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11.
T. Kenkmann F. Kiebach M. Rosenau U. Raschke A. Pigowske K. Mittelhaus D. Eue 《Meteoritics & planetary science》2007,42(11):1995-2012
Abstract— Our current understanding of marine‐impact cratering processes is partly inferred from the geological structure of the Lockne crater. We present results of a mapping campaign and structural data indicating that this crater is not pristine. In the western part of the crater, pre‐impact, impact, and post‐impact rocks are incorporated in Caledonian thrust slices and are subjected to folding and faulting. A nappe outlier in the central crater depression is a relic of the Caledonian nappe cover that reached a thickness of more than 5 km. The overthrusted crater is gently deformed. Strike of strata and trend of fold axes deviate from standard Caledonian directions (northeast‐southwest). Radially oriented crater depressions, which were previously regarded as marine resurge gullies formed when resurging seawater erosively cut through the crater brim, are interpreted to be open synclines in which resurge deposits were better preserved. The presence of the impact structure influenced orogenesis due to morphological and lithological anomalies of the crater: i) a raised crater brim zone acted as an obstacle during nappe propagation, (ii) the occurrence of a central crater depression caused downward sagging of nappes, and (iii) the lack of an appropriate detachment horizon (alum shale) within the crater led to an enhanced mechanical coupling and internal deformation of the nappe and the overthrusted foreland. Preliminary results of 3‐D‐analogue experiments suggest that a circular high‐friction zone representing the crater locally hinders nappe propagation and initiates a circumferentially striking ramp fault that delineates the crater. Crustal shortening is also partitioned into the crater basement and decreases laterally outward. Deformation of the foreland affected the geometry of the detachment and could be associated with the activation of a deeper detachment horizon beneath the crater. Strain gradients both vertically and horizontally result in non‐plane strain deformation in the vicinity of the crater. The strain tensors in the hanging and foot walls may deviate up to 90° from each other and rotated by up to 45° with respect to the standard regional orientation. The observed deflection of strata and fold axes within the Lockne crater area as revealed by field mapping is in agreement with the pattern of strain partitioning shown in the analogue models. 相似文献
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Mathias Raschke 《Journal of Seismology》2013,17(4):1157-1182
We introduce a new approach for ground motion relations (GMR) in the probabilistic seismic hazard analysis (PSHA), being influenced by the extreme value theory of mathematical statistics. Therein, we understand a GMR as a random function. We derive mathematically the principle of area equivalence, wherein two alternative GMRs have an equivalent influence on the hazard if these GMRs have equivalent area functions. This includes local biases. An interpretation of the difference between these GMRs (an actual and a modeled one) as a random component leads to a general overestimation of residual variance and hazard. Beside this, we discuss important aspects of classical approaches and discover discrepancies with the state of the art of stochastics and statistics (model selection and significance, test of distribution assumptions, extreme value statistics). We criticize especially the assumption of logarithmic normally distributed residuals of maxima like the peak ground acceleration (PGA). The natural distribution of its individual random component (equivalent to exp(ε 0) of Joyner and Boore, Bull Seism Soc Am 83(2):469–487, 1993) is the generalized extreme value. We show by numerical researches that the actual distribution can be hidden and a wrong distribution assumption can influence the PSHA negatively as the negligence of area equivalence does. Finally, we suggest an estimation concept for GMRs of PSHA with a regression-free variance estimation of the individual random component. We demonstrate the advantages of event-specific GMRs by analyzing data sets from the PEER strong motion database and estimate event-specific GMRs. Therein, the majority of the best models base on an anisotropic point source approach. The residual variance of logarithmized PGA is significantly smaller than in previous models. We validate the estimations for the event with the largest sample by empirical area functions, which indicate the appropriate modeling of the GMR by an anisotropic point source model. The constructed distances like the Joyner–Boore distance do not work well for event-specific GMRs. We discover also a strong relation between magnitude and the squared expectation of the PGAs being integrated in the geo-space for the event-specific GMRs. One of our secondary contributions is the simple modeling of anisotropy for a point source model. 相似文献
