ALBERT

All Library Books, journals and Electronic Records Telegrafenberg

Your email was sent successfully. Check your inbox.

An error occurred while sending the email. Please try again.

Proceed reservation?

Export
Filter
  • Other Sources  (262)
  • Elsevier  (199)
  • Univ. Köln  (61)
  • American Institute of Physics (AIP)
  • Institut für Meereskunde
  • Nature Publishing Group (NPG)
  • 2010-2014  (237)
  • 1985-1989  (25)
  • 2010  (237)
  • 1989  (25)
  • 1
    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.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 2
    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.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 3
    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.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 4
    Publication Date: 2020-10-07
    Description: The first part of the thesis is concerned with the fate of singularities in quantum cosmology. The second part addresses the derivation of predictions from quantum cosmology. In the first part, two classes of cosmological models were studied. In the first class of models, the universe evolves to or emerges from a big-rip singularity. Here, energy density, pressure and scale factor diverge after a finite amount of time. This type of singularity arises rather generically in cosmological models with phantom dark energy. For each of these phantom-field models, the corresponding scenario with ordinary scalar field was studied. The scalar field induced a big-bang singularity. The second class of models studied was dominated by a big-brake singularity. At the big brake, the universe evolution comes to a halt due to an infinite deceleration. The motivation behind this choice of models was the occurrence of a singularity at large scale factor. The major question pursued was whether these types of singularity were resolved on the quantum level. If such singularities were resolved in quantum cosmology, this would imply that quantum gravitational effects can occur in the macroscopic universe. After devising classical models that contain the respective singularity, I subjected these models to quantization which was carried out in the geometrodynamical approach. The governing equation is then the WheelerDeWitt equation ...
    Description: Zsfassung in dt. und engl. Sprache
    Description: thesis
    Keywords: 523 ; TEC 800 ; Quantenkosmologie {Astronomie: Kosmologie}
    Language: English
    Type: monograph , publishedVersion
    Format: 228 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 5
    facet.materialart.
    Unknown
    Univ. Köln
    Publication Date: 2021-03-29
    Description: According to current knowledge, star formation occurs preferentially in clustered environments. As a byproduct of the star formation process young stars are found to be surrounded by accretion discs that are potential birth places of planets and planetary systems. Located in the hosting cluster, these protoplanetary discs are potentially subject to stellar interactions. These interactions give rise to a fundamental question of clustered star formation: How far does the cluster environment affect the evolution of protoplanetary discs and the formation of planets? The question is addressed in the present investigation in terms of the effect of stellar encounters on stars and their disc in young clusters by combining numerical simulations of isolated star-disc encounters and stellar dynamics of young star clusters. The investigation is composed of three key aspects. First, simulations of a dynamical model of the Orion Nebula Cluster (ONC) show that disc destruction is dominated by encounters with high-mass stars that act as gravitational foci for the lower mass stars in the cluster centre. The massive stars are thus subject to repeated encounters which can lead to a total disc destruction ...
    Description: thesis
    Keywords: 523 ; THX 000 ; TIC 000 ; Extrasolare Planetensysteme {Astronomie: Sterne} ; Sternhaufen {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 137 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 6
    Publication Date: 2021-03-29
    Description: The work presented in my thesis covers two aspects of modern astronomy: Observations and instrumentation. Part I of this thesis addresses the design, the development and the qualification of the Low Resolution Spectroscopy Double Prism Assembly (LRSDPA). From an instrumentational point of view, the purpose of the LRSDPA is to make an integration of two prisms, made of Germanium and Zincsulfide, into the imaging module of the mid infrared instrument of the James Webb Space Telescope possible. My design of the LRSDPA answers to several challenging specifications, joining together available envelope, mechanical, thermal, optical and alignment aspects. Both prisms are mounted separately onto a holder via a semi-kinematic interface. The Aluminium components of the demonstration, qualification and flight model all have been manufactured at the mechanical workshop of the 1st Institute of Physics. As it is demanded of all space equipment, the function and performance of the LRSDPA has to be thoroughly demonstrated. The qualification campaign that was conducted in collaboration with the Centre Spatial de Liège, has just been brought to a successful finish. A brief introduction to the James Webb Space Telescope and its mid infrared instrument are given in Chapters 1 and 2. Chapter 3 then describes in detail the scientific capabilities, the design and the qualification of the LRSDPA. The low resolution spectroscopy mode will provide prism slit spectroscopy at a resolution of R=100 and cover the wavelength range from 5æm-10æm. This mode is particularly aiming at spectroscopic analyses of very low surface brightness objects, such as the first light-emitting galaxies that re-ionized the universe shortly after the big bang ...
    Description: thesis
    Keywords: 522 ; TCE 230 ; TIE 400 ; TBG 000 ; TCE 380 ; Weltraumbasierte UV-, Optische und Infrarotteleskope {Astronomische Instrumente} ; Spektren und Leuchtkraft von Sternsystemen {Astronomie} ; Infrarot-Astronomie ; CCD, Photodetektoren {Astronomische Instrumente}
    Language: English
    Type: monograph , publishedVersion
    Format: 146 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 7
    Publication Date: 2021-03-29
    Description: In this doctoral thesis, multi-frequency very long baseline interferometry observations together with multi-frequency total flux-density variability data of compact relativistic jets in active galactic nuclei are presented and analyzed. The main goal of the thesis is to investigate the physical mechanisms in relativistic jets responsible for such phenomena as the co-existence of moving and stationary jet components, jet wiggling and precession. We also aim to study the connection between the structural changes in the relativistic jets and flares in the total flux-density light curves and to find observational evidences for the appearance of a primary perturbation in the base of the jet and its further propagation. In this thesis we also investigate which physical mechanisms are responsible for periodical total flux-density variability and to search for periodicities as a sign of jet precession. In order to study the jet physics we used the multi-frequency very long baseline interferometry technique which gives the highest possible in astronomy resolution. We also compared jet structural changes with single-dish multi-frequency observations spanning more than 30 years together with optical and gamma-ray data. In particular, analysis of the long-term kinematics of two active galactic nuclei S5 1803+784 and 0605-085 shows evidence for jet precession ...
    Description: thesis
    Keywords: 523 ; TBC 000 ; TIE 500 ; Radioastronomie ; Aufbau und Struktur von Sternsystemen {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 201 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 8
    facet.materialart.
    Unknown
    Univ. Köln
    Publication Date: 2021-03-29
    Description: The understanding of gravitational stability of galactic disks against star formation, the interplay of atomic and molecular components of the interstellar medium in a galaxy and its physical conditions, namely temperature and density, are important to gain a deeper insight into star formation. Nearby galaxies like the spiral galaxy M51 or the southern starburst galaxies NGC4945 and Circinus offer excellent opportunities to investigate these topics over a complete galactic disk or parts of the galaxy. A suitable tracer to study the molecular part of the gaseous component of galaxies is the CO molecule. It is the second most abundant molecule after H2 in the interstellar medium, its lower lying transition are excited at typical conditions of molecular clouds and the rotational transitions lie in the radio window. Thus, CO emission can penetrate throughout galactic disks and is observable from the ground. Apart from complementary data from the literature, we use observations of 12CO 21, 12CO 4--3, and 13CO 2--1 in this thesis. Additionally, the [CI] 3P1-3P0 fine structure line was observed to study the physical conditions in the central regions of galaxies. In the first part of this thesis, the nearby spiral galaxy M51 is used as a sample source to investigate the onset of star formation. CO, HI, radio-continuum, dust, and stellar maps of M51 are combined to study star formation rate, the H2/HI transition, the gas-to-dust ratios, the stability of the disk against gravitational collapse, and properties of the giant molecular clouds. Parts of the results have been published in Astronomy and Astrophysics (461,143) in 2007 and are submitted to Astronomy and Astrophysics, 2008 for publication. We use the first complete 12CO 2--1 map of M51 including the companion galaxy NGC5195 observed with HERA at the IRAM-30m telescope to trace the molecular gas. Complementary HI VLA data is used to study the atomic gas distribution and the combined total gas surface density ...
    Description: thesis
    Keywords: 523 ; TEG 000 ; Kosmogonie {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 180 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 9
    Publication Date: 2021-03-29
    Description: This thesis is focussed on the development of optimized techniques to overcome limitations of astrophysical observations. The goal is an optimal signal estimation in noisy measurements by the consideration of underlying physical processes. This principle was applied to two different fields in astrophysics: intrumental design and analysis of polarimetric observations. In the observational part of this thesis near-infrared images of young stellar objects in the Orion constellation are studied. Limitations in resolution and sensitivity of current astronomical instruments prohibit the detailed analysis of interesting proto-stellar sources to improve theories of star formation. Radiation from the astronomical targets is not only characterized by its spectral energy, but also by polarization properties. The modeling of typical configurations of star-disk systems and the simulation of their polarization patterns helped to understand and interprete features, that were found in observations. For the case of a proto-stellar systems with both a disk and an envelope analysis techniques were developed, which are based on polarimetric effects of the scattering of light by dust. These techniques substantially improve the sensitivity and resolution and are reliable under different observing conditions. Although the obtained data did not allow investigations of substructures of the circumstellar material, the techniques are suitable to obtain constraints on star formation processes ...
    Description: thesis
    Keywords: 523 ; THK 000 ; Spektren und Spektroskopie von Sternen {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 168 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 10
    Publication Date: 2021-03-29
    Description: Astronomische Beobachtungen im Bereich der THz-Frequenzen geben Aufschluss über die Entwicklung der interstellaren Materie in unserem Universum. Als wichtigste Kühllinie dichter Molekülwolken ist die Detektion des Feinstrukturübergangs von einfach-ionisiertem atomarem Kohlenstoff CII bei der Frequenz von 1,9 THz von fundamentaler Bedeutung. Wünschenswert ist das Studium astronomischer Quellen hinsichtlich ihrer Dynamik, Temperatur und Dichte mit möglichst hoher sowohl räumlicher als auch spektraler Auflösung. Heterodynempfänger sind für diese Aufgabe am besten geeignet. Bei dieser Technologie wird das astronomische Signal mittels eines Lokaloszillatoren (LO) auf eine Zwischenfrequenz von wenigen GHz umgesetzt und dann rauscharm weiterverstärkt. Gegenstand der vorliegenden Arbeit ist die Entwicklung und der Aufbau des LOs für den 1,9 THz Frequenzkanal des Mehrkanalheterodynempfängers German REceiver for Astronomy at THz-Frequencies (GREAT) der auf dem Flugzeugobservatorium Stratospheric Observatory For Infrared Astronomy (SOFIA) zum Einsatz kommen wird. Für den Aufbau des LOs wurde auf eine Kombination zweier THz-Strahlungsquellen bestehend aus einem Rückwärtswellenoszillator (Backward-Wave Oscillator, BWO) und einem Frequenzverdreifacher zurückgegriffen. Dieser Ansatz erforderte die Entwicklung einer astigmatisch-abbildenden Submillimeteroptik, um die Leistungsankopplung zwischen BWO und Frequenzverdreifacher zu verbessern...
    Description: thesis
    Keywords: 522 ; 550 ; TBG 000 ; Infrarot-Astronomie
    Language: German
    Type: monograph , publishedVersion
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 11
    Publication Date: 2021-03-29
    Description: The central part of the Milky Way is a unique environment where an interplay of different astrophysical phenomena can be studied, starting from the physics of the interstellar medium, stellar physics and star formation, to high energetic processes associated with the accretion onto the supermassive black hole Sgr A*. In this thesis I focus onto the central parsec of the Milky Way, observed at 3.8 micrometer (L'-band) during several epochs from 2002 to 2007. This particular wavelength is interesting because one can observe the (very dense) Galactic stellar nuclear cluster, as well as the thermal component of the interstellar medium which is not visible at shorter near-infrared wavelengths. Our images revealed a high number of very narrow filamentary structures associated with the streamers of gas and dust (called mini-spiral), and sometimes also with stars. We also detected several stellar sources that are barely observable at shorter wavelengths, but well defined in the dust-dominated L'-band. The goal of this thesis was to use multi-epoch observations in order to measure motions of filamentary structures, as well as of those very red stars. The proper motion analysis allows us to come a step further in understanding the real nature of these enigmatic sources. The high-resolution observations were obtained with the NAOS/CONICA Adaptive Optics system at the ESO Very Large Telescope at Paranal, Chile. The first part of the thesis deals with the narrow dust filaments. The analysis of their morphology and proper motions shows that they are (i) probably not due to a projectional effect and (ii) are influenced by other forces than just the gravitational force of the central black hole...
    Description: thesis
    Keywords: 523 ; 550 ; TIE 662 ; Struktur der Milchstrasse {Astronomie}
    Language: German
    Type: monograph , publishedVersion
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 12
    facet.materialart.
    Unknown
    Univ. Köln
    Publication Date: 2021-03-29
    Description: The meaning of my thesis was to obtain new insights about the supermassive Black Hole in the center of our Milky Way and its accretion flow. The non-thermal radio, X-ray, and near-infrared source Sagittarius A* (Sgr A*) is the electro-magnetic manifestation of the Black Hole. Sgr A* is a unique source to study the accretion onto a very massive compact object as it is the closest galactic nucleus. For this work I conducted observations as well as theoretical computations. The near-infrared camera CONICA in combination with the adaptive optics device NAOS at ESO's Very Large Telescope in Chile were used for the observations. The goal of our group was in particular to find further evidence for a quasi-periodic signal of ~17 minutes in radiation outbursts from Sgr A* that has been reported for the first time in 2003. The radiation outbursts - most often termed `flares' - are periods of ~50 - 130 minutes in which the flux of Sgr A* in the near-infrared rises up to a factor of ten. The quasi-periodic sub-structure thereby manifests itself as sub-flares with a constant separation superimposed on the larger, underlying flare. In 2005 and 2006 we were able to detect a significant periodicity, hence the previous findings are supported ...
    Description: thesis
    Keywords: 522 ; TBG 000 ; THK 000 ; Infrarot-Astronomie ; Spektren und Spektroskopie von Sternen {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 125 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 13
    Publication Date: 2021-03-29
    Description: This thesis describes the development and manufacturing of the IF circuits for two different heterodyne receivers used for sub-mm radio astronomy. The first project is the broadband 4-8 GHz IF circuitry for the mixer units for band 2 of the Heterodyne Instrument for the Far Infrared (HIFI). This instrument will be operating onboard of ESA’s Herschel space observatory. The band 2 mixer units for HIFI, built by KOSMA, implement low noise SIS mixers in a very compact, modular design. The complete IF path in the mixer units consist of the mixer block (with the SIS mixer chip) and the bias-T, which is needed to apply a bias voltage to the SIS-junction and to extract the IF signal. The detailed investigation of the IF performance of the mixer block must consider the geometric capacitances of the SIS-junction and the tuning structure as well as the inductance of the bond wires used to establish the contact between the mixer chip and the SMA output connector. The calculations presented in this thesis show that the design can be used for IF frequencies up to 12 GHz. The bias-T, which is implemented in the mixer unit, is a dedicated, new development with high performance and high reliability complying with the special requirements for a spaceborne instrument. These include the survival under high mechanical stress such as vibration during the launch and extensive thermal cycling to cryogenic temperatures during the tests of the mixer unit and the instrument.
    Description: thesis
    Keywords: 522 ; 550 ; TBC 000 ; TCE 230 ; Radioastronomie ; Weltraumbasierte UV-, Optische und Infrarotteleskope {Astronomische Instrumente}
    Language: English
    Type: monograph , publishedVersion
    Format: 173 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 14
    Publication Date: 2021-03-29
    Description: A pattern recognition and classification software was developed to detect dust devils automatically in surface images from Mars. The amount of images taken by spacecraft orbiting Mars is increasing continuously and the expenditure of time is too high to search every image for spatially and temporally highly variable features like dust devils. The pattern recognition method was therefore used to conduct a completely new kind of search for dust devils. Images from the three different Mars missions Viking, Mars Global Surveyor and Mars Express can be processed and for the first time automatically scanned for the desired objects. Viking images including dust devils were used as the database to filter unique dust devil features and the derived parameters built the feature vector. Various Classification methods have been tested resulting in a two-layer perceptron (neural network) as the best classifier. Necessary adjustments and increments complete the software so that it can be applied to Mars Global Surveyor Mars Orbiter Camera (MOC), Mars Express High Resolution Stereo Camera (HRSC) and probably coming images from future missions. It was shown that the standard dust devil is filtered and correctly classified. The two main features, the bright spot representing the dust column and the shadow, must be filterable from the background. Crater rims and hills are the most false-positive objects...
    Description: thesis
    Keywords: 523 ; TGG 545 ; TGG 515 ; TCM 000 ; TCE 380 ; Marsoberfläche {Astronomie} ; Marsbeobachtung, Raumflüge zum Mars {Astronomie} ; Mathematische und EDV-Verfahren {Astronomie} ; CCD, Photodetektoren {Astronomische Instrumente}
    Language: English
    Type: monograph , publishedVersion
    Format: 158 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 15
    Publication Date: 2021-03-29
    Description: The work presented here is concerned with issues related to the interplay of galaxy structure and the accretion phenomenon onto supermassive black holes (SMBH), i.e. active galactic nuclei (AGN). There is statistical evidence for a coevolution of SMBHs and the galaxy bulges they reside in. The detailed knowledge of the involved physical processes, however, is still far from being satisfactory. In order to test and improve theoretical models of how this coevolution is arising, high angular resolution observations of the host galaxies of AGN are necessary. Imaging and spectroscopy of the innermost region of galaxies have the power to reveal information on the structure, the chemical composition, and the dynamics of stars and gas in the presence of an SMBH, and allow us to separate energetic signatures related either to star formation or to the accretion onto the SMBH. Considering such observations over cosmological distances (redshifts) -- i.e. looking into the past because of the finite light-travel time -- we are also able to assess evolutionary effects on the beforementioned properties ...
    Description: thesis
    Keywords: 523 ; TIE 400 ; Spektren und Leuchtkraft von Sternsystemen {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 174 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 16
    Publication Date: 2021-03-29
    Description: This thesis consists of two parts. The first part reports on the development of a fringe tracking system for LINC-NIRVANA, the near-infrared homothetic imaging camera for the Large Binocular Telescope (LBT). LINC-NIRVANA allows for a coherent combination of the light entering the two primary mirrors. The fringe pattern in the focal plane is required to be stable in time to preserve the high spatial frequency information in long exposure images. Atmospheric differential piston causes the position of the fringes to change with time. A fringe tracker is a servo system that measures and corrects for atmospheric differential piston in real-time. In the first part, numerical simulations of atmospheric turbulence are used to investigate the problem of angular anisoplanatism of differential piston. The fringe tracking concept and the top-level requirements are introduced, followed by a presentation of the mechanical design of the system. This design includes a solution for a device that is capable of positioning a detector with high precision within a cryogenic environment. A fitting algorithm determines the amount of differential piston in the point-spread function of a reference target. The performance of this algorithm under different signal-to-noise conditions is investigated. First polychromatic fringes obtained with a testbed interferometer conclude the first part ...
