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  • 1
    Call number: 9780128191101 (e-book)
    Type of Medium: 12
    Pages: 1 Online-Ressource (806 Seiten)
    Edition: 2nd edition
    ISBN: 9780128191101
    Language: English
    Note: Contents List of contributors Preface 1 Antarctic Climate Evolution - second edition 1.1 Introduction 1.2 Structure and content of the book Acknowledgements References 2 Sixty years of coordination and support for Antarctic science - the role of SCAR 2.1 Introduction 2.2 Scientific value of research in Antarctica and the Southern Ocean 2.3 The international framework in which SCAR operates 2.4 The organisation of SCAR 2.5 Sixty years of significant Antarctic science discoveries 2.6 Scientific Horizon Scan 2.7 Summary References Appendix 3 Cenozoic history of Antarctic glaciation and climate from onshore and offshore studies 3.1 Introduction 3.2 Long-term tectonic drivers and ice sheet evolution 3.3 Global climate variability and direct evidence for Antarctic ice sheet variability in the Cenozoic 3.3.1 Late Cretaceous to early Oligocene evidence of Antarctic ice sheets and climate variability 3.3.2 The Eocene-Oligocene transition and continental-scale glaciation of Antarctica 3.3.3 Transient glaciations of the Oligocene and Miocene 3.3.4 Pliocene to Pleistocene 3.4 Regional seismic stratigraphies and drill core correlations, and future priorities to reconstruct Antarctica's Cenozoic 3.4.1 Ross Sea 3.4.2 Amundsen Sea 3.4.3 Bellingshausen Sea and Pacific coastline of Antarctic Peninsula 3.4.4 The Northern Antarctic Peninsula and South Shetland Islands 3.4.5 The Eastern Margin of the Antarctic Peninsula 3.4.6 The South Orkney Microcontinent and adjacent deep-water basins 3.4.7 East Antarctic Margin 3.4.7.1 Weddell Sea 3.4.7.1.1 Gondwana break-up, Weddell Sea opening and pre-ice-sheet depositional environment 3.4.7.1.2 The Eocene-Oligocene transition and paleoenvironment during increasing glacial conditions 3.4.7.1.3 Recent geophysical survey beneath the Ekström Ice Shelf and future directions for drilling 3.4.7.2 Prydz Bay 3.4.7.2.1 Early Cenozoic greenhouse and earliest glacial phase in late Eocene 3.4.7.2.2 Oligocene-Miocene ice-sheet development 3.4.7.2.3 The Polar Ice Sheet (late Miocene(?)-Pleistocene) 3.4.7.3 East Antarctic Margin - Sabrina Coast 3.4.7.4 Wilkes Land margin and Georges V Land 3.5 Summary, future directions and challenges Acknowledgements References 4 Water masses, circulation and change in the modern Southern Ocean 4.1 Introduction 4.1.1 Defining the Southern Ocean 4.2 Water masses - characteristics and distribution 4.2.1 Upper ocean 4.2.2 Intermediate depth waters 4.2.3 Deep water 4.2.4 Bottom water 4.3 Southern Ocean circulation 4.3.1 Antarctic Circumpolar Current (ACC) 4.3.2 Southern Ocean meridional overturning circulation (SOMOC) 4.3.3 Deep western boundary currents 4.3.3.1 Pacific deep western boundary current 4.3.3.2 Indian deep western boundary currents 4.3.3.3 Atlantic deep western boundary current 4.3.4 Subpolar circulation - gyres, slope and coastal currents 4.3.4.1 Gyres 4.3.4.2 Antarctic slope and coastal currents 4.4 Modern Southern Ocean change 4.4.1 Climate change 4.4.2 Ocean change 4.4.3 Change in dynamics and circulation 4.5 Concluding remarks References 5 Advances in numerical modelling of the Antarctic ice sheet 5.1 Introduction and aims 5.2 Advances in ice sheet modelling 5.2.1 Grounding line physics 5.2.2 Adaptive grids 5.2.3 Parallel ice sheet model - PISM 5.2.4 Coupled models 5.3 Model input - bed data 5.4 Advances in knowledge of bed processes 5.5 Model intercomparison 5.6 Brief case studies 5.7 Future work References 6 The Antarctic Continent in Gondwana: a perspective from the Ross Embayment and Potential Research Targets for Future Investigations 6.1 Introduction 6.2 The Antarctic plate and the present-day geological setting of the Ross Embayment 6.3 