesagt, dass sehr hochenergetische -Strahlung durch Annihilation der WIMPs in konzentrierten Ansammlungen dunkler Materie produziert wird. Im Rahmen der vorliegenden Arbeit wurden anhand von Beobachtungen im Energiebereich von 100 GeV bis 100 TeV mit dem System abbildender Cherenkov-Teleskope des H.E.S.S.-Experiments (aus dem Englischen: High Energy Stereoscopic System) verschiedene Objekte untersucht, ob die gemessene Strahlung ihren Ursprung in der Annihilation von Teilchen dunkler Materie haben konnte. Das Zentrum unserer Galaxie ist ein in der Literatur viel diskutierter Bereich, in dem sehr hochenergetische -Strahlung aus Annihilation dunkler Materie entstehen konnte. Es wurde mit H.E.S.S. sehr hochenergetische -Strahlung aus dieser Richtung nachgewiesen. Es wird aber gezeigt, dass die gemessene Strahlung aus der Richtung des galaktischen Zentrums nicht ausschlie lich von dunkler Materie erzeugt wird. Daher wurde zusatzlich untersucht, welche Aussagen mit der Hypothese getro en werden konnen, dass nur ein Anteil aus dieser Strahlung besteht. Es konnten interessante Einschrankungen auf das Dichtepro l der hypothetischen DM-Ansammlung gewonnen werden; ein Dichtepro l nach Moore kann fur viele Parametersatze der untersuchten Modelle ausgeschlossen werden. Auf den Wirkungsquerschnitt der Annihilation kann keine relevante Einschrankung erzielt werden..
    Description: thesis
    Keywords: 523 ; 550 ; TII 100 ; TIE 650 ; Dunkle Materie {Astronomie: Interstellare Materie} ; Milchstrasse {Astronomie}
    Language: German
    Type: monograph , publishedVersion
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  • 12
    Publication Date: 2021-03-29
    Description: In this work, nonanalytical line profiles for both cool and hot, dense atmospheres are added to the opacity calculations of the multipurpose stellar atmosphere code PHOENIX. Their influence on model atmospheres and synthetic spectra is studied. Model atmospheres are necessary in order to calculate synthetic spectra and to derive reliable stellar parameters. For cool, dense atmospheres, i.e., of objects of spectral type similar to and lower than latetype M, vanderWaals broadening is the most important pressure broadening mechanism. The spectra of these objects below ~1 micro-meter are dominated by alkali resonance lines. The profiles of the alkali resonance lines, especially of Na ID and KI, determine mostly the pseudo continuum in this wavelength range. Up to this work, classical analytical impact approximated alkali near line wing profiles perturbed by H2, He, and HI, which are the dominant perturbing particles, have been applied. In this work, various nonanalytical alkali line profiles, including far line wing and near line wing profiles, for Na I D, Li I, KI, and Rb I are included in order to describe the strong alkali absorption features which are characteristic for latetype dwarfs. For the alkali resonance line profiles, different theoretical approaches were used describing the far and near line wings. Non analytical alkali profiles for the far and near line wings perturbed by H2 and He are provided in the unified semiclassical theory...
    Description: thesis
    Keywords: 523 ; 550 ; THN 400 ; THK 000 ; Sternatmosphären {Astronomie} ; Spektren und Spektroskopie von Sternen {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 156 S.
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  • 13
    facet.materialart.
    Unknown
    Univ. Berlin
    Publication Date: 2021-03-29
    Description: This work covers the dominant aspects of landforms and processes related to the cold-climate (periglacial) and hyperarid environment of Mars and relates the knowledge obtained from terrestrial research to possible Martian analogue landforms. Among the plethora of landforms related to cold-climate environments and subsurface permafrost on Mars, those features have been investigated in detail that are related to the creep of ice and debris at the Martian dichotomy escarpment and the southern-hemispheric impact basins, especially Hellas Planitia, and which have been described controversially as either glacial or periglacial in nature. Structures related to seasonal freeze-thaw cycles on Mars which are generally known as thermal contraction polygons form a second major focus of this work. Research presented on this topic focuses on the northern hemispheric Utopia Planitia area and the south-polar cap of Mars. This work was carried out on the basis of observational and geomorphometrical analyses by utilizing imaging-sensor and topographic data in order to address questions regarding the history, development, and current state of cold-climate landforms on Mars. This work provides new insights with respect to age, composition, source of debris and ice, and the deformational and degradational history of lobate debris aprons and similar landforms. It is shown that processes which led to creep of debris and ice at the northern hemispheric dichotomy boundary are transitional in nature and are not easily categorized using standard definitions commonly used in terrestrial research...
    Description: thesis
    Keywords: 523 ; 550 ; V 600 ; VAR 800 ; TGG 545 ; Grenzgebiete. Beziehungen. Wirkungen. Einflüsse {Geologische Wissenschaften} ; Periglazialerscheinungen ; Marsoberfläche {Astronomie}
    Language: German
    Type: monograph , publishedVersion
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  • 14
    Publication Date: 2021-03-29
    Description: The subject of this work is the physical characterization of asteroids, with an emphasis on the thermal inertia of near-Earth asteroids (NEAs). Thermal inertia governs the Yarkovsky effect, a non-gravitational force which significantly alters the orbits of asteroids up to ~20 km in diameter. Yarkovsky-induced drift is important in the assessment of the impact hazard which NEAs pose to Earth. Yet, very little has previously been known about the thermal inertia of small asteroids including NEAs.Observational and theoretical work is reported. The thermal emission of asteroids has been observed in the mid-infrared (5-35 æm) wavelength range using the Spitzer Space Telescope and the 3.0 m NASA Infrared Telescope Facility, IRTF; techniques have been established to perform IRTF observations remotely from Berlin. A detailed thermophysical model (TPM) has been developed and extensively tested; this is the first detailed TPM shown to be applicable to NEA data.
    Description: thesis
    Keywords: 523 ; 550 ; TGG 900 ; Planetoide {Astronomie}
    Language: English
    Type: monograph , publishedVersion
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  • 15
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 523 ; 550 ; TH0 000 ; THP 000 ; THT 600 ; Asteroseismologie, Oszillation {Sterne} ; Thermodynamische Vorgänge in Sternen {Astronomie} ; Riesensterne {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 135 S.
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  • 16
    Publication Date: 2021-03-29
    Description: In dieser Doktorarbeit wurden im Rahmen des MAGIC Experimentes neue Datenanalysemethoden implementiert, die sich insbesondere fuer die Analyse von Ereignissen niedriger Gammastrahlungsenergie eignen. Die Methoden konnten erfolgreich in Monte Carlo Studien getestet und auf Beobachtungsdaten des Krebsnebels und der extragalaktischen Gammastrahlungsquelle PG1553+113 angewandt werden. Diese Methoden reichen von ''image cleaning'' Techniken und der Nutzung neuer Bildparameter bis zu fortgeschrittenen g/h-Separations- und Energieabschaetzungsverfahren. Zum ersten Mal wurden die Vorteile von Klassifikations- und Regressionsbaeumen in der Gamma-Astrophysik ausgenutzt, um existierende klassische Methoden zu verbessern. Die Analyse - getestet an Monte Carlo Daten - bewies ihre Zuverlaessigkeit bei der Untersuchung der Gammastrahlungsemission des Krebsnebels, wobei ein hochsignifikanter Exzess im Energiebereich unterhalb 100 GeV in nur 1.7 h nachgewiesen werden konnte. Die Analyse von Daten des BL Lac Objekts PG1553+113 ergab signifikante Exzesse fuer Beobachtungen in den Jahren 2005 und 2006. Das kombinierte alpha-Histogramm zeigt ein Signal mit einer Signifikanz, die 8 sigma ueberschreitet...