    Description: thesis
    Keywords: 523 ; TII 500 ; Emissionsnebel {Astronomie: Interstellare Materie}
    Language: English
    Type: monograph , publishedVersion
    Format: 186 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 17
    Publication Date: 2021-03-29
    Description: The focus of this thesis lies on the analysis and interpretation of near- and mid-infrared images of the Galactic center, with a view to improving the understanding of this region, especially at longer wavelengths. Multi-band (H, K, L and M, i.e. 1.6, 2.1, 3.78 and 4.66æm) photometry of images with a large field of view results in a new L-band calibration which eliminates anomalous color effects found in previous surveys of the Galactic center stellar cluster. The color data obtained indicates that the average extinction toward the region containing the Northern Arm and Sgr A* is lower than previously assumed, confirming the findings of Scoville et al. (2003). The stellar population of the inner few arcseconds is compared to that situated up to approximately 0.5 arcminutes out from the position of Sgr A*, revealing that the extinction does not increase significantly over the entire field of view of the ISAAC instrument (i.e. 70" x 70"). Using the large number of sources (over 500), the M-band extinction is calculated from the average L-M colors, resulting in a higher value than that of the "standard" extinction law of Rieke & Lebofsky (1985). The L-M color is shown to be a useful diagnostic tool in distinguishing hot and cool stars, when more precise methods (e.g. spectroscopy) are not available. The unusual morphology of the bright mid-infrared source IRS 3 is also discussed...
    Description: thesis
    Keywords: 522.683 ; 550 ; TBG 000 ; TIE 400 ; Infrarot-Astronomie ; Spektren und Leuchtkraft von Sternsystemen {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 117 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 18
    Publication Date: 2021-03-29
    Description: Design and performance of waveguide mixers at 1.4 THz and 1.9 THz based on NbTiN phonon-cooled hot electron bolometers (HEB) fabricated on a 2 æm thick Si_3N_4 membrane. The membrane is bonded to a silicon frame in the mixer block using a flip chip process. Simulated RF coupling is compared with experimental results, showing good agreement. Receiver noise temperature measurements show uncorrected values of 1600 K at 1.4 THz and 2100 K at 1.9 THz, both at 1.5 GHz intermediate frequency. Device cooling on the membrane seems not to be problematic. The mixers are used in receivers for SOFIA (GREAT & CONDOR) and APEX (CONDOR).
    Description: thesis
    Keywords: 523 ; TBG 000 ; Infrarot-Astronomie
    Language: German
    Type: monograph , publishedVersion
    Format: 153 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 19
    Publication Date: 2021-03-29
    Description: Sternentstehung findet im dichten Teil der Molekülwolken des interstellaren Mediums statt. In diesen Gebieten werden die ablaufenden physikalischen und chemischen Prozesse maßgeblich von der Wechselwirkung zwischen der Materie und dem Strahlungsfeld eingebetteter junger Sterne bestimmt. Konsequenz der Bestrahlung mit FUV-Photonen (6eV〈E〈13.6eV) ist die Aufheizung des Staubes und des atomaren bzw. molekularen Gases. Dabei fÓhrt die auf StaubkÒrnern umgesetzte Photonenenergie zur Emission von IR-Kontinuumsstrahlung, wohingegen die vom atomaren bzw. molekularen Gas aufgenommene Energie zu einer Anregung charakteristischer ÃbergÑnge im submm-Bereich fÓhrt. Beobachtbar sind astronomisch relevante Linien wie z.B. CO-RotationsÓbergÑnge, aber auch starke Linienemissionen von HyperfeinstrukturÓbergÑngen von z.B. [OI] und [CII], die im THz-Bereich liegen. Die Verteilung und die IntensitÑten lassen sich mit gÑngigen Modellen Óber so genannte Photonen-dominierte Regionen beschreiben und liefern wichtige Informationen fÓr unser VerstÑndnis Óber z.B. Sternentstehungsgebiete. Mit dem German REceiver for Astronomy at THz-Frequencies (GREAT), einem Einpixel-HeterodynempfÑnger fÓr zwei Frequenzen, wird der Wissenschaft der Zugang zu diesen Linien spektral hochaufgelÒst (R〉10^6) ermÒglicht. Dabei ist zu beachten, dass Frequenzen im Bereich von 1-10THz erdgebunden aufgrund der Absorption des atmosphÑrischen Wassersdampfs nicht beobachtbar sind.
    Description: thesis
    Keywords: 522 ; TJI 000 ; TBG 000 ; Werkstofforschung und Verfahrenstechnik im Weltraum ; Infrarot-Astronomie
    Language: German
    Type: monograph , publishedVersion
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 20
    Publication Date: 2021-03-29
    Description: Sowohl in der Radioastronomie als auch in der Atmosphärenforschung gibt es einen Bedarf für breitbandige Spektrometer mit einer Bandbreite von bis zu 10 GHz und einer moderaten Auflösung. In der Radioastronomie wurde durch die stete Weiterentwicklung der Heterodynempfangssysteme der THz-Bereich für die Beobachtung zugänglich. Dies erfordert bei zahlreichen Beobachtungen, z.B. des galaktischen Zentrums, breitbandige Spektrometer, da die Geschwindigkeitsverteilung von Molekül- und Atomlinien in diesen turbulenten Gebieten sehr hoch ist. Die Auflösung des Spektrometers kann dabei in einen Bereich von 50-100 MHz liegen. Auch in der Atmosphärenforschung werden breitbandige Spektrometer benötigt, um die vollständige Information aus den Flügeln der druckverbreiterten Linienprofile zu gewinnen. Ziel dieser Arbeit war es daher ein Spektrometer zu entwickeln, das die Möglichkeit einer breitbandigen Frequenzanalyse bietet. Dies wird durch die Modulation eines Lasers mit einem externen Phasenmodulator möglich. Der Phasenmodulator kann das Laserlicht mit Frequenzen über 10 GHz modulieren. Zur Frequenzanalyse der so erzeugten Seitenbänder dient ein Fabry-Perot Etalon. Durch die Ausleuchtung des Etalons mit einer Zylinderlinse konnte erreicht werden, dass das vom Etalon erzeugte Ringsystem auf eine Zeile transformiert wird. Dies ermöglicht eine effiziente Ausnutzung des Signallichts. Um die Eigenschaften des in dieser Arbeit entwickelten Spektrometers zu charakterisieren und die Ausleuchtung des Etalons zu optimieren wurde ein Simulationsprogramm entwickelt. Mit Hilfe der Simulation ist es möglich eine Aussage über die Mindestgröße der Apertur des Etalons zu treffen, um die "walk-off" Verluste zu reduzieren. Es konnte zudem an Hand der Simulation gezeigt werden, welchen Einfluss die Ausleuchtung des Etalons auf die Auflösung und Intensitätsverteilung über das gesamte Band hat.
    Description: thesis
    Keywords: 523 ; TCE 320 ; TUD 000 ; Photometer, Polarimeter, spektroskopische Instrumente {Astronomische Instrumente} ; Meteorologische Instrumente
    Language: German
    Type: monograph , publishedVersion
    Format: 97 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 21
    Publication Date: 2021-03-29
    Description: All projects aim at pushing the limits of our knowledge about the interaction between a galaxy and a supermassive black hole (SMBH) at its center. The development of a new instrument can be as valuable as combining different datasets. I follow both approaches and developed projects which deal with new instrumentation and telescope technology, combine datasets from different wavelengths and resolutions, and incorporate recent theoretical models and predictions, which can be verified empirically. The first two of the six chapters compile astrophysical and technical background of the individual projects, which are presented in the following four chapters. While the first project (Chapter 3) deals with observations of the innermost parsec of our Galaxy, Chapter 4 presents data of the inner kpc of an active galaxy. The subjects of Chapters 5 and 6 are very luminous AGN/host systems, so-called QSOs. Whereas Chapter 5 presents global, spatially unresolved properties of SMBH/host systems, the radio jet, analyzed in the final Chapter 6, combines all size scales. It is investigated from close to its origin out to several kpc. The accretion onto the black hole of the Milky Way (Chapter 3) is extremely inefficient and the SMBH possibly interacts dominantly via tidal forces only. The next discussed system (Chapter 4) is the prototype of moderately luminous Seyfert 2 AGN, NGC 1068. Here a strong local influence of the nuclear X-ray radiation is observed. Chapter 5 deals with the possible global importance of radiative interaction between highly luminous QSO AGN and the host. The radio jet in Chapte 6 definitely shows signs of interaction with the matter of its host several kpc away from the nucleus. Chapters 3-6 include a dedicated introductory and a conclusive section, which put the results obtained in the larger astrophysical context of the observation ...
    Description: thesis
    Keywords: 523 ; TEG 440 ; TIE 662 ; Schwarze Löcher {Astronomie: Kosmogonie} ; Struktur der Milchstrasse {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 147 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 22
    Publication Date: 2021-03-29
    Description: A time-dependent 3D magnetohydrodynamic (MHD) model has been developed to investigate the temporal periodic interaction between Europa and the Jovian magnetosphere. The temporal variations are caused by the periodic variations of the magnetospheric plasma at Europa. As a new feature compared to existing stationary models, periodic induced magnetic fields, caused by electromagnetic induction in a potential subsurface ocean, are included. The MHD-flow problem and the internal induction problem are solved simultaneously by making use of the periodicity and the quasi-stationarity of the problem. The ideal MHD equations have been extended in order to account for the effects of Europa's neutral atmosphere and the internal periodic induced magnetic fields on the plasma interaction. At the beginning of this work, Galileo magnetometer data acquired on four passes by Europa were used to investigate whether a fixed permanent dipole moment is present in the interior of the moon in addition to the induced dipole moment previously identified. We thereby confirm the presence of an inductive response and find that the dipole coefficients of the constant intrinsic field contribute at best in a very minor way to the magnetic field. The induced magnetic fields caused by the time variable plasma interaction are calculated in an interactive process...
    Description: thesis
    Keywords: 523.45 ; 550 ; TGG 605 ; Jupitermonde {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 161 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 23
    Publication Date: 2021-03-29
    Description: The topic of this work is the development of Hot Electron Bolometer (HEB) mixers on freestanding membrane substrates for terahertz high resolution heterodyne receiver systems. The radio astronomy in the THz frequency spectrum is still in the beginning. At present much effort is put into the development of novel telescopes as well as in detector technologies. This work focuses on the development of THz waveguide detectors with superconducting Hot Electron Bolometer (HEB) mixers. These are primarily aimed for the use in the airborne Stratospheric Observatory For Infrared Astronomy (SOFIA) (1.9 THz) and the Atacama Pathfinder EXperiment (APEX) telescope (1.4 THz) in northern Chile ...
    Description: thesis
    Keywords: 523 ; TBC 000 ; Radioastronomie
    Language: English
    Type: monograph , publishedVersion
    Format: 169 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 24
    Publication Date: 2021-03-29
    Description: This doctoral thesis deals with crinoids from the Middle Devonian (U. Eifelian to L. Givetian) of the Eifel Synclines (western Rhenish Massif, Germany) and secondary with U. Eifelian to U. Givetian crinoids of the eastern Rhenish Massif. The study focuses on new recovered material and on material deposit in historical collections. Since the classic monographs of the early 19th century, crinoids are nearly unstudied in modern view. They are only periphery mentioned within the standard works Treatise on Invertebrate Paleontology and Fossil Crinoids. The Eifel has to be characterised as the global hotspot of Middle Devonian crinoids. Because of the high diversity, selected groups of each of the four occurring Palaeozoic subclasses are studied in the course of this work: 1. The subfamily Cupressocrininae (subclass Cladida); 2. the family Hexacrinitidae (subclass Camerata); 3. the genus Stylocrinus (subclass Disparida); 4. the genus Ammonicrinus (subclass Flexibilia). Altogether, four families, eight genera and 66 species are described taxonomically. 10 new species are erected newly. Based on the excellent three-dimensional preservation of the partly autochthon conserved skeletons and their ecological-/facial response, the Eifel crinoids gave important information about the palaeodiversity, palaeobiology and palaeoecology: Regeneration processes in cupressocrinitids and hexacrinitids correspond with that features defined for recent echinoderms. Because of their important functions, the regeneration of injured arms is more perfect than those of affected cups. Hexacrinites contra balanced the general smallness of the regenerative arms by an increased pinnulated surface ...
    Description: thesis
    Keywords: 560 ; VZB 121 ; VWG 600 ; VXR 000 ; Rheinisches Schiefergebirge {Paläontologie} ; Devon {Stratigraphische Paläontologie} ; Echinodermata {Paläozoologie}
    Language: German
    Type: monograph , publishedVersion
    Format: 263 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 25
    Publication Date: 2017-06-09
    Description: Atmosphärische Aerosolpartikel spielen eine bedeutende Rolle in verschiedenen Fragestellungen der Luftreinhaltung. Einen wesentlichen Bestandteil ihrer Masse bilden anorganische Komponenten wie Sulfat, Ammonium und Nitrat, die in der maritimen planetaren Grenzschicht u.a. durch Natrium und Chlorid ergänzt werden. Die Wirkung eines Aerosols ist vom Phasenzustand der Partikel, ihrem Wassergehalt und der Partitionierung flüchtiger Komponenten zwischen Gas- und Partikelphase abhängig. Zur Bestimmung dieser Eigenschaften wird ein thermodynamisches Modell ...
    Description: thesis
    Keywords: VJH 200 ; Thermodynamische Prozesse, Verteilungskoeffizienten {Physikalische Geochemie}
    Language: German
    Type: monograph , publishedVersion
    Format: 282 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 26
    Publication Date: 2021-03-29
    Description: In meiner Arbeit untersuche ich die Bildung SiO2-reicher Objekte (SRO) in chondritischen Meteoriten (--〉 Chondrite). Diese Phasen werden nach den heutigen Modellen des frühen Sonnsystems nicht in diesen erwartet. Trotzdem enthalten einige kohlige Chondrite darunter insbesondere die CH-Chondrite und einige gewöhnliche Chondrite Objekte mit freiem SiO2. Die SRO habe ich mit der Elektronenstrahl-Mikrosonde und dem Sekundärionen-Massenspektrometer zur Bestimmung der chemischen Zusammensetzung, sowie mit dem Mikro-Raman Spektrometer und dem Transmissionselektronen-Mikroskop zur Bestimmung der SiO2-Polymorphie untersucht. In den kohligen Chondriten treten die SRO fast nur in den CH- und CR-Chondriten auf. Deren Population in den CH-Chondriten beträgt ~0.1 Vol.%. Die Paragenese besteht fast ausschließlich aus SiO2 und einem etwa Pyroxen-normativen Silikat. Diese beiden Phasen zeigen oftmals Entmischungsstrukturen. Diese SRO sind meist an den refraktären Elementen Ca, Al und Ti verarmt, bis zu 0.015 x CI. In gleichem Maße sind die Seltenen Erd-Elemente (SEE) verarmt und zeigen unfraktionierte, flache Muster. Das Si/Mg-Verhältnis ist stark fraktioniert, mit 3 4 x CI. Die SRO sind außerdem verarmt an volatilen Elementen, jedoch haben zwei SRO-Chondren sehr hohe Mn-Konzentrationen, und das, obwohl die CH-Chondrite die Mn-ärmsten Gesamt-Zusammensetzungen aller Chondrite haben. Eine dieser Mn-reichen Chondren enthält Pyroxen mit den höchsten, je aus einem Meteoriten berichteten Mn-Konzentrationen von 6.68 Gew.%. Das SiO2 tritt in den SRO hauptsächlich als Glas und in seinen Hoch- und Mitteltemperatur-Polymorphen Cristobalit und Tridymit auf. Die Bildung dieser SRO kann über einen zweistufigen Mechanismus verstanden werden, bei dem zuerst eine fraktionierte Kondensation die Precursor der SRO bildete, die anschließend im zweiten Schritt zu Temperaturen 〉1968 K wieder aufgeheizt wurden und danach rasch abkühlten ...
    Description: thesis
    Keywords: 523 ; TGL 600 ; TJM 000 ; VJG 221 ; Meteorite {Astronomie} ; Kosmochemie {Weltraumforschung} ; Geochemie der Chondrite
    Language: German
    Type: monograph , publishedVersion
    Format: 137 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 27
    Publication Date: 2021-03-29
    Description: Vor dem Hintergrund des Globalen Wandels sind räumliche und zeitliche Informationen über die Stickstoffverfügbarkeit im Boden und die Nitratauswaschung von entscheidender Bedeutung für die Entwicklung von Maßnahmen zur integrierten Bewirtschaftung der (Grund-)Wasserressourcen. Im Rahmen des Projekts GLOWA-Danube untersucht diese Arbeit die Reaktionen des Bodenstickstoffhaushalts auf Klimaänderungen im Einzugsgebiet der Oberen Donau. Als Komponente des integrativen Entscheidungsunterstützungssystems DANUBIA wurde das objektorientierte und prozessbasierte Bodenstickstoffmodell SNT auf der Grundlage des Modells CERES Maize 2.0 entwickelt. SNT bildet die wichtigsten Prozesse (Mineralisierung/Immobilisierung, Denitrifizierung, Nitrifizierung, Harnstoffhydrolyse und Nitratverlagerung) und die Dynamik von zwei mineralischen (Nitrat und Ammonium) sowie zwei organischen (frische Biomasse und Humus) Stickstoffreserven im Boden ab. Die Validierung des Modells erfolgte durch einen multikriteriellen und skalenübergreifenden Vergleich mit Messreihen, die ein breites Spektrum pedologischer und meteorologischer Bedingungen in Deutschland abdeckten. In einer Sensitivitätsanalyse wurde die Reaktivität des Modells gegenüber Eingabedaten und physikochemischen Bodenparametern bestimmt ...
    Description: thesis
    Keywords: 577.22 ; 577.145 ; VJI 000 ; VOBB 400 ; VPB 200 ; Geochemische Kreislaufmodelle ; Anorganische Bodenchemie, Anorganische Bodenbestandteile ; Deutschland {Bodenkunde}
    Language: German
    Type: monograph , publishedVersion
    Format: 216 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 28
    Publication Date: 2021-03-29
    Description: In the unglaciated areas of Antarctica, lake sediments act as archives of the regional environmental and climatic history. In most cases, the records are restricted to the Holocene. Amongst the few exceptions are lakes in the McMurdo Dry Valleys, southern Victoria Land, which are known to have remained mostly ice-free during the Last Glacial Maximum. Within the scope of an U.S.-American-German expedition in austral summer 2002/2003, several sediment cores were recovered from the three major lakes in the Taylor Valley: lakes Fryxell, Hoare, and Bonney. In order to reconstruct the late Quaternary regional environmental and climate history, sedimentological, biogeochemical, mineralogical, and chronological investigations were conducted on the sediment sequences recovered from Lake Hoare (core Lz1020) and East Lake Bonney (core Lz1023) within the scope of this thesis. Sediment cores from Lake Hoare with a maximum length of 2.3 m mainly consist of coarse-grained material and penetrate back into the late Weichselian, when Taylor Valley was occupied by the large proglacial Lake Washburn. This lake was dammed by the advanced Ross Sea ice sheet at the valley outlet and was mainly fed by meltwater of the ice sheet. During the Pleistocene-Holocene transition, enhanced evaporation led to a significant lake level drop of Lake Washburn ...
    Description: thesis
    Keywords: 551 ; 550 ; TWC 500 ; VDI 200 ; VAU 000 ; VEY 200 ; VBN 500 ; VBL 500 ; Klimaschwankungen und Klimaänderungen im Quartär ; Quartär ; Paläolimnologie {Geologie} ; Antarktis {Geologie} ; Geochronologie einzelner Regionen im allgemeinen ; Geologische Bohrungen in einzelnen Regionen
    Language: English
    Type: monograph , publishedVersion
    Format: 121 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 29
    Publication Date: 2021-03-29
    Description: Eleven lakes and ponds and three lacustrine sediment sequences from coastal East and North-East Greenland were studied for recent hydrological and phytoplankton characteristics and for palaeolimnology, respectively. The limnological survey of lakes and ponds from Store Koldewey in summer 2003 revealed cold, monomictic, thermally unstratified, alkaline and likely oligotrophic water bodies. The diatom phytoplankton, present in six lakes and dominated by four species, varied distinctly between the lakes. The results give information about the recent status of the ecology of these High Arctic freshwater bodies. The sediment sequences were investigated for their chronology, changes in physical and biogeochemical properties, macro- and microfossils, grain-size distribution and in the case of one sequence for its elemental profiles using XRF. The palaeolimnological studies address different time intervals at various temporal resolutions with particular attention to the latitudinal differences of late Quaternary climatic and environmental changes along the coast of East and North-East Greenland. The results include information about the Late Weichselian ice-front environments on southern Store Koldewey with information about the temporal and spatial evolution of the Greenland Ice Sheet margin west of the island ...
