Mark Z. Jacobson: Fundamental of Atmospheric Modeling     

Eberhard Renner 《Journal of Atmospheric Chemistry》2000,37(2):214-215

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Shock waves—Phenomenology,experimental, and numerical simulation     

Klaus Thoma  Ulrich Hornemann  Martin Sauer  Eberhard Schneider 《Meteoritics & planetary science》2005,40(9-10):1283-1296

Abstract— The purpose of this paper is to review the results of long‐term cooperation between Dieter Stöffler and the authors in the field of shock wave deformation of minerals and rocks. First, the principal phenomena of shock wave generation and propagation, predominantly in solid media, are presented, and then analytical and numerical mathematical treatment of shock wave processes on the basis of mass, momentum, and energy conservation laws will be described and discussed. Experimental methods of shock wave investigations by means of impact and explosive techniques are summarized, including hypervelocity acceleration facilities and high‐pressure explosive devices. Shock pressure barometry by means of mineralogical evidence of distinct material phase transitions and characteristic shock structures is also discussed.  相似文献   

Petrogenesis of Evolved Basalts and Rhyolites at Austurhorn, Southeastern Iceland: the Role of Fractional Crystallization   总被引：6，自引：0，他引：6  

FURMAN  TANYA; FREY  FRED A.; MEYER  PETER S. 《Journal of Petrology》1992,33(6):1405-1445

The Austurhorn intrusive complex in southeastern Iceland representsthe evolved hypabyssal remains of an eroded Tertiary (6–7Ma) central volcano. The complex consists of a layered gabbrointrusion, a composite granophyric stock, and abundant maficand felsic dikes. Mineralogical and geochemical trends amongcontemporaneous, compositionally diverse liquids from the complexprovide insight into the genesis of evolved basalts and rhyolitesin Iceland that are difficult to infer from studies of onlylavas. Mafic and felsic samples have comparable ranges in incompatibletrace element ratios (Ba/La and P/Ce) and Sr- and Pb-isotopes(O'Nions and Pankhurst, 1973; B. Hanan, pers. comm., 1988),suggesting derivation from a common parental composition. Majorand trace element variations throughout the Austurhorn suiteare consistent with fractional crystallization of the observedphenocrysts. Quartz-normative basalts were derived from parentalbasalt containing 7.8 wt.% MgO by extensive low-pressure crystallizationof olivine, augite, plagioclase, magnetite, and ilmenite. Thefractionating assemblage is consistent with the observed mineralogyof associated gabbro. Moreover, the cumulus mineralogy of thegabbro provides evidence for fractionation processes in a compositionalinterval not represented by dikes and sills (i.e., 54–63wt.% SiO₂).Diversity among the mafic dikes reflects severaladditional factors: (1) crystallization under conditions ofvariable oxygen fugacity; (2) separate mantle melting eventsthat produce different Ce/Yb values; (3) contamination of somemafic dikes at depth, presumably by interaction with felsicmagmas. Major and trace element trends among most felsic samples canbe modeled by fractionation of the observed mineral phases:plagioclase, K-feldspar, clinopyroxene, ilmenite, apatite, allanite,and zircon. Although crustal melting has been proposed for generatingIcelandic rhyolites, most Austurhorn felsic samples are unlikeliquids derived by melting of hydrated basalts. In particular,apatite and zircon have controlled the abundances of Zr, Hf,and the REE in the felsic rocks, but they are unlikely to beresidual phases during partial melting of basalt. One felsicdike, interpreted as a melt of an evolved source, shows petrographicevidence of in situ anatexis and also has anomalous trace elementabundances and unusually high ₂₀₆Pb/₂₀₄Pb.  相似文献   

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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Reaction progress in chloritic material: an electron microbeam study of the Taveyanne greywacke, Switzerland     

SCHMIDT  LIVI  & FREY 《Journal of Metamorphic Geology》1999,17(2):229-241

Chlorite and associated minerals from the volcanogenic Taveyanne metasediment of the western Helvetic nappes, Switzerland, were investigated by electron microprobe (EMP) and transmission electron microscopy (TEM) in order to determine their textural and chemical evolution during low-temperature metamorphism. EMP analyses of chloritic material from sub-greenschist facies outcrops show a decrease of Si and Σ(Ca, Na, K) with increasing metamorphic grade. A number of conclusions may be drawn from combined TEM images and analytical electron microscopy (AEM) data. 1 In diagenetic-grade samples, chlorite crystals (observed maximum defect-free distance=80 nm) always contain some 1 nm layers (with a maximum of 29% of all layers) and less frequently some 0.7 nm berthierine-like layers. With increasing grade, the amounts of 1 and 0.7 nm layers decrease, and most chlorite from the epizone is structurally pure or contains less than 2% of 1 nm layers. 2 A positive correlation was found between the amount of 1 nm layers and the Ca+K+Na content, indicating that the 1 nm layers are saponite. 3 Observations and calculations suggest that the transformation reaction of saponite to chlorite takes place by the replacement of the interlayer cations in saponite by brucite-like layers resulting in a local volume decrease. In contrast, the destruction of berthierine has only minor influence on the local bulk volume. These results confirm recent studies which show that the change in composition measured by EMP of diagenetic-grade chloritic material are mainly the result of mixtures of chlorite and saponite. The use of chlorite ‘geothermometry’ in such systems is greatly influenced by the presence of saponite and hence is not based on reaction equilibria, even though temperatures calculated in this study agree with temperatures derived from other methods. Therefore, chlorite evolution should be treated as a kinetically controlled grade indicator and developed as a qualitative scale similar to the illite crystallinity index.  相似文献   

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   

Orogenic Lherzolites and Mantle Processes: Editorial     

MENZIES  M. A.; VANNUCCI  R.; BODINIER  J. L.; FREY  F. A.; SHIMIZU  N.; KELEMEN  P. B.; RAMPONE  E.; RIVALENTI  G.; HOFFMAN  A. W. 《Journal of Petrology》2001,42(1):3-4

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