Electron impact polarization of X-ray lines from hydrogen-like ions during solar flares     

Eberhard Haug 《Solar physics》1981,71(1):77-89

The linear polarization of X-ray lines from highly charged hydrogenic ions is calculated under the assumption that the ions are collisionally excited by nonthermal electrons with an anisotropic pitch-angle distribution around magnetic field lines. The results are applied to the conditions in solar flares. The maximum degree of polarization to be expected is quite low, of the order of some percent. In case of favourable conditions it should be feasible to detect line polarization during flares if the short-wavelength fine-structure component of the L doublet is observed.  相似文献   

Böden der Rauhen Alb     

Diplomlandwirt Dr. Eberhard Ostendorff 《International Journal of Earth Sciences》1930,21(5):299-302

Ohne Zusammenfassung  相似文献   

The Chan Hol cave near Tulum (Quintana Roo,Mexico): evidence for long‐lasting human presence during the early to middle Holocene          下载免费PDF全文

Fabio Hering  Wolfgang Stinnesbeck  Jens Folmeister  Eberhard Frey  Sarah Stinnesbeck  Jerónimo Avilés  Eugenio Aceves Núñez  Arturo González  Alejandro Terrazas Mata  Martha Elena Benavente  Carmen Rojas  Adriana Velázquez Morlet  Norbert Frank  Patrick Zell  Julia Becker 《第四纪科学杂志》2018,33(4):444-454

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Galileo in-situ dust measurements in Jupiter’s gossamer rings     

Harald Krüger  Douglas P. Hamilton  Eberhard Grün 《Icarus》2009,203(1):198-213

Galileo was the first artificial satellite to orbit Jupiter. During its late orbital mission the spacecraft made two passages through the giant planet’s gossamer ring system. The impact-ionization dust detector on board successfully recorded dust impacts during both ring passages and provided the first in-situ measurements from a dusty planetary ring. During the first passage—on 5 November 2002 while Galileo was approaching Jupiter—dust measurements were collected until a spacecraft anomaly at 2.33R_J (Jupiter radii) just 16 min after a close flyby of Amalthea put the spacecraft into a safing mode. The second ring passage on 21 September 2003 provided ring dust measurements down to about 2.5R_J and the Galileo spacecraft was destroyed shortly thereafter in a planned impact with Jupiter. In all, a few thousand dust impacts were counted with the instrument accumulators during both ring passages, but only a total of 110 complete data sets of dust impacts were transmitted to Earth. Detected particle sizes range from about 0.2 to 5 μm, extending the known size distribution by an order of magnitude towards smaller particles than previously derived from optical imaging [Showalter, M.R., de Pater, I., Verbanac, G., Hamilton, D.P., Burns, J.A., 2008. Icarus 195, 361-377; de Pater, I., Showalter, M.R., Macintosh, B., 2008. Icarus 195, 348-360]. The grain size distribution increases towards smaller particles and shows an excess of these tiny motes in the Amalthea gossamer ring compared to the Thebe ring. The size distribution for the Amalthea ring derived from our in-situ measurements for the small grains agrees very well with the one obtained from images for large grains. Our analysis shows that particles contributing most to the optical cross-section are about 5 μm in radius, in agreement with imaging results. The measurements indicate a large drop in particle flux immediately interior to Thebe’s orbit and some detected particles seem to be on highly-tilted orbits with inclinations up to 20°. Finally, the faint Thebe ring extension was detected out to at least 5R_J, indicating that grains attain higher eccentricities than previously thought. The drop interior to Thebe, the excess of submicron grains at Amalthea, and the faint ring extension indicate that grain dynamics is strongly influenced by electromagnetic forces. These findings can all be explained by a shadow resonance as detailed by Hamilton and Krüger [Hamilton, D.P., Krüger, H., 2008. Nature 453, 72-75].  相似文献   

多层是不够的！喙嘴龙翼膜中新的软组织结构     

Helmut TISCHLINGER  Eberhard FREY 《地球学报》2010,31(Z1):64-64

Since the multilayered and multifunctional nature of the pterosaurian flight membrane was first described on the basis of superbly preserved material from the Solnhofen Lithographic Limestone (Upper Jurassic, South Germany) and the Lower Cretaceous Santana Formation of NE Brazil (Martill & Unwin 1989, Tischlinger & Frey 2002), subsequent investigations of several Rhamphorhynchus specimens under ultraviolet light have confirmed the presence of several layers and launched the first biomechanical analysis of the pterosaurian flight membrane (Frey et al. 2007).  相似文献   