    Description: thesis
    Keywords: 551 ; 550 ; TWC 500 ; VDI 200 ; VAU 000 ; VEY 110 ; VBN 500 ; VBL 500 ; Klimaschwankungen und Klimaänderungen im Quartär ; Quartär ; Paläolimnologie {Geologie} ; Grönland {Geologie} ; Geochronologie einzelner Regionen im allgemeinen ; Geologische Bohrungen in einzelnen Regionen
    Language: English
    Type: monograph , publishedVersion
    Format: 148 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 30
    Publication Date: 2021-03-29
    Description: Die mio-pliozänen Ablagerungen im NNW SSE streichenden Monastir-Florina-Ptolemais-Kozani/Servia-Graben beherbergen das größte zusammenhängende Braunkohlevorkommen in Bereich des Balkans. Das Becken erstreckt sich von Monastir (F.Y.R.O.M.) im Norden bis hin zur Region von Elassona im Süden (Makedonien/GR). Es umfasst eine Gesamtfläche von ca. 120 kmø. Mittlerweile werden ca. 71 % des elektrischen Energiebedarfs der Hauptstadt Athen durch die Energiegewinnung aus dem MFPK/S-G gedeckt. Diese rhythmisch entwickelten Lignitvorkommen zeigen, neben den bedeutenden wirtschaftlichen Aspekten, ein großes Potential für eine Paläoklima-Analyse des nordöstlichen mediterranen Raums. Das Neogen zeigt einen multiplen Wechsel von Kalt- und Warmzeiten mit vereinzelt deutlich höheren Temperaturen als heute an (Bradley, 1999). Die Ursachen hierfür können u.a. auf Variationen der Erdbahnparameter zurückgeführt werden, welche Schwankungen in der Insolation verursachen und somit das atmosphärisch-ozeanische System steuern. Zeitreihenanalysen belegten bereits in den 70er bis späten 90er Jahren des letzten Jahrhunderts diese Variationen innerhalb mariner (Hays et al., 1976; Imbrie & Imbrie, 1980) und kontinentaler Ablagerungen (Santarelli et al., 1988, van Vugt et al., 1998. Die Ursachen und Steuerungsprozesse dieser Variationen sind von Milankovitch (1920, 1930, 1941) eingehenst diskutiert worden ...
    Description: thesis
    Keywords: 551.69 ; 551 ; 550 ; TSF 300 ; TOT 310 ; VEF 300 ; VKB 372 ; VKB 376 ; VKB 326 ; VDI 110 ; Griechenland und griechische Inseln {Geophysik} ; Gesteinsmagnetismus {Geophysik} ; Griechenland und griechische Inseln {Geologie} ; Karbonatische Sedimentgesteine ; Organogene Sedimentgesteine ; Magnetische Stratigraphie {Sedimentologie} ; Paläogen
    Language: German
    Type: monograph , publishedVersion
    Format: 131 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 31
    Publication Date: 2021-03-29
    Description: thesis
    Keywords: 551.5 ; 550 ; TVK 900 ; TYZ 100 ; Vertikale Komponenten der Luftbewegung {Meteorologie} ; Atlantischer Ozean {Meteorologie und Klimatologie}
    Language: German
    Type: monograph , publishedVersion
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 32
    Publication Date: 2021-03-29
    Description: Die hyperaride und weitgehend vom Menschen unveränderte Western Desert Ägyptens ist ein Hauptuntersuchungsgebiet des interdisziplinär angelegten Sonderforschungsbereichs 389 (ACACIA) und bietet somit ein ideales Feld zur Entwicklung und Prüfung neuer Methoden. In dieser Arbeit wurden erstmalig flächenhafte digitale Höheninformationen in hoher Auflösung für das Untersuchungsgebiet abgeleitet, aufbereitet und hinsichtlich ihrer Qualität und Einsatzmöglichkeiten untersucht. Dabei konnten über die Fragestellung der Arbeit hinaus weitere Einsatzmöglichkeiten zur Beantwortung geomorphologischer und geoarchäologischer Fragestellung herausgearbeitet werden. Beide Höhenmodelle (ASTER / SRTM-3) zeigen für die jeweilige Auflösung geringe Höhenfehler, sie unterscheiden sich jedoch hinsichtlich ihres nutzbaren Maßstabsbereiches. Hier konnte eine Trennung im Bereich von ca. 1:100.000 festgelegt werden. Während die SRTM-3-Daten durch ihre flächenhafte Verfügbarkeit für großräumige Fragestellungen geeignet sind, fallen die ASTER-Höhendaten in die chorische Maßstabsebene und eignen sich besonders zur Beantwortung regionaler Fragestellungen. Die abgeleiteten methodischen Ergebnisse zum Einsatz und der Überprüfung der Höhendaten können problemlos auf andere aride Räume übertragen werden. Zur Ableitung holozäner Nutzungspotentiale wurde ein offenes Modell entwickelt, das die spezielle Fragestellung aufgreift, jedoch ebenfalls mit anderen Datensets und in anderen Regionen nutzbar ist. Es beinhaltet die Verknüpfung geomorphometrischer mit anderen raumbezogenen Daten in einem statistischen Verfahren. Die kanonische Korrespondenzanalyse wurde dabei als geeignete statistische Methode vorgestellt, um ein solches Datenset zu analysieren und einen Mehrwert an Information aus den Daten abzuleiten. Für das holozäne Nutzungspotential der Western Desert konnten durch die Untersuchung zweier archäologischer Fundregionen verschiedene Erkenntnisse gewonnen werden ...
    Description: thesis
    Keywords: 910
    Language: German
    Type: monograph , publishedVersion
    Format: 197 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 33
    Publication Date: 2021-03-29
    Description: Mit dem Ziel der Rekonstruktion des jungquartären Klimawandels im südlichen Kaokoland (NW-Namibia) und einer daraus resultierend zu erstellenden regionalen Klimastratigraphie wurden sedimentologische und geochronologische Untersuchungen von äolischen Sandablagerungen und fluvial/aquatisch abgelagerten Beckensedimenten durchgeführt. Das Untersuchungsgebiet im nordwestlichen Namibia ist durch ein arides Klima gekennzeichnet, kann aber aufgrund der geologisch bedingten Kleinkammerung seines Reliefs in klimatische Gunst- und Ungunsträume für menschliche Besiedlung gegliedert werden. Die bislang vorliegenden Rekonstruktionen der Klimageschichte dieser Region gehen von einer seit dem Tertiär andauernden Aridität aus. Die quartäre Klimaentwicklung ist durch hygrische Fluktuationen geringer Ausprägung gekennzeichnet. Anhand der sedimentologischen und geochronologischen Ergebnisse wurde eine bis 16 700 Jahre vor heute zurückreichende Stratigraphie erarbeitet, in der Änderungen des Klimas dokumentiert sind. So sind um 8000 und um 4500 Jahre vor heute zwei feuchtere Phasen nachweisbar. Die Ergebnisse der Untersuchungen äolischer Sande belegen für die Folgezeit die seit mindestens 2000 Jahren vor heute andauernde Trockenheit mit ausgeprägter äolischer Dynamik. Die fluvial/aquatische Ablagerung der Beckensedimente endet im südlichen Kaokoland um 15 500 Jahre vor heute. Die nachfolgend einsetzende Phase äolischer Aktivität kann mit dem Aufbau der Wüstenlösse’ im nördlichen Kaokoland korreliert werden. Weiterhin wurde gezeigt, dass die feuchteren Phasen am Namib-Rand nicht die Intensität und Dauer aufweisen, wie sie östlich des Untersuchungsgebietes festgestellt wurden. Nicht zuletzt wird anhand der sedimentologischen Ergebnisse der untersuchten Dünen eine bisher nicht beschriebene Genese von Pseudoechodünen’ aus Sandrampen aufgezeigt.
    Description: thesis
    Keywords: 551.79 ; 551
    Language: German
    Type: monograph , publishedVersion
    Format: 176 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 34
    Publication Date: 2021-03-29
    Description: Weather and climate in West Africa are determined by the pronounced contrast between tropical, moist air masses over the Gulf of Guinea in the south and the dry desert climate over the Sahara in the north. The sharp border between the two air masses exhibits a pronounced meridional annual cycle and follows the path of the sun northward. This circulation system is called "West African monsoon". In the past, the knowledge about the factors that control the monsoon and its strength was limited due to the small number of high-quality observations. Therefore, little is known about the reasons for the significant decline of annual rainfall over the Sahel area during the past 40 years which represents the most pronounced climatic signal worldwide. During the past few years, intensive atmospheric observations were performed in the framework of the international project "African Monsoon Multidisciplinary Analyses" (AMMA) in order to obtain high-quality data and to improve the process understanding. This work gathered and analyzed ground-based remote sensing observations which were performed in Benin and Niger during the AMMA field campaigns. These data give an insight into diurnal and annual cycles of atmospheric parameters, such as water vapor, temperature profiles, cloud cover, cloud liquid water content, or wind with a temporal resolution never reached before. Particular attention is paid to the atmospheric water which is recognized to be a critical parameter for many other atmospheric variables, e.g. the vertical temperature distribution, the long-wave radiation balance, and many more ...
    Description: Zsfassung in dt. und engl. Sprache
    Description: thesis
    Keywords: 551.5 ; TYO 000 ; TVB 110 ; Westafrika, Sudan und Guinealänder {Meteorologie und Klimatologie} ; Grenzschicht {Meteorologie: Troposhäre}
    Language: German
    Type: monograph , publishedVersion
    Format: 120 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 35
    Publication Date: 2021-03-29
    Description: The distribution of hydrometeors is highly variable in space and time, since it is the result of a complex chain of processes with scales from microphysical (1e-6 m) to synoptical (1e3 m). It is a challenging task to observe these highly variable atmospheric constituents on a global scale with a temporal and spatial resolution sufficient for numerical weather prediction (NWP) and hydrological purposes. This study investigates the potential of the millimeter- and submillimeter-wavelength range on space-borne sensors for hydrometeor and surface precipitation rate observations. The approach is based on simulations with cloud resolving models (CRMs) coupled to a radiative transfer (RT) model. The simulations are performed for mid-latitude cases covering a broad band of precipitation events such as heavy convective and light stratiform winter precipitation. Realistic atmospheric conditions were simulated with two mesoscale CRMs: the Meso-scale NonHydrostatic model (Meso-NH) on a 10 km and the COSMO-DE (COnsortium for Small-scale MOdeling-DEutschland) on a 2.8 km horizontal resolution. When calculating brightness temperatures for satellite observations with the one-dimensional radiative transfer model MWMOD (MicroWave MODel), the detailed cloud microphysics and the three-dimensional fields of temperature, humidity, and pressure of the CRMs are considered in the calculation of the interaction parameters ...
    Description: thesis
    Keywords: 551.5 ; TUA 800 ; TUA 850 ; Radarmeteorologie ; Satellitenmeteorologie
    Language: English
    Type: monograph , publishedVersion
    Format: 138 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 36
    facet.materialart.
    Unknown
    Univ. Köln
    Publication Date: 2021-03-29
    Description: Dense cold molecular clouds reckoned to be stellar nurseries are the scene of an extreme molecular deuteration. Despite the cosmic D/H ratio of 10^{-5}, molecular species in prestellar cores are observed to contain nearly as much deuterium as hydrogen. This astonishing deuterium enrichment promoted by low temperatures is the work of H3+. It is the key species which unlocks the deuterium from its HD reservoir via reactions like H3+ + HD -〉 H2D+ + H_2 and drags it further to other species in successive reactions. For this reason, the H3+ + H2 isotopic system is outstandingly critical for the astrochemistry of cold environments. However, its understanding is yet incomplete and insufficient. This thesis thus focuses on the H3+ + H2 isotopic system from a theoretical, experimental and astronomical point of view giving a particular look into the role of nuclear spins...
    Description: thesis
    Keywords: 523 ; TJM 000 ; Kosmochemie {Weltraumforschung}
    Language: English
    Type: monograph , publishedVersion
    Format: 202 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 37
    facet.materialart.
    Unknown
    Univ. Köln
    Publication Date: 2021-03-29
    Description: Wasserdampf ist eines der wichtigsten atmosphärischen Spurengase. Sein Einfluss auf das Klima, die Chemie und den Energiehaushalt ist bedeutend. Von besonderem Interesse ist dabei die Wasserdampfverteilung in der oberen Troposphäre insbesondere in den Tropen. Die wichtigste Wasserdampfquelle für die tropische obere Troposphäre ist tropische Konvektion. Ihr wirkt das grossräumige Absinken entgegen, das seine Ursache sowohl in der Dynamik als auch im Strahlungshaushalt hat. Es gleicht die konvektive Aufwärtsbewegung aus und transportiert dabei relativ trockene Luft nach unten. Über den Netto-Effekt dieser beiden Prozesse ist wenig bekannt, vorallem wegen eines Mangels an zuverlässigen Messungen in dieser Region. In dieser Arbeit werden der Wasserdampfgehalt und die Mechanismen, die für die Wasserdampfverteilung in der oberen tropischen Troposphäre verantwortlich sind, mithilfe einer grossen Menge an in-situ Feuchtemessungen untersucht. Die Messungen wurden auf Linienflugzeugen im Rahmen des EU Projektes MOZAIC durchgeführt (Measurements of Ozone and Water Vapor by Airbus In-Service AirCraft; Messungen von Ozon und Wasserdampf auf Airbus Linienflugzeugen). Eine Klimatologie der gemessenen Parameter über dem tropischen Atlantik zeigt, dass die Feuchte auf allen zeitlichen und räumlichen Skalen sehr variabel ist. Die bimodale Verteilung der Feuchte in den Tropen unterscheidet sich ausserdem deutlich von der Verteilung in den Sub-Tropen oder mittleren Breiten...
    Description: thesis
    Keywords: 551.5 ; 550 ; TVB 100 ; TVL 100
    Language: English
    Type: monograph , publishedVersion
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 38
    Publication Date: 2021-03-29
    Description: According to a model by Cerling (1991, 1999), the carbon isotope composition of calcretes should depend on the soil type and the CO2-concentration in the atmosphere. We have tested Cerling’s model by investigating 14 Palaeozoic sections with soil profiles. A large number of carbonate types of different genetic origin exist in the localities examined. Comparing the Palaeozoic samples with recent and subrecent calcretes, it can be demonstrated that anhedral, cryptocrystalline (〈10 μm) and subhedral microcrystalline (10 - 40 μm) carbonates are clearly of pedogenic origin. Crystals of larger size with a poikilotopic texture are of groundwater or burial diagenetic origin. Macro- and micromorphological features, typical of recent calcretes, occur in several soil profiles, but thin section microscopy reveals a strong diagenetic overprint of most pedogenic carbonates. Time equivalent sections with comparable soil types (protosols, calcisols and vertisols) show large variations in carbon isotope composition. On the other hand, different carbonate generations at one site do not differ much. Therefore Palaeozoic calcretes appear to be unsuitable for a deduction of the Palaeozoic CO2-concentration.
    Description: German Research Foundation (DFG)
    Description: research
    Keywords: 551.9 ; 552.5 ; VKB 350 ; VJJ 110 ; VCA 300 ; VKB 332 ; VKA 300 ; VKB 371 ; VEA 000 ; VKB 372 ; Lithogenese {Sedimentologie} ; Geochemie der Stabilen Isotopen ; Paläozoische Geologie ; Sedimentationsbedingungen ; Petrogenese ; Klastische Sedimentgesteine ; Europa insgesamt {Geologie} ; Karbonatische Sedimentgesteine ; Kohlenstoffkreislauf ; C-isotope ; Jungpaläozoikum ; Paläopedologie ; Kalkkruste ; CO2 ; calcrete ; carbon cycle ; upper Paleozoic ; paleosol ; C-13/C-12 ; Europa ; paläoklima ; Europe ; 38.41 ; 38.61 ; 38.32
    Language: English
    Type: article
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 39
    facet.materialart.
    Unknown
    Univ. Köln
    Publication Date: 2021-03-29
    Description: In the framework of this PhD thesis, the study of the distribution of an extended mass close to the super-massive black hole (SMBH) at the centre of our Galaxy is addressed using observational data and theoretical modelling. The main emphasize is on establishing a distinction between the fraction of dark mass present in the form of a black hole and that in an extended form. Despite the significant observational and theoretical progress in the understanding of SMBHs in the last ten years, the formation of SMBHs and the interplay with their host galaxy are still poorly understood. The work presented here extends our understanding of the dynamics in the vicinity of the SMBH. Already in 1974, it was proposed that the radio source SgrA* could be a SMBH. With observations during the following years, it became more clear that the centre of our Galaxy hides an amount of dark mass close to 3 million solar masses. However, the strongest evidence for the existence of a SMBH, was only after it became possible to trace for the first time stellar orbits of fast moving stars, the so-called S-stars, around SgrA*. This was achievable using the SHARP near-infrared speckle camera at la Silla in Chile as well as the near-infrared camera NAOS/CONICA at the Very Large Telescope (VLT) at Paranal in Chile.
    Description: thesis
    Keywords: 523 ; TEG 000 ; TIC 000 ; TEG 440 ; Kosmogonie {Astronomie} ; Sternhaufen {Astronomie} ; Schwarze Löcher {Astronomie: Kosmogonie}
    Language: English
    Type: monograph , publishedVersion
    Format: 122 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 40
    Publication Date: 2021-03-29
    Description: In this thesis the design and analysis of SIS-mixers (SIS: superconductor-isolator-superconductor) for the use as low-noise and broad-band detectors in the submm-region for astronomical observations is described. The SIS-mixers have been developed for the frequency band 2 (636-802 GHz) of the Heterodyne Instrument for the Far Infrared (HIFI) on ESA’s space-observatory Herschel. The required performance baseline has been defined by the HIFI-consortium in terms of the estimated noise temperature contribution of the mixer to be 110 K at 636 GHz and 150 K at 802 GHz. In the frequency region between 80 GHz and 900 GHz Heterodyne SIS mixers are established as the best devices for low noise mixing with a high spectral resolution (mixing of the signal radiation with local oscillator, LO). For the HIFI band 2 mixers, the technology of Nb/Al-Al2O3/Nb-junctions has been used with junction areas of 0.5-1.0 um2, a target value for the current density jc of 15 kA/cm2 and a gap-voltage of 2.75-2.77 mV. For the compensation of the SIS-junction’s intrinsic capacitance and the optimized power coupling to the tunnel junction, two types of matching circuits have been theoretically modelled and experimentally studied: (1) three-step transformer single junction devices and (2) double-junction devices. This has been done for two material combinations: for an all-superconductive micro strip NbTiN/SiO2/Nb, and for the superconductor/normal-conductor combination NbTiN/SiO2/Al...