East Antarctica 6.3.1 The Main Geological Units during the Paleoproterozoic-Early Neoproterozoic Rodinia Assemblage 6.3.2 From Rodinia breakup to Gondwana (c. 800-650 Ma) 6.3.3 The 'Ross Orogen' in the Transantarctic Mountains during the late Precambrian-early Paleozoic evolution of the paleo-Pacific margin of Gondwana (c. 600-450 Ma) 6.4 West Antarctic Accretionary System 6.4.1 West Antarctica in the Precambrian to Mesozoic (c. 180 Ma) evolution of Gondwana until the middle Jurassic breakup 6.4.1.1 Precambrian to Cambrian metamorphic basement 6.4.1.2 Devono-Carboniferous arc magmatism ('Borchgrevink Event') (c. 370-350 Ma) 6.4.1.3 Beacon Supergroup (Devonian-Permo-Triassic-earliest Jurassic) 6.4.1.4 The Ellsworth-Whitmore Mountains Terrane and the Permo-Triassic arc magmatism 6.4.1.5 Ferrar Supergroup and the Gondwana breakup (c. 180Ma) 6.4.1.6 The Antarctic Andean Orogen 6.5 Mesozoic to Cenozoic Tectonic Evolution of the Transantarctic Mountains 6.6 Tectonic evolution in the Ross Sea Sector during the Cenozoic 6.7 Concluding remarks, open problems and potential research themes for future geoscience investigations in Antarctica 6.7.1 Persistent challenges for onshore geoscience investigations 6.7.2 Antarctica and the Ross Orogen in the Transantarctic Mountains 6.7.3 Antarctica after Gondwana fragmentation Acknowledgements References 7 The Eocene-Oligocene boundary climate transition: an Antarctic perspective 7.1 Introduction 7.2 Background 7.2.1 Plate tectonic setting 7.2.2 Antarctic paleotopography 7.2.3 Paleoceanographic setting 7.2.4 Global average and regional sea level response 7.2.5 Proxies to reconstruct past Antarctic climatic and environmental evolution 7.2.6 Far-field proxies 7.3 Antarctic Sedimentary Archives 7.3.1 Land-based outcrops 7.3.1.1 Antarctic Peninsula Region 7.3.1.2 King George (25 de Mayo) Island, South Shetland Islands 7.3.1.3 The Ross Sea Region 7.3.2 Sedimentary archives from drilling on the Antarctic Margin 7.3.2.1 Drill cores in the western Ross Sea 7.3.2.2 The Prydz Bay Region 7.3.2.3 Weddell Sea 7.3.2.4 Wilkes Land 7.4 Summary of climate signals from Antarctic sedimentary archives 7.4.1 Longer-term changes 7.4.2 The climate of the Eocene-Oligocene transition 7.5 The global context of Earth and climate system changes across the EOT 7.5.1 Climate modelling 7.5.2 Relative sea-level change around Antarctica 7.6 Summary 7.6.1 Early-middle Eocene polar warmth 7.6.2 Late Eocene cooling 7.6.3 Eocene-Oligocene transition Acknowledgements References 8 Antarctic Ice Sheet dynamics during the Late Oligocene and Early Miocene: climatic conundrums revisited 8.1 Introduction 8.2 Oligocene-Miocene Transition in Antarctic geological records and its climatic significance 8.3 Conundrums revisited 8.3.1 What caused major transient glaciation of Antarctica across the OMT? 8.3.2 Apparent decoupling of Late Oligocene climate and ice volume? 8.4 Concluding remarks Acknowledgements References 9 Antarctic environmental change and ice sheet evolution through the Miocene to Pliocene - a perspective from the Ross Sea and George V to Wilkes Land Coasts 9.1 Introduction 9.1.1 Overview and relevance 9.1.2 Far-field records of climate and ice sheet variability 9.1.2.1 The Early Miocene 9.1.2.2 The mid-Miocene 9.1.2.3 The Late Miocene 9.1.2.4 The Pliocene 9.1.3 Southern Ocean Paleogeography and Paleoceanography 9.1.4 Land elevation change and influences on Antarctic Ice Sheet evolution 9.2 Records of Miocene to Pliocene climate and ice sheet variability from the Antarctic margin 9.2.1 Introduction to stratigraphic records 9.2.2 George V Land to Wilkes Land Margin 9.2.2.1 Geological setting 9.2.2.2 Oceanography of the Adelie coast 9.2.2.3 Seismic stratigraphy off the George V Land to Wilkes Land Margin 9.2.2.4 Drill core records from the George V Land to Wilkes Land Margin 9.2.2.5 Neogene history of the George V Land to Wilkes Land margin 9.2.3 The Ross Sea Embayment and Southern Victoria Land 9.2.3.1 Geological setting 9.2.3.2 Oceanography and climate in the Ross Sea Region 9.2.3.3 Seismic stratigraphic records in the Ross Sea 9.2.3.4 Stratigraphic records from drill cores in the Ross Sea 9.2.3.5 Terrestrial records from Southern Victoria Land 9.2.3.6 Neogene history in the Ross Sea Region 9.3 Numerical modelling 9.3.1 Miocene