Untersuchungen der seismischen Aktivität im Nordteil der Geotraverse IA     

Prof. Dr. Otto Förtsch  Dr. Eberhard Schmedes 《International Journal of Earth Sciences》1976,65(1):748-755

Zusammenfassung Mit Hilfe von vier seismologischen Stationen in Bad Reichenhall (BHG), Garmisch-Partenkirchen (GAP), Innsbruck (IBK) und Schlegeis (SCE) werden Kleinbeben im nördlichen Teil der Geotraverse I a beobachtet, die vom internationalen Erdbebendienst nicht registriert werden. In der Zeit von Januar 1972 bis Januar 1975 wurden etwa 200 Beben mit Herden im Untersuchungsgebiet aufgezeichnet. Seit März 1973 konnten die Epizentren von etwa 30 Beben bestimmt werden. Bei zwei Beben wurden makroseismische Untersuchungen durchgeführt. Es wurde die zeitliche und räumliche Verteilung der Beben bestimmt, um daraus auf rezente Bewegungen und Bewegungszonen in diesem Teil der Ostalpen zu schließen.

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In the northern part of the Geotraverse I a microearthquakes are investigated with four seismological stations situated in Bad Reichenhall (BHG), Garmisch-Partenkirchen (GAP), Innsbruck (IBK) and Schlegeis (SCE). Between January 1972 and January 1975 about 200 earthquakes were recorded with origins within the region under investigation. Since March 1973 the epicenters of about 30 earthquakes were determined. For two events macroseismic investigations were carried out. A seismicity map shows the nowadays mobile regions in this part of the eastern Alps.

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Résumé Grâce à quatre stations séismologiques situées à Bad Reichenhall (BHG), Garmisch-Partenkirchen (GAP), Innsbruck (IBK) et Schlegeis (SCE) environ 200 tremblements de terre ont été enrigistrés dans la région nord de la Geotraverse I a entre janvier 1972 et janvier 1975. Depuis mars 1973 les épicentres de 30 tremblements de terre ont été déterminés. A deux reprises des recherches macroséismiques ont eu lieu. La carte de la séismicité montre les régions actuellement actives dans cette partie des Alpes orientales.

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The role of radiation in an inversion-capped planetary boundary layer     

Eberhard Schaller  Helmut Kraus 《Boundary-Layer Meteorology》1981,20(4):485-495

In an inversion-capped planetary boundary layer (PBL), the structure of the turbulent fluxes as well as the height of the inversion are determined by the interaction of turbulent mixing in the PBL, large-scale subsidence above the PBL and radiational cooling. Here the sensitivity of the inversion height and of the turbulent fluxes due to radiational processes is investigated with the aid of a three-layered model for a well mixed PBL. For an example of the Trade-Wind region, the inversion height (i.e., the difference between surface pressure and pressure at the inversion level) varies between 46 and 257 mb and the surface flux of moist static energy between 417 and 99 W m^-2, if the (mean) radiative net flux divergence for both the inversion and the well-mixed layer is changed over a reasonable range of values. None of the parameterization schemes existing in the literature is able to describe these radiational effects in an appropriate way. This is due to the fact that these parameterizations are either not or not flexibly enough linked to the thermodynamical model parameter. Therefore the demand for an adequate parameterization of the radiational influence in a well-mixed PBL under a subsidence inversion is obvious.  相似文献   

Time and height variability of the sensible heat flux in the surface layer     

Eberhard Schaller 《Boundary-Layer Meteorology》1977,11(3):329-354

The energy-budget concept is used together with a high resolution spectral radiation model to study the time and height variation of the sensible heat flux and of the eddy thermal diffusivity for an actual case up to 50 m above ground. A data set of 32 h is chosen for this study. Time-height cross-sections of the local enthalpy changes, and the radiative and the sensible heat flux divergences are presented, which show the interaction of the two energy fluxes. It can be seen, for example, that during the transient hours from night to day the sensible heat flux divergence plays an outstanding role in the warming of the atmosphere, while during the clear night radiative cooling exceeds the cooling caused by the sensible heat flux. For the layer under consideration (0-50 m) a constancy of the sensible heat flux within 10% is obtained for seven hours only, namely for the time around noon and in the early afternoon. Selected night-time profiles of the thermal diffusivity are shown, which have their maximum below 48.3 m.The accuracy of the energy-budget method is studied in detail. The tests show that a high accuracy, with errors even less than 10% for some hours, can be expected, if special micrometeorological studies are made during the field phase and a layer depth of 50 cm or less is used in the radiation model.  相似文献   