    Description: thesis
    Keywords: 523 ; TBG 000 ; TCE 230 ; Infrarot-Astronomie ; Weltraumbasierte UV-, Optische und Infrarotteleskope {Astronomische Instrumente}
    Language: English
    Type: monograph , publishedVersion
    Format: 183 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 41
    Publication Date: 2021-03-29
    Description: In der Radioastronomie und in der Atmosphärenforschung erlauben moderne Heterodyn-Empfangssysteme die Beobachtung von Atom- und Molekülübergangslinien mit ZF-Bandbreiten von bis zu 4 GHz. Zur Abdeckung dieser großen Bandbreiten wurden bisher Echtzeitspektrometer eingesetzt, die entweder nur eine geringe Auflösung aufweisen oder Hybrid-Spektrometer, die die Bandbreite durch das Zusammenschalten mehrerer Subsysteme erreichen. Solche Hybrid-Spektrometer sind zum einen sehr komplex und zum anderen zeigt diese Art von Spektrometern einen Platforming-Effekt. Ziel dieser Arbeit war es deshalb, ein Echtzeitspektrometer zu entwickeln, das auf Akusto-Optik basierend intrinsisch eine Bandbreite von 〉= 3 GHz bei moderater Auflösung (〈 3 MHz) zur VerfÓgung stellt. Zur Entwicklung des Prototypen des Breitbandigen Akusto-Optischen Spektrometers (BAOS) war es notwendig von der bisher in AOS verwendeten LaserwellenlÑnge im Infraroten zu einer kÓrzen WellenlÑngen im Blauen zu wechseln. Des weiteren wird fÓr das BAOS eine Bragg-Zelle verwendet, die nicht auf Lithium-Niobat basiert, sondern auf Rutil. Im Rahmen dieser Arbeit wurde ein mathematisches Modell entwickelt, das in Fraunhofer-NÑherung das zweidimensionale Beugungsbild des Bragg-gebeugten Laserlichts auf dem CCD beschreibt und somit die MÒglichkeit bietet, im Vorfeld der Spektrometer Entwicklung die optimale Ausleuchtung der Bragg-Zelle und die erwartet Effizienz des BAOS zu bestimmen. Mittels dieser Berechnungen wurde der optische Aufbau des Prototypen-BAOS konstruiert und die Kenndaten des Spektrometers experimentell bestimmt. Wie sich zeigt, erfÓllt der Prototyp des BAOS die Erwartungen hinsichtlich Bandbreite, AuflÒsung, Noise Dynamic Range (NDR) und StabilitÑt voll und ganz ...
    Description: thesis
    Keywords: 523 ; TBC 000 ; Radioastronomie
    Language: German
    Type: monograph , publishedVersion
    Format: 156 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 42
    Publication Date: 2021-03-29
    Description: The Herschel satellite observatory will explore the universe at far-infrared, submillimetre, and millimetre wavelengths. This regime of the electromagnetic spectrum is difficult to observe, because water vapour in the Earth’s atmosphere absorbs the signals of almost all the astronomical sources. With the 3.5m telescope (the largest ever placed aboard a spacecraft), it will be possible to observe various atomic and molecular lines with exceptionally high spatial resolution. The receiver system employs the heterodyne technique, and the spectral information is obtained by means of real-time spectrometers. Within this thesis, the requirements, specifications, design concept, and development of a wide bandwidth array acousto-optical spectrometer (WBS) is discussed...
    Description: thesis
    Keywords: 523 ; TC 200 ; TBG 000 ; Astronomische Beobachtungen vom Weltraum aus ; Infrarot-Astronomie
    Language: English
    Type: monograph , publishedVersion
    Format: 177 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 43
    Publication Date: 2021-03-29
    Description: Die Erde und viele andere planetare Körper besitzen Eisennickel-Kerne. Diese resultieren aus einer zumindest partiellen Aufschmelzung in der Frühphase ihrer Geschichte. Durch die Gravitation hat sich dabei das schwerere Metall vom leichteren Silicat abgetrennt und ist in den Mittelpunkt des Körpers gesunken. Auf diese Weise entstand daraus der Metallkern. Während dieses Segregationsprozesses stand das Metall im Gleichgewicht mit dem Silicat. Eine geringe Menge des Elements Silicium wird abhängig von Temperatur und Sauerstoffpartialdruck aus der Oxidationsstufe +IV zum elementaren Silicium reduziert. Dieses Si wandert in die Metallphase und wird mit ihr in den Kern extrahiert. Die Menge des Si im Fe-Ni-Kern ist demnach ein empfindlicher Indikator für Temperatur und Sauerstoffpartialdruck bei der Kernbildung. Die meisten Gruppen der Eisenmeteorite werden als Derivate solcher Metallkerne angesehen, die sich während des Aufschmelzens von Planetesimalen gebildet haben. Der Si-Gehalt in Eisenmeteoriten sollte daher Temperatur und Sauerstoffpartialdruck bei ihrer Bildung widerspiegeln. Bisher waren die Si-Gehalte in Eisenmeteoriten nicht bekannt, weil diese unter den Nachweisgrenzen der verwendeten analytischen Methoden (Elektronenstrahl- Mikroanalyse) liegen. Auch der zu weiteren Berechnungen notwendige Aktivitätskoeffizient von Silicium in Eisennickel-Legierungen war bisher nicht ausreichend bekannt ...
    Description: thesis
    Keywords: 523 ; TG 200 ; TJM 000 ; VJG 100 ; Kosmogonie des Sonnensystems {Astronomie} ; Kosmochemie {Weltraumforschung} ; Geochemie des Sonnensystems
    Language: German
    Type: monograph , publishedVersion
    Format: 134 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 44
    Publication Date: 2021-03-29
    Description: Die Erde, der Mond und die anderen terrestrischen Planeten haben einen eisen-nickelreichen, metallischen Kern, der sich in der Frühphase der Geschichte dieser Planeten von der Silikat-phase, die heute den Mantel bildet, abgetrennt hat. Diese Metall/Silikat-Trennung ist eine der umwälzensten Ereignisse in der Geschichte der terrestrischen Planeten. Umso erstaunlicher ist es, dass die Prozesse, die zur Kernbildung geführt, und die Bedingungen, die bei der Kernbil-dung geherrscht haben, bis heute noch nicht vollständig verstanden sind. Als Schlüssel zum Verständnis des Kernbildungsprozesses werden die siderophilen (eisenliebenden) Elemente (z.B. Ni, Co, Ge, PGEś) angesehen. Herrscht chemisches Gleichgewicht zwischen einer Metall- und einer Silikatphase, wandern die siderophilen Elemente bevorzugt in die Metallphase was zu ihrer Verarmung in der Silikatphase führt. Die Affinität eines Elements zur Metallphase wird mit dem Metall/Silikat-Verteilungskoeffizienten (Dmet/Sil), dem Quotienten aus der Konzentration des untersuchten Elementes in der Metallphase und der Konzentration des untersuchten Elements in der Silikatphase, ausgedrückt. Vergleicht man die aus den experimentell ermittelten Metall/Silikat-Verteilungskoeffizienten (1 atm., 1600 ʿC und eine Sauerstofffugazität 2.3 logarithmische Einheiten unterhalb der des Eisen-Wüstit-Puffers) errechneten Konzentrationen der siderophilen Elemente mit den tatsächlichen Konzentrationen im Erdmantel, sieht man, dass die Konzentrationen der siderophilen Elemente im Erdmantel teilweise mehrere Größenordnungen höher als die errechneten liegen. Dieses Phänomen wird als siderophile Elementanomalie bezeichnet. Unter den siderophilen Elementen nehmen Nickel und Kobalt eine Sonderstellung ein, denn sie haben nicht nur eine höhere Konzentration im Erdmantel als erwartet, sondern sie weisen ein beinahe chondritisches Verhältnis (~18.2) auf. Das chondritische Ni/Co-Verhältnis im Erdmantel erklären LI&AGEE (1996) durch eine verschieden starke Druckabhängigkeit der Verteilungskoeffizienten von Nickel und Kobalt ...
    Description: thesis
    Keywords: TG 200 ; TJM 000 ; VJG 100 ; Kosmogonie des Sonnensystems {Astronomie} ; Kosmochemie {Weltraumforschung} ; Geochemie des Sonnensystems
    Language: German
    Type: monograph , publishedVersion
    Format: 143 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 45
    Publication Date: 2021-03-29
    Description: The main focus of this work is the development of ultrathin NbN and NbTiN films. A reproducible and reliable deposition process for ultrathin NbN and NbTiN films for the use in phonon-cooled HEB devices was established. The ultrathin films were deposited on silicon (Si) substrates and on 2æm Si3N4 membranes by DC reactive magnetron sputtering. A method for the precise control of the nitrogen partial pressure by monitoring the target voltage has been introduced to deposit high quality, ultrathin NbN (3-4nm, Tc=8.5 K) and NbTiN (4-5nm, Tc=8K) films. Substrate heating of at least 600ʿC during the deposition is essential for the fabrication of ultrathin NbN and NbTiN films on Si substrates and Si3N4 membranes. The fabrication process required for HEB devices to be used in a quasi-optical mixer was developed. The ultrathin film was patterned by electron beam lithography (EBL), resulting in bolometer devices that measure areas of about 0.4 æm x 4 æm. The nature of the contact determines the interface transparency between the bolometer and the contact structure. Different cleaning processes have been performed and the influence on the contact resistance has been instigated. A better interface transparency gives less RF losses and could improve the HEB sensitivity and local oscillator (LO) requirement ...
    Description: thesis
    Keywords: 523 ; TBC 000 ; Radioastronomie
    Language: English
    Type: monograph , publishedVersion
    Format: 165 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 46
    Publication Date: 2021-03-29
    Description: Gegenstand der vorliegenden Arbeit ist die technische Weiterentwicklung des durchstimmbaren Infrarot-Heterodynsystems THIS (Tuneable Heterodyne Infrared Spectrometer) sowie die Planung, Vorbereitung und Durchführung diverser Beobachtungseinsätze des Instruments an unterschiedlichen Teleskopen. Auf technischer Seite konnte der sehr erfolgreiche Einsatz von Quanten- Kaskadenlasern als Lokaloszillatoren, die Empfindlichkeit des Systems erstmals auf das Niveau von CO2-Laser gepumpten Instrumenten bringen. Frequenzstabilität und radiometrisches Verhalten des Instruments konnten für Beobachtungszeiträume von einigen Stunden nachgewiesen werden.Weiterhin wurde ein in den Empfänger integriertes, optisches Guide-System für den Einsatz an Teleskopen entwickelt und aufgebaut. Die neu entwickelte Optik macht THIS durch die Verwendung einer integrierten optischen Kamera sowie eines Scannerspiegels zur Auswahl von Beobachtungspositionen am Himmel weitgehend unabhängig vom Teleskoptyp und damit vielseitig einsetzbar. Die technischen Neuerungen und die mechanische Stabilität des neuen Aufbaus wurden u. a. während Messperioden am Observatorium Hoher List bei Daun/Eifel sowie am McMath-Pierce Solar Telescope auf dem Kitt Peak nahe Tucson/Arizona erstmalig außerhalb des Labors genutzt und getestet. Es konnten Molekül-Absorptionen aus Sonnenflecken aufgenommen und aus den vollständig aufgelösten Linienprofilen die Anregungstemperaturen des Materials bestimmt werden. In diesem Zusammenhang wurde eine theoretische Analyse der Kalibration von am Teleskop gewonnenen Spektren durchgeführt und auf die gemessenen Daten angewandt ...
    Description: thesis
    Keywords: 523 ; TBG 000 ; Infrarot-Astronomie
    Language: German
    Type: monograph , publishedVersion
    Format: 147 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 47
    Publication Date: 2021-03-29
    Description: The thesis focuses on two case studies of the host galaxies of the quasi-stellar objects (QSOs) I Zw 1 and 3C 48. The studies are motivated by the hypothesis that ultra-luminous infrared galaxies (ULIRGs) might represent the early stage of QSO evolution (Sanders et al. 1988). According to this hypothesis, galaxy mergers and interactions trigger gas inflow which is followed by starburst activity and by the formation of an active nucleus. As likely transitionary objects between the ultra-luminous infrared stage and the QSO stage, I Zw 1 and 3C 48 are promising candidates to investigate the active nucleus, the starburst, and the merger properties as the essential links between all stages of the proposed evolutionary sequence. The case study of I Zw 1 has an observational focus and is based on near-infrared (NIR) imaging and spectroscopy, carried out with ISAAC (Infrared Spectrometer and Array Camera) at the Very Large Telescope of the European Southern Observatory (ESO) on Cerro Paranal in Chile. The two-armed spiral host galaxy of I Zw 1 shows two bright knots in the north and in the west of the optical disk region, respectively. Here, the new ISAAC spectra indicate that the northern object is a projected foreground star, as previously assumed but recently challenged. In the surroundings of the western source, the ISAAC J-band image displays tidal features. This gives further support for the scenario that I Zw 1 is presently in a minor merger process with this source. The new spectra and the NIR colors of the western source indicate an old stellar population. The host of I Zw 1 is analyzed in a one-dimensional structural decomposition into bulge, disk, and halo components, which results in mean J-band mass-to-light ratios ...
    Description: thesis
    Keywords: 523 ; THS 000 ; TIE 900 ; TIE 400 ; Sternpopulationen {Astronomie} ; Sonstige Sternensysteme {Astronomie} ; Spektren und Leuchtkraft von Sternsystemen {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 123 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 48
    Publication Date: 2021-03-29
    Description: This PhD thesis presents a study of active galaxies carried out from cm- to mm-wavelengths with high angular resolution. The mechanism of the activity in these objects is supposed to be strongly correlated with the accretion of matter onto a super-massive black hole in their centres. One approach to increase the understanding of these highly interesting sources is to observe and analyse the molecular gas. The characteristics of its distribution and dynamics are indispensible diagnostic tools to investigate the accretion processes at different angular scales. A second approach is the study of emission originating in the direct vicinity of the black hole, such as non-thermal radio emission. To account for different activity levels, five objects were chosen ranging from nearby, Low Luminosity Active Galaxies (LLAGs; NGC3718 at z=0.003 and NGC1068 at z=0.004) to higher redshifted, High LAGs (HLAGs; HE1029-1831 at z=0.039, 3C48 at z=0.367, and Q0957+561 at z=1.414). The first two sources are part of the NU(clei of)-GA(laxy) project, that aims at analysing the distribution and kinematics of the molecular gas at high angular resolution/sensitivity in a sample of 30 nearby LLAGs. HE1029-1831 is part of a complementary sample of nearby HLAGs with similar aims. All sources were observed in carbon-monoxide (CO), known to be a good molecular gas tracer, with the IRAM Plateau de Bure Interferometer (PdBI) providing high sensitivity and high angular resolution. CO emission was detected in all five galaxies. In NGC3718, the molecular gas disk, having roughly two hundred million solar masses, is highly warped. The distribution of the gas reveals large scale asymmetries witnessing a possible tidal tail interaction with a close companion, and as well small scale asymmetries most likely tracing accretion onto the nucleus ...
    Description: thesis
    Keywords: 523 ; TIE 400 ; Spektren und Leuchtkraft von Sternsystemen {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 207 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 49
    Publication Date: 2021-03-29
    Description: In den Marsmeteoriten ALHA 77005, ALH 84001, Chassigny, EETA 79001A, Governador Valadares, Lafayette, Nakhla, Sayh al Uhaymir 005, Shergotty und Zagami sowie den Chondriten Grüneberg, Morávka, Naragh und Neuschwanstein wurden die Konzentrationen der langlebigen kosmogenen Radionuklide Be-10, Al-26 und Mn-53 gemessen. Die Analyse fand mittels ultrasensitiver Beschleuniger-Massenspektrometrie (Accelerator-Mass-Spectrometry: AMS) statt. Dazu mussten die Elemente Al, Be, Ca, Fe, Mn und Ni mittels eines radiochemischen Trennungsgangs separiert werden. Daraufhin wurden hochreine Oxid-, Hydrid- und Fluorid-Proben für die AMS-Messung präpariert und in den Beschleunigerlabors der TU-München und der ETH Zürich gemessen. Darüber hinaus wurden die Konzentrationen der kosmogenen Anteile der Edelgase He-3, Ne-21, Ne-22, Ar-36, Ar-38, Kr-80 und Kr-83 zusammengestellt, die im Rahmen eines gemeinsamen Forschungsvorhabens am MPI Mainz an den gleichen Proben analysiert und auf ihren kosmogenen Anteil korrigiert wurden. Dadurch wurde ein umfassender same-sample-Datensatz mit teilweise erstmaligen Daten für kosmogene Nuklide in den untersuchten zehn Marsmeteoriten geschaffen, der in diesem Umfang bisher nicht erhältlich war. Zur Interpretation der gemessenen Radionuklidkonzentrationen diente das von Leya et al. [LEY00b] entwickelte physikalische Modell, welches auf der Basis nuklearer Daten die Produktionsrate kosmogener Nuklide in Meteoroiden berechnet. Mit Hilfe der analysierten Daten und der Modellrechnungen war es möglich, die Bestrahlungsgeschichten detailliert zu entschlüsseln ...
    Description: thesis
    Keywords: 523 ; TGL 600 ; VJG 200 ; Meteorite {Astronomie} ; Geochemie der Meteorite
    Language: German
    Type: monograph , publishedVersion
    Format: 179 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 50
    Publication Date: 2021-03-29
    Description: Models of the thermal behavior of a cometary nucleus, the evolution of the neutral gas coma, the ionized cometary coma and of the interaction of the cometary plasma with the solar wind are studied in this work. The general aim is to develop a global model of the comet and its environment in order to characterize the physical conditions around comets 67P/Churyumov-Gerasimenko and 46P/Wirtanen with respect to the heliocentric distance. The results also provide estimates of the effects of the cometary environment on the radio science investigations experiment (RSI) aboard the spacecraft Rosetta. After the launch that is scheduled for February 2004, the Rosetta mission is planned to encounter comet 67P/Churyumov-Gerasimenko and accompany it on its orbit. Comet 46P/Wirtanen has been the original target comet, but serves now as back-up target due to the postponement of the Rosetta launch in January 2003. The model of the heat diffusion within the cometary nucleus is one-dimensional. A grid of one-dimensional models is distributed over the nucleus in order to determine the temperature distribution and the sublimation characteristics of the comet on the whole surface of the comet. A heat balance equation is applied as boundary condition on the surface. Many parameters that have to be accounted for in a heat diffusion model are not precisely known to date. The variation of these parameters within reasonable limits yields a wide range of possible results. The heat diffusion within the cometary nucleus is derived from an energy conservation equation that includes heat conduction through the porous cometary material and heat convection due to the transport of latent heat by the gas phase within the nucleus. Model results are evaluated by a comparison of modeled and observed global gas production rates ...
    Description: thesis
    Keywords: 523 ; TGL 280 ; TC 200 ; Einzelne Kometen {Astronomie} ; Astronomische Beobachtungen vom Weltraum aus
    Language: English
    Type: monograph , publishedVersion
    Format: 153 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 51
    facet.materialart.