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  • 2
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Between 34 and 15 million years (Myr) ago, when planetary temperatures were 3–4 °C warmer than at present and atmospheric CO2 concentrations were twice as high as today, the Antarctic ice sheets may have been unstable. Oxygen isotope records from deep-sea ...
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 126 (1996), S. 0 
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: Numerous short features in the ocean magnetic anomaly patterns (25–100 nT amplitude, 8–25 km wavelength: tiny wiggles) have been identified in several independent magnetic profiles, and have been modelled either as short polarity intervals (‘cryptochrons’) or as palaeointensity fluctuations (Cande & Kent 1992). In the last few years, several authors (e.g. Tauxe et al. 1994; Lowrie & Lanci 1994; Hartl, Tauxe & Constable 1993) have identified, on high-resolution magnetostratigraphic sections, short polarity intervals, correlated with cryptochrons deriving from the ocean floor. The record of a previously undetected short normal-polarity event, lasting about 11 kyr, from an upper Tortonian-lower Messinian sedimentary sequence (e.g. Compagnoni et al. 1992) in central Italy (42.0°N, 13.0°E), is reported here. The north virtual geomagnetic polar (VGP) path of the R-N transition appears to be strongly confined to a meridian band passing over the Americas about 90° away from the site longitude, as reported in recent years for a large number of reversals. This short feature is lacking in the corresponding ocean-floor magnetic anomaly patterns, probably because of the difficulties of resolving polarity intervals as short as this one in ocean magnetic profiles.
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 123 (1995), S. 0 
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: A revision of the magnetostratigraphy in the Valle Ricca (Monterotondo, Rome) Plio-Pleistocene section was carried out. This section, consisting mainly of blue-grey marly clays, was previously investigated for palaeomagnetic effects by Arias et al. (1980, 1990), who detected a normal polarity interval, close to a volcanic ash layer, which was correlated to the Reunion subchron. This interpretation conflicts, however, with new biostratigraphic data and palaeomagnetic observations. In order to investigate the possible origin of these discrepancies, we performed a detailed sampling for palaeomagnetic and rock-magnetic analyses in the controversial interval around the volcanic ash layer. The present results show strong variations in the rock-magnetic parameters and suggest significant changes in the magnetic mineralogy. Two levels with a high-intensity, low-temperature, normal component of magnetization were distinguished. At these two levels, the rock-magnetic parameters are typical of greigite, and a widespread occurrence of framboids of micron-sized iron sulphide grains was found by mineralogical analyses. A high-temperature reversed component of magnetization, carried by magnetite, was isolated for the whole interval investigated. We demonstrate that the previously recognized normal polarity interval is the effect of changes in the magnetic mineralogy and it does not represent a true reversal of the Earth's magnetic field. The origin of the low-temperature normal component of magnetization is discussed in light of the present knowledge about greigite formation and remanence acquisition.