    Description: thesis
    Keywords: 523 ; TBK 000 ; THT 200 ; Hochenergieastronomie ; Sterne einzelner Spektralklassen {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 195 S.
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  • 17
    Publication Date: 2021-03-29
    Description: Die H.E.S.S. Kollaboration betreibt ein stereoskopisches System aus vier großen abbildenden Cherenkov-Teleskopen für den Nachweis sehr hochenergetischer Gamma-Strahlung (VHE; 〉 100 GeV). In dieser Arbeit wird über den Nachweis zweier neuer Quellen sehr hochenergetischer Gamma-Strahlung mit den H.E.S.S.-Teleskopen berichtet. Die extragalaktische Quelle 1ES0347-121 gehört zur Klasse der BL Lac Objekte und ist der aktive Kern einer entfernten Galaxie. Detektiert mit einer Signifikanz von mehr als 10 Standard-Abweichungen, ist es die bisher am weitesten entfernte Quelle sehr hochenergetischer Gamma-Strahlung (Rotverschiebung z = 0.1880). Ihr Energiespektrum läßt sich gut durch ein Potenzgesetz mit Photonindex Gamma = 3.08 +/- 0.23_stat +/- 0.1_sys beschreiben. Der integrale Fluss I(E 〉250GeV) entspricht ~2% des Flusses des Krebsnebels. Mit Hilfe des hochenergetische Gamma-Strahlungsspektrum von 1ES 0347-121 werden Einschränkungen auf die Dichte des extragalaktischen diffusen Photonfeldes bestimmt (s. unten). Bei der zweiten Quelle handelt es sich um die ausgehnte Quelle HESS J1023-577, die mit dem jungen, massiven Sternenhaufen Westerlund 2 und dessen Umgebung assoziert wird. Junge und massereichen Sterne strahlen starke Sternenwinde ab, die durch Schockbeschleunigung hochenergetische Teilchen produzieren können. Zum erstenmal konnte eine Quelle sehr hochenergetischer Gamma-Strahlung mit einer solchen Umgebung sicher identifiziert werden. Das Energiespekrum reicht von ~400GeV bis ~20TeV und läßt sich gut durch eine Potenzgesetz mit Photonindex Gamma=2.53 +/- 0.16_stat +/- 0.1_syst beschreiben.
    Description: thesis
    Keywords: 523 ; TIE 400 ; TBK 000 ; TCE 240 ; Spektren und Leuchtkraft von Sternsystemen {Astronomie} ; Hochenergieastronomie ; Röntgen- und Gammateleskope {Astronomische Instrumente}
    Language: English
    Type: monograph , publishedVersion
    Format: 123 S.
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  • 18
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 523 ; THP 000 ; Thermodynamische Vorgänge in Sternen {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 76 S.
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  • 19
    facet.materialart.
    Unknown
    Univ. Berlin
    Publication Date: 2021-03-29
    Description: Comets belong to the most pristine objects in the Solar System. The study of comets therefore allows one to put constraints to the physical and chemical conditions in the pre-planetary disc. In this work, a one-dimensional simplified multi-fluid model for the analysis of the chemistry in cometary comae was constructed. This model was used for the study of the formation of the C3 and C2 radicals. For this purpose, radial profiles of the optical emissions of C3 and C2 in comets C/2001 Q4 NEAT, C/2002 T7 LINEAR, and 9P/Tempel 1 at heliocentric distances between 1.0 AU and 1.5 AU were analysed. These profiles were obtained by means of long-slit spectroscopy. A reaction network for the formation of C3 and C2 at larger heliocentric distances (Helbert 2002) was updated and extended. Molecules and radicals were identified for which photodissociation reaction rates have to be further constrained before the formation of C3 and C2 can be understood. As comets of special interest, the comets 67P/Churyumov-Gerasimenko and 9P/Tempel 1 were studied in more detail. Both comets are targets of space missions...
    Description: thesis
    Keywords: 523 ; TGL 200 ; Kometen {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 227 S.
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  • 20
    Publication Date: 2021-03-29
    Description: Diese Arbeit beschreibt die Verbesserung der Richtungsstabilisierung des Flugzeugteleskops SOFIA. Das Ziel des Flugzeugteleskops SOFIA sind astronomische Beobachtungen im Infrarotbereich. Da der Wasserdampf der Erdatmosphäre den Großteil der Infrarotstrahlung absorbiert, sind solche Beobachtungen mit herkömmlichen Teleskopen von der Erdoberfläche aus kaum möglich. Um unerwünschte Drehbewegungen des Flugzeugteleskops, z.B. hervorgerufen durch Luftturbulenzen, auszugleichen, ist zuerst eine genaue Messung bzw. Schätzung derselben notwendig. Diese Informationen werden dann mittels Computer in Echtzeit weiterverarbeitet. Anschließend sorgen dann Motoren dafür, das Teleskop wieder in die gewünschte Lage zu drehen. Die Motoren können das Teleskop nur so genau ausrichten, wie es die Genauigkeit des Meßsystems zuläßt. Die Messung der Drehbewegungen geschieht mit drei zueinander senkrecht angeordneten Gyroskopen. Diese weisen jedoch Fehler auf, so daß sich die Ausrichtgenauigkeit verschlechtert. Deshalb werden mit Hilfe einer auf das Teleskop montierten Kamera in regelmäßigen Zeitabständen Bilder des Sternhimmels aufgenommen. Aus diesen Bildern wird dann mit Hilfe der dort sichtbaren Sterne die aktuelle Orientierung des Teleskops bestimmt. Mittels dieser Orientierung werden dann die Fehler der Gyroskope korrigiert und der lineare Fehleranteil für die Zukunft extrapoliert. Dieser Fehler wird dann schon im Voraus vom Teleskoplageregler berücksichtigt. Dadurch wird der quasikonstante Fehleranteil minimiert. Je besser dieser Fehler geschätzt wird, desto geringer ist die Drift des Teleskops um seine Achsen. Dadurch erhöht sich die Richtungsstabilisierung ...
    Description: thesis
    Keywords: 522 ; TCE 200 ; Teleskope {Astronomische Instrumente}
    Language: German
    Type: monograph , publishedVersion
    Format: 125 S.
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  • 21
    facet.materialart.
    Unknown
    Univ. Hamburg
    Publication Date: 2021-03-29
    Description: Unter stellarer Aktivität werden eine Reihe von Phänomenen in den unterschiedlichen Atmosphärenschichten zusammengefasst, die eng mit dem Magnetfeld des einzelnen Sterns verbunden sind. Da eine direkte Auflösung der Sternoberfläche, wie uns dies bei der Sonne möglich ist, für aktive Sterne noch in ferner Zukunft liegt, können diese Phänomene im Normalfall nicht direkt beobachtet werden. Es können aber aus der Spektralanalyse indirekt Informationen über die Aktivität eines Sterns gewonnen werden. Die vorliegende Arbeit beschäftigt sich mit koronaler und chromosphärischer Aktivität von mittleren und späten M Sternen und deren Nachweis und Analyse in UVES Echelle-Spektren von 3030 bis 3880 und 4580 bis 6680 A. Dabei widmet sich der erste Teil der Arbeit dem Nachweis der verbotenen koronalen Fe XIII Linie bei 3388 A. Das mehrere Millionen Kelvin heiße koronale Gas wird normalerweise - und am leichtesten - im Röntgenbereich beobachtet...
    Description: thesis
    Keywords: 523 ; THK 000 ; THN 400 ; Spektren und Spektroskopie von Sternen {Astronomie} ; Sternatmosphären {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 101 S.
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  • 22
    facet.materialart.