    Unknown
    Univ. Köln
    Publication Date: 2021-03-29
    Description: Während der Kreide wurden zahlreiche Störungen des globalen Kohlenstoffkreislaufes aufgezeichnet. Diese Störungen führten zu organisch reichen Ablagerungen, den sogenannten ozeanischen anoxischen Ereignissen (OAEs). Der OAE 1b, abgelagert in der Unteren Kreide, ist einer dieser bedeutenden CO2- Störungen und wird mit der Sedimentation von Schwarzschiefern in Verbindung gebracht. Beschrieben wurde OAE 1b in Ablagerungen des Unteren Albs für die Regionen des Nord- und Zentral Atlantiks sowie im westlichen Einzugsbereich der Tethys und wird deshalb als überregionaler Schwarzschiefer beschrieben. OAE 1b ist assoziiert mit einer abrupten Verschiebung zu ausgeprägt negativen Werten innerhalb zahlreicher Kohlenstoffisotopenreservoirs. Negative Piks in den Kohlenstoffisotopen wurden ebenfalls für das OAE im Toarcium und das OAE 1a im Frühen Apt beschrieben und werden in Zusammenhang mit spontaner Freisetzung von Methan aus marinen Gashydraten gebracht. In dieser hier präsentierten Studie wurden hochauflösende geochemische Profile von zwei paläogeographisch getrennten und klimatisch differenzierten Gebieten (Mazagan Plateau DSDP Site 545 und dem Vokontischen Becken) erstellt. Der Beginn der Sedimentation und der Abschluss fallen zeitgleich mit den negativen Isotopen Piks für beide Untersuchungsgebiete einher. Auffallend ist ein plötzlicher Anstieg der Meeresoberflächentemperatur um 3 ʿC, gemessen an der tropisch gelegenen Site 545 mit dem TEX86 Temperaturproxie, zeitgleich mit dem negativen Piks in den Kohlenstoffisotopen zu Beginn des OAE 1b ...
    Description: Zsfassung in dt. und engl. Sprache
    Description: thesis
    Keywords: 551 ; VJI 000 ; VDH 310 ; VJB 313 ; VKB 380 ; Geochemische Kreislaufmodelle ; Unterkreide ; Geochemie der Sedimente ; Sedimente bestimmter Regionen
    Language: English
    Type: monograph , publishedVersion
    Format: 135 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 52
    Publication Date: 2021-03-29
    Description: Mit Hilfe des mesoskaligen meteorologischen Modells FOOT3DK und eines Erkennungsverfahrens der sogenannten Circulation Weather Types (CWTs) wird eine statistisch-dynamische Regionalisierung des Niederschlags und der Evapotranspiration für das Drâatal südlich des Hohen Atlas in Marokko durchgeführt. Damit können Informationen über das Niederschlags- und Evapotranspirationsverhalten während eines zukünftigen Zeitraums gewonnen werden. Zu diesem Zweck wird FOOT3DK zunächst an die Simulationsregion angepasst. Darüber hinaus wird die Anzahl der möglichen Landnutzungsklassen auf 17 vergrößert und eine erweiterte Karte der Bodenarten in das FOOT3DK-Kataster implementiert. Anschließend wird die Sensitivität der Evapotranspiration hinsichtlich verschiedener Parameter untersucht und die Ergebnisse bei den darauf folgenden Simulationen berücksichtigt. Für die statistisch-dynamische Regionalisierung wird eine objektive Klassifikation der bodennahen Strömung in CWTs durchgeführt. Die dazu benötigten Bodendruckdaten stammen aus Reanalyse- und Modelldaten. Die Modelldaten basieren dabei auf verschiedenen SRES-Szenarien - A1B und B1. Im Folgenden werden Repräsentanten (Episodensimulationen von jeweils 24 Stunden Länge) für die verschiedenen CWTs bestimmt. Es werden Repräsentanten mit und Repräsentanten ohne Niederschlag im Untersuchungsgebiet nachsimuliert. Eine Validierung wird für das Jahr 2002 vorgenommen, weil für dieses Jahr Messwerte verschiedener Klimastationen im Simulationsgebiet und Antriebsdaten für FOOT3DK zur Verfügung stehen. Die Rekombination von Niederschlag und Evapotranspiration berücksichtigt die Häufigkeitsverteilung der verschiedenen CWTs und deren Wahrscheinlichkeit, mit bzw. ohne Niederschlag aufzutreten ...
    Description: thesis
    Keywords: 551.5 ; TYN 000 ; TUA 500 ; Nordafrika {Meteorologie und Klimatologie} ; Meteorologische Modelle
    Language: German
    Type: monograph , publishedVersion
    Format: 142 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 53
    Publication Date: 2021-03-29
    Description: To enhance interpretation capabilities of transient electromagnetic (TEM) methods, a multidimensional inverse solution is introduced, which allows for a explicit sensitivity calculation with reduced computational effort. The main conservation of computational load is obtained by solving Maxwell's equations directly in time domain. This is achieved by means of a high efficient Krylov-subspace technique that is particularly developed for the fast computation of EM fields in the diffusive regime. Traditional modeling procedures for Maxwell's equations yields solutions independently for every frequency or, in the time domain, at a given time through explicit time stepping. Because of this, frequency domain methods are rendered extremely time consuming for multi-frequency simulations. Likewise the stability conditions required by explicit time stepping techniques often result in highly inefficient calculations for large diffusion times and conductivity contrasts. The computation of sensitivities is carried out using the adjoint Green functions approach. For time domain applications, it is realized by convolution of the background electrical field information, originating from the primary signal, with the impulse response of the receiver acting as secondary source. In principle, the adjoint formulation may be extended allowing for a fast gradient calculation without calculating and storing the whole sensitivity matrix but just the gradient of the data residual. This technique, which is also known as migration, is widely used for seismic and, to some extend, for EM methods as well. However, the sensitivity matrix, which is not easily given by migration techniques, plays a central role in resolution analysis and would therefore be discarded ...
    Description: thesis
    Keywords: 550.28 ; 550 ; TQD 000 ; Elektrische Verfahren {Geophysik}
    Language: English
    Type: monograph , publishedVersion
    Format: 233 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 54
    Publication Date: 2021-03-29
    Description: Sedimentkerne aus zwei hocharktischen Seen (Duck und Hjort Lake) auf Store Koldewey, einer Insel auf Nordostgrönland, wurden auf ihre fossilen Chironomiden-Vergesellschaftungen untersucht. Im gesamten Holozän konnten 18 Chironomiden-Arten im Duck Lake und 21 im Hjort Lake identifiziert werden. Erste Chironomiden erscheinen im Hjort Lake bei ca. 9500 Kalenderjahre BP und ca. 500 Jahre später im Duck Lake. Für diese Periode wird in Ostgrönland eine signifikante Erwärmung angenommen. Jedoch bleiben die Abundanz und die Diversität der Chironomiden im Laufe des Frühholozäns in beiden Seen gering. Eine mögliche Ursache könnte der Einfluss der kalten, Meereis führenden Ostgrönlandströmung sein, welche vom Arktischen Ozean in Richtung Süden an Ostgrönland entlang verläuft. Der Beginn des Mittelholozäns wird durch eine steigende Abundanz von Chironomiden im Hjort Lake ab ca. 8000 Kalenderjahren BP und im Duck Lake ab ca. 6800 Kalenderjahren BP angezeigt. Die Chironomiden-Vergesellschaftung im Mittelholozän ähnelt derer von heutzutage leicht wärmeren Seen. Die zeitliche Verschiebung der Chironomiden-Vergesellschaftungen zwischen beiden Seen ist vermutlich auf Nährstoffschwankungen zurückzuführen. Eine wahrscheinlich höhere Schmelzwasserzufuhr in den Hjort Lake, aufgrund eines größeren Einzugsgebietes, führte diesem See möglicherweise mehr Nährstoffe als dem Duck Lake zu, wodurch sich die Chironomiden-Vergesellschaftungen im Hjort Lake vermutlich früher entfalten konnten ...
    Description: thesis
    Keywords: 560.179 ; 551.793 ; 560 ; TWC 500 ; TYY 100 ; VEY 110 ; VAU 000 ; VXP 000 ; VZY 110 ; VDI 220 ; VWI 200 ; Klimaschwankungen und Klimaänderungen im Quartär ; Arktis {Meteorologie und Klimatologie} ; Grönland {Geologie} ; Paläolimnologie {Geologie} ; Arthropoda {Paläozoologie} ; Grönland {Paläontologie} ; Holozän ; Quartär {Stratigraphische Paläontologie}
    Language: German
    Type: monograph , publishedVersion
    Format: 128 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 55
    Publication Date: 2021-03-29
    Description: The first major differentiation in primitive planetesimals is the formation of metal- or metal-sulfide cores. To constrain the time of asteroidal differentiation, meteoritic metals and silicates coexisting with metals were analyzed for Wisotopes and Hf and W concentrations. The study focused on silicate inclusions in non-magmatic IAB iron meteorites and the corresponding metal phases as well as on winonaites and acapulcoites were analyzed. IAB iron meteorites formed by crystallization of metal ponds under low pressure conditions at or near the surface of their asteroidal parent body. The presence of abundant silicate inclusions reflects either incomplete metal-silicate separation or mixing of metal and silicates by impacts. Hafnium-W measurements were performed on magnetic and non-magnetic separates from seven IAB iron meteorites to constrain the exact timing of metal separation, silicate differentiation and metamorphism. IAB metals have a deficit in 182W of - 3.1 ± 0.2 -units (relative to terrestrial standard materials)...
    Description: thesis
    Keywords: 523 ; TGG 900 ; TG 200 ; Planetoide {Astronomie} ; Kosmogonie des Sonnensystems {Astronomie}
    Language: English
    Type: monograph , publishedVersion
    Format: 118 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 56
    Publication Date: 2021-03-29
    Description: Der Einsatz geophysikalischer Verfahren zur Untersuchung von Altlasten hat in den letzten Jahren stark zugenommen. Durch Kombination verschiedener Verfahren einerseits und verschiedener Geo-Wissenschaften andererseits können solche Untersuchungen in ihrer Effizienz jedoch deutlich erhöht und Kosten drastisch reduziert werden. Zu diesem Zwecke wurde das EU-Altlastprojekt NORISC (’Network Oriented Risc assessment with In-situ Screening of Contaminated sites’) ins Leben gerufen. In den Jahren 2001 bis 2003 wurde unter der Federführung der Stadt Köln (Europabüro und Umweltamt) ein mehrteiliges Software-Paket entwickelt, welches sowohl Gutachtern im Feld als auch Umweltämtern und Ingenieurbüros zu Gute kommen soll. Dieses Paket enthält u.a. ein Werkzeug zur optimalen Methodenauswahl (DSS ’Decision Support System’) und ein 3D-Visualisierungswerkzeug (’GSI3D’) zur Darstellung aller gemessenen Parameter im Feld. Dieses Visualisierungswerkzeug wurde im Rahmen dieser Arbeit mit der Möglichkeit zur digitalen Bearbeitung geophysikalischer Daten (Inversion, Darstellung von Modellen und Rohdaten, Erstellung von Startmodellen) innerhalb des GIS Programms versehen, welches während der Projektphase noch nicht möglich war. So können nun geoelektrische und radiomagnetotellurische Daten mit geologischen und chemischen Informationen kalibriert werden, um dadurch ein genaueres Untergrundbild vor Ort zu erhalten. Weiterhin wurden Routinen zur Darstellung von 1D-, 2D- und 3D-Datensätzen implementiert, welche die Möglichkeiten der Visualsierung und Kalibration geophysikalischer Daten erweitern. Die während des Projekts gesammelten Daten wurden nach Abschluss der Erweiterung des GIS-Programms neu bearbeitet, um die Effizienz der eingebauten Module zu testen und zu verifizieren.
    Description: thesis
    Keywords: 628.55 ; 550.28 ; 550 ; TQ 000 ; Angewandte Geophysik
    Language: German
    Type: monograph , publishedVersion
    Format: 242 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 57
    Publication Date: 2021-03-29
    Description: Die Arbeit beschreibt Konzeption, Entwicklung, Aufbau und Betrieb eines generischen Informationsmodells in der Verwaltung der Stadt Köln. Das Modell ist praxiserprobt und in der Fachwelt bekannt. Einige Komponenten beginnen, sich als Standard für Geoinformationssysteme durchzusetzen. In seiner Gesamtheit ist das Modell einzigartig. Über Lizenzen findet es Verbreitung in Städten und Unternehmen. Teile waren immer wieder Richtungsgeber und Schrittmacher der technologischen Entwicklung. Der Verfasser, nach Konzeption, Entwicklung und Aufbau des Modells nun mit den nicht minder schwierigen Alltäglichkeiten des Betriebs befasst, schaut visionär voraus. Er sieht zusätzlich zur technischen Weiterentwicklung die Öffnung des bisher verwaltungsinternen Informationsmodells nach außen als erstrebenswert an. Informationsbeteiligung wäre nicht nur ein auch politikwirksames Zeichen modernen Verwaltungsmanagements, sondern sicherlich auch ein willkommener Beitrag zur wohlverstandenen Informationsgesellschaft. Ein generisches Informationsmodell kann flexibel auf raumbezogene Informations-wünsche reagieren. Allein Geodaten reichen dazu aber nicht aus; sie sind um Sach-daten aus den Verwaltungsverfahren zu ergänzen. Erst dadurch ist es möglich, die umfangreichen Datenschätze einer Kommunalverwaltung in Werte umzusetzen und für vielfältige geographische Fragestellungen zu nutzen. Als Grundlage des als Semantic Data Dictionary bezeichneten Informationsmodells war ein raumbezogenes Data Warehouse zu konzipieren, zu realisieren und aufzu-bauen. Das Besondere daran ist die Verbindung eines Spatial Data Warehouse mit einem Business Data Warehouse ...
    Description: thesis
    Keywords: 910
    Language: German
    Type: monograph , publishedVersion
    Format: 222 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 58
    Publication Date: 2021-03-29
    Description: This thesis had two primary objectives: One objective was to explore and develop applications of Fourier transform infrared spectroscopy (FTIRS) for the quantification of biogeochemical properties in lake sediment; the other objective was to assess the Lake Ohrid (Albania/Macedonia) sediment record with an emphasis on tephrostratigraphy and inferences of climatic and environmental changes using a 15 m long sediment succession (core Co1202) from the north-eastern part of the lake. Studies presented in this thesis were conducted within the scope of an envisaged deep drilling campaign at Lake Ohrid and therefore represent important preliminary studies. FTIR spectra of lacustrine sediment samples were calibrated to infer concentrations of total organic carbon (TOC), total inorganic carbon (TIC), total nitrogen (TN), and biogenic silica (BSi). To test the applicability of the FTIRS technique, site-specific FTIRS calibrations and FTIRS calibrations based on a surface sediment dataset from 94 northern Swedish lakes were constructed. Both approaches demonstrated significant correlations between FTIRS-inferred and conventionally assessed biogeochemical property concentrations, ranging between R2 = 0.79 0.99 for TOC, R2 = 0.85 0.99 for TIC, R2 = 0.62 0.84 for TN, and R2 = 0.68 0.94 for BSi ...
    Description: Zsfassung in dt. und engl. Sprache
    Description: thesis
    Keywords: 551 ; 551 ; 550 ; VKB 380 ; VAU 000 ; TWC 500 ; VEE 600 ; TQG 000 ; Sedimente bestimmter Regionen ; Paläolimnologie {Geologie} ; Klimaschwankungen und Klimaänderungen im Quartär ; Südosteuropa nach politischen Ländern {Geologie} ; Geophysikalische Bohrlochmessungen
    Language: English
    Type: monograph , publishedVersion
    Format: 147 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 59
    Publication Date: 2021-03-29
    Description: The focus of this thesis lies on the joint application of ground-based and airborne electromagnetic methods for the investigation of a glacial valley. For the first time two different airborne electromagnetic (AEM) surveying methods were employed to determine the resistivity structure of a single geological target: the frequency-domain helicopter-borne electromagnetic (HEM) system operated by the Federal Institute for Geosciences and Natural Resources (BGR), Germany, and the time-domain SkyTEM system developed at the University of Aarhus, Denmark. For verification of the airborne results, ground-based transient electromagnetics (TEM) and 2D resistivity surveying were also performed. The target survey area was the Cuxhaven valley in northern Germany, a significant local groundwater reservoir. The course of this buried valley was revealed by drillings, and the shape determined by reflection seismics along several transects across the valley. Electrical and electromagnetic methods were applied to investigate the structure of the valley fill, consisting of gravel, sand, silt and clay. Here, the extension and the thickness of clay layers are of particular interest. They have a low hydraulic permeability and often serve as protection for underlying aquifers against pollution from the surface ...
    Description: thesis
    Keywords: 550 ; TQD 000 ; TQH 000 ; TSB 000 ; Elektrische Verfahren {Geophysik} ; Aerogeophysik ; Mitteleuropa {Geophysik}
    Language: English
    Type: monograph , publishedVersion
    Format: 125 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 60
    Publication Date: 2021-03-29
    Description: In der vorliegenden Arbeit werden Ergebnisse von Messungen der Wind- und Turbulenzverhältnisse zwischen 30 und 100 m Höhe über See im Gebiet der Deutschen Bucht auf Basis von vier Jahren Daten präsentiert. Die mittleren gemessenen Größen der Windgeschwindigkeit (Jahresmittel 9,9 m/s in 90 m Höhe) und -richtung (Hauptwindrichtung aus West-Südwest) entsprechen im Wesentlichen den z. B. vom Bundesamt für Seeschifffahrt und Hydrografie (BSH) getroffenen Vorhersagen für diese Region. Erstmals konnten zusätzlich Vertikalprofile der Windgeschwindigkeit, der Turbulenzintensität, der extrapolierten Extremereignisse der Windgeschwindigkeit und anderer wichtiger Größen im Bereich zwischen dem unteren Ende der Rotorfläche (etwa 30 m) und der Nabenhöhe (etwa 90-100 m) der geplanten Offshore-Windkraftanlagen der 5 MW Klasse auf Basis eines mehrjährigen, qualitativ hochwertigen Datensatzes mit einer Höhenauflösung von 10 m für verschiedene Windgeschwindigkeitsbereiche und atmosphärische Stabilitätsverhältnisse bestimmt werden. Für einige der untersuchten Größen wurde auch die Abhängigkeit vom Wellenalter betrachtet. Der Vertikalgradient der Windgeschwindigkeit ist zwischen 30 und 100 m Höhe in den meisten Situationen vor allem aufgrund der geringen Oberflächenrauhigkeit über See deutlich geringer als über den meisten Landoberflächen ...
    Description: thesis
    Keywords: 333.7 ; TVK 100 ; TVK 700 ; ZHB 340 ; Windmessungen und Beobachtungsergebnisse im Allg. {Meteorologie} ; Windwirkungen {Meteorologie} ; Windenergie {Energietechnik}
    Language: German
    Type: monograph , publishedVersion
    Format: 126 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 61
    Publication Date: 2021-03-29
    Description: In this thesis I study the physical and chemical properties of molecular gas in star forming regions. This work takes advantage of the newly developed CONDOR receiver, which allows spectrally resolved observations of emission lines at frequencies of about 1.4 THz. Thus the thesis contains observational data obtained with CONDOR as well as observations motivated by the science one can do with receivers at terahertz frequencies are largely included. In the massive star forming region NGC 2024, seven emission lines of 12CO and 13CO have been observed, including 12CO J=13-12 (f=1.497 THz) observations with CONDOR. These high-J CO data reveal a thin layer of hot (~300 K) and dense (~10e6 cm-3) molecular gas, which has not been detected with any other tracer before. This newly discovered component is located at the interface between an HII region and the molecular cloud. Furthermore, the narrow line width indicates that this layer is heated by radiation rather than by shocks. On the background of well established physical scenarios, such as the ''Blister Model'' and the PDR scenario, I developed a model of NGC 2024, using radiative transfer computations. This model explains both, the spatial distribution of density and temperature along the line of sight and the velocity structure of the source...
