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  • 1
    Publication Date: 2020-10-05
    Description: Die Bibliografische Datenbank GeoRef und die Virtuelle Fachbibliothek GEO-LEO eignen sich bei paralleler Nutzung für eine weitgehend erschöpfende Informationsrecherche im Bereich Geowissenschaften. Während GeoRef im Wesentlichen als Nachweisinstrument für Zeitschriftenartikel dient, werden bei GEO-LEO Bibliothekskataloge abgefragt und digitale Volltexte verfügbar gemacht. Der direkte Dokumentzugriff und die Verzeichnung von Webseiten, ein Instrument zur Erkundung von Wissen durch systematische Darstellung von Einzeldisziplinen und eine Publikationsplattform bei GEO-LEO ergänzen sich mit hervorragender Erschließung und großer thematischer Abdeckung bei GeoRef.
    Description: study
    Keywords: 551 ; V 200 ; Geowissenschaften ; Virtuelle Bibliothek ; Literaturdatenbank ; Vergleich ; 38.04
    Language: German
    Type: article_first
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  • 2
    facet.materialart.
    Unknown
    Universitätsverlag Göttingen
    Publication Date: 2020-10-05
    Description: For about four decades marble has been used as thin veneer cladding. The durability of such thin slabs (mostly 30-40 mm) is satisfactory at most constructions. However, on numerous buildings all over the world, the long-term deformation (expansion, bowing) of some claddings is associated with structural weakening and strength loss which led to an inevitable restoration of the affected facades and to an image problem of marble used as a structural building stone. Up to now, the existing knowledge about the causes for this special kind of marble weathering is mostly restricted to research on Carrara marble and to the effect of individual parameters. This thesis presents the first study of the combined influence of extrinsic (environmental) and intrinsic (material specific) parameters on marble bowing. The respective impact of these factors on the weathering process is elucidated by damage mapping of four different marble facades. The work focuses on the influence of the microfabric on the damage dynamics of veneer marble and particularly considers moisture as an essential climatic parameter. In order to characterize and understand the weathering process, an array of different marble samples had to be studied with regard to their petrographic, rock physical and microstructural properties. Besides both fresh and artificially weathered marble samples this survey also included demounted façade panels from the investigated buildings with varying degrees of pre-deterioration...
    Description: Die seit etwa vier Jahrzehnten dauernde Verwendung von Marmor als dünnplattige Fassadenverkleidung hat weltweit an zahlreichen Gebäuden zu Problemen mit der Langzeitstabilität solcher Fassaden geführt. Das dabei oft auftretende Phänomen des Verbiegens von Marmorplatten geht mit einer Materialentfestigung einher, was langfristig die Sanierung der betroffenen Fassaden zur Folge hat und mittlerweile ein Imageproblem für den Werkstoff Marmor darstellt. Die bislang vorhandenen Kenntnisse zu den Ursachen dieser speziellen Form der Marmorverwitterung beschränken sich meist auf Untersuchungen an Carrara Marmor und auf die Wirkung einzelner Faktoren. In der vorliegenden Arbeit wurde der kombinierte Einfluss von umweltbedingten (extrinsischen) und materialspezifischen (intrinsischen) Parametern untersucht. Ihr Wirkungsgrad wird am Beispiel von vier Schadenskartierungen an Marmorfassaden aufgezeigt. Der Schwerpunkt liegt auf dem Einfluss des Mikrogefüges auf die Schadensdynamik von Fassadenmarmor unter besonderer Berücksichtigung der Feuchtigkeit als essentieller Klimafaktor. Basis für die Charakterisierung und Interpretation des Verwitterungsprozesses ist die Erfassung von petrographischen, gefügekundlichen und petrophysikalischen Eigenschaften an bruchfrischen und künstlich verwitterten Marmorproben sowie an demontierten Fassadenplatten unterschiedlicher Vorschädigung von den untersuchten Marmorfassaden...
    Description: thesis
    Keywords: 551 ; VKB 210 ; VBP 200 ; RVC 810 ; VAE 130 ; ZTI 000 ; VAH 000 ; VKA 170 ; Fassade ; Marmor ; Gefüge 〈Gesteinskunde〉 ; Petrophysik ; Physikalische Verwitterung ; Deformation 〈Geologie〉 ; 38.25 ; 56.47 ; 38.58
    Language: German
    Type: monograph , publishedVersion , monograph
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  • 3
    facet.materialart.