    Unknown
    Univ. Hamburg
    Publication Date: 2021-03-29
    Description: The high ionization state of the intergalactic medium (IGM) is maintained by the metagalactic UV background radiation. This ionizing radiation field is supposed to be the integrated radiation of quasars and young star-forming galaxies, which is reprocessed and attenuated by the intergalactic gas. Since the UV background is inaccessible to direct observations, it is impossible to test theoretical predictions of its spectral energy distribution in great detail. However, constraints can be derived from studies of metal absorption systems, the HI Lyman alpha opacity, or the HeII Lyman alpha forest, respectively. Observations of the HeII/HI column density ratio eta particularly probe the variations of the UV background. Since unobscured quasars permitting observation of HeII absorption are rare, there are only two lines of sight, towards the quasars HE2347-4342 and HS1700+6416, where the HeII Lyman alpha forest can be resolved. This work presents a study of the UV background at redshifts z 〈 3 investigating the HeII absorption towards the quasars HS1700+6416 (z = 2.72), which provides the second line of sight where the HeII Lyman alpha forest is resolved. The numerous metal line systems detected in the spectra of this QSO are studied in order to avoid biases due to unrecognized metal line absorption in the HeII forest. In this connection, several shapes of the ionizing radiation are tested for each system. The majority of the considered systems, in particular those at z 〉 2, is best reproduced with an ionizing radiation similar to the UV background of Haardt & Madau (2001), where the HeII break, formally located at 4 Ryd, is shifted to lower energies (~ 3 Ryd), probably due to the opacity of the higher HeII Lyman series lines ...
    Description: thesis
    Keywords: 523 ; TIE 400 ; TBI 000 ; Spektren und Leuchtkraft von Sternsystemen {Astronomie} ; Ultraviolett-Astronomie
    Language: English
    Type: monograph , publishedVersion
    Format: 131 S.
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  • 23
    Publication Date: 2021-03-29
    Description: Die Untersuchung der Oberflächenzusammensetzung von Ganymed basiert auf Daten des abbildenden Spektrometers NIMS an Bord der Raumsonde Galileo, das die Ganymedoberfläche im Spektralbereich des Nahen Infrarot detektiert. Die Verarbeitung der vorliegenden Spektraldaten einschließlich der quantitativen Analyse der spektralen Signaturen in den Reflexionsspektren von Ganymed wie deren Charakterisierung in Abhängigkeit der geologischen Oberflächenstrukturen bildet den zentralen Teil der Arbeit. Die Ergebnisse zeigen, dass Veränderungen der Reflexionseigenschaften der Ganymedoberfläche auf den wechselnden Anteil von Wassereis und Gesteinsmaterial und dem Gehalt an CO2 zurückzuführen sind. Die simultane Analyse der Absorptionen von Wassereis erlaubt es ferner, erstmals Veränderungen des relativen Anteils und der Partikelgröße von Wassereis getrennt voneinander zu erfassen...
    Description: thesis
    Keywords: 523.45 ; 550 ; TGG 605 ; Jupitermonde {Astronomie}
    Language: German
    Type: monograph , publishedVersion
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  • 24
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 523 ; TIE 900 ; TBG 000 ; TC 200 ; Sonstige Sternensysteme {Astronomie} ; Infrarot-Astronomie ; Astronomische Beobachtungen vom Weltraum aus
    Language: English
    Type: monograph , publishedVersion
    Format: 181 S.
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  • 25
    facet.materialart.
    Unknown
    Univ. Berlin
    Publication Date: 2021-03-29
    Description: AM Herculis stars (or 'polars') are close binaries consisting of a white dwarf with a strong magnetic field and a main sequence star (the 'secondary') which is losing mass to the white dwarf. The magnetic field channels the matter to the magnetic poles, where the released potential energy is radiated away - mainly in X-rays and the UV. The spatial structure of these objects cannot be observed directly, because their apparent size is too small. Indirect imaging methods are capable of restoring information which is only contained in observational data as projections onto a sub-space. These tomographic methods are known from medicine, but can also be applied to astronomical data, when a number of measurements can be regarded as views of the same object under different aspect angles. In this work tomographic methods are applied to time-resolved spectroscopic data of polars. Spectral lines seen in the radiation emitted by the constituents of these systems are notably Doppler-shifted. The Doppler-shift is depending on the viewing angle of the system ('inclination') and is varying with orbital phase. Time-series of one-dimensional data (spectra) can be used to create a two-dimensional map of the intensity distribution in velocity-space (Doppler-tomography), or a map of the line-flux on the assumed surface of the mass-losing star (Roche-tomography) from the line profile changes ...
    Description: thesis
    Keywords: 523 ; THT 900 ; THU 155 ; Doppelsterne {Astronomie} ; Eruptionsveränderliche {Astronomie: Sterne}
    Language: English
    Type: monograph , publishedVersion
    Format: 124 S.
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  • 26
    Publication Date: 2021-03-29
    Description: The aim of this thesis is to obtain as much information as possible, about global solutions of the Cauchy problem for the Einstein-Vlasov-scalar field system with spherical, plane and hyberbolic symmetries written in areal coordinates. The sources of this system are generated by both a distribution function and a linear scalar field subject to the Vlasov and wave equations respectively. This system describes the evolution of self-gravitating collisionless matter and scalar waves within the context of general relativity. We consider the cosmological case. That is spacetimes possess a compact Cauchy hypersurface and then, data are given on a compact 3-manifold. We extend the local-in-time results obtained by G. Rein for the Einstein-Vlasov system with collisionless matter alone. This extension concerns pointwise estimates for hyperbolic equations by the method of characteristics. This means that the system is transformed to a system of ordinary differential equations which are integrated along characteristics ...
    Description: thesis
    Keywords: 523 ; TFA 000 ; Relativistische Astrophysik, Gravitation
    Language: English
    Type: monograph , publishedVersion
    Format: 85 S.
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  • 27
    Publication Date: 2021-03-29
    Description: Die physikalischen Ursachen für das Auftreten massiver Winde bei entwickelten Sternen sind weitgehend unverstanden. Aus diesem Grund ist es bisher noch nicht gelungen, von einer empirischen Beschreibung des Phänomens zu einem befriedigenden hydrodynamischen Ansatz überzugehen. Auch die üblichen diagnostischen Methoden ergeben kein einheitliches Bild der Windeigenschaften und können charakteristische Feinstrukturen in hochaufgelösten Spektren nicht erklären. Zudem ist nicht verstanden, ob die widersprüchlichen Ergebnisse der Analysen von Einzelsternen und Doppelsternsystemen von intrinsischer Natur sind oder methodische Unzulänglichkeiten widerspiegeln. Die in den Winden beobachteten Überschallturbulenzen scheinen eine zentrale Rolle für das Verständnis der dynamischen Prozesse zu spielen. In den üblichen Analyseverfahren wird diese Geschwindigkeitskomponente in der einfachen mikroturbulenten Approximation beschrieben. Es ist allerdings fraglich, ob die komplexe Struktur der Winde dadurch adäquat erfasst wird. Ein von Traving (1975) entwickeltes alternatives Turbulenzmodell gestattet es, Geschwindigkeitskorrelationen in einer stochastischen Näherung zu berücksichtigen ...
    Description: thesis
    Keywords: 523 ; THP 000 ; Thermodynamische Vorgänge in Sternen {Astronomie}
    Language: German
    Type: monograph , publishedVersion
    Format: 137 S.
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  • 28
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; VBQ 900 ; VBQ 800 ; VEO 170 ; Hydrogeologie einzelner Regionen ; Aquifere {Hydrogeologie} ; Sudan {Geologie}
    Language: English
    Type: monograph , publishedVersion
    Format: 133 S.