    Description: Zsfassung in dt. und engl. Sprache
    Description: thesis
    Keywords: 523 ; TII 040 ; TEG 000 ; TJM 000 ; Physikalische Eigenschaften {Astronomie: Interstellare Materie} ; Kosmogonie {Astronomie} ; Kosmochemie {Weltraumforschung}
    Language: German
    Type: monograph , publishedVersion
    Format: 163 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 62
    Publication Date: 2021-03-29
    Description: Das nördliche Alpenvorland gilt als klassische Region der Quartärforschung. Hier wurde das System der quartären Eiszeiten anhand der Terrassenstratigraphie entwickelt (PENCK & BRÜCKNER 1901/1909). Die drei letzten Eiszeiten sind die Mindel-, die Riss- und die Würm-Eiszeit. Während das Alter der Vergletscherungen bis heute mit Sauerstoffisotopengehalten in marinen Sedimentbohrkernen korreliert wird, erlauben neuere Datierungsmethoden eine direkte Altersbestimmung der Sedimente. Ziel dieser Untersuchung war es, erstmals eine unabhängige Chronologie der quartären Schotterkörper im Alpenvorland mittels optischer Datierung zu erstellen. Dazu war eine detaillierte methodische Analyse der Lumineszenzeigenschaften der Proben notwendig. Die vergleichende Datierung der Quarz- und Feldspatfraktion derselben Probe diente der Validierung der Ergebnisse. Die Datierungsergebnisse weisen auf zeitlich voneinander zu unterscheidende Terrassenakkumulationen hin. Darüber hinaus haben die vielfältigen experimentellen Untersuchungen zu wichtigen neuen Erkenntnissen bezüglich des Lumineszenzverhaltens der Sedimente im Alpenvorland geführt, die in Zukunft zur Etablierung einer eigenständigen Chronologie der pleistozänen Ablagerungen im Alpenvorland genutzt werden können.
    Description: thesis
    Keywords: 551.701 ; VBN 500 ; VAR 912 ; Geochronologie einzelner Regionen im allgemeinen ; Alpenregion und Alpenvorland {Glazialgeologie}
    Language: German
    Type: monograph , publishedVersion
    Format: 222 S.
    Format: application/pdf
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 63
    Publication Date: 2017-07-18
    Description: The granule floatation is a serious issue of the anammox (anaerobic ammonium oxidation) process when high loading rates are applied that results in instability or even system collapse. The present study reports the granule floatation in an anammox reactor when high loading rates were applied. The comparison of enlarged photos taken for the settling and floating granules showed that the two kinds of granules both contained macroscopic gas pockets accounting for 11 +/- 14% of total volume. The settling granules had gas tunnels that could release the gas bubbles, while the floating granules did not. The presence of gas bubbles enclosed in the gas pockets led to the small density of 979.2 +/- 15.8 mg L(-1) and flotation of anammox granules. Consequently, the flotation caused washout of anammox granules and the deterioration of anammox process (volumetric removal rate decreased from 4.00 to 2.46 kg N m(-3) d(-1)). The collection of floating granules, breaking them into small pieces and then returning to the anammox reactor proved an effective control strategy. The volumetric removal rate was finally up to 16.5 kg N m(-3) d(-1) after the control strategy was put into use.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 64
    Publication Date: 2018-03-06
    Description: A geochemical proxy for surface ocean nutrient concentrations recorded in coral skeleton could provide new insight into the connections between sub-seasonal to centennial scale nutrient dynamics, ocean physics, and primary production in the past. Previous work showed that coralline P/Ca, a novel seawater phosphate proxy, varies synchronously with annual upwelling-driven cycles in surface water phosphate concentration. However, paired contemporaneous seawater phosphate time-series data, needed for rigorous calibration of the new proxy, were lacking. Here we present further development of the P/Ca proxy in Porites lutea and Montastrea sp. corals, showing that skeletal P/Ca in colonies from geographically distinct oceanic nutrient regimes is a linear function of seawater phosphate (PO4 SW) concentration. Further, high-resolution P/Ca records in multiple colonies of Pavona gigantea and Porites lobata corals grown at the same upwelling location in the Gulf of Panamá were strongly correlated to a contemporaneous time-series record of surface water PO4 SW at this site (r2 = 0.7–0.9). This study supports application of the following multi-colony calibration equations to down-core records from comparable upwelling sites, resulting in ±0.2 and ±0.1 μmol/kg uncertainties in PO4 SW reconstructions from P. lobata and P. gigantea, respectively. Inter-colony agreement in P/Ca response to PO4 SW was good (±5–12% about mean calibration slope), suggesting that species-specific calibration slopes can be applied to new coral P/Ca records to reconstruct past changes in surface ocean phosphate. However, offsets in the y-intercepts of calibration regressions among co-located individuals and taxa suggest that biologically-regulated “vital effects” and/or skeletal extension rate may also affect skeletal P incorporation. Quantification of the effect of skeletal extension rate on P/Ca could lead to corrected calibration equations and improved inter-colony P/Ca agreement. Nevertheless, the efficacy of the P/Ca proxy is thus supported by both broad scale correlation to mean surface water phosphate and regional calibration against documented local seawater phosphate variations.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 65
    Publication Date: 2018-06-26
    Description: We present the latest 3D velocity field of the Fennoscandian glacial isostatic adjustment (GIA) process from BIFROST. It is derived from more than 4800 days (13 years) of data at more than 80 permanent GPS sites. We use the GAMIT/GLOBK and the GIPSY/OASIS II software packages for GPS analysis and compare the results. The solution has an internal accuracy at the level of 0.2 mm/year (1 sigma) for horizontal velocities at the best sites. We also present a revised GIA prediction model. At the best sites, the optimal model agrees with the observations to within 0.4 mm/year. However, the model systematically overpredicts the magnitude of horizontal rates in the north. We discuss limitations in computed and presented GNSS station velocities, where especially possible instability over time causing non-linear pattern in vertical time series are considered. In extension, preliminary results from an investigation applying revised analysis strategies on a sparse subset of the database are presented, indicating possible improvements for the future.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 66
    Publication Date: 2018-03-08
    Description: The flow of groundwater beneath barrier islands has been cited as a possible pathway for salt water and chemical exchange between a protected embayment and the open sea. Evidence is presented that identifies an exchange of groundwater through a highly permeable paleoinlet along the barrier beach of Cavallino, which separates the northern Venice Lagoon from the Adriatic Sea. We utilized both point measurements of submarine groundwater discharge (SGD) and a geophysical investigation of the subsurface resistivity to analyze the movement of saline groundwater. Discharge of groundwater and associated nutrients, was higher at the site of a former inlet than at a similar site along the barrier and modulated by the difference in tidal water level between the lagoon and Adriatic Sea. If the measured conditions are typical, storm surge barriers could potentially result in a saline groundwater flow of up to 1.5×106 m3 d−1 into the lagoon.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 67
    Publication Date: 2017-11-24
    Description: Like other low-elevation passive margins, the French Atlantic margin is characterized by a gradual topographic transition from the coast to low-altitude interior plains or plateaus. Here we propose a morphostratigraphic analysis to constrain long-term landscape evolution and denudation rates, through the characterization of palaeotopographies and related palaeoweatherings in an area restricted to the southeast Armorican Massif. Two regional-scale palaeosurfaces are recognized: (i) the Infraliassic palaeosurface, the truncated weathering profiles of which are sealed by Liassic marine deposits; (ii) the Eocene palaeosurface, underlain by thick kaolinite- and iron-rich palaeosaprolites and by siliceous duricrusts (silcretes). Quantitative constraints on large-scale tectonic uplift and long-term denudation are obtained from these morphostratigraphic markers. Mean uplift and denudation rates calculated on post-Eocene times range between 0.5 and 2 m.Ma-1. These low values imply high landscape stability of the inland margin over most of the Cenozoic.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 68
    Publication Date: 2018-05-04
    Description: The objective of this study was to investigate the geochemical and hydrogeological effects of earthquakes on fluids in aquifers, particularly in a seismically active area such as Eskisehir (Turkey) where the Thrace–Eskisehir Fault Zone stretches over the region. The study area is also close to the North Anatolian Fault Zone generating devastating earthquakes such as the ones experienced in 1999, reactivating the Thrace–Eskisehir Fault. In the studied area, Rn and CO2 gas concentrations, redox potential, electrical conductivity, pH, water level, water temperature, and the climatic parameters were continuously measured in five stations for about a year. Based on the gathered data from the stations, some ambiguous anomalies in geochemical parameters and Rn concentration of groundwater were observed as precursors several days prior to an earthquake. According to the mid-term observations of this study, well-water level changes were found to be a good indicator for seismic estimations in the area, as it comprises naturally filtered anomalies reflecting only the changes due to earthquakes. Also, the results obtained from this study suggest that both the changes in well-water level and gas–water chemistry need to be interpretated together for more accurate estimations. Valid for the studied area, it can be said that shallow earthquakes with epicentral distances of 〈30 km from the observation stations have more influence on hydrochemical parameters of groundwater and well-water level changes. Although some hydrochemical anomalies were observed in the area, it requires further observations in order to be able to identify them as precursors.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 69
    facet.materialart.
    Unknown
    Elsevier
    In:  Journal of Environmental Radioactivity, 101 (7). pp. 519-520.
    Publication Date: 2018-03-08
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 70
    Publication Date: 2018-03-15
    Description: A novel flow injection ion chromatograph (FI-IC) system has been developed to fully automate pretreatment procedures for multi-elemental analysis of trace metals in seawater by inductively coupled plasma mass spectrometer (ICPMS). By combining 10-port, 2 position and 3-way valves in the FI-IC manifold, the system effectively increase sample throughput by simultaneously processing three seawater samples online for: sample loading, injection, buffering, preconcentration, matrix removal, metal elution, and sample collection. Forty-two seawater samples can be continuously processed without any manual handing. Each sample pretreatment takes about 10 min by consuming 25 mL of seawater and producing 5 mL of processed concentrated samples for multi-elemental offline analysis by ICPMS. The offline analysis improve analytical precision and significantly increase total numbers of isotopes determined by ICPMS, which include the metals Al, Cd, Co, Cr, Cu, Fe, Mn, Ni, Pb, Ti, V, and Zn. The blank value and detection limits of trace metals using the system with ICPMS analysis all range from 0.1 to 10 parts per trillion (ppt), except Al, Fe, and Zn. The accuracy of the pretreatment system was validated by measuring open-ocean and coastal reference seawater, NASS-5 and CASS-4. Using the system with ICPMS analysis, we have obtained reliable trace metal concentrations in the water columns of the South China Sea. Possessing the features of full automation, high throughput, low blank, and low reagent volume used, the system automates and simplifies rigorous and complicated pretreatment procedures for multi-elemental analysis of trace metals in seawater and effectively enhances analytical capacity for trace metal analysis in environmental and seawater samples.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 71
    facet.materialart.
    Unknown
    Elsevier
    In:  Geochimica et Cosmochimica Acta, 74 (23). pp. 6801-6813.
    Publication Date: 2017-03-09
    Description: Copper and Zn metals are produced in large quantities for different applications. During Cu production, large amounts of Cu and Zn can be released to the environment. Therefore, the surroundings of Cu smelters are frequently metal-polluted. We determined Cu and Zn concentrations and Cu and Zn stable isotope ratios (δ65Cu, δ66Zn) in three soils at distances of 1.1, 3.8, and 5.3 km from a Slovak Cu smelter and in smelter wastes (slag, sludge, ash) to trace sources and transport of Cu and Zn in soils. Stable isotope ratios were measured by multicollector inductively coupled plasma mass spectrometry (MC-ICP-MS) in total digests. Soils were heavily contaminated with concentrations up to 8087 μg g−1 Cu and 2084 μg g−1 Zn in the organic horizons. The δ65Cu values varied little (−0.12‰ to 0.36‰) in soils and most wastes and therefore no source identification was possible. In soils, Cu became isotopically lighter with increasing depth down to 0.4 m, likely because of equilibrium reactions between dissolved and adsorbed Cu species during transport of smelter-derived Cu through the soil. The δ66ZnIRMM values were isotopically lighter in ash (−0.41‰) and organic horizons (−0.85‰ to −0.47‰) than in bedrock (−0.28‰) and slag (0.18‰) likely mainly because of kinetic fractionation during evaporation and thus allowed for separation of smelter-Zn from native Zn in soil. In particular in the organic horizons large variations in δ66Zn values occur, probably caused by biogeochemical fractionation in the soil–plant system. In the mineral horizons, Zn isotopes showed only minor shifts to heavier δ66Zn values with depth mainly because of the mixing of smelter-derived Zn and native Zn in the soils. In contrast to Cu, Zn isotope fractionation between dissolved and adsorbed species was probably only a minor driver in producing the observed variations in δ66Zn values. Our results demonstrate that metal stable isotope ratios may serve as tracer of sources, vertical dislocation, and biogeochemical behavior in contaminated soil.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 72
    facet.materialart.
    Unknown
    Elsevier
    In:  Precambrian Research, 183 (1). pp. 44-49.
    Publication Date: 2020-06-10
    Description: The sensitive high-resolution ion microprobe (SHRIMP) developed at the Australian National University (ANU) was the first of the high-resolution ion microprobes. The impact of this instrument on geochronological research over the last twenty years has been immense. This is particularly so for lunar geochronology where it has opened up avenues of research that were not possible using conventional TIMS techniques. The great advantage of SHRIMP is that it provides a means for determining precise U–Pb isotopic ratios on selected micron-size areas on polished grains of zircon and other U-bearing minerals. One of the first projects undertaken on the newly invented SHRIMP I was an investigation of U–Pb ages of lunar zircon. Using SHRIMP, multiple analyses could be made on areas of individual zircons to test the stability of U–Pb systems in shocked grains. Also, by analysing grains “in situ”, textural relationships between the analysed zircon and the components of the sample breccia could be used in the interpretation of the SHRIMP data. As a result of this research it was realised that most lunar zircons have ages up to 500Ma older than the Imbrium and Serenitatis impacts at ca. 3.9 Ga, demonstrating that the zircons have not been affected by the these impact events although heating and shock effects have profoundly disturbed other dating systems. This has opened the way for research into the early lunar magmatic and bombardment record. For example, recent SHRIMP results have revealed profound differences in the ages of zircons from breccias from the Apollo 14 and Apollo 17 sample sites, raising new questions about the evolution of lunar magmatism. Also, multiple SHRIMP analyses on complex lunar zircons have shown that these grains can record U–Pb disturbance by later impact events. SHRIMP U–Pb age determinations on phosphates in lunar meteorites has identified lunar events not recognised in samples from the Apollo program. SHRIMP-based research on lunar materials is ongoing and, in combination with other chemical and structural evidence, continues to stimulate new ideas on the early evolution of the Moon.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 73
    Publication Date: 2018-03-08
    Description: Geochemical cycles occurring at the interface between terrestrial and marine groundwaters, in the so-called subterranean estuary (STE), are not well understood for most elements. This is particularly true of the transition metals, many of which have particular ecological relevance as micronutrients or toxicants. To gain a first approximation of trace metal geochemistry in the mixing zone, we examined the distribution of nine dissolved metals (Fe, Mn, Mo, V, Co, Ni, Cu, Pb, and Al) through a shallow STE in Great South Bay, New York, USA. We also performed a simple kinetic and chemical separation of labile and organic-complexed metal species in the STE. Dissolved Mn showed marked subsurface enrichment (up to 755 µM at 15 cm depth) that was suggestive of diagenetic remobilization. Dissolved Fe, however, was higher by more than three orders-of-magnitude in fresh groundwater (90 µM) as compared to marine groundwater (0.02 µM), and pH-mediated removal was evident as slightly acidic fresh groundwater (pH 6.8) mixed with marine groundwater (pH ∼ 8.0). Dissolved Mo, Co, and Ni were primarily cycled with Mn, and highly elevated concentrations relative to bay surface waters (up to 300, 75, and 44 nM, respectively) were observed in the STE. High levels of dissolved Pb (up to 4250 pM) observed in the fresh groundwater were nearly quantitatively removed within the salinity mixing zone, in conjunction with marked reduction of dissolved Al. Dissolved Cu exhibited non-conservative removal throughout the STE, and was correlated with the redox potential of the porewaters. Substantial percentages (〉 15%) of organic-metal species were only observed for Cu and Ni, suggesting that these complexes were not generally very important for metal cycling in the STE. Kinetically labile species were observed for all metals examined except Cu and Pb, and represented an approximately constant proportion (between 10% and 70%) of the total dissolved pool for each metal, indicating equilibrium between labile and non-labile species throughout the mixing zone. The non-conservative behavior observed for all metals examined in this study suggests that reactions occurring in the STE are vastly important to the source/sink function of permeable sediments, and studies seeking to quantify SGD-derived trace metal fluxes must take into account biogeochemical processes occurring in the subterranean estuary.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 74
    Publication Date: 2018-03-08
    Description: Ra isotopes are a powerful tool for quantifying the flux of submarine groundwater discharge (SGD) into the sea. Previous studies of 223Ra and 224Ra mass balances in coastal embayments have shown that the Ra balance is dominated by supply via SGD, exchange with the open ocean and radioactive decay. The current study shows that a single time series over a tidal cycle at the principal inlet to Great South Bay (NY, US) is sufficient to determine the net flux of Ra across the inlet, and also can be used to estimate the decay of short-lived Ra in the bay. Estimates of the net Ra flux obtained from a single tidal time-series by using three different approaches agree with those determined from a more time-consuming survey of Ra within the bay, and may represent a first step of estimating SGD in bays and coastal lagoons.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 75
    Publication Date: 2017-12-04
    Description: Core PRAD 1-2, located on the western flank of the Mid-Adriatic Deep, contains a continuous sediment record extending back to upper MIS-11. The upper part of the record which spans the mid Holocene to MIS 5–4 (the last ca 105,000 years) has been investigated for tephra content. A total of 25 discrete tephra layers were discovered, only one of which was visible in the core sequence. The other 24 are not visible to the naked eye, nor were the majority detected by routine down-core scanning methods. A total of 625 geochemical measurements obtained from individual glass shards using WDS-EPMA enabled 21 of the 25 tephras to be assigned to known volcanic events emanating from the Campanian Province (Campi Flegrei, Somma-Vesuvius and Ischia Island). The results provide an independent basis for establishing an age–depth profile for the upper part of the PRAD 1-2 record. This study demonstrates that the number of non-visible tephra layers can significantly exceed the number of visible layers in some deep marine sequences. Routine testing for the presence of non-visible tephra layers can therefore prove rewarding, leading to the detection of additional isochrons for dating and correlating marine sequences, and for their synchronisation with terrestrial records.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 76
    facet.materialart.
    Unknown
    Elsevier
    In:  Geochimica et Cosmochimica Acta, 74 (13). pp. 3735-3750.
    Publication Date: 2018-02-22
    Description: Calcium isotopes in tissues are thought to be influenced by an individual’s diet, reflecting parameters such as trophic level and dairy consumption, but this has not been carefully assessed. We report the calcium isotope ratios (δ44/42Ca) of modern and archaeological animal and human bone (n = 216). Modern sheep raised at the same location show 0.14 ± 0.08‰ higher δ44/42Ca in females than in males, which we attribute to lactation by the ewes. In the archaeological bone samples the calcium isotope ratios of the herbivorous fauna vary by location. At a single site, the archaeological fauna do not show a trophic level effect. Humans have lower δ44/42Ca than the mean site fauna by 0.22 ± 0.22‰, and the humans have a greater δ44/42Ca range than the animals. No effect of sex or age on the calcium isotope ratios was found, and intra-individual skeletal δ44/42Ca variability is negligible. We rule out dairy consumption as the main cause of the lower human δ44/42Ca, based on results from sites pre-dating animal domestication and dairy availability, and suggest instead that individual physiology and calcium intake may be important in determining bone calcium isotope ratios.
