Untersuchungen über die Absorptionsanisotropie Longitudinaler Wellen in Sandsteinen     

Eckart Hurtig  Zdeněk Pros  Jiří Vaněk 《Studia Geophysica et Geodaetica》1967,11(3):281-290

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Heat flow map of Central and Eastern Europe (revised version)     

Vladimír Čermák  Eckart Hurtig  Reviewer A. Janáčková 《Studia Geophysica et Geodaetica》1977,21(3-4):394-397

Summary Revised version of the map showing the distribution of the surface heat flow on the territories of Bulgaria, Czechoslovakia, the German Democratic Republic, Hungary, Poland, Roumania and the European part of the USSR is presented and its general features are briefly discussed.  相似文献   

Mikrosondenuntersuchungen von Saussuriten in Abhängigkeit vom Metamorphosegrad und vom geochemischen Milieu     

Eckart Braun 《Contributions to Mineralogy and Petrology》1974,46(4):301-327

Zusammenfassung In einem Profil ansteigender Metamorphose werden im Stavanger-Gebiet/SW-Norwegen zwei Gesteinstypen, repräsentiert durch 17 Meta-Arkosen und Quarz-Feldspat-Gneise, sowie 19 metamorphe Tuffe und Tuffite, modellhaft auf ihre Saussuritparagenesen hin analysiert.Mikroskopische und mikroanalytische Untersuchungen zeigen eine weitestgehende Eduktabhängigkeit der Saussuritparagenesen. In calcitarmen granitoiden Edukten bilden sich schon im sehr schwach-metamorphen Stadium folgende mit Ab-reichem Plagioklas koexistierende Saussuritmineralien: 4 An-reicher Plagioklas+K-Feldspat+4 Eisenhydroxid + H₂O 2 Fe(III)Al₂-Epidot+Muskovit+Hämatit+2 Quarz. In calcitführenden Meta-Arkosen gewinnt die Mineralreaktion: An-Plagioklas+K-Feldspat+2 Eisenhydroxid+CO₂Calcit+Muskovit+ Hämatit+Quarz an Bedeutung. Im reduzierenden geochemischen Milieu der Meta-Tuffe und -Tuffite tritt in diesem metamorphen Bereich als charakteristische Neubildung Biotit neben Muskovit auf. Auch in den calcitreichen tuffitischen Proben koexistieren die Saussuritkomponenten Calcit, Muskovit, Hämatit, Quarz und Biotit.Die mikroanalytisch untersuchten Saussuritmineralien Plagioklas und Epidot zeigen anhand von annähernd 800 chemischen Vollanalysen in der Entwicklung ihrer Chemismen während der Metamorphose für beide Sedimente gleiche Trends. Im niedrigtemperierten Bildungsstadium der Saussurite können die An-Gehalte der Feldspäte in Abhängigkeit vom Edukt und aufgrund unterschiedlich intensiver Rekristallisation der Sedimente relativ stark schwanken. Die Epidote sind je nach primärem Fe(III)-Angebot mehr oder weniger eisenreich. In Richtung ansteigender Metamorphose stellen sich in den Epidoten beim Übergang zu oligoklasführenden Paragenesen maximale Fe(III)-Gehalte ein, die in Form eines rhythmischen Zonarbaus die wechselnden -Bedingungen im Verlauf der Metamorphose widerspiegeln. Bereits hier setzt der retrograde Saussuritisierungsprozeß ein: es reagieren Fe(III)Al₂-Epidot, Muskovit, Quarz, Hämatit und Albit/Oligoklas zu anorthitreicherem Plagioklas, Biotit und Wasser. Zusätzlich bildet sich durch die Zersetzung des Al-reichen Epidots Mikroklin.Die Untersuchung zur Wechselbeziehung zwischen dem Eisengehalt des Eduktes und dem der Epidote ergibt, daß die Fe(III)-Einbaurate der Epidote in keiner Weise von den Fe(III)-Konzentrationen der Meta-Sedimente beeinflußt wird, vielmehr können eduktspezifische Intervalle für die Eisenanreicherung der Epidote nachgewiesen werden.