Geologische Bearbeitung Südwest-Ägyptens     

Prof. Dr. Eberhard Klitzsch 《International Journal of Earth Sciences》1978,67(2):509-520

Zusammenfassung In einem auf die Klärung stratigraphischer, fazieller, paläogeographischer, hydrogeologischer und paläoklimatischer Fragen ausgerichteten Forschungsprogramm wird eine Bearbeitung Südwest-Ägyptens durchgeführt. Neben dem Nachweis einer altpaläozoischen — vermutlich ordovizischen — Vereisung und jüngerer, mariner paläozoischer Schichten erfolgte bisher eine Gliederung der ehemaligen Nubischen Serie dieses Gebietes in mehrere marine und kontinentale Sedimentationszyklen von jurassischem bis oberkretazischem Alter. Eine detaillierte geologische Karte von Südwest-Ägypten ist in Vorbereitung.

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First results of geological research in Southwestern Egypt are presented, which are part of a programme dedicated to stratigraphical, sedimentological, paleogeographical and hydro geological as well as paleoclimatical questions. The research programme is sponsored by Deutsche Forschungsgemeinschaft, it is carried out in cooperation with the Academy of Science of Egypt and it is backed by Continental Oil Company.Apart from the proof of an Early Paleozoic glaciation of probably Ordovician age, marine sediments of younger Paleozoic ages were found. The former Nubian Sandstone was subdivided into several formations of shallow marine to continental origin of Jurassic to Late Cretaceous age. A detailed geological map of Southwestern Egypt is under preparation.

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Résumé Les premiers résultats de recherche géologique dans le Sud-Ouest de l'Egypte sont présentés; ils font partie d'un programme d'étude des questions stratigraphiques, sédimentologiques, paléogéographiques, hydrogéologiques et paléoclimatiques. Ce programme est subventionné par la Deutsche Forschungsgemeinschaft, réalisé en coopération avec l'Académie des Sciences d'Egypte et assisté par Conoco.Outre la preuve d'une glaciation d'âge paléozoique — probablement ordovicien — et de sédiments marins paléozoiques plus jeunes, une division de l'ancien «Grès Nubie» de cette région en plusieurs cycles de sédimentation marine et continentale du Jurassique au Crétacé supérieur fut effectuée. Une carte géologique détaillée du Sud-Ouest de l'Egypte est en préparation.

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Decadal-scale variations of water mass properties in the deep Weddell Sea   总被引：2，自引：0，他引：2  

Eberhard?FahrbachEmail author  Mario?Hoppema  Gerd?Rohardt  Michael?Schr?der  Andreas?Wisotzki 《Ocean Dynamics》2004,54(1):77-91

Data from cruises between 1989 and 2003 with FS Polarstern were used to construct section-wide potential temperature and salinity time series of the main water masses in the Weddell Gyre. In tandem with these CTD data, two time series between 1989 and 1995 are presented from moored instruments in the central Weddell Sea. The regional and methodological consistency of the dataset allows us to quantify variations which are not visible in less homogeneous datasets. The data reveal significant temperature and salinity variations of the Warm Deep Water and the Weddell Sea Bottom Water on a decadal time scale. The longest time series were obtained at the prime meridian. Here warming is observed in the Warm Deep Water from 1992 to 1998 followed by cooling. In the Weddell Sea proper, measurements of instruments moored in the Weddell Sea Bottom Water layer recorded a temperature increase over 6 years at a rate of 0.01 °C a^–1. After the mooring period, CTD casts in 1998 point to a weakening of the trend. The warming trend in the bottom water occurs over most of the Weddell Sea, as detected in the additional CTD surveys. The variations are close to the detection level in the voluminous Weddell Sea Deep Water. The initial warming trend of the Warm Deep Water is consistent with warming trends reported in literature of subsurface waters of the Antarctic Circumpolar Current. The reversal of the trend in the Weddell Sea seems to be related to variations of the atmospheric conditions which can affect both the intrusion of Circumpolar Deep Water from the north and the circulation of the Weddell Gyre. Because the Warm Deep Water is the major source water for the formation of deep and bottom water in the Weddell Sea, it is suggested that its increase in temperature and salinity is likely to at least partly cause the variations which were observed in the bottom water.Responsible Editor: Jörg-Olaf Wolff  相似文献