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  • 29
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 560 ; VDH 200 ; VEX 100 ; VWH 200 ; VZX 100 ; VKB 380 ; Jura ; Anden {Geologie} ; Jura {Stratigraphische Paläontologie} ; Anden {Paläontologie} ; Sedimente bestimmter Regionen
    Language: German
    Type: monograph , publishedVersion
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  • 30
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 910 ; 551 ; VBQ 900 ; VEB 213 ; VJC 110 ; Hydrogeologie einzelner Regionen ; Brandenburg, Sachsen-Anhalt & Mecklenburg-Vorpommern {Geologie} ; Geochemie des Grundwassers, Porenwassers
    Language: German
    Type: monograph , publishedVersion
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  • 31
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 549 ; VGB 700 ; VGA 300 ; VHB 820 ; Spektroskopische Methoden {Mineralogie} ; Kristallstrukturen ; Inselsilikate {Mineralogie}
    Language: German
    Type: monograph , publishedVersion
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  • 32
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 549 ; VHB 850 ; VGF 200 ; Kettensilikate {Mineralogie} ; Phasengleichgewichte und Umbildungen {Mineralogie}
    Language: English
    Type: monograph , publishedVersion
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  • 33
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; VQC 000 ; VRA 110 ; VTG 000 ; Lagerstättengenese ; Eisenerz {Lagerstättenkunde} ; Osteuropa und Asiatische Teile der ehemaligen Sowjetrepubliken {Rohstoffgeologie}
    Language: German
    Type: monograph , publishedVersion
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  • 34
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; VGA 420 ; Optische Methoden {Mineralogie: Kristallographie}
    Language: German
    Type: monograph , publishedVersion
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  • 35
    facet.materialart.
    Unknown
    Univ. Hamburg
    Publication Date: 2021-03-29
    Description: The Levantine Basin - a seismic investigation of the crustal structure and the evolution of the Messinian evaporites ABSTRACT This work presents an analysis of the crustal structure of the Levantine Basin, based on refraction seismic and gravity data, and an analysis of the evolution of the Messinian evaporites, based on reflection seismic data. Forward and inverse modelling of refraction seismic traveltimes along two profiles yielded 2-D velocity-depth-profiles. Gravity modelling along these profiles provided further information on the crustal structure. A great number of reflection seismic profiles was used for the analysis of the Messinian evaporites, which allowed an exhaustive investigation of the geometry of the evaporite layers, depositional phases of the evaporites and of their structural evolution. The Levantine Basin is located in the Southeastern Mediterranean Sea. The basin and its margin are key areas for the understanding of the geodynamic evolution of the Eastern Mediterranean. The opening of the Levantine Basin is closely related to the opening of the Neo-Tethys. Many geodynamic reconstructions of this area have been developed, but the key question, the origin of the crust, remained open. The Levantine Basin is also a world class site for studying the initial stages of salt tectonics driven by differential sediment load. The Messinian evaporites are comparatively young (deposited during the Messinian Salinity Crisis 5.9 - 5.3 Ma ago), the sediment load varies along the basin margin, they are hardly tectonically overprinted, and the geometry of the basin and the overburden is well-defined...
    Description: thesis
    Keywords: 550 ; TSF 000 ; VAE 820 ; VEF 000 ; Südeuropa und Mittelmeergebiet {Geophysik} ; Sedimentationsbecken als Erdkrustentypen {Geologie} ; Südeuropa und Mittelmeergebiet {Geologie}
    Language: English
    Type: monograph , publishedVersion
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  • 36
    Publication Date: 2021-03-29
    Description: Central Asia is characterized by a number of spectacular tectonic units such as the Tibetan Plateau, the Tien Shan intra-continental mountain belt and the Altyn Tagh strike-slip fault. Deformation of the lithosphere of these units is not well understood. In this dissertation, an attempt is made to answer the following tectonic questions: To what extent do the tectonic units formed in the upper crust in the course of the convergence between India and Eurasia weaken the underlying lithosphere? How is the Tibetan Plateau gravita-tionally compensated along its northern boundary? Do the Altyn Tagh and/or West Kunlun faults persist as vertical strike-slips throughout the crust and mantle lithosphere, thus representing a fundamental plate boundary? Which dynamic processes in the crust and mantle of the Tien Shan are responsible for intra-continental mountain building? What characterizes the local stress field in the Tien Shan and what causes the deformation of these mountains? To answer these questions, the elastic plate theory is used to interpret gravity and topography data, and in turn to derive specific characteristics of the lithospheric structure in Central Asia. Theoretical deflection of the elastic plate or plates were calculated using the 3D and 2D finite-difference methods. Variable-rigidity elastic plates are subjected to vertical and horizontal loads, shear forces, and terminal bending moments. Surface topo-graphic data from the Topo30 dataset is used as vertical surface loading to calculate the flexure of the elastic lithosphere...
    Description: thesis
    Keywords: 551.8 ; 622.15 ; 551 ; 550 ; VAE 400 ; VEK 000 ; TQA 000 ; TSK 000 ; VAE 400 ; VEK 000 ; TQA 000 ; TSK 000 ; Tektogenese {Geologie} ; Zentralasien {Geologie} ; Gravimetrische Verfahren {Geophysik} ; Zentralasien {Geophysik}
    Language: English
    Type: monograph , publishedVersion
    Format: 136 Bl.
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  • 37
    Publication Date: 2021-03-29
    Description: Mit der Annahme schwacher Anisotropie vereinfachen sich die Lösungen der Modellierung und Inversion anisotroper Medien. Üblicherweise werden Perturbation-Methoden zur Beschreibung der Wellen-Ausbreitung in schwach anisotropen Medien verwendet, ein anisotropes Medium wird ersetzt durch ein isotropes Hintergrundmodell. Hier lässt sich die Wellenausbreitung leicht behandeln und die anisotropen Effekte werden mit Hilfe der Perturbations-Methode berechnet. Um die jeder Perturbations-Methode anhaftenden Fehler zu minimieren, sollte das gewählte isotrope Hintergrundmedium dem korrektem anisotropen Medium so ähnlich wie möglich sein. Zur Bestimmung des optimalen isotropen Mediums wurden Formeln für sektoriell best angepasste isotrope Medien entwickelt. Deren Anwendung wurde anhand von Modellen mit transversal isotropen und orthorombischen Symmetrien gezeigt...
    Description: thesis
    Keywords: 551.22 ; 550 ; Seismische Wellen {Geophysik} ; Übertragungsmedien {Seismologie}
    Language: English
    Type: monograph , publishedVersion
    Format: 134 S.
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  • 38
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551.1 ; 550 ; VKA 150 ; TOO 000 ; Physikalische Petrologie ; Geothermik {Geophysik}
    Language: German
    Type: monograph , publishedVersion
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  • 39
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 622.15 ; 552.5 ; 624.51 ; 550 ; VBP 800 ; TQJ 000 ; Ingenieurgeologie bei der unterirdischen Speicherung und Lagerung ; Geophysikalische Methoden in anderen Wissenschaftsgebieten
    Language: German
    Type: monograph , publishedVersion
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  • 40
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551.5 ; 550 ; TUA 700 ; TVH 300 ; Verfahren zur Untersuchung der freien Atmosphäre {Meteorologie} ; Lufttemperatur {Meteorologie}
    Language: English
    Type: monograph , publishedVersion
    Format: 153 S.