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E. Raschke P. Flamant Y. Fouquart P. Hignett H. Isaka P. R. Jonas H. Sundquist P. Wendling 《Surveys in Geophysics》1998,19(2):89-138
The dominant role of clouds in modulating and interacting with radiative energy transports within the atmosphere, in providing precipitation, transporting water and influencing air-chemical processes is still not understood well enough to be accurately represented within atmospheric circulation and climate models over all regions of the globe. Also the extraction of real-world cloud properties from satellite measurements still contains uncertainties. Therefore, various projects have been developed within the Global Energy and Water Cycle Experiment (GEWEX), to achieve more accurate solutions for this problem by direct measurements within cloud fields and other complementary studies. They are based on the hypothesis, that most relevant properties of cloud fields can be parametrized on the basis of the prognostic field variables of atmospheric circulation models, and that the cloud microphysical properties can directly be related – with additional parameters on the particle shapes etc. – to the radiative transfer properties.One of these projects has been the European Cloud and Radiation Experiment (EUCREX) with its predecessor ICE (International Cirrus Experiment).The EUCREX and ICE provided a common platform for research groups from France, Germany, Sweden and the United Kingdom to concentrate their efforts primarily on high, cold cirrus. They showed, with data from satellites, that this cloud species enhances the atmospheric greenhouse-effect. Numerical mesoscale models were used in sensitivity studies on cloud developments. In-situ measurements of cloud properties were made during more than 30 aircraft missions, where also in-flight comparisons of various instruments were made to ensure the quality of data sets measured from different aircraft. The particle sampling probes, used for in-cloud measurements, showed a disagreement in total number density in all ranges between about 20–50%, while all other instruments agreed quite satisfactorily. A few measured holographic data provided information on typical ice-crystal shapes, which were used in numerical simulations of their absorption and scattering properties.Several new instruments for both in-situ and remote measurement, such as a polar nephelometer, a chopped pyrgeometer and an imaging multispectral polarimeter (POLDER) for cloud and radiation measurements were tested and improved. New algorithms were developed for cloud classifications in multispectral satellite images and also for simulations of the scattering of radiation by non-spherical particles.This paper primarily summarizes the EUCREX results obtained between 1989 and 1996, and provides examples of the many results which have been obtained so far. It is not a complete review of the world-wide state in this field, but it tries to place the EUCREX results into the world-wide development. Therefore many references are made to the results of other groups, which in turn influenced the work within EUCREX. 相似文献
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Summary The large desert regions over North Africa are of particular importance to our climate and are therefore modelled numerically as part of sensitivity studies. The result of these models needs verification, but diagnostic studies of atmospheric energetics also require accurate values of the radiation budget at the upper boundary of the climate system.The radiation anomaly above Northern Africa is now established from various satellite data. However, it is suspected that there are serious errors caused in particular by angular and temporal sampling. A sample of NIMBUS-7 ERB—measurements (16.–30. June 1979) was therefore reanalysed, including the missing diurnal cycle which was reconstructed from the corresponding METEOSAT measurements. These more complete data on diurnal cycles change the results on outgoing thermal fluxes and net radiation by up to almost 60 Wm–2, thus changes of the sign of net radiation also occur over several regions.