    Unknown
    Universitätsverlag Göttingen
    Publication Date: 2020-10-05
    Description: Seit nunmehr 20 Jahren findet regelmäßig alle zwei Jahre das Symposium ‚Tektonik — Strukturgeologie — Kristallingeologie‘ (TSK) statt. Die Tagung soll insbesondere jungen Nachwuchswissenschaftlern die Möglichkeit bieten, ihre Ergebnisse zu diskutieren und einem breiten Fachpublikum vorzustellen. Dies ist natürlich besonders attraktiv, wenn auch die ‚alten Hasen‘ der Zunft eifrig dabei sind. In diesem Jahr wird schon TSK 11 — nach Tübingen, Erlangen, Graz, Frankfurt, Salzburg, Freiberg, Freiburg und Aachen nun zum zweiten Mal nach 1994 wieder in Göttingen durchgeführt. Wir freuen uns, auch dieses Mal wieder ein vielseitiges Tagungsprogramm präsentieren zu können. Die vorgestellten Arbeiten befassen sich mit Geländebeobachtungen, Laboranalysen und -experimenten bis hin zu Computermodellierungen. Im Maßstab reichen sie vom submikroskopischen Bereich bis hin zu ganzen Orogenen. Dabei werden sowohl duktile als auch spröde Deformationsprozesse beleuchtet. Regionale Geologie ist ebenso Thema wie auch eher angewandte Fragestellungen. Um die einzelnen Beiträge schnell auffinden zu können, wurden diese alphabetisch nach Erstautoren geordnet. Aus Zeitgründen konnte nur der kleinere Teil der mehr als einhundert eingegangen Beiträge in das Vortragsprogramm aufgenommen werden. Auf parallele Vortragssitzungen haben wir bewusst verzichtet. Besonderen Raum für anregende Diskussionen sollen auch die thematisch zusammengestellten Postersitzungen bieten, für die wir spezielle Zeiten eingeräumt haben. Hierzu werden Poster jeweils vorher im Plenum kurz vorgestellt. Die eingegangenen Manuskripte wurden, wie bei TSK üblich, für die Publikation keinem Gutachterverfahren unterzogen. Daher sind die jeweiligen Autoren allein für den Inhalt verantwortlich. Wir wünschen allen Teilnehmenden anregende Diskussionen und interessante Kontakte sowie einen schönen Aufenthalt in der ‚Stadt, die Wissen schafft‘!
    Description: conference
    Keywords: 551 ; VAE 000 ; VAC 100 ; Tektonik ; Strukturgeologie ; Kristallin ; Kongress ; 38.36 ; 38.37
    Language: German
    Type: anthology , publishedVersion
    Format: 273 S.
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  • 4
    facet.materialart.
    Unknown
    Univ. Köln
    Publication Date: 2020-10-07
    Description: The Radio Science technique enables to estimate the mass and other gravitational parameters of a solar system body from spacecraft observations very precisely. It uses the radio link between ground station and spacecraft. The frequency shift of the radio signal is proportional to the relative velocity change between spacecraft and ground station. If a spacecraft performs a close flyby at a solar system body, the velocity of the spacecraft is changed by the gravitational attraction of the body. If all other contributions on the radio signal are known, the remaining frequency change is solely due to the gravitational attraction. A least square fit can be performed on the frequency residuals to derive from it gravitational parameters. Within this thesis models were developed and merged into a software package with which it is possible to determine the orbit of a spacecraft precisely and to predict accurately the frequency to be observed at a ground station. Models for extracting the frequency shift caused by the propagation of the radio signal through the ionosphere and troposphere of the Earth were incorporated...
    Description: thesis
    Keywords: 522 ; TBC 000 ; TGL 000 ; Radioastronomie ; Interplanetare Materie {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 151 S.
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  • 5
    Publication Date: 2020-10-07
    Description: The thesis at hand presents the results of a study of galaxies with active galactic nuclei (AGN) carried out in the radio and mm wavelength regimes at low and high angular resolutions. The studied objects cover a broad range of mechanisms responsible for powering the engines of the respective galaxies: ULIRGs (UltraLuminous Infrared Galaxies), a product of mergers between galaxies that are supposedly powered by starbursts, AGN or a mixture of the two, and QSOs (quasi-stellar objects) which are powered by AGN. Since ULIRGs and QSOs show similar properties (especially the infrared luminosities), it was proposed that they form the early and late phase of an evolutionary sequence where supposedly ULIRGs are the dust enshrouded progenitors of QSOs. As a prototypical ULIRG, Arp 220 represents an early-to-intermediate phase object in the scheme of the ULIRG-to-QSO evolution. For this object observations at multiple mm wavelengths and angular resolutions with the IRAM Plateau de Bure Interferometer (PdBI) are presented and analyzed. Arp 220 as a whole is studied in CO emission of the more extended structure. Furthermore, Arp 220-East is analyzed in more detail in the CO gas. Indications for emission ~10" towards the south, as well as to the north and to the west of the two nuclei, were found in the low resolution CO(1-0) maps ...
    Description: Zsfassung in dt. und engl. Sprache
    Description: thesis
    Keywords: 523 ; TBC 000 ; TIE 900 ; Radioastronomie ; Sonstige Sternensysteme {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 152 S.