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  • 41
    Publication Date: 2021-03-29
    Description: With regard to geodesy optimizing procedures for nonlinear adjustment problems are presented. The procedures can be divided into local and global optimization techniques according to the type of the problem. If good initial values are given, the usage of local optimization techniques, (e.g., the Gauß-Newton procedure) is justified. If this is not the case, and the minimizing function has various local minimums, a global strategy must be implemented. Applying global optimization techniques one will not yield the global solution with certainty; only a probabilistic solution will be obtained. Nevertheless, combining local and global strategy and inclusion of all available a priori-information, a global optimizing system can be established that yields practical results for a wide area of problems. With the increase of the capacity of modern computers the efficiency of global optimization algorithms comes along ...
    Description: thesis
    Keywords: 526.9 ; 550 ; UND 000 ; Fehlertheorie {Praktische Geodäsie}
    Language: German
    Type: monograph , publishedVersion
    Format: 85 S.
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  • 42
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 622.15 ; 550 ; Elektrische Verfahren {Geophysik} ; Mitteleuropa {Geophysik}
    Language: German
    Type: monograph , publishedVersion
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  • 43
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551.6 ; 550 ; TVF 000 ; TWB 000 ; TWH 100 ; Allgemeine Zirkulation der Atmosphäre {Meteorologie} ; Statistische Klimatologie und Klimatologische Modelle ; Einfluss der Verteilung von Land und Meer {Klimatologie}
    Language: German
    Type: monograph , publishedVersion
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  • 44
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551.5 ; 550 ; EIGA 100 ; TVH 100
    Language: German
    Type: monograph , publishedVersion
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  • 45
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551.701 ; 549 ; 550 ; VBN 500 ; Geochronologie einzelner Regionen im allgemeinen
    Language: German
    Type: monograph , publishedVersion
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  • 46
    Publication Date: 2021-03-29
    Description: Am Ausgangspunkt dieser Arbeit stand die Frage, ob und in welcher Form beim Bau der Autobahnen vor 1933 in Deutschland, Frankreich und Italien die Wahrnehmung von Landschaft' berücksichtigt wurde. Da die Diskussion um die veränderte Wahrnehmung von Landschaft' bei steigender Reisegeschwindigkeit erstmals intensiv im Zusammenhang mit dem Bau der Eisenbahnen im 19. Jahrhundert geführt wurde, leitet ein Rückblick auf diese Zeit die Arbeit ein. Hier konnte die historische Dimension des Untersuchungsthemas verdeutlicht sowie dessen wesentliche Diskussionspunkte aufzeigt werden, die - in modifizierter Form - ein knappes Jahrhundert später bei der Planung und beim Bau der Autobahnen erneut aufgegriffen wurden. Der italienische Futurismus wurde anschließend daraufhin untersucht, ob er neue Darstellungsformen für die veränderte Wahrnehmung von Landschaft' hervorgebracht hat. Das nachfolgende Kapitel diente dazu, die Bedeutung des Themas der Arbeit aufzuzeigen. Eine zusammenstellende Übersicht über den Status des Autobahnbaus und der Autobahnplanungen in Deutschland Frankreich und Italien vor 1933, die bis dato fehlte, wurde hier gegeben. Von zentraler Bedeutung war im Rahmen dieser Arbeit die Analyse der Gestaltungselemente ...
    Description: thesis
    Keywords: 944 ; QEB 000 ; Geographische Umweltwahrnehmung und Raumbewertung
    Language: German
    Type: monograph , publishedVersion
    Format: 307 S.
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  • 47
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; VAE 890 ; VAE 130 ; VBE 000 ; TOE 000 ; TSX 500 ; VEX 500 ; Ozeanische Kruste {Tektonik} ; Geomechanik ; Modellierung von Prozessen in der Geosphäre ; Physikalisches Verhalten der Erde {Geophysik} ; Chile {Geophysik} ; Chile {Geologie}
    Language: English
    Type: monograph , publishedVersion
    Format: 118 S.
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  • 48
    facet.materialart.
    Unknown
    GFZ, Helmholtz-Zentrum
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; TSX 500 ; VEX 100 ; VEX 500 ; VAE 500 ; TOH 800 ; Chile {Geophysik} ; Anden {Geologie} ; Chile {Geologie} ; Geotektonische Entwicklung der Erdkruste {Geologie} ; Paläoerdbeben {Geophysik}
    Language: English
    Type: monograph , publishedVersion
    Format: 108 S.
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  • 49
    facet.materialart.
    Unknown
    GFZ, Helmholtz-Zentrum
    Publication Date: 2021-03-29
    Description: Ein transversales Störungssystem im Nahen Osten, die Dead Sea Transform (DST), trennt die Arabische Platte von der Sinai-Mikroplatte und erstreckt sich von Süden nach Norden vom Extensionsgebiet im Roten Meer über das Tote Meer bis zur Taurus-Zagros Kollisionszone. Die sinistrale DST bildete sich im Miozän vor etwa 17 Ma und steht mit dem Aufbrechen des Afro-Arabischen Kontinents in Verbindung. Das Untersuchungsgebiet liegt im Arava Tal zwischen Totem und Rotem Meer, mittig über der Arava Störung (Arava Fault, AF), die hier den Hauptast der DST bildet. Eine Reihe seismischer Experimente, aufgebaut aus künstlichen Quellen, linearen Profilen über die Störung und entsprechend entworfenen Empfänger-Arrays, zeigt die Untergrundstruktur in der Umgebung der AF und der Verwerfungszone selbst bis in eine Tiefe von 3-4 km. Ein tomographisch bestimmtes Modell der seismischen Geschwindigkeiten von P-Wellen zeigt einen starken Kontrast nahe der AF mit niedrigeren Geschwindigkeiten auf der westlichen Seite als im Osten. Scherwellen lokaler Erdbeben liefern ein mittleres P-zu-S Geschwindigkeitsverhältnis und es gibt Anzeichen für Änderungen über die Störung hinweg ...
    Description: thesis
    Keywords: 551 ; VAE 850 ; TQC 220 ; TSI 000 ; VEI 400 ; Festländische Lineamente {Geologie} ; Reflexionsseismik {Geophysik} ; Vorderasien {Geophysik} ; Israel, Palästina {Geologie}
    Language: English
    Type: monograph , publishedVersion
    Format: 142 S.
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  • 50
    facet.materialart.
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    GFZ, Helmholtz-Zentrum
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551
    Language: German
    Type: monograph , publishedVersion
    Format: 145 S.
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  • 51
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; TQG 000 ; TOO 000 ; TOD 410 ; TSV 200 ; TSZ 300 ; Geophysikalische Bohrlochmessungen ; Geothermik {Geophysik} ; Oberer Erdmantel {Geophysik} ; USA {Geophysik} ; Pazifischer Ozean {Geophysik}
    Language: German
    Type: monograph , publishedVersion
    Format: 94 S.
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    Publication Date: 2021-03-29
    Description: report
    Keywords: 551 ; TQH 000 ; TQA 000 ; TOF 000 ; Aerogeophysik ; Gravimetrische Verfahren {Geophysik} ; Schwerkraft {Geophysik}
    Language: English
    Type: article , publishedVersion
    Format: 48 S.
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    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551
    Language: German
    Type: monograph , publishedVersion
    Format: 116 S.
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    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; VAE 811 ; VEX 100 ; VEX 300 ; Alpidische Orogene {Geologie} ; Anden {Geologie} ; Bolivien und Paraguay {Geologie}
    Language: German
    Type: monograph , publishedVersion
    Format: 128 S.
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    Publication Date: 2021-03-29
    Description: report
    Keywords: 551
    Language: English
    Type: article , publishedVersion
    Format: 106 S.
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    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 538.78 ; 551 ; 550
    Language: German
    Type: monograph , publishedVersion
    Format: 102 S.
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  • 57
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; TQD 000 ; TSR 000 ; VAE 814 ; VER 200 ; Elektrische Verfahren {Geophysik} ; Südafrika {Geophysik} ; Präkambrische Orogene {Geologie} ; Namibia {Geologie}
    Language: German
    Type: monograph , publishedVersion
    Format: 133 S.