    Type: Article , PeerReviewed
    Format: text
    Format: text
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 77
    Publication Date: 2017-08-07
    Description: Porangahau Ridge, located offshore the Wairarapa on the Hikurangi Margin, is an active ocean-continent collision region in northeastern New Zealand coastal waters. Bottom simulating reflections (BSRs) in seismic data indicate the potential for significant gas hydrate deposits across this part of the margin. Beneath Porangahau Ridge a prominent high-amplitude reflection band has been observed to extend from a deep BSR towards the seafloor. Review of the seismic data suggest that this high-amplitude band is caused by local shoaling of the base of gas hydrate stability due to advective heat flow and it may constitute the location of elevated gas hydrate concentrations. During R/V Tangaroa cruise TAN0607 in 2006 heat flow probing for measurements of vertical fluid migration, sediment coring for methane concentrations, and additional seismic profiles were obtained across the ridge. In a subsequent 2007 expedition, on R/V Sonne cruise SO191, a controlled source electromagnetic (CSEM) experiment was conducted along the same seismic, geochemical, and heat flow transect to reveal the electrical resistivity distribution. CSEM data highlight a remarkable coincidence of anomalously high resistivity along the western, landward flank of the ridge which point to locally higher gas hydrate concentration above the high amplitude reflection band. Measured sediment temperature profiles, also along the western flank, consistently show non-linear and concave geothermal gradients typical of advective heat flow. Geochemical data reveal elevated methane concentrations in surface sediments concomitant with a rapid decline in sulfate concentrations indicating elevated methane flux and oxidation of methane in conjunction with sulfate reduction at the landward ridge base. Together, these data sets suggest that the western rim of Porangahau Ridge is a tectonically driven zone of rising fluids that transport methane and cause an upward inflection of the base of gas hydrate stability and the formation of locally enriched gas hydrate above the reflective zone.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 78
    Publication Date: 2016-09-19
    Description: The relationship of sea-level changes and short-term climatic changes with turbidite deposition is poorly documented, although the mechanisms of gravity-driven sediment transport in submarine canyons during sea-level changes have been reported from many regions. This study focuses on the activity of the Dakar Canyon off southern Senegal in response to major glacial/interglacial sea-level shifts and variability in the NW-African continental climate. The sedimentary record from the canyon allows us to determine the timing of turbidite events and, on the basis of XRF-scanning element data, we have identified the climate signal at a sub-millennial time scale from the surrounding hemipelagic sediments. Over the late Quaternary the highest frequency in turbidite activity in the Dakar Canyon is confined to major climatic terminations when remobilisation of sediments from the shelf was triggered by the eustatic sea-level rise. However, episodic turbidite events coincide with the timing of Heinrich events in the North Atlantic. During these times continental climate has changed rapidly, with evidence for higher dust supply over NW Africa which has fed turbidity currents. Increased aridity and enhanced wind strength in the southern Saharan–Sahelian zone may have provided a source for this dust.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 79
    Publication Date: 2020-03-24
    Description: Vertical distributions of iron and iron binding ligands were determined in 2 size classes (dissolved 〈 0.2 μm, soluble 〈 200 kDa, e.g., ~ 0.03 μm) in the Southern Ocean. Colloidal iron and complexing capacity (〉 200 kDa–〈 0.2 μm) were inferred as the difference between the dissolved and soluble fractions. Dissolved iron and ligands exist primarily in the soluble size range in the surface waters, although iron-complexing colloids still represent a significant portion of the dissolved pool and this fraction increases markedly with depth. This work presents evidence for the colloidal nature of a significant portion (37–51% on average) of the ‘dissolved’ organic Fe pool in these oceanic waters. From the data it was not possible to discern whether iron colloids exist as discrete organic complexes and/or inorganic amorphous colloids. Iron-complexing colloids are the most saturated with iron at the thermodynamic equilibrium, whereas soluble organic ligands occur in larger excess compared to soluble iron. It suggests that the exchangeable fraction for iron uptake through dissociation of Fe complexes likely occurs in the soluble fraction, and that soluble ligands have the potential to buffer iron inputs to surface waters whereas iron colloids may aggregate and settle. Expectations based on Fe diffusion rates, distributions and the stability of the soluble iron complexes and iron colloids also suggest that the weaker soluble Fe complexes may be more bio-available, while the strongest colloids may be a major route for iron removal from oceanic waters. Investigations of the size classes of the dissolved organic iron thus can significantly increase our understanding of the oceanic iron cycle.
    Type: Article , PeerReviewed
    Format: text
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 80
    Publication Date: 2017-09-27
    Description: Accurate constraints on past ocean temperatures and compositions are critical for documenting climate change and resolving its causes. Most proxies for temperature are not thermodynamically based, appear to be subject to biological processes, require regional calibrations, and/or are influenced by fluid composition. As a result, their interpretation becomes uncertain when they are applied in settings not necessarily resembling those in which they were empirically calibrated. Independent proxies for past temperature could provide an important means of testing and/or expanding on existing reconstructions. Here we report measurements of abundances of stable isotopologues of calcitic and aragonitic benthic and planktic foraminifera and coccoliths, relate those abundances to independently estimated growth temperatures, and discuss the possible scope of equilibrium and kinetic isotope effects. The proportions of 13C–18O bonds in these samples exhibits a temperature dependence that is generally similar to that previously been reported for inorganic calcite and other biologically precipitated carbonatecontaining minerals (apatite from fish, reptile, and mammal teeth; calcitic brachiopods and molluscs; aragonitic coral and mollusks). Most species that exhibit non-equilibrium 18O/16O (d18O) and 13C/12C (δ13C) ratios are characterized by 13C–18O bond abundances that are similar to inorganic calcite and are generally indistinguishable from apparent equilibrium, with possible exceptions among benthic foraminiferal samples from the Arctic Ocean where temperatures are near-freezing. Observed isotope ratios in biogenic carbonates can be explained if carbonate minerals generally preserve a state of ordering that reflects the extent of isotopic equilibration of the dissolved inorganic carbon species.
    Type: Article , PeerReviewed
    Format: text
    Format: text
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 81
    Publication Date: 2013-05-15
    Description: Climate-dependent chemical weathering trends have a strong impact on the dissolved Pb isotopic composition of continental runoff during glacial terminations, so that this tracer can be used to reconstruct the impact of the North American deglaciation on aspects of freshwater runoff and ocean chemistry. Here we present authigenic Fe–Mn oxyhydroxide-derived Pb isotope records from lower Laurentian Fan sediments that trace the local deglacial continental runoff signal through the Gulf of St. Lawrence. We use these records to investigate changes in the Pb isotopic composition of the North American runoff, and their relationship to deglacial processes. The new Pb isotope records are very similar to those from the subtropical deep NW Atlantic locations, though the new data are at higher resolution and exhibit much greater amplitudes of change due to their Laurentide Ice Sheet-proximal setting. Unradiogenic compositions (206Pb/204Pb as low as 18.8 at 18.5 ka) during the latest glacial change towards highly radiogenic compositions during the early Holocene (206Pb/204Pb = 20.1 at 11.2 ka). Late Holocene 206Pb/204Pb values return to intermediate values around 206Pb/204Pb = 19.6. These new data support previous inferences that the Pb isotopic composition of the deep Atlantic is controlled during deglaciation by changes in the pattern and intensity of continental chemical weathering. In more detail, the most significant change in the entire Pb isotope record starts at 12.5 ka and lasts until about 11 ka. This observation, of strong Pb isotopic changes across a climatically cold period in the North Atlantic region, suggests that at this location Pb isotopic compositions recorded in deep marine authigenic Fe–Mn oxyhydroxides not only trace deglacial changes in chemical weathering intensity but also highly depend on major freshwater runoff routes in interior North America. Our data suggest a gradual opening of the eastward freshwater runoff route in the course of the Younger Dryas.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 82
    Publication Date: 2017-08-08
    Description: Many biological seep studies focused on the distribution, structure, nutrition and food web architecture of seep communities as well as on their interaction with the seep geochemistry. However, overall respiration at cold seeps received only little attention. We conducted in-situ oxygen flux measurements in combination with ex-situ oxygen micro-profiles, respiration measurements, as well as rate determinations of microbial methane and sulfate turnover to assess respiration pathways as well as carbon turnover at a seep habitat that was recently discovered alongside the Hikurangi Margin offshore northern New Zealand. This habitat is dominated by dense beds of tube-building, heterotrophic ampharetid polychaetes. Average total oxygen uptake (TOU) from this habitat was very high (83.7 mmol m− 2 day− 1). TOU at a non-seep reference site ranged between 2.7 and 5.8 mmol m− 2 day− 1. About 37% (30.8 mmol m− 2 day− 1) of the average TOU was consumed by ampharetids. Considering mean diffusive oxygen uptake (8.5 mmol m− 2 day− 1) the remaining fraction of ~ 53% of the TOU (44.4 mmol m− 2 day− 1) might be explained by respiration of epibenthic organisms as well as aerobic methane and sulfide oxidation at the sediment–water interface. The strongly negative carbon isotopic signatures (− 52.9 ± 5‰ VPDB) of the ampharetid tissues indicate a methane derived diet. However, carbon production via anaerobic oxidation of methane (AOM) was too low (0.1 mmol C m− 2 day− 1) to cover the mean carbon demand of the ampharetid communities (21 mmol C m− 2 day− 1). Likely, organic carbon generated via aerobic methane oxidation represents their major carbon source. This is in contrast to other seep habitats, where energy bound in methane is partly transferred to sulfide via AOM and finally consumed by sulfide-oxidizing chemoautotrophs providing carbon that subsequently enters the benthic food web.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 83
    Publication Date: 2019-09-23
    Description: Estimating the magnitude of Agulhas leakage, the volume flux of water from the Indian to the Atlantic Ocean, is difficult because of the presence of other circulation systems in the Agulhas region. Indian Ocean water in the Atlantic Ocean is vigorously mixed and diluted in the Cape Basin. Eulerian integration methods, where the velocity field perpendicular to a section is integrated to yield a flux, have to be calibrated so that only the flux by Agulhas leakage is sampled. Two Eulerian methods for estimating the magnitude of Agulhas leakage are tested within a high-resolution two-way nested model with the goal to devise a mooring-based measurement strategy. At the GoodHope line, a section halfway through the Cape Basin, the integrated velocity perpendicular to that line is compared to the magnitude of Agulhas leakage as determined from the transport carried by numerical Lagrangian floats. In the first method, integration is limited to the flux of water warmer and more saline than specific threshold values. These threshold values are determined by maximizing the correlation with the float-determined time series. By using the threshold values, approximately half of the leakage can directly be measured. The total amount of Agulhas leakage can be estimated using a linear regression, within a 90% confidence band of 12 Sv. In the second method, a subregion of the GoodHope line is sought so that integration over that subregion yields an Eulerian flux as close to the float-determined leakage as possible. It appears that when integration is limited within the model to the upper 300 m of the water column within 900 km of the African coast the time series have the smallest root-mean-square difference. This method yields a root-mean-square error of only 5.2 Sv but the 90% confidence band of the estimate is 20 Sv. It is concluded that the optimum thermohaline threshold method leads to more accurate estimates even though the directly measured transport is a factor of two lower than the actual magnitude of Agulhas leakage in this model.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 84
    Publication Date: 2020-10-21
    Description: Here we present the first radiometric age data and a comprehensive geochemical data set (including major and trace element and Sr–Nd–Pb–Hf isotope ratios) for samples from the Hikurangi Plateau basement and seamounts on and adjacent to the plateau obtained during the R/V Sonne 168 cruise, in addition to age and geochemical data from DSDP Site 317 on the Manihiki Plateau. The 40Ar/39Ar age and geochemical data show that the Hikurangi basement lavas (118–96 Ma) have surprisingly similar major and trace element and isotopic characteristics to the Ontong Java Plateau lavas (ca. 120 and 90 Ma), primarily the Kwaimbaita-type composition, whereas the Manihiki DSDP Site 317 lavas (117 Ma) have similar compositions to the Singgalo lavas on the Ontong Java Plateau. Alkalic, incompatible-element-enriched seamount lavas (99–87 Ma and 67 Ma) on the Hikurangi Plateau and adjacent to it (Kiore Seamount), however, were derived from a distinct high time-integrated U/Pb (HIMU)-type mantle source. The seamount lavas are similar in composition to similar-aged alkalic volcanism on New Zealand, indicating a second wide-spread event from a distinct source beginning ca. 20 Ma after the plateau-forming event. Tholeiitic lavas from two Osbourn seamounts on the abyssal plain adjacent to the northeast Hikurangi Plateau margin have extremely depleted incompatible element compositions, but incompatible element characteristics similar to the Hikurangi and Ontong Java Plateau lavas and enriched isotopic compositions intermediate between normal mid-ocean-ridge basalt (N-MORB) and the plateau basement. These younger (not, vert, similar52 Ma) seamounts may have formed through remelting of mafic cumulate rocks associated with the plateau formation. The similarity in age and geochemistry of the Hikurangi, Ontong Java and Manihiki Plateaus suggest derivation from a common mantle source. We propose that the Greater Ontong Java Event, during which not, vert, similar1% of the Earth’s surface was covered with volcanism, resulted from a thermo-chemical superplume/dome that stalled at the transition zone, similar to but larger than the structure imaged presently beneath the South Pacific superswell. The later alkalic volcanism on the Hikurangi Plateau and the Zealandia micro-continent may have been part of a second large-scale volcanic event that may have also triggered the final breakup stage of Gondwana, which resulted in the separation of Zealandia fragments from West Antarctica.
    Type: Article , PeerReviewed
    Format: text
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 85
    Publication Date: 2019-01-24
    Description: Three novel natural products, sorbifuranones A–C (4–6), were isolated from a Penicillium chrysogenum fungus isolated from the marine sponge Ircinia fasciculata. Sorbifuranones B (5) and C (6) and 2′,3′-dihydrosorbicillin, a putative precursor to sorbifuranone B, were also found in the culture of another Penicillium strain, which was isolated from the sponge Tethya aurantium. Their constitutions were elucidated mainly by 2D NMR. NOE correlations in combination with quantum chemical calculations and comparison of experimental and calculated electronic circular dichroism (CD) spectra permitted assignment of the absolute configuration of sorbifuranone C. The structures hint at a two-step cleavage-cyclization sequence of sorbifuranone A (4) leading to the spiro compound sorbifuranone C, while sorbifuranone B is likely to be the respective cleavage product of a putative 2′,3′-dihydrosorbifuranone A, which cannot cyclize further.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 86
    facet.materialart.
    Unknown
    Elsevier
    In:  Comparative Biochemistry and Physiology Part B: Biochemistry and molecular biology, 155 (4). pp. 413-418.