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Electron microprobe investigations of saussurites dependent on metamorphic stage and geochemical environment

In a profile of ascending metamorphism, the saussuritic parageneses of two characteristic rock types, 17 acid meta-arkoses and 19 basic meta-tuffs and meta-tuffites, were investigated by microscopical and microanalytical methods.Microscopic studies reveal that the specific saussurite mineral association is dependent on the petrographic substratum. In very low stage metamorphism, granitic rocks show the following saussurite minerals coexisting with albite-rich plagioclase: 4 An-rich plagioclase+K-feldspar +4 ironhydroxide+H₂O2 Fe (III) Al₂-epidote + muscovite + hematite + 2 quartz. Phyllitic and calciferous meta-arkoses exhibit predominantly the following saussurite reaction: An-plagioclase + K-feldspar + 2 ironhydroxide + CO₂ calcite + muscovite + hematite + quartz. In the reducing environment of the meta-tuffs and meta-tuffites, biotite is formed in addition to muscovite.The changing chemical composition of the saussurite minerals (plagioclase and epidote) at different stages of metamorphism was determined by 800 quantitative electron microprobe analyses. The changes found in both rock types are nearly the same. During low metamorphic stage, the An-content of the plagioclases depends on the substratum and the variable intensity of recrystallization. The Fe-content of the epidotes is dependent on the amount of iron available.The epidotes are enriched in Fe toward the transition to oligoclase-bearing parageneses. These Fe-contents cause rhythmical zoning, representing varying conditions during metamorphism. With increasing metamorphic grade the retrograde process of saussuritization is initiated. The reactants are Fe (III) Al₂-epidote, muscovite, quartz, hematite, and albite/ oligoclase. The decomposition of these minerals leads to An-rich plagioclase, biotite, microcline, and H₂O.

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Herrn Prof. Dr. G. Müller, Clausthal, danke ich für viele anregende Diskussionen sowie für die kritische Durchsicht des Manuskriptes.

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Mein Dank gilt auch Herrn Dr. A. Schneider, Geochemisches Institut der Universität Göttingen, der mir freundlicherweise das Rucklidge-Korrekturprogramm für Silikatanalysen zur Verfügung stellte. Zu danken habe ich auch Herrn Dr. F. Wurm, Geologisches Landesamt Baden-Württemberg, für sein großzügiges Entgegenkommen und die tatkräftige Unterstützung bei der ergänzenden Probennahme im Gebiet der nordwestlichen Inseln des Boknfjords.

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Der Deutschen Forschungsgemeinschaft schulde ich Dank für die finanzielle Unterstützung dieser Arbeit.  相似文献   

Early Miocene carbonate ramp development in a warm ocean,North West Shelf,Australia     

Rosine Riera  Julien Bourget  Tony Allan  Eckart Hkansson  Moyra E. J. Wilson 《Sedimentology》2022,69(1):219-253

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The massive black hole at the galactic center     

A. Eckart  R. Genzel 《Journal of Astrophysics and Astronomy》1999,20(3-4):187-196

At the dynamic center of the Milky Way high spatial resolution, near-infrared imaging and spectroscopy have made it possible in the last few years to measure stellar velocities down to separations of less than five light days from the compact radio source SgrA* (in the constellation Sagittarius). These measurements make a compelling case for the presence of a compact, central dark mass of 2.6 × 10⁶ solar masses. Simple physical considerations show that this dark mass cannot consist of a stable cluster of stars, stellar remnants, substellar condensations or a degenerate gas of elementary particles. Energy equipartition requires that at least 105 solar masses must be associated with SgrA* itself and is enclosed within less than 8 light minutes (equivalent to 15 Schwarzschild radii of a million solar mass black hole). If one accepts these arguments it is hard to escape the conclusions that there must be a massive black hole at the core of the Milky Way.  相似文献   