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    Oxford UK : Blackwell Science Ltd
    Sedimentology 47 (2000), S. 0 
    ISSN: 1365-3091
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Type of Medium: Electronic Resource
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  • 6
    Publication Date: 2013-07-02
    Description: The Monte Cagnero sedimentary section, which crops out in the northeastern Apennines near Urbania in the Umbria–Marche Basin (Italy), contains well-exposed strata spanning the middle Eocene to lower Oligocene interval. We use an integrated magnetobiostratigraphic approach to generate a high-resolution age model for the Monte Cagnero section, with the goal of obtaining a reliable chronostratigraphic framework for studying Eocene–Oligocene palaeoceanographic changes during the switch from greenhouse to icehouse conditions. The studied sediments consist of alternating reddish and greenish limestones and marlstones. A new integrated age model for the section is based on high-resolution palaeomagnetic analyses, combined with detailed planktonic foraminiferal and calcareous nannofossil biostratigraphic results. Rock magnetic measurements show that the magnetic mineralogy is dominated by a mixture of high- and low-coercivity minerals, probably representing a combination of hematite and magnetite. A robust magnetostratigraphic signal, together with the identification of key planktonic foraminiferal and nannofossil biostratigraphic events, allows construction of a detailed age model for the section. Based on these results, we infer that the section spans a continuous interval (within magnetochron resolution) from the middle Eocene to lower Oligocene (c. 41–27 Ma; Chrons C18r–C12r). The Monte Cagnero section, therefore, represents a sequence that is suitable for studying the impact of the Neo-Tethyan gateway closure on subtropical Eocene circulation and determining the nature and timing of palaeoceanographic changes in the Tethys through the late middle Eocene to early Oligocene interval.
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  • 7
    Publication Date: 2016-02-22
    Description: Geological records from the Antarctic margin offer direct evidence of environmental variability at high southern latitudes and provide insight regarding ice sheet sensitivity to past climate change. The early to mid-Miocene (23–14 Mya) is a compelling interval to study as global temperatures and atmospheric CO2 concentrations were similar to those projected for coming centuries. Importantly, this time interval includes the Miocene Climatic Optimum, a period of global warmth during which average surface temperatures were 3–4 °C higher than today. Miocene sediments in the ANDRILL-2A drill core from the Western Ross Sea, Antarctica, indicate that the Antarctic ice sheet (AIS) was highly variable through this key time interval. A multiproxy dataset derived from the core identifies four distinct environmental motifs based on changes in sedimentary facies, fossil assemblages, geochemistry, and paleotemperature. Four major disconformities in the drill core coincide with regional seismic discontinuities and reflect transient expansion of grounded ice across the Ross Sea. They correlate with major positive shifts in benthic oxygen isotope records and generally coincide with intervals when atmospheric CO2 concentrations were at or below preindustrial levels (∼280 ppm). Five intervals reflect ice sheet minima and air temperatures warm enough for substantial ice mass loss during episodes of high (∼500 ppm) atmospheric CO2. These new drill core data and associated ice sheet modeling experiments indicate that polar climate and the AIS were highly sensitive to relatively small changes in atmospheric CO2 during the early to mid-Miocene.
    Print ISSN: 0027-8424
    Electronic ISSN: 1091-6490
    Topics: Biology , Medicine , Natural Sciences in General
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  • 8
    Publication Date: 2011-12-01
    Description: Since its first field season (2006–2007), the ANDRILL (Antarctic Geological Drilling) program has implemented an innovative educational and public outreach (EPO) program known as ARISE (ANDRILL Research Immersion for Science Educators), which has actively involved a group of selected educators in every phase of the research, from participation in field activities to discussion of the scientific results. This method of research immersion has led to an impressive list of achievements, including the development of quality outreach initiatives and diverse educational materials, the involvement of a large number of schools using these resources, the creation of an international network of strongly motivated polar geoscience educators, and the realization of new and unexpected professional opportunities for educators. In Italy this program initiated a specific project (progettosmilla.it), in accordance with the objectives of the ARISE Program. Thanks to the use of both a wide range of instruments (online and material) and the network of personal relationships provided by teachers involved in the program, ARISE has resulted in many short-term accomplishments. The development of new partnerships with local and national institutions has led to a number of middle- and long-term processes, rarely seen in similar EPO projects, resulting in the attainment of other goals. Research immersion experiences promote close interactions between teachers and scientists, and provide the potential for accomplishing other long-term educational outcomes. The shared development of educational resources by scientists and educators through ARISE has created an opportunity to advance scientific education within schools and, through outreach, in the general populace.