    Publication Date: 2020-08-04
    Description: Thermal tolerance was determined in two closely related amphipod species from contrasting environments (sub-littoral and supra-littoral zones of the sea) using HSP expression and the activity of antioxidant enzymes. The levels of HSP70 and small HSPs present in untreated control animals were higher in the supra-littoral Orchestia gammarellus than in the sub-littoral Gammarus oceanicus. Under the acute thermal stress, HSP levels increased less strongly in O. gammarellus than in G. oceanicus. Activities of antioxidant enzymes peroxidase, catalase and glutathione S-transferase, were more pronounced in the supra-littoral O. gammarellus then in the sub-littoral G. oceanicus. We conclude that the environmental temperature regime modifies key cellular defense mechanisms in amphipods. Higher levels of constitutive HSP synthesis and higher levels of antioxidant enzymes in the supra-littoral species likely reflects adaptation to this highly thermally variable environment.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 87
    Publication Date: 2020-07-09
    Description: We present recently-acquired high-resolution seismic data and older lower-resolution seismic data from Rock Garden, a shallow marine gas hydrate province on New Zealand's Hikurangi Margin. The seismic data reveal plumbing systems that supply gas to three general sites where seeps have been observed on the Rock Garden seafloor: the ‘LM3’ sites (including LM3 and LM3-A), the ‘Weka’ sites (including Weka-A, Weka-B, and Weka-C), and the ‘Faure’ sites (including Faure-A, Faure-B, and Rock Garden Knoll). At the LM3 sites, seismic data reveal gas migration from beneath the bottom simulating reflection (BSR), through the gas hydrate stability zone (GHSZ), to two separate seafloor seeps (LM3 and LM3-A). Gas migration through the deeper parts of GHSZ below the LM3 seeps appears to be influenced by faulting in the hanging wall of a major thrust fault. Closer to the seafloor, the dominant migration pathways appear to occupy vertical chimneys. At the Weka sites, on the central part of the ridge, seismic data reveal a very shallow BSR. A distinct convergence of the BSR with the seafloor is observed at the exit point of one of the Weka seep locations (Weka-A). Gas supply to this seep is predicted to be focused along the underside of a permeability contrast at the BGHS caused by overlying gas hydrates. The Faure sites are associated with a prominent arcuate slump feature. At Faure-A, high-amplitude reflections, extending from a shallow BSR towards the seafloor, are interpreted as preferred gas migration pathways that exploit relatively-high-permeability sedimentary layers. At Faure-B, we interpret gas migration to be channelled to the seep along the underside of the BGHS — the same scenario interpreted for the Weka-A site. At Rock Garden Knoll, gas occupies shallow sediments within the GHSZ, and is interpreted to migrate up-dip along relatively high-permeability layers to the area of seafloor seepage. We predict that faulting, in response to uplift and flexural extension of the ridge, may be an important mechanism in creating fluid flow conduits that link the reservoir of free gas beneath the BGHS with the shallow accumulations of gas imaged beneath Rock Garden Knoll. From a more regional perspective, much of the gas beneath Rock Garden is focused along a northwest-dipping fabric, probably associated with subduction-related deformation of the margin.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 88
    Publication Date: 2017-08-07
    Description: The southern Hikurangi Subduction Margin is characterized by significant accretion with predicted high rates of fluid expulsion. Bottom simulating reflections (BSRs) are widespread on this margin, predominantly occurring beneath thrust ridges. We present seismic data across the Porangahau Ridge on the outer accretionary wedge. The data show high-amplitude reflections above the regional BSR level. Based on polarity and reflection strength, we interpret these reflections as being caused by free gas. We propose that the presence of gas above the regional level of BSRs indicates local upwarping of the base of gas hydrate stability caused by advective heatflow from upward migrating fluids, although we cannot entirely rule out alternative processes. Simplified modelling of the increase of the thermal gradient associated with fluid flow suggests that funnelling of upward migrating fluids beneath low-permeability slope basins into the Porangahau Ridge would not lead to the pronounced thermal anomaly inferred from upwarping of the base of gas hydrate stability. Focussing of fluid flow is predicted to take place deep in the accretionary wedge and/or the underthrust sediments. Above the high-amplitude reflections, sediment reflectivity is low. A lack of lateral continuity of reflections suggests that reflectivity is lost because of a destruction of sediment layering from deformation rather than gas-hydrate-related amplitude blanking. Structural permeability from fracturing of sediments during deformation may facilitate fluid expulsion on the ridge. A gap in the BSR in the southern part of the study area may be caused by a loss of gas during fluid expulsion. We speculate that gaps in otherwise continuous BSRs that are observed beneath some thrusts on the Hikurangi Margin may be characteristic of other locations experiencing focussed fluid expulsion.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 89
    Publication Date: 2017-08-08
    Description: The imbricated frontal wedge of the central Hikurangi subduction margin is characteristic of wide (ca. 150 km), poorly drained and over pressured, low taper (not, vert, similar 4°) thrust systems associated with a relatively smooth subducting plate, a thick trench sedimentary sequence (not, vert, similar 3–4 km), weak basal décollement, and moderate convergence rate (not, vert, similar 40 mm/yr). New seismic reflection and multibeam bathymetric data are used to interpret the regional tectonic structures, and to establish the geological framework for gas hydrates and fluid seeps. We discuss the stratigraphy of the subducting and accreting sequences, characterize stratigraphically the location of the interplate décollement, and describe the deformation of the upper plate thrust wedge together with its cover sequence of Miocene to Recent shelf and slope basin sediments. We identify approximately the contact between an inner foundation of deforming Late Cretaceous and Paleogene rocks, in which widespread out-of-sequence thrusting occurs, and a 65–70 km-wide outer wedge of late Cenozoic accreted turbidites. Although part of a seamount ridge is presently subducting beneath the deformation front at the widest part of the margin, the morphology of the accretionary wedge indicates that frontal accretion there has been largely uninhibited for at least 1–2 Myr. This differs from the offshore Hawkes Bay sector of the margin to the north where a substantial seamount with up to 3 km of relief has been subducted beneath the lower margin, resulting in uplift and complex deformation of the lower slope, and a narrow (10–20 km) active frontal wedge. Five areas with multiple fluid seep sites, referred to informally as Wairarapa, Uruti Ridge, Omakere Ridge, Rock Garden, and Builders Pencil, typically lie in 700–1200 m water depth on the crests of thrust-faulted, anticlinal ridges along the mid-slope. Uruti Ridge sites also lie in close proximity to the eastern end of a major strike-slip fault. Rock Garden sites lie directly above a subducting seamount. Structural permeability is inferred to be important at all levels of the thrust system. There is a clear relationship between the seeps and major seaward-vergent thrust faults, near the outer edge of the deforming Cretaceous and Paleogene inner foundation rocks. This indicates that thrust faults are primary fluid conduits and that poor permeability of the Cretaceous and Paleogene inner foundation focuses fluid flow to its outer edge. The sources of fluids expelling at active seep sites along the middle slope may include the inner parts of the thrust wedge and subducting sediments below the décollement. Within anticlinal ridges beneath the active seep sites there is a conspicuous break in the bottom simulating reflector (BSR), and commonly a seismically-resolvable shallow fault network through which fluids and gas percolate to the seafloor. No active fluid venting has yet been recognized over the frontal accretionary wedge, but the presence of a widespread BSR, an extensive protothrust zone (〉 200 km by 20 km) in the Hikurangi Trough, and two unconfirmed sites of possible previous fluid expulsion, suggest that the frontal wedge could be actively dewatering. There are presently no constraints on the relative fluid flux between the frontal wedge and the active mid-slope fluid seeps. Article Outline
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 90
    Publication Date: 2016-11-01
    Description: Understanding the upward motion of CO2 droplets or CH4 bubbles in oceanic waters is prerequisite to predict the vertical distribution of the two most important greenhouse gases in the water column after these have been released from the seabed. One of the key parameters governing the fate of droplets or bubbles dissolving into the surrounding seawater as they rise, is the terminal velocity, uT. The latter is strongly influenced by the ability of both compounds to form skins of gas hydrate, if pressure and temperature satisfy thermodynamic framework conditions. Experimental efforts aiming to elucidate the rise properties of CO2 droplets and CH4 bubbles and specifically the influence of hydrate skins open the possibility to obtain a parameterization of uT applicable to both hydrate-coated and pure fluid particles of CH4 and CO2. With the present study, we report on experimentally determined terminal velocities of single CH4 bubbles released to pressurized and temperature-regulated seawater. Hydrate skins were identified by high bubble sphericities and changed motion characteristics. Based on these experiments as well as published data on the rise of hydrate-coated and pure liquid CO2 droplets and physical principles previously successfully used for clean bubbles near atmospheric pressures, a new parameterization of uT is proposed. Model predictions show a good agreement with the data base established from the laboratory-based measurements.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 91
    Publication Date: 2017-02-21
    Description: This paper presents magnetic fabric analysis to examine the internal structure of the accretionary prism toe in the Nankai Trough, off the east coast of Japan. Two sites (C0006 and C0007) drilled during Integrated Ocean Drilling Program (IODP) Expedition 316 penetrated the sediment section, including intra wedge thrusts and the frontal thrust. Anisotropy of magnetic susceptibility (AMS) measurements provides insight into recorded strain during sedimentary and tectonic processes. Results from the upper part of the wedge show sedimentary acquired compaction fabric in general. In the lower part, AMS fabrics occasionally rotate almost ninety degrees and suggest horizontal compression. In contrast, magnetic fabrics did not show any correspondence to the thrusts or minor normal faults, which implies that those faults develop with concentrated shear deformation without disturbing surrounding sediments. Two adjacent drilling sites and dense sampling demonstrated clearly the change in strain field which is reported by previous studies. Based on these results, we propose a model of structural evolution at the toe of the prism. Underthrusting sediments induce horizontal stress in the lower part of the wedge, which reduces the effective stress and forms a high pore pressure anomaly and zones of fracturing. The frontal thrust is bent geometrically and terminates its activity in response to an increase of friction that triggers initiation of the next-generation frontal thrust. The upper part of the wedge tilts accordingly, resulting in an unstable slope.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 92
    Publication Date: 2017-08-09
    Description: The Kamchatka Peninsula in far eastern Russia represents the most volcanically active arc in the world in terms of magma production and the number of explosive eruptions. We investigate large-scale silicic volcanism in the past several million years and present new geochronologic results from major ignimbrite sheets exposed in Kamchatka. These ignimbrites are found in the vicinity of morphologically-preserved rims of partially eroded source calderas with diameters from ∼ 2 to ∼ 30 km and with estimated volumes of eruptions ranging from 10 to several hundred cubic kilometers of magma. We also identify and date two of the largest ignimbrites: Golygin Ignimbrite in southern Kamchatka (0.45 Ma), and Karymshina River Ignimbrites (1.78 Ma) in south-central Kamchatka. We present whole-rock geochemical analyses that can be used to correlate ignimbrites laterally. These large-volume ignimbrites sample a significant proportion of remelted Kamchatkan crust as constrained by the oxygen isotopes. Oxygen isotope analyses of minerals and matrix span a 3‰ range with a significant proportion of moderately low-δ18O values. This suggests that the source for these ignimbrites involved a hydrothermally-altered shallow crust, while participation of the Cretaceous siliceous basement is also evidenced by moderately elevated δ18O and Sr isotopes and xenocryst contamination in two volcanoes. The majority of dates obtained for caldera-forming eruptions coincide with glacial stages in accordance with the sediment record in the NW Pacific, suggesting an increase in explosive volcanic activity since the onset of the last glaciation 2.6 Ma. Rapid changes in ice volume during glacial times and the resulting fluctuation of glacial loading/unloading could have caused volatile saturation in shallow magma chambers and, in combination with availability of low-δ18O glacial meltwaters, increased the proportion of explosive vs effusive eruptions. The presented results provide new constraints on Pliocene–Pleistocene volcanic activity in Kamchatka, and thus constrain an important component of the Pacific Ring of Fire.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 93
    Publication Date: 2019-09-23
    Description: Iodine and its radioisotope 129I have been successfully used to trace the origin of pore waters in submarine fluid escape structures because of their close association with organic material in deeply buried sediments. We report here halogen concentrations and 129I/I ratios for fluids of five mud volcanoes sampled along an E–W transect across the Gulf of Cadiz in the NE Atlantic Ocean. Concentrations of iodide and bromide increase consistently seaward accompanied by a decrease in 129I/I ratios from 6490 × 10− 15 to 663 × 10− 15. The exceptionally high 129I/I ratios at the near-shore locations reflect the presence of fissiogenic 129I, produced in situ by spontaneous fission of 238U within terrigenous sediments and released into pore water during clay mineral diagenetic processes. The observed 129I/I and halogen trends, together with similar changes in 87Sr/86Sr ratios, indicate a progressive seaward transition from inorganic-terrigenous to organic-marine fluid sources. Comparison of our results with literature data for varying geological settings reveals a general relationship between fissiogenic 129I, radiogenic 87Sr and the lithology or provenance of rocks and sediments, respectively. While 129I/I ratios in continental rock-hosted aquifers and terrigenous sedimentary systems are dominated by in situ production of fissiogenic 129I, iodine isotopes in oceanic settings or volcanogenic marine sediments reflect the release of ‘old’ iodine from deeply buried organic matter. The Gulf of Cadiz represents the full transition between these continental and oceanic 129I/I and 87Sr/86Sr end members. This is the first systematic investigation of fissiogenic 129I production in marine sedimentary environments.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 94
    Publication Date: 2019-09-23
    Description: Lithium concentration and isotope data (δ7Li) are reported for pore fluids from 18 cold seep locations together with reference fluids from shallow marine environments, a sediment-hosted hydrothermal system and two Mediterranean brine basins. The new reference data and literature data of hydrothermal fluids and pore fluids from the Ocean Drilling Program follow an empirical relationship between Li concentration and δ7Li (δ7Li = −6.0(±0.3) · ln[Li] + 51(±1.2)) reflecting Li release from sediment or rocks and/or uptake of Li during mineral authigenesis. Cold seep fluids display δ7Li values between +7.5‰ and +45.7‰, mostly in agreement with this general relationship. Ubiquitous diagenetic signals of clay dehydration in all cold seep fluids indicate that authigenic smectite–illite is the major sink for light pore water Li in deeply buried continental margin sediments. Deviations from the general relationship are attributed to the varying provenance and composition of sediments or to transport-related fractionation trends. Pore fluids on passive margins receive disproportionally high amounts of Li from intensely weathered and transported terrigenous matter. By contrast, on convergent margins and in other settings with strong volcanogenic input, Li concentrations in pore water are lower because of intense Li uptake by alteration minerals and, most notably, adsorption of Li onto smectite. The latter process is not accompanied by isotope fractionation, as revealed from a separate study on shallow sediments. A numerical transport-reaction model was applied to simulate Li isotope fractionation during upwelling of pore fluids. It is demonstrated that slow pore water advection (order of mm a−1) suffices to convey much of the deep-seated diagenetic Li signal into shallow sediments. If carefully applied, Li isotope systematics may, thus, provide a valuable record of fluid/mineral interaction that has been inherited several hundreds or thousands of meters below the actual seafloor fluid escape structure.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 95
    Publication Date: 2019-09-23
    Description: The Arctic Ocean has wide shelf areas with extensive biological activity including a high primary productivity and an active microbial loop within the surface sediment. This in combination with brine production during sea ice formation result in the decay products exiting from the shelf into the deep basin typically at a depth of about 150 m and over a wide salinity range centered around S not, vert, similar33. We present data from the Beringia cruise in 2005 along a section in the Canada Basin from the continental margin north of Alaska towards the north and from the International Siberian Shelf Study in 2008 (ISSS-08) to illustrate the impact of these processes. The water rich in decay products, nutrients and dissolved inorganic carbon (DIC), exits the shelf not only from the Chukchi Sea, as has been shown earlier, but also from the East Siberian Sea. The excess of DIC found in the Canada Basin in a depth range of about 50–250 m amounts to 90±40 g C m−2. If this excess is integrated over the whole Canadian Basin the excess equals 320±140×1012 g C. The high DIC concentration layer also has low pH and consequently a low degree of calcium carbonate saturation, with minimum aragonite values of 60% saturation and calcite values just below saturation. The mean age of the waters in the top 300 m was calculated using the transit time distribution method. By applying a future exponential increase of atmospheric CO2 the invasion of anthropogenic carbon into these waters will result in an under-saturated surface water with respect to aragonite by the year 2050, even without any freshening caused by melting sea ice or increased river discharge.
    Type: Article , PeerReviewed , info:eu-repo/semantics/article
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 96
    Publication Date: 2019-09-23
    Description: Several known gas seep sites along the Hikurangi Margin off the east coast of New Zealand were surveyed by marine controlled source electromagnetic (CSEM) experiments. A bottom-towed electric dipole–dipole system was used to reveal the occurrence of gas hydrate and methane related to the seeps. The experiments were part of the international multidisciplinary research program “New Vents” carried out on German R/V Sonne in 2007 (cruise SO191) to study key parameters controlling the release and transformation of methane from marine cold vents and shallow gas hydrate deposits. Two CSEM lines have been surveyed over known seep sites on Opouawe Bank in the Wairarapa region off the SE corner of the North Island. The data have been inverted to sub-seafloor apparent resistivity profiles and one-dimensional layered models. Clearly anomalous resistivities are coincident with the location of two gas seep sites, North Tower and South Tower on Opouawe Bank. A layer of concentrated gas hydrate within the uppermost 100 m below the seafloor is likely to cause the anomalous resistivities, but free gas and thick carbonate crusts may also play a role. Seismic data show evidence of fault related venting which may also indicate the distribution of gas hydrates and/or authigenic carbonate. Geochemical profiles indicate an increase of methane flux and the formation of gas hydrate in the shallow sediment section around the seep sites. Takahe is another seep site in the area where active venting, higher heat flow, shallow gas hydrate recovered from cores, and seismic fault planes, but only moderately elevated resistivities have been observed. The reasons could be a) the gas hydrate concentration is too low, even though methane venting is evident, b) strong temporal or spatial variation of the seep activity, and c) the thermal anomaly indicates rather temperature driven fluid expulsion that hampers the formation of gas hydrate beneath the vent.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 97
    Publication Date: 2020-08-07
    Description: We have generated 104-year long (1895–1999) monthly δ18O and Sr/Ca time series from a fast-growing Diploria strigosa coral core drilled off Guadeloupe Island, Lesser Antilles. Coral Sr/Ca reliably records interannual to decadal surface air temperature (SAT) variations in the region and shows a pronounced warming of approximately 1.5 °C since 1950, with the strongest warming (1.2 °C) occurring since 1975. This warming is also evident in SAT measured at Guadeloupe, which ends in 1951. Thus, our Sr/Ca series extends the air temperature record by 56 years. We find that the past few decades are the warmest years over the entire period of record. The accelerated warming since 1950 is accompanied by a pronounced decrease in regional precipitation. This dampens the warming signal indicated by coral δ18O, which is too low (only 0.7– 0.8 °C since 1951). Consistently, δ18Osw estimated from the coral proxies also shows a strong decrease since 1950. Our data suggest an inverse relationship between SAT and precipitation (i.e. warmer and drier) for the latter half of the 20th century with the strongest trends since the mid-1970s. This is consistent with recent observational and model data, which report that while over the tropical oceans rainfall has increased due to an increase in sea surface temperatures, precipitation over land regions is reduced. A continuation of this warming and drying trend over Caribbean land regions would have severe societal consequences, especially in the context of anthropogenic warming. The El Niño Southern-Oscillation (ENSO) and the North Atlantic Oscillation (NAO) are the two major climate modes affecting large-scale SST variability in the northern tropical Atlantic. Both Sr/Ca and δ18O show a close relationship to ENSO and the NAO. A quantitative comparison between extremes in mean March–May coral δ18O and the Nino3 and NAO indices imply that climate variability in the northern tropical Atlantic is mainly forced by tropical Pacific and North Atlantic variability. Spectral analysis suggests that the relative importance of ENSO and the NAO is frequency dependent, with ENSO dominating at interannual, and the NAO dominating at interdecadal time scales.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 98
    Publication Date: 2017-08-08
    Description: Fluid escape structures on the Nile Deep Sea Fan were investigated during the MEDIFLUX MIMES expedition in 2004. Mud volcanoes, pockmarks and authigenic carbonate structures were surveyed for the first time with a high-resolution deep-towed 75 kHz sidescan sonar and a 2–8 kHz Chirp sediment echosounder. In combination with existing multibeam bathymetry and detailed seafloor in situ geological observations, these new data allowed detailed seep analyses. About 60 gas flares were detected acoustically in the water column from the sidescan sonar raw data atwater depths from 770 to 1700 m. These gas flares coincide at the seabed with 1) the centres of the mud volcanoes where mud is also extruded, 2) the borders of the mud volcanoes where the emitted gases contribute to the precipitation of authigenic carbonates, and 3) to the edges of broad sheets of authigenic carbonates. Subsurface sediments are commonly disturbed by ascending fluids throughout the delta, with an abundance of seep-related carbonate structures on the seafloor. The feeder channels below mud volcanoes, similar to the gas conduits below the widespread carbonate crust structures and pockmarks, are relatively narrow and, for the vast majority of them, do not exceed a few metres in diameter. The seeps on the Nile Deep Sea Fan clearly follow lineations on the seafloor that ee can relate to faults.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 99
    Publication Date: 2017-08-08
    Description: Seismic attenuation across the central Costa Rican margin wedge is determined fromamplitude analysis ofwideangle seismic data. Travel time and amplitude modeling are applied to ocean bottom hydrophones along two trench-parallel profiles, located 30 km (P21) and 35 km (P18) landward of the deformation front northeast of Quepos Plateau. Tomographic inversion images a progressively thinning margin wedge from the coast to the lower slope at the trench. A 1–1.5 km thick décollement zone with seismic velocities of 3.5–4.5 km/s is sandwiched between the marginwedge and the subducting Cocos plate. For strike line P21, amplitude modeling indicates a Qp value of 50–150 for the upper margin wedge with seismic velocities ranging from 3.9 km/s to 4.9 km/s. Along strike line P18, Qp values of 50–150 are determined with velocities of 4.3–5.0 km/s in the upper margin wedge, increasing to 5.1–5.4 km/s in the lower margin wedge. Quantitative amplitude decay curves support the observed upper plate Qp values. In conjunction with earlier results from offshore Nicoya Peninsula, our study documents landward decreasing attenuation across the margin wedge, consistent with a change in lithology from the sediment-dominated frontal prism to the igneous composition of the forearc middle prism
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 100
    facet.materialart.
    Unknown
    Elsevier
    In:  Journal of Experimental Marine Biology and Ecology, 395 (1-2). pp. 10-20.
    Publication Date: 2017-07-11
    Description: Predicting the relevance of initial colonization and subsequent species interactions for succession in marine sessile communities is difficult because the effects of both factors depend on highly variable environmental processes (e.g. currents, topography, upwelling and others). Depending on the successional stage at which a new species arrives, it can either rapidly colonize in large numbers or its colonization success might be suppressed by resident species. In order to assess the roles of (i) initial colonization and (ii) subsequent species interactions on community development, we examined the succession of fouling assemblages that established on artificial substrata during two different seasonal periods, i.e. austral winter/spring and spring/summer. At 16 weeks of age communities that were initiated in different seasons varied significantly in composition and diversity. During each period (winter/spring and spring/summer), multispecies fouling consortia of different ages (hereafter termed “old” and “young”) were reciprocally transplanted between two neighbouring study sites and their succession was documented. After 8 weeks of transplantation communities of different ages maintained their differences in diversity even in the face of environmental change. However, during winter/spring the spreading of the dominant species P. chilensis caused more rapid convergence between all communities at both sites. During the spring/summer period, the high initial abundances of the weak competitor Bugula neritina led to the maintenance of differences between resident and transplanted assemblages within each site. Later colonizers, including the dominant competitor P. chilensis, however, could recruit onto B. neritina and started to spread in the communities. These results suggest that the early and intermediate succession of fouling communities in highly productive marine environments such as the Humboldt Current System is driven by the temporal and spatial variability of propagule supply, while the long-term stability of these communities depends on the identity of colonizers and their competitiveness.
    Type: Article , PeerReviewed
    Format: text
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
Close ⊗
This website uses cookies and the analysis tool Matomo. More information can be found here...