Obituary for Dr. Wolfgang Engel     

Philip E. LaMoreaux  Gunter Dörhöfer  Jörg Matschullat 《Environmental Geology》2006,50(4):459-459

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GGM02 – An improved Earth gravity field model from GRACE     

B. Tapley  J. Ries  S. Bettadpur  D. Chambers  M. Cheng  F. Condi  B. Gunter  Z. Kang  P. Nagel  R. Pastor  T. Pekker  S. Poole  F. Wang 《Journal of Geodesy》2005,79(8):467-478

A new generation of Earth gravity field models called GGM02 are derived using approximately 14 months of data spanning from April 2002 to December 2003 from the Gravity Recovery And Climate Experiment (GRACE). Relative to the preceding generation, GGM01, there have been improvements to the data products, the gravity estimation methods and the background models. Based on the calibrated covariances, GGM02 (both the GRACE-only model GGM02S and the combination model GGM02C) represents an improvement greater than a factor of two over the previous GGM01 models. Error estimates indicate a cumulative error less than 1 cm geoid height to spherical harmonic degree 70, which can be said to have met the GRACE minimum mission goals. Electronic Supplementary Material Supplementary material is available in the online version of this article at  相似文献   

The thermodynamic properties of H2O in magnesium and iron cordierite     

G. B. Skippen  Avril E. Gunter 《Contributions to Mineralogy and Petrology》1996,124(1):82-89

 The equilibrium water content of cordierite has been measured for 31 samples synthesized at pressures of 1000 and 2000 bars and temperatures from 600 to 750° C using the cold-seal hydrothermal technique. Ten data points are presented for pure magnesian cordierite, 11 data points for intermediate iron/magnesium ratios from 0.25 to 0.65 and 10 data points for pure iron cordierite. By representing the contribution of H₂O to the heat capacity of cordierite as steam at the same temperature and pressure, it is possible to calculate a standard enthalpy and entropy of reaction at 298.18° K and 1 bar for, (Mg,Fe)₂Al₄Si₅O₁₈+H₂O ⇄ (Fe,Mg)₂Al₄Si₅O₁₈.H₂O Combining the 31 new data points with 89 previously published experimental measurements gives: ΔH ^° _r =–37141±3520 J and ΔS ^° _r =–99.2±4 J/degree. This enthalpy of reaction is within experimental uncertainty of calorimetric data. The enthalpy and entropy of hydration derived separately for magnesian cordierite (–34400±3016 J, –96.5±3.4 J/degree) and iron cordierite (–39613±2475, –99.5±2.5 J/degree) cannot be distinguished within the present experimental uncertainty. The water content as a function of temperature, T(K), and water fugacity, f(bars), is given by n _H2O=1/[1+1/(K ⋅ f _H2O)] where the equilibrium constant for the hydration reaction as written above is, ln K=4466.4/T–11.906 with the standard state for H₂O as the gas at 1 bar and T, and for cordierite components, the hydrous and anhydrous endmembers at P and T. Received: 2 August 1994/Accepted: 7 February 1996  相似文献   

探测冰盖和多年冻土层的融冰探头研发     

Norbert I. K 《冰川冻土》2004,26(Z1):310-318

The exploration of ice sheets by melting vertical holes into the ground has some tradition in terrestrial glaciology. Such probes have been used since the 1960's to investigate the vertical structure of the ice in Greenland and Antarctica and in alpine glaciers. In this paper we look into the possibility to develop similar devices for use on extraterrestrial icy bodies, like e.g. the polar areas on Mars or the icy satellites of the outer solar system. We report on some basic experiments performed in the cryo-vacuum laboratory of the Space Research Institute of the Austrian Academy of Sciences, Graz. In these experiments the penetration of a simple melting probe into compact and porous water ice (with a snow-like texture) was monitored, both under vacuum conditions and under air pressure. The observed penetration speeds for a given power supply are compared with a simple mathematical model. We conclude that a miniature melting probe with small overall dimensions and a reasonable power demand could well be part of the payload of a future planetary mission, for example to the poles of Mars. Such missions are currently under discussion in several space agencies. Moreover such probes could also e? ectively be used in terrestrial environments. A possible design is presented at the end of the paper.  相似文献   

Turbulent Humidity Fluctuations in the Convective Boundary Layer: Case Studies Using Water Vapour Differential Absorption Lidar Measurements     

Shravan Kumar Muppa  Andreas Behrendt  Florian Späth  Volker Wulfmeyer  Simon Metzendorf  Andrea Riede 《Boundary-Layer Meteorology》2016,158(1):43-66

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An approach for estimating time-variable rates from geodetic time series   总被引：1，自引：0，他引：1  

Olga Didova  Brian Gunter  Riccardo Riva  Roland Klees  Lutz Roese-Koerner 《Journal of Geodesy》2016,90(11):1207-1221

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Complex zoning and resorption in Breunnerite from hall in Tyrol,Austria: Evidence from back-scattered electron microscopy     

Mag. Ch. Spötl 《Mineralogy and Petrology》1989,40(3):225-233

Summary Back-scattered electron imagery (BSE) coupled with energy-dispersive X-ray elemental analysis was applied to petrographic investigations of recrystallized, anchimetamorphic breunnerites (ferroan magnesites). Analyses of polished thin sections allowed the recognition of a complex zoning pattern, invisible by transmitted or reflected light microscopy. Breunnerite precipitation and replacement started with (Mg_0.90Fe_0.07Ca_0.01Mn_0.02) CO₃ and proceeded towards (Mg_0.73Fe_0.22Ca_0.00Mn_0.05)CO₃. This precipitation sequence was interrupted by