The ALFA Laser Guide Star: Operation and Results     

R. Davies  A. Eckart  W. Hackenberg  T. Ott  D. Butler  M. Kasper  A. Quirrenbach 《Experimental Astronomy》2000,10(1):103-121

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Book reviews     

Gwyn Rowley  Mushtaqur Rahman  Fouad Ibrahim  Günther Schlee  Eckart Ehlers  Yola Verhasselt  Andreas G. Koestler  G. L. Kamukala  Wolf Tietze 《GeoJournal》1995,36(1):102-96

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VLT-SINFONI observations of Mrk 609 – A showcase for X-ray active galaxies chosen from a sample of AGN suitable for adaptive optics observations with natural guide stars     

J. Zuther  C. Iserlohe  J.-U. Pott  A. Eckart  W. Voges 《New Astronomy Reviews》2006,49(10-12):508

We will present first results of ESO-VLT AO-assisted integral-field spectroscopy of a sample of X-ray bright AGN with redshifts of 0.04 < z < 1. We constructed this sample by cross-correlating the SDSS and ROSAT surveys and utilizing typical AO constraints. This sample allows for a detailed study of the NIR properties of the nuclear and host environments with high spectral resolution on the 100 pc scale. These objects can then be compared directly to the local (z < 0.01) galaxy populations (observed without AO) at the same linear scale. As a current example, we will present observations of the z = 0.034 Seyfert 1.8 galaxy Mrk 609 with the new AO-assisted integral-field spectrometer SINFONI at the VLT. The successful observations show, that in the future – while having observed more objects – we will be able to determine the presence, frequency and importance of nuclear bars and/or circum-nuclear star forming rings in these objects and address the question of how these X-ray luminous AGN and their hosts are linked to optically/UV-bright QSOs, low-z QSOs/radio galaxies, or ULIRGs.  相似文献   

Stereo analysis of high-resolution SAR images for building height estimation in cases of orthogonal aspect directions     

Uwe Soergel  Eckart Michaelsen  Antje Thiele  Erich Cadario  Ulrich Thoennessen 《ISPRS Journal of Photogrammetry and Remote Sensing》2009,64(5):490-500

SAR stereo image analysis for 3D information extraction is mostly carried out based on imagery taken under same-side or opposite-side viewing conditions. For urban scenes in practice stereo is up to now usually restricted to the first configuration, because increasing image dissimilarity connected with rising illumination direction differences leads to a lack of suitable features for matching, especially in the case of low or medium resolution data. However, due to two developments SAR stereo from arbitrary viewing conditions becomes an interesting option for urban information extraction. The first one is the availability of airborne sensor systems, which are capable of more flexible data acquisition in comparison to satellite sensors. This flexibility enables multi-aspect analysis of objects in built-up areas for various kinds of purpose, such as building recognition, road network extraction, or traffic monitoring. The second development is the significant improvement of the geometric resolution providing a high level of detail especially of roof features, which can be observed from a wide span of viewpoints. In this paper, high-resolution SAR images of an urban scene are analyzed in order to infer buildings and their height from the different layover effects in views taken from orthogonal aspect angles. High level object matching is proposed that relies on symbolic data, representing suitable features of urban objects. Here, a knowledge-based approach is applied, which is realized by a production system that codes a set of suitable principles of perceptual grouping in its production rules. The images are analyzed separately for the presence of certain object groups and their characteristics frequently appearing on buildings, such as salient rows of point targets, rectangular structures or symmetries. The stereo analysis is then accomplished by means of productions that combine and match these 2D image objects and infer their height by 3D clustering. The approach is tested using real SAR data of an urban scene.  相似文献   

Deep infrared imaging and spectroscopy of the nearby late M‐dwarf DENIS‐P J104814 –395606     

R. Neuhuser  E.W. Guenther  J. Alves  N. Grosso  Ch. Leinert  Th. Ratzka  Th. Ott  M. Mugrauer  F. Comern  A. Eckart  W. Brandner 《Astronomische Nachrichten》2002,323(5):447-452

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