With 11 Figures 相似文献
Zusammenfassung Die ausgedehnten Wüstengebiete in Nordafrika sind von großer Wichtigkeit für unser Klima und daher Gegenstand zahlreicher numerischer Empfindlichkeitsstudien. Entsprechende Modellergebnisse können mit Hilfe von Messungen der Strahlungsbilanz am Oberrand der Atmosphäre verifiziert werden. Messungen dienen aber auch als Eingangsdaten für diagnostische Untersuchungen der Energietransporte in der Atmosphäre.Die Strahlungsanomalität über Nordafrika ist mittlerweile durch zahlreiche Satellitenmessungen bestätigt. Jedoch beinhalten ältere Studien z.T. Fehler auf Grund der Nichtberücksichtigung der speziellen Eigenschaften der Stichprobenentnahme durch das Satelliteninstrument. Aus diesem Grund wurde ein Datensatz des NIMBUS-7 ERB Experimentes (16.–30. Juni 1979) neu ausgewertet unter zusätzlicher Verwendung von METEOSAT-1-Messungen, um den Tagesgang der Strahlungsparameter berücksichtigen zu können. Diese zusätzlichen Daten bewirken Änderungen im kurz- und langwelligen Fluß sowie in dem daraus resultierenden Nettofluß von bis zu 60 Wm–2, was für einige Gebiete eine Vorzeichenumkehr des Nettoflusses bedeutet.
With 11 Figures 相似文献
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Geochemical studies of impact breccias and country rocks from the El'gygytgyn impact structure,Russia 
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下载免费PDF全文 Ulli Raschke Ralf Thomas Schmitt Iain McDonald Wolf Uwe Reimold Dieter Mader Christian Koeberl 《Meteoritics & planetary science》2015,50(6):1071-1088
The complex impact structure El'gygytgyn (age 3.6 Ma, diameter 18 km) in northeastern Russia was formed in ~88 Ma old volcanic target rocks of the Ochotsk‐Chukotsky Volcanic Belt (OCVB). In 2009, El'gygytgyn was the target of a drilling project of the International Continental Scientific Drilling Program (ICDP), and in summer 2011 it was investigated further by a Russian–German expedition. Drill core material and surface samples, including volcanic target rocks and impactites, have been investigated by various geochemical techniques in order to improve the record of trace element characteristics for these lithologies and to attempt to detect and constrain a possible meteoritic component. The bedrock units of the ICDP drill core reflect the felsic volcanics that are predominant in the crater vicinity. The overlying suevites comprise a mixture of all currently known target lithologies, dominated by felsic rocks but lacking a discernable meteoritic component based on platinum group element abundances. The reworked suevite, directly overlain by lake sediments, is not only comparatively enriched in shocked minerals and impact glass spherules, but also contains the highest concentrations of Os, Ir, Ru, and Rh compared to other El'gygytgyn impactites. This is—to a lesser extent—the result of admixture of a mafic component, but more likely the signature of a chondritic meteoritic component. However, the highly siderophile element contribution from target material akin to the mafic blocks of the ICDP drill core to the impactites remains poorly constrained. 相似文献
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K. Raschke 《Theoretical and Applied Climatology》1956,7(2):240-268
Zusammenfassung Die Energieumsätze eines Alocasiablattes setzen sich im wesentlichen aus dem sichtbaren und dem infraroten Strahlungsaustausch, den Konvektionsumsätzen und den Transpirationsverlusten zusammen. Sie wurden, getrennt in die Werte von Ober- und Unterseite des Blattes, unter verschiedenen Bedingungen in natürlichen Verhältnissen gemessen. Die Ergebnisse werden sowohl in der Form von Tagesläufen der Einzelkomponenten als auch in Bilanzen dargeboten.Die Ermittlungen wurden nach zwei Grundmethoden durchgeführt. Beide basierten einmal auf direkten Strahlungsmessungen, zum anderen entweder auf Bestimmungen der Wärmeübergangszahlen und der relativen Wasserbedeckungsfaktoren der Blattseiten oder auf Messungen der Temperatur- und Feuchtegradienten in Blattnähe. Beide Verfahren setzen die Kenntnis des Verhältnisses der Konvektionsverluste der beiden Blattseiten (das für das waagrechte Blatt meistens den Wert 1,0 annimmt) voraus, das zweitgenannte Verfahren dazu noch die des Verhältnisses der Austauschkoeffizienten für Wasserdampf und Wärme (das zu 1,00±0,05 gefunden wurde).Aus den Ergebnissen lassen sich Aussagen über die Eigenschaften des Alocasiablattes als Strahlungspartner im Sichtbaren und im Infraroten und über das Verhältnis der Transpirations- und der Konvektionsverluste eines besonnten Blattes und dessen Auswirkung auf die Blattemperatur herleiten. Die transpirationsbeeinflussende Wirkung der Strahlung erweist sich als groß, die des Windes als sehr gering, während die unabhängig voneinander reagierenden Stomata zu eigenartigen Schwankungen des Verhältnisses zwischen Ober- und Unterseitentranspiration Anlaß geben. Schließlich werden Wechselwirkungen zwischen Mikroklima und Wärmehaushalt besprochen.