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  • 58
    Publication Date: 2021-03-29
    Description: report
    Keywords: 551 ; TOB 300 ; TOD 500 ; TOF 000 ; TOT 400 ; Polbewegungen {Geophysik: Erde} ; Erdkern {Geophysik} ; Schwerkraft {Geophysik} ; Magnetfeld der Erde im allgemeinen {Geophysik}
    Language: English
    Type: article , publishedVersion
    Format: 15 S.
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    Publication Date: 2021-03-29
    Description: lecture
    Keywords: 551
    Language: English
    Type: anthology , publishedVersion
    Format: 675 S.
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    Publication Date: 2021-03-29
    Description: report
    Keywords: 551 ; TOB 100 ; Drehbewegungen {Geophysik: Erde}
    Language: English
    Type: article , publishedVersion
    Format: 8 S.
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    Publication Date: 2021-03-29
    Description: report
    Keywords: 551 ; TOB 300 ; Polbewegungen {Geophysik: Erde}
    Language: English
    Type: article , publishedVersion
    Format: 9 S.
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    Publication Date: 2021-03-29
    Description: report
    Keywords: 551
    Language: English
    Type: article , publishedVersion
    Format: 39 S.
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    Publication Date: 2021-03-29
    Description: report
    Keywords: 551
    Language: English
    Type: article , publishedVersion
    Format: 28 S.
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    Publication Date: 2021-03-29
    Description: report
    Keywords: 551 ; VRG 000 ; ZHB 380 ; Geothermalfelder ; Geothermische Energie {Energietechnik}
    Language: German
    Type: monograph , publishedVersion
    Format: 70 S.
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    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; VRG 000 ; Geothermalfelder
    Language: German
    Type: monograph , publishedVersion
    Format: 175 S.
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    GFZ, Helmholtz-Zentrum | [Bibliothek des Wiss.-Parks Albert Einstein] [Vertrieb], [Potsdam]
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551.792 ; 551 ; VAU 000 ; TWC 500 ; VKB 380 ; VKB 378 ; VBO 000 ; VEB 167 ; Paläolimnologie {Geologie} ; Klimaschwankungen und Klimaänderungen im Quartär ; Sedimente bestimmter Regionen ; Rhytmite {Sedimentologie} ; Isotopengeologie ; Westalpen {Geologie}
    Language: German
    Type: monograph , publishedVersion
    Format: 91 S.
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    GFZ, Helmholtz-Zentrum | [Bibliothek des Wiss.-Parks Albert Einstein] [Vertrieb], [Potsdam]
    Publication Date: 2021-03-29
    Description: The glacial-isostatic adjustment in Iceland resulting from the recent melting of the Vatnajökull ice cap is controlled by the viscosity distribution in the earth's interior and by the details of the melting history. Interpretations of the results of GPS and gravity measuring campaigns in the time interval 1991-2000 and 1992-1999, respectively, by means of laterally homogeneous earth models for the determination of the lithosphere thickness, the asthenosphere thickness and the asthenosphere viscosity have so far been not fully satisfactory. In particular near the ice margin, the fitting of the computed land uplift and gravity change to the observational data was inadequate, which may be related to the neglegt of the Iceland plume in the laterally homogeneous earth models. In the present study, a program package is used for the modelling of the land uplift and gravity change that allows the computation of load-induced perturbations of a Maxwell-viscoelastic, incompressible, self-gravitating, spherical earth model. To simulate the presence of the plume below the Vatnajökull, an axisymmetric viscosity distribution is used, where the plume radius and the plume viscosity are free parameters. Based on seismic results, a 6-km-thick lithosphere is assumed above the plume, which thickens to 35 km in the peripheral region of the plume. The melting history of the Vatnajökull is founded on interpretations of geomorphological and climatological investigations and is simulated by a load co-axial with the plume with parabolic profile and time-dependent radius. The results of the modelling favour a plume radius of ~80 km and a plume viscosity of (0.3-1.0) x 10^{18} Pa s.
    Description: report
    Keywords: 551
    Language: English
    Type: article , publishedVersion
    Format: 20 S.
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    GFZ, Helmholtz-Zentrum | [Bibliothek des Wiss.-Parks Albert Einstein] [Vertrieb], [Potsdam]
    Publication Date: 2021-03-29
    Description: report
    Keywords: 551 ; VAE 300 ; TQI 000 ; UNH 100 ; Epirogenese {{Geologie}} ; Geophysikalische Satellitenfernerkundung ; GPS {Praktische Geodäsie}
    Language: English
    Type: article , publishedVersion
    Format: 28 S.
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    Publication Date: 2021-03-29
    Description: report
    Keywords: 551
    Language: English
    Type: article , publishedVersion
    Format: 228 S.
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    GFZ, Helmholtz-Zentrum | [Bibliothek des Wissenschaftsparks Albert Einstein] [Vertrieb], [Potsdam]
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; TOH 530 ; VAE 200 ; VAE 130 ; Häufigkeit und Verbreitung von Erdbeben {Geophysik} ; Geodynamik der Lithosphäre {Geologie} ; Geomechanik
    Language: English
    Type: monograph , publishedVersion
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  • 71
    Publication Date: 2021-03-29
    Description: The Aggregated Carbon Cycle, Atmospheric Chemistry, and Climate model (ACC2) (Tanaka and Kriegler et al., 2007a) describes physical-biogeochemical processes in the Earth system at a global-annual-mean level. Compared to its predecessors NICCS (Hooss, 2001) and ICM (Bruckner et al., 2003), ACC2 adopts more detailed parameterizations of atmospheric chemistry involving a set of agents (CO2, CH4, N2O, O3, SF6, 29 species of halocarbons, sulfate aerosols (direct effect), carbonaceous aerosols (direct effect), all aerosols (indirect effect), stratospheric H2O, OH, and pollutants NOx, CO, and VOC). In contrast to the Impulse Response Function (IRF) approaches in the predecessor models, ACC2 uses DOECLIM (Kriegler, 2005), a land-ocean Energy Balance Model (EBM), to calculate temperature change. The carbon cycle is described by box models based on the IRF approach. A temperature feedback is newly implemented to ocean and land CO2 uptake. The most novel aspect of ACC2 is its inverse estimation, the first attempt to estimate uncertain parameters simultaneously for the carbon cycle, atmospheric chemistry, and climate system by taking their interactions into account. Theoretical underpinning of the ACC2 inversion is the probabilistic inverse estimation theory (Tarantola, 2005), which characterizes the ACC2 inversion as an integration of the existing Earth system knowledge. This includes parameter estimates, observational databases, reconstructions, and physical-biogeochemical laws...
    Description: thesis
    Keywords: 551.5 ; TUA 500 ; TOY 000 ; TVA 200 ; VJD 000 ; Meteorologische Modelle ; Energiebilanzen in der Geodynamik {Geophysik} ; Zusammensetzung der Atmosphäre {Meteorologie} ; Geochemie der Atmosphäre
    Language: English
    Type: monograph , publishedVersion
    Format: 300 S.