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  • 6
    Publication Date: 2020-10-07
    Description: In cosmic ray experiments the arrival directions, among other properties, of cosmic ray particles from detected air shower events are reconstructed. The question of uniformity in the distribution of arrival directions is of large importance for models that try to explain cosmic radiation. In this thesis, methods for the reconstruction of parameters of a dipole-like flux distribution of cosmic rays from a set of recorded air shower events are studied. Different methods are presented and examined by means of detailed Monte Carlo simulations. Particular focus is put on the implications of spurious experimental effects. Modifications of existing methods and new methods are proposed. The main goal of this thesis is the development of the horizontal Rayleigh analysis method. Unlike other methods, this method is based on the analysis of local viewing directions instead of global sidereal directions. As a result, the symmetries of the experimental setup can be better utilised. The calculation of the sky coverage (exposure function) is not necessary in this analysis. The performance of the method is tested by means of further Monte Carlo simulations. The new method performs similarly good or only marginally worse than established methods in case of ideal measurement conditions. However, the simulation of certain experimental effects can cause substantial misestimations of the dipole parameters by the established methods, whereas the new method produces no systematic deviations. The invulnerability to certain effects offers additional advantages, as certain data selection cuts become dispensable.
    Description: thesis
    Keywords: 523 ; TFE 000 ; Kosmische Elektrodynamik {Astrophysik}
    Language: English
    Type: monograph , publishedVersion
    Format: 177 S.
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  • 7
    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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  • 8
    facet.materialart.
    Unknown
    Univ. Potsdam
    Publication Date: 2020-10-07
    Description: Central stars of planetary nebulae are low-mass stars on the brink of their final evolution towards white dwarfs. Because of their surface temperature of above 25,000 K their UV radiation ionizes the surrounding material, which was ejected in an earlier phase of their evolution. Such fluorescent circumstellar gas is called a "Planetary Nebula". About one-tenth of the Galactic central stars are hydrogen-deficient. Generally, the surface of these central stars is a mixture of helium, carbon, and oxygen resulting from partial helium burning. Moreover, most of them have a strong stellar wind, similar to massive Pop-I Wolf-Rayet stars, and are in analogy classified as [WC]. The brackets distinguish the special type from the massive WC stars.
    Description: thesis
    Keywords: 523 ; TEG 000 ; Kosmogonie {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 102 S.
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  • 9
    facet.materialart.
    Unknown
    Univ. Bielefeld
    Publication Date: 2020-10-07
    Description: In this thesis we apply methods from statistical physics to stochastic inflation. Those methods, the replica field theory and the Gaussian variational methods, have to our knowledge never been applied before in this context, and allow us to compute the power spectrum of a scalar test field in the most general set-up. It provides a framework to perform calculations in regions of arbitrarily large quantum fluctuations and may also serve as a starting point to address the issue of back reaction. We first give an introduction to cosmological inflation, cosmological perturbation theory and cosmic microwave background anisotropies. Then we explain the idea of stochastic inflation, including some detailed derivations, and give an overview over major progress in this field. This is followed by an introduction to replica field theory, presented in a way directly applicable to stochastic inflation. Our work continues with a detailed calculation of the power spectrum of a scalar test field in a Friedmann Universe. We show the effect of the quantum fluctuations on the spectrum and derive explicit expressions showing its dependence on time and other important parameters. The effect of self-interactions and possible effects on the cosmic microwave background are discussed. We conclude with a summary of our results and give an outlook. One part of our major results has been published in Phys. Rev. D 78, 103501 (2008), where for the first time we present a replica field-theoretical approach to stochastic inflation in which we find a manifestation of the phenomena of so-called dimensional reduction. It implies under certain conditions inevitable infra-red divergencies of correlation functions on large-scales. These conditions are examined in detail in Phys. Rev. D 79, 44009 (2009), where we find that generically for a wide class of circumstances the divergencies are pushed exponentially fast well beyond observable scales ...
    Description: thesis
    Keywords: 523 ; TA 100 ; TEC 000 ; Theoretische Grundlagen {Astronomie} ; Kosmologie {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 132 S.
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  • 10
    facet.materialart.
    Unknown
    Univ. Köln
    Publication Date: 2021-03-29
    Description: Neutron stars are unique stellar remnants with extreme properties, as their density and magnetic field. Their study can be the key to a number of unanswered problems in fundamental physics and astronomy, ranging from stellar evolution to strong field gravity. One of the best ways of studying these objects is with observations at radio wavelengths, the efficiency of which can be vastly improved with the combination of data from multiple radiotelescopes. In this thesis, we use the largest European radiotelescopes for performing high quality studies of the properties of objects belonging into two separate categories of neutron stars, millisecond pulsars and magnetars. In the first part of this thesis, a complete description of the observing systems and calibration procedures for the multiple telescopes used is presented. Specifically, all observations were made with the European Pulsar Timing Array (EPTA) telescopes, which are the Effelsberg 100m radiotelescope in Germany, the Lovell 76m radiotelescope in UK, the Westerbork 94m equivalent synthesis radiotelescope in the Netherlands and the Nanc cay 94m equivalent decimetric radiotelescope in France...
    Description: Zsfassung in dt. und engl. Sprache
    Description: thesis
    Keywords: 523 ; THU 400 ; THK 000 ; TBC 000 ; Pulsare, Neutronensterne {Astronomie} ; Spektren und Spektroskopie von Sternen {Astronomie} ; Radioastronomie
    Language: English
    Type: monograph , publishedVersion
    Format: 152 S.
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