    Electronic ISSN: 1553-040X
    Topics: Geosciences
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  • 9
    Publication Date: 2012-03-01
    Description: Paleoenvironmental and paleoclimate changes that occurred during the late postevaporitic stage of the Mediterranean Basin in the Messinian foreland domain of the Adriatic region offer a new perspective on the relationship between orbital forcing and climate response. The magnetic susceptibility record of the Fonte dei Pulcini A section (Maiella Mountains, Italy) allows us to orbitally tune the record between 5.394 and 5.336 Ma and to temporally constrain the paleoenvironmental and paleoclimate changes evidenced by quantitative paleontological (palynomorphs, ostracods, and calcareous nannofossils), stable isotope (d18O and d13C), and X-ray diffraction (XRD) analyses. The base of the Fonte dei Pulcini A section is characterized by Paratethyan ostracods and dinocysts, which point to the late Messinian Lago-Mare biofacies (Loxocorniculina djafarovi zone) of the Mediterranean Messinian stratigraphy. From paleontological and geochemical (d18O) analyses, there is no evidence of a marine incursion in the Fonte dei Pulcini A section. The major changes in terms of paleodepth, paleosalinity, evaporation versus precipitation, aridity versus humidity, and reworking processes occurred in the upper part of the Fonte dei Pulcini A section, during the last Messinian insolation cycle (i-cycle 511/512), which is characterized by high-amplitude oscillations. In contrast, the lower part of the Fonte dei Pulcini A section, which was deposited during relatively low-amplitude insolation cycles, is characterized by more stable environmental conditions. Comparing summer insolation with the paleoenvironmental changes at the Fonte dei Pulcini A section, we identify delays of several thousands of years between orbital forcing and climate response.
    Print ISSN: 0016-7606
    Electronic ISSN: 1943-2674
    Topics: Geosciences
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  • 10
    Publication Date: 2018-06-13
    Description: Diagenetic alteration of magnetic minerals occurs in all sedimentary environments and tends to be severe in reducing environments. Magnetic minerals provide useful information about sedimentary diagenetic processes, which makes it valuable to use magnetic properties to identify the diagenetic environment in which the magnetic minerals occur and to inform interpretations of paleomagnetic recording or environmental processes. We use a newly developed first-order reversal curve unmixing method on well-studied samples to illustrate how magnetic properties can be used to assess diagenetic processes in reducing sedimentary environments. From our analysis of multiple data sets, consistent magnetic components are identified for each stage of reductive diagenesis. Relatively unaltered detrital and biogenic magnetic mineral assemblages in surficial oxic to manganous diagenetic environments undergo progressive dissolution with burial into ferruginous and sulfidic environments and largely disappear at the sulfate-methane transition. Below the sulfate-methane transition, a weak superparamagnetic to largely noninteracting stable single domain (SD) greigite component is observed in all studied data sets. Moderately interacting stable SD authigenic pyrrhotite and strongly interacting stable SD greigite are observed commonly in methanic environments. Recognition of these characteristic magnetic components enables identification of diagenetic processes and should help to constrain interpretation of magnetic mineral assemblages in future studies. A key question for future studies concerns whether stable SD greigite forms in the sulfidic or methanic zones, where formation in deeper methanic sediments will cause greater delays in paleomagnetic signal recording. Authigenic pyrrhotite forms in methanic environments, so it will usually record a delayed paleomagnetic signal. ©2018. American Geophysical Union. All Rights Reserved.
    Print ISSN: 2169-9313
    Electronic ISSN: 2169-9356
    Topics: Geosciences , Physics
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