Mit 8 Textabbildungen
Diese Arbeit wurde durch ein Stipendium der indischen Regierung im Rahmen des Indo-German Industrial Cooperation Scheme ermöglicht. 相似文献
Summary The energy-balance of an Alocasia leaf is made up primarily of the radiation exchange in the visible and infra-red, of the convective transfer, and of the losses by transpiration. Each of these items has been split up into the values for the upper and for the lower surfaces of the leaf and was measured under different conditions in situ. Results are presented in the form of graphs showing the diurnal variations of the different energy components as well as in the form of balance sheets.Two methods were applied, both of which required direct radiation measurements. The first method further utilised determinations of the heat transfer coefficients and the relative wetness factors of the leaf surfaces, whereas the other method was based on measurements of the gradients of temperature and humidity close to the leaf. For both cases the ratio of the convective losses from both the surfaces of the leaf must be known (which for a horizontal leaf almost always is equal to unity). In addition to this, the second method requires information about the ratio of the Austausch coefficients for water vapour and heat (experimentally it was found to be 1,00±0.05).The results give some insight regarding the radiative properties of an Alocasia leaf in the visible and infra-red and regarding the ratio of the losses by transpiration and by convection and its effects on leaf temperature in sunshine. The effect of radiation on transpiration proves to be strong; wind, however, has only little effect. The stomata of both the leaf surfaces were functioning independently of each other, which resulted in peculiar variations in the ratio of the water lost by the upper and lower surfaces. Finally mutual relationships between energy exchange and microclimate are discussed.
Résumé Le bilan énergétique d'une feuille d'Alocasia se compose principalement des échanges radiatifs de la lumière visible et infra-rouge ainsi que des échanges convectifs et des pertes de transpiration. Les composantes furent mesurées, séparément sur les surfaces supérieure et inférieure de la feuille, dans des conditions différentes en milieu naturel. Les résultats sont représentés par des bilans et, sous forme de graphiques, par les variations diurnes des différentes composantes d'énergie.A cet effet on a utilisé deux méthodes différentes qui se basent d'une part chacune sur des mesures directes du rayonnement, d'autre part, ou bien sur la détermination des échanges convectifs et des facteurs relatifs du recouvrement d'eau des surfaces de la feuille, ou bien sur des mesures des gradients de température et d'humidité a proximité de la feuille. Dans les deux méthodes on est sensé connaître le rapport des pertes de convection des deux surfaces de la feuille qui, en position horizontale est généralement de 1,0. Dans la seconde il faut encore connaître le rapport des coéfficients d'échange pour la vapeur d'eau et pour la chaleur qui fut trouvé être de 1,00±0,05.Les résultats obtenus permettent de nous renseigner au sujet des propriétés de la feuille d'Alocasia en ce qui concerne la radiation dans le domaine visible et infra-rouge, et le rapport des pertes de transpiration et de convection d'une feuille exposée au soleil et d'en déduire les effets sur la température de celle-ci. La radiation se révèle comme ayant une forte influence sur la transpiration, tandis que celle du vent est très faible. Les stomas des surfaces supérieure et inférieure réagissant séparément, provoquent de curieuses fluctuations du rapport de la transpiration de celles-ci. Finalement l'auteur discute encore les relations réciproques entre le microclimat et l'économie thermique.