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  • 72
    Publication Date: 2021-03-29
    Description: Durch den Prozess der Urbanisierung verändert die Menschheit die Erdoberfläche in großem Ausmaß und auf unwiederbringliche Weise. Die optische Fernerkundung ist eine Art der Erdbeobachtung, die das Verständnis dieses dynamischen Prozesses und seiner Auswirkungen erweitern kann. Die vorliegende Arbeit untersucht, inwiefern hyperspektrale Daten Informationen über Versiegelung liefern können, die der integrierten Analyse urbaner Mensch-Umwelt-Beziehungen dienen. Hierzu wird die Verarbeitungskette von Vorverarbeitung der Rohdaten bis zur Erstellung referenzierter Karten zu Landbedeckung und Versiegelung am Beispiel von Hyperspectral Mapper Daten von Berlin ganzheitlich untersucht. Die traditionelle Verarbeitungskette wird mehrmals erweitert bzw. abgewandelt. So wird die radiometrische Vorverarbeitung um die Normalisierung von Helligkeitsgradienten erweitert, welche durch die direktionellen Reflexionseigenschaften urbaner Oberflächen entstehen. Die Klassifikation in fünf spektral komplexe Landnutzungsklassen wird mit Support Vector Maschinen ohne zusätzliche Merkmalsextraktion oder Differenzierung von Subklassen durchgeführt...
    Description: thesis
    Keywords: 550.28 ; 622.159 ; 550 ; TQH 000 ; Aerogeophysik
    Language: English
    Type: monograph , publishedVersion
    Format: 276 S.
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  • 73
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; 550 ; TOD 400 ; TOE 000 ; TSB 000 ; Erdmantel {Geophysik} ; Physikalisches Verhalten der Erde {Geophysik} ; Mitteleuropa {Geophysik}
    Language: English
    Type: monograph , publishedVersion
    Format: 147 S.
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  • 74
    Publication Date: 2021-03-29
    Description: Aim of the study was to test the capability of multiple trace gas analyses for the assessment of regional carbon budgets. Therefore, air samples were taken by airborne and ground level activities during several field campaigns within Europe. Basic elements for the data acquisition were the development of an adapted sampling system and of an enhanced investigation strategy. By the study important processes like insufficient mixing and advection were identified which could seriously effect the measurements and thus the calculated budgets. The concluding results prompt for improvements regarding appropriate flux estimation techniques and application of the enhanced investigation strategy within a frame of combined measurement activities.
    Description: thesis
    Keywords: 551.5 ; 550 ; TUA 700 ; VJI 000 ; VJD 100 ; TVA 210 ; Verfahren zur Untersuchung der freien Atmosphäre {Meteorologie} ; Geochemische Kreislaufmodelle ; Geochemie der Ungestörten Atmosphäre ; Chemische Zusammensetzung der Atmosphäre {Meteorologie}
    Language: English
    Type: monograph , publishedVersion
    Format: 344 S.
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  • 75
    Publication Date: 2021-03-29
    Description: The southeastern Mediterranean Sea and the northern section of Egypt constitutes one of the most complex tectonic areas in the Mediterranean. This study is an attempt to achieve a better understanding of tectonics, and geodynamical processes along a complex tectonization region. These include crustal structure, thickness of sediments, transition between oceanic and continental crust and regional integrated model of the gravity field observed. A wide range of field work from the geophysical data has been acquired and used in this study with respect to the gravity and magnetic data as well as the results of deep seismic soundings. A comparison between the marine gravity data and the gravity data derived from satellite altimetry was made to ensure that the marine gravity data compiled from different marine surveys were compatible...
    Description: thesis
    Keywords: 622.15 ; 551.1 ; 550 ; TSZ 100 ; VAE 880 ; TSZ 100 ; VAE 880 ; Atlantischer Ozean {Geophysik} ; Passive und aktive Kontinentalränder {Geologie}
    Language: English
    Type: monograph , publishedVersion
    Format: 184 Bl.
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  • 76
    Publication Date: 2021-03-29
    Description: Die dynamische Entwicklung des neotektonisch und vulkanisch aktiven südchilenischen Plattenrandes wird durch die schiefe Subduktion der ozeanischen Nazca Platte unter den südamerikanischen Kontinent gesteuert. Die Deformationen in der Oberplatte sind von der Verformungsaufteilung (strain partitioning) des Konvergenzvektors in Bewegungen und Deformationen senkrecht und parallel zum Plattenrand sowie von diversen anderen in Wechselwirkung zueinander stehenden exogenen und endogenen Faktoren abhängig. Das Untersuchungsgebiet (Arauco-Bíobío Trench-Arc-System), das sich zwischen den Küstenstädten Concepción und Valdivia (36ʿ45`-40ʿS) und bis in den magmatischen Bogen an der chilenisch-argentinischen Grenze (73ʿ30`-71ʿW) erstreckt, bietet die Möglichkeit, die neogene Entwicklung eines Subduktionssystems zu studieren und die für die differenzierten Deformationen verantwortlichen Faktoren zu evaluieren. Mit Hilfe von detaillierten strukturgeologischen Untersuchungen der räumlichen und zeitlichen Zusammenhänge der andinen und auch prä-andinen Strukturen konnten kinematische Modelle für die verschiedenen Einheiten des Trench-Arc-Systems entwickelt werden. Tektonische Untersuchungsmethoden wurden durch die Analyse von Fernerkundungsdaten sowie geomorphologischen und sedimentologischen Studien ergänzt. Die neotektonische Aktivität wurde durch gängige paläoseismologische Beobachtungen,..
    Description: thesis
    Keywords: 550 ; TOH 800 ; VAE 880 ; TSX 500 ; VEX 500 ; Paläoerdbeben {Geophysik} ; Passive und aktive Kontinentalränder {Geologie} ; Chile {Geophysik} ; Chile {Geologie}
    Language: German
    Type: monograph , publishedVersion
    Format: 169 S.
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    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 910 ; QGJ 120 ; Teilfragen zu Indien {Geographie}
    Language: German
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    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; VDG 810 ; VKB 340 ; VEB 110 ; Unter-Perm ; Fazieskunde ; Norddeutsche Senke {Geologie}
    Language: German
    Type: monograph , publishedVersion
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    Publication Date: 2021-03-29
    Description: report
    Keywords: 551 ; ZHB 380 ; VRG 000 ; TOO 000 ; Geothermische Energie {Energietechnik} ; Geothermalfelder ; Geothermik {Geophysik}
    Language: German
    Type: article , publishedVersion
    Format: 110 S.
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    Publication Date: 2021-03-29
    Description: report
    Keywords: 551
    Language: German
    Type: article , publishedVersion
    Format: 148 S.
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    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; TOF 000 ; TQA 000 ; TQI 000 ; Schwerkraft {Geophysik} ; Gravimetrische Verfahren {Geophysik} ; Geophysikalische Satellitenfernerkundung
    Language: German
    Type: monograph , publishedVersion
    Format: 141 S.
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    Publication Date: 2021-03-29
    Description: report
    Keywords: 551 ; ZHB 380 ; Geothermische Energie {Energietechnik}
    Language: German
    Type: article , publishedVersion
    Format: 206 S.
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  • 83
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; VAE 130 ; VAE 400 ; VAE 120 ; VEI 700 ; Geomechanik ; Tektogenese {Geologie} ; Methodik {Strukturgeologie} ; Iran {Geologie}
    Language: German
    Type: monograph , publishedVersion
    Format: 159 S.
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  • 84
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 521.1 ; 550 ; TOF 000 ; TQA 000 ; TJ 900 ; Schwerkraft {Geophysik} ; Gravimetrische Verfahren {Geophysik} ; Einzelne Weltraumprojekte
    Language: German
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    Publication Date: 2021-03-29
    Description: report
    Keywords: 551 ; VRG 000 ; TOO 000 ; Geothermalfelder ; Geothermik {Geophysik}
    Language: German
    Type: article , publishedVersion
    Format: 150 S.
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    Publication Date: 2021-03-29
    Description: report
    Keywords: 551
    Language: German
    Type: article , publishedVersion
    Format: 72 S.
