Gesellschaftsmitteilungen     

M. Stemprok  W. Franke 《International Journal of Earth Sciences》1995,84(1):220-222

Ohne Zusammenfassung  相似文献   

Literal solution for Hill's lunar problem     

Dieter S. Schmidt 《Celestial Mechanics and Dynamical Astronomy》1979,19(3):279-289

A computer program for the manipulation of power series in several variables is used to find the first order solution to Hill's lunar problem. The ratiom of the mean motion of the Sun to that of the Moon is kept as a formal parameter. The series inm are known to converge very poorly. It is shown how efficient algorithms among them the Lie transformation allow us to compute the series inm as far as they are needed. When the series are evaluated at Brown's numerical value form the results achieve or exceed his accuracy.  相似文献   

An Alternate Procedure for Analyzing Aquifer Tests Using the Theis Nonequilibrium Solution     

O. L. Franke 《Ground water》1987,25(3):314-320

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Preface     

Jean Chapront  Jacques Henrard  Dieter Schmidt 《Celestial Mechanics and Dynamical Astronomy》1982,26(1):2-3

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Site Correction for Long Period Seismometers, Tiltmeters and Strainmeters     

Geoffrey King  Walter Zurn  Russ Evans  Dieter Emter 《Geophysical Journal International》1976,44(2):405-411

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Ein Entwicklungssatz als Mittel zur Prognose auf Grund der hydro-thermodynamischen Gleichungen einer trockenen,reibungslosen, baroklinen,kompressiblen modellatmosphäre     

Martin Franke Dipl.-Met. 《Pure and Applied Geophysics》1956,35(1):94-125

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Exact Brans-Dicke-Bianchi types-II,VIII, and IX stiff matter solutions     

Dieter Lorenz-Petzold 《Astrophysics and Space Science》1984,98(2):281-286

Exact solutions of the Brans-Dicke field equations of Bianchi types-II, VIII, and IX are derived. The solutions represent locally rotationally symmetric universes with stiff matter content.  相似文献   

The eastern continuation of the Cadomian orogen: U–Pb zircon evidence from Saxo-Thuringian granitoids in south-western Poland and the northern Czech Republic     

Żelaźniewicz  Andrzej  Dörr  Wolfgang  Bylina  Paweł  Franke  Wolfgang  Haack  Udo  Heinisch  Helmut  Schastok  Janina  Grandmontagne  Klaus  Kulicki  Cyprian 《International Journal of Earth Sciences》2004,93(5):773-781

We report U–Pb single zircon ages from three pre-Variscan granitoids in the NE part of the Bohemian Massif. The Platerówka granodiorite from the Lausitz-Izera Unit, the Polish Sudetes, has been dated at 533±9 Ma. The Bitouchov granite form the SW part of the South Krkonoe Unit, the Czech Sudetes, gave an age of 540+11/–10 Ma, and the Wdroe granodiorite in the Fore-Sudetic Block yielded 548±9 Ma. All these latest Vendian/Early Cambrian granitoids represent the post-tectonic expression of a late Proterozoic Cadomian orogenic cycle and demonstrate the eastward extent of the Cadomian basement into the Variscan orogen. Granodiorites of similar age have so far been reported from Brittany and especially from the Saxo-Thuringian Terrane to the NE and SW of the Elbe Fault Zone. We conclude that the Saxo-Thuringian Terrane extends across the Elbe and Sudetic Marginal Fault Zones into the Fore-Sudetic Block.  相似文献   

Provenance of Palaeozoic sandstones from the Carnic Alps (Austria): petrographic and geochemical indicators   总被引：1，自引：0，他引：1  

Dieter?MaderEmail author  Franz?Neubauer 《International Journal of Earth Sciences》2004,93(2):262-281

An integrated approach of petrographic analysis, whole rock geochemistry and microprobe analysis has been applied to obtain information on the geodynamic development and the provenance for Ordovician to Permian siliciclastic successions exposed within the Carnic Alps (Austria). Sandstone detrital mode and geochemical results refine previous geodynamic interpretations. Late Ordovician samples indicate a stable craton and recycled orogenic and, possible, extensional setting. The Early Carboniferous is interpreted to represent a compressional environment, followed by a Late Carboniferous molasse-type foreland basin, and a Permian extensional geodynamic setting. Contrasting geochemical patterns of post-Variscan and Permian sequences suggest a rift setting. Electron microprobe data of detrital white mica also indicate changes in the provenance. Compositional data reflect a shift from low- to medium-grade metamorphic (Ordovician) to high-grade metamorphic (Carboniferous) to low- to medium-grade metamorphic and plutonic source rocks (Permian). Additionally, our data show that various chemical discrimination diagrams do not include all possible ranges of sandstones, and that high contents of detrital mica and ultra-stable heavy minerals may cause misclassification. Consequently, we propose the use of multi-method approach for provenance studies, including the control of geochemical data by modal analysis and heavy mineral investigations.  相似文献   

SNR Surface Density Distribution in Nearby Galaxies     

Manami Sasaki  Dieter Breitschwerdt  Rodrigo Supper 《Astrophysics and Space Science》2004,289(3-4):283-286

Since supernova remnants (SNRs) are believed to be the primary sources of Galactic cosmic rays (CRs), their distribution in galaxies is an important basis for modelling and understanding the distribution of the CRs and their γ-ray spectrum. We analysed the radial surface density of X-ray and radio selected SNRs in the Large Magellanic Cloud (LMC) and M 33. Both in X-rays and in radio, the surface densities of the SNRs are in excellent agreement in both galaxies, showing an exponential decay in radius. The results were compared to the SNR distribution in the spiral galaxies M 31 and NGC 6946 as well. The radial scale length of the distribution is $\frac{1} {4} $ ? $\frac{1} {3} $ of the radius of the galaxies, fully consistent with values derived for the Milky Way, the LMC, and M 33. Therefore, not only the radio SNRs, but also the X-ray detected SNR sample can be interpreted to be representative for the CR sources within a galaxy.  相似文献