The Canyon System off Fimbulisen

In der vorliegenden Arbeit werden Daten einer systematischen Vermessung in der Lazarev Sea nahe des Fimbul-Ice-Shelfs (Fimbulisen) genutzt, die während der Expedition ANT XIX-2 mit dem Fächersonarsystem Hydrosweep DS-2 und dem Sedimentecholot Parasound erhoben wurden. Nach kurzer Darstellung der Hintergründe dieser durchgeführten Untersuchungen in dem Messgebiet wird allgemein auf wesentliche Aspekte der Hydroakustik hinsichtlich der Anwendung von Echolotsystemen eingegangen. Schwerpunktmäßig soll dabei der parametrischen Effekt, das Messprinzip parametrischer Sedimentecholote, behandelt werden. Nach anschließender Anführung zweier praktischer Anwendungen hydroakustischer Messverfahren anhand des Hydrosweep DS-2 und des Parasound-Systems wird eingehend deren Positionierung auf FS 'Polarstern' dargestellt, da sich bei der Aufbereitung der Messungen zeigte, dass sich das größte Problem der Daten beider Systeme in der minderwertigen Qualität der Navigationsdaten abzeichnete. Aus den bereinigten Tiefendaten der Fächersonarmessung wird ein digitales Geländemodell (DGM) mit einer Rasterweite von 100 m generiert. Dieses Modell liegt für die weitere Bearbeitung digital und in Form einer bathymetrischen Karte im Maßstab 1:250,000 vor, bei der die Topographie des Canyon-Systems nahe dem Fimbulisen durch Isolinien mit einer Aquidistanz von 50 m dargestellt wird. Die als Ergebnis der prozessierten Parasound-Daten erhaltenen Seismogramme, die gefiltert im digitalen Bildformat mit bekannter Start- und Endposition für einen definierten Tiefenbereich vorliegen, können zusammen mit dem DGM in einem dreidimensionalen Modell dargestellt werden. Dieses in digitaler Form vorliegende Modell kann durch den Nutzer interaktiv durchschritten und die darin enthaltenen Messergebnisse in ihrer Gesamtheit sowie in Detailansichten aus verschiedenen Perspektiven betrachtet werden, was das gegenseitige Verständnis und Einschätzung der Ergebnisse aus den beiden Messverfahren fördert. Diese gemeinsame Darstellungsweise eines digitalen Geländemodells in Kombination mit den Seismogramm-Bildern des Sedimentecholotes Parasound bietet sich auch hinsichtlich einer geologischen Klassifizierung der verschiedenen Echotypen und einer anschließenden Interpretation der Sedimentationsvorgänge in einem flächenhaft vermessenen Gebiet an.

Accumulation rates of ODP Site 177-1090

Dust has the potential to modify global climate by influencing the radiative balance of the atmosphere and by supplying iron and other essential limiting micronutrients to the ocean (Martin et al., 1990, doi:10.1038/345156a0; Martin, 1990, doi:10.1029/PA005i001p00001). Indeed, dust supply to the Southern Ocean increases during ice ages, and 'iron fertilization' of the subantarctic zone may have contributed up to 40 parts per million by volume (p.p.m.v.) of the decrease (80-100 p.p.m.v.) in atmospheric carbon dioxide observed during late Pleistocene glacial cycles (Watson et al., 2000, doi:10.1038/35037561; Kohfeld et al., 2005, doi:10.1126/science.1105375; Martínez-Garcia et al., 2009, doi:10.1029/2008PA001657; Sigman et al., 2010, doi:10.1038/nature09149; Hain et al., 2010, doi:10.1029/2010gb003790). So far, however, the magnitude of Southern Ocean dust deposition in earlier times and its role in the development and evolution of Pleistocene glacial cycles have remained unclear. Here we report a high-resolution record of dust and iron supply to the Southern Ocean over the past four million years, derived from the analysis of marine sediments from ODP Site 1090, located in the Atlantic sector of the subantarctic zone. The close correspondence of our dust and iron deposition records with Antarctic ice core reconstructions of dust flux covering the past 800,000 years (Lambert et al., 2008, doi:10.1038/nature06763; Wolf et al., 2006, doi:10.1038/nature04614) indicates that both of these archives record large-scale deposition changes that should apply to most of the Southern Ocean, validating previous interpretations of the ice core data. The extension of the record beyond the interval covered by the Antarctic ice cores reveals that, in contrast to the relatively gradual intensification of glacial cycles over the past three million years, Southern Ocean dust and iron flux rose sharply at the Mid-Pleistocene climatic transition around 1.25 million years ago. This finding complements previous observations over late Pleistocene glacial cycles (Martínez-Garcia et al., 2009; Lambert et al., 2008; Wolff et al., 2006), providing new evidence of a tight connection between high dust input to the Southern Ocean and the emergence of the deep glaciations that characterize the past one million years of Earth history.

Description of sampling sites in Northern Russia

The youngest ice marginal zone between the White Sea and the Ural mountains is the W-E trending belt of moraines called the Varsh-Indiga-Markhida-Harbei-Halmer-Sopkay, here called the Markhida line. Glacial elements show that it was deposited by the Kara Ice Sheet, and in the west, by the Barents Ice Sheet. The Markhida moraine overlies Eemian marine sediments, and is therefore of Weichselian age. Distal to the moraine are Eemian marine sediments and three Palaeolithic sites with many C-14 dates in the range 16-37 ka not covered by till, proving that it represents the maximum ice sheet extension during the Weichselian. The Late Weichselian ice limit of M. G. Grosswald is about 400 km (near the Urals more than 700 km) too far south. Shorelines of ice dammed Lake Komi, probably dammed by the ice sheet ending at the Markhida line, predate 37 ka. We conclude that the Markhida line is of Middle/Early Weichselian age, implying that no ice sheet reached this part of Northern Russia during the Late Weichselian. This age is supported by a series of C-14 and OSL dates inside the Markhida line all of >45 ka. Two moraine loops protrude south of the Markhida line; the Laya-Adzva and Rogavaya moraines. These moraines are covered by Lake Komi sediments, and many C-14 dates on mammoth bones inside the moraines are 26-37 ka. The morphology indicates that the moraines are of Weichselian age, but a Saalian age cannot be excluded. No post-glacial emerged marine shorelines are found along the Barents Sea coast north of the Markhida line.

Age determination of sediment cores from the western Svalbard margin

The deglaciation of the continental shelf to the west of Spitsbergen and the main fjord, Isfjorden, is discussed based on sub-bottom seismic records and sediment cores. The sea floor on the shelf to the west of Isfjorden is underlain by less than 2 m of glaciomarine sediments over a firm diamicton interpreted as till. In central Isfjorden up to 10 m of deglaciation sediments were recorded, whereas in cores from the innermost tributary, Billefjorden, less than a meter of ice proximal sediments was recognized between the till and the 'normal' Holocene marine sediments. We conclude that the Barents Sea Ice Sheet terminated along the shelf break during the Late Weichselian glacial maximum. Radiocarbon dates from the glaciomarine sediments above the till indicate a stepwise deglaciation. Apparently the ice front retreated from the outermost shelf around 14.8 ka. A dramatic increase in the flux of line-grained glaciomarine sediments around 13 ka is assumed to reflect increased melting and/or current activity due to a climatic warming. This second stage of deglaciation was interrupted by a glacial readvance culminating on the mid-shelf area shortly after 12.4 ka. The glacial readvance, which is correlated with a simultaneous readvance of the Fennoscandian ice sheet along the western coast of Norway, is attributed to the so-called 'Older Dryas' cooling event in the North Atlantic region. Following this glacial readvance the outer part of Isfjorden became rapidly deglaciated around 12.3 ka. During the Younger Dryas the inner fjord branches were occupied by large outlet glaciers and possibly the ice front terminated far out in the main fjord. The remnants of the Barents Sea Ice Sheet melted quickly away as a response to the Holocene warming around 10 ka.