Mit 8 Textabbildungen
Diese Arbeit wurde durch ein Stipendium der indischen Regierung im Rahmen des Indo-German Industrial Cooperation Scheme ermöglicht. 相似文献
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Andrei A. Andreev Elena Raschke Boris K. Biskaborn Stuart A. Vyse Jeremy Courtin Thomas Böhmer Kathleen Stoof-Leichsenring Stefan Kruse Lyudmila A. Pestryakova Ulrike Herzschuh 《Boreas: An International Journal of Quaternary Research》2021,50(3):652-670
This paper presents two new pollen records and quantitative climate reconstructions from northern Chukotka documenting environmental changes over the last 27.9 ka. Open tundra- and steppe-like habitats dominated between 27.9 and 18.7 cal. ka BP. Betula and Alnus shrubs might have grown in sheltered microhabitats but disappeared after 18.7 cal. ka BP. Although the climate was rather harsh, local herb-dominated communities supported herbivores as is evident by the presence of coprophilous spores in the sediments. The increase in Salix and Cyperaceae ~16.1 cal. ka BP suggests climate amelioration. Shrub Betula appeared ~15.9 cal. ka BP, and became dominant after ~15.52 cal. ka BP, whilst typical steppe communities drastically reduced. Very high presence of Botryococcus in the Lateglacial sediments reflects widespread shallow habitats, probably due to lake level increase. Shrub Alnus became common after ~13 cal. ka BP reflecting further climate amelioration. Simultaneously, herb communities gradually decreased in the vegetation reaching a minimum ~11.8 cal. ka BP. A gradual decrease of algae remains suggests a reduction of shallow-water habitats. Shrubby and graminoid tundra was dominant ~11.8–11.1 cal. ka BP, later Salix stands significantly decreased. The forest-tundra ecotone established in the Early Holocene, shortly after 11.1 cal. ka BP. Low contents of green algae in the Early Holocene sediments likely reflect deeper aquatic conditions. The most favourable climate conditions were between ~10.6 and 7 cal. ka BP. Vegetation became similar to the modern after ~7 cal. ka BP but Pinus pumila came to the Ilirney area at about 1.2 cal. ka BP. It is important to emphasize that the study area provided refugia for Betula and Alnus during MIS 2. It is also notable that our records do not reflect evidence of Younger Dryas cooling, which is inconsistent with some regional environmental records but in good accordance with some others. 相似文献
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Ulli Raschke Patrice Tristan Zaag Ralf Thomas Schmitt Wolf Uwe Reimold 《Meteoritics & planetary science》2014,49(6):978-1006
El'gygytgyn is a 3.6 Ma, 18 km diameter, impact crater formed in an approximately 88 Ma old volcanic target in Northeast Siberia. The structure has been the subject of a recent ICDP drilling project. In parallel to those efforts, a Russian‐German expedition was undertaken in summer 2011 to investigate the permafrost soil, lake terraces, and the volcanic rocks of the southern and eastern crater rim. This provided the unique opportunity for mapping and sampling of the volcanic target rocks around a large part of this complex impact structure. Samples from 43 outcrops were collected and analyzed petrographically and geochemically. The results were combined with earlier mapping outcomes to create a new geological map of this impact structure and its immediate environs, at the scale of 1:50,000. Compositions of our rock suites are compared with the lithologies of the 2009 ICDP drill core. The ignimbrite described as lower bedrock in the ICDP drill core shows petrographically and chemically strong similarities to the rhyolitic and rhyodacitic ignimbrites observed on surface. The suevite sequence exposed in the ICDP drill core is a mixture of all observed target rocks at their respective proportions in the area. In contrast to previous studies, the calculated average target composition of El'gygytgyn takes the contribution of the basic target rocks into consideration: mafic and intermediate rocks approximately 7.5%, and felsic rocks approximately 92.5%. 相似文献