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  • 87
    Publication Date: 2021-03-29
    Description: report
    Keywords: 551 ; VRG 000 ; VBV 000 ; Geothermalfelder ; Nationales und internationales Recht in der Geologie
    Language: German
    Type: article , publishedVersion
    Format: 95 S.
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  • 88
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    Publication Date: 2021-03-29
    Description: report
    Keywords: 551 ; TOO 000 ; VBL 500 ; TQG 000 ; VEB 213 ; Geothermik {Geophysik} ; Geologische Bohrungen in einzelnen Regionen ; Geophysikalische Bohrlochmessungen ; Brandenburg, Sachsen-Anhalt & Mecklenburg-Vorpommern {Geologie}
    Language: German
    Type: anthology , publishedVersion
    Format: 190 S.
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  • 89
    Publication Date: 2021-03-29
    Description: Die südlichen Anden sind Teil des aktiven Kontinentalrandes von Südamerika, der durch eine Kombination subduktionsgebundener Prozesse gebildet wurde. Die andine Gebirgskette erstreckt sich über den gesamten südamerikanischen Kontinent, variiert jedoch merklich in Höhe und Krustenmächtigkeit. Während die Zentralen Anden, vor allem auch die tieferen Strukturen bis in den oberen Mantel, vergleichsweise gut erforscht sind (SFB267), ist über den geophysikalischen Aufbau der südlichen Anden bisher relativ wenig bekannt. Aus diesem Grund wurde das seismische Experiment ISSA2000 in den südlichen Anden durchgeführt. In dieser Arbeit wurde mithilfe der Methode der lokalen Erdbebentomographie ein 3-D Modell der seismischen Geschwindigkeitstruktur erstellt. Die gleichzeitig durchgeführte Lokalisierung der registrierten Erdbeben, ergibt darüberhinaus ein detailliertes Bild der Verteilung der Seismizität im Untersuchungsgebiet. Im Rahmen des ISSA2000-Experimentes wurde ein seismologisches Netzwerk mit 62 Seismographen betrieben, das die Subduktionszone von der Küste bis in den backarc zwischen 36ʿ und 40ʿS überdeckt. Die Hypozentren der 440 lokalen Erdbeben zeigen eine ~30ʿ geneigte Wadati-Benioff-Zone mit kontinuierlicher Seismizität bis in 120km Tiefe, die vereinzelt bis in 200km Tiefe zu beobachten ist. Sowohl die generell geringe Seismizität im Untersuchungsgebiet als auch die geringe Tiefenerstreckung der Wadati-Benioff-Zone u.a. im Vergleich zu den Zentralen Anden sowie die Konzentration der mitteltiefen Erdbeben in 60km Tiefe, spiegeln wahrscheinlich den Einfluß des jungen Alters und des damit verbundenen hohen thermischen Zustandes der Nazca-Platte auf das Subduktionsregime wider. Das tomographische Vp Modell zeigt zum ersten Mal die Geschwindigkeitsstruktur der südlichen Anden bis in eine Tiefe von 100km. Die Nazca-Platte ist durch die Lage der Erdbeben definiert und durch hohe Vp Geschwindigkeiten gekennzeichnet (7,2-8,3km/s). Die durchschnittlichen Geschwindigkeiten in der kontinentalen Kruste sind im gesamten Vp Modell relativ hoch (5,5-6,5km/s) ...
    Description: thesis
    Keywords: 551
    Language: German
    Type: monograph , publishedVersion
    Format: 137 S.
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  • 90
    Publication Date: 2021-03-29
    Description: After a gap of nearly two decades since the Magsat mission in 1980, the dedicated low-orbit potential field mission CHAMP is now in the third of its seven year mission. Already, the new magnetic total intensity and vector data have yielded maps of the global crustal field of unprecedented accuracy and resolution. Here, we assess the value of these maps to infer deep crustal structure of regions overlain by younger cover. A GIS based modelling technique has been developed to model the various geological units of the continents starting from the geological map of the world. Depending upon the known rock types of the region, they are assigned a standard susceptibility value and using the global seismic crustal structure, a vertically integrated susceptibility (VIS) model is computed at each point of the region. Starting with this initial VIS model, the vertical field anomaly is computed at a satellite altitude of 400 km and compared with the corresponding CHAMP vertical field anomaly map. The first comparison is carried out against a model using the lateral extent of a cratonic region as given by published tectonic maps. In the subsequent modelling step, depending upon the extent of the observed anomaly pattern of that region, the surface geology is extended beneath the sediments until the recomputed map fits the observed magnetic anomaly map. Here, we focus on modelling results for the selected few provinces of the world where the initial model does not agree with the observed anomaly map. Similar modelling of CHAMP satellite magnetic anomalies can constrain the subsurface structure hidden by Phanerozoic cover in many parts of the world.
    Description: thesis
    Keywords: 551 ; TOD 200 ; TOT 330 ; TOT 100 ; TQI 000 ; TQB 000 ; Erdkruste {Geophysik} ; Anomalien {Geophysik: Erdmagnetismus} ; Methodik {Geophysik: Erdmagnetismus} ; Geophysikalische Satellitenfernerkundung ; Erdmagnetische Verfahren {Geophysik}
    Language: German
    Type: monograph , publishedVersion
    Format: 137 S.
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  • 91
    Publication Date: 2021-03-29
    Description: report
    Keywords: 551
    Language: German
    Type: article , publishedVersion
    Format: 39 S.
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  • 92
    Publication Date: 2021-03-29
    Description: report
    Keywords: 551
    Language: English
    Type: article , publishedVersion
    Format: 30 S.
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  • 93
    Publication Date: 2021-03-29
    Description: report
    Keywords: 551
    Language: English
    Type: article , publishedVersion
    Format: 190 S.
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  • 94
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; VEX 100 ; VAE 811 ; TSX 100 ; TQC 200 ; Anden {Geologie} ; Alpidische Orogene {Geologie} ; Anden {Geophysik} ; Prospektionsseismik {Geophysik}
    Language: English
    Type: monograph , publishedVersion
    Format: 139 S.
    Format: application/pdf
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  • 95
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; VAE 120 ; VAE 140 ; VBP 500 ; VBP 200 ; Methodik {Strukturgeologie} ; Gesteinsdeformation {Strukturgeologie} ; Bodenmechanik, Erdbaumechanik, Baugrunddynamik ; Ingenieurgeologische Bewertung von Gesteinen als Baugrund und Baustoff
    Language: English
    Type: monograph , publishedVersion
    Format: 95,S.
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  • 96
    Publication Date: 2021-03-29
    Description: report
    Keywords: 551
    Language: German
    Type: article , publishedVersion
    Format: 54 S.
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  • 97
    Publication Date: 2021-03-29
    Description: report
    Keywords: 551 ; TVI 000 ; Jahreszeiten als meteorologische Erscheinung
    Language: English
    Type: article , publishedVersion
    Format: 16 S.
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  • 98
    Publication Date: 2021-03-29
    Description: report
    Keywords: 551 ; TVI 000 ; TM 600 ; Jahreszeiten als meteorologische Erscheinung ; Grenzgebiete. Beziehungen. Einflüsse. Wirkungen {Geophysik}
    Language: English
    Type: article , publishedVersion
    Format: 17 S.
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  • 99
    Publication Date: 2021-03-29
    Description: report
    Keywords: 551 ; TOB 100 ; Drehbewegungen {Geophysik: Erde}
    Language: English
    Type: article , publishedVersion
    Format: 43 S.
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  • 100
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    GFZ, Helmholtz-Zentrum | [Bibliothek des Wiss.-Parks Albert Einstein] [Vertrieb], [Potsdam]
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551 ; VBJ 000 ; Satellitenbildgeologie
    Language: German
    Type: monograph , publishedVersion
    Format: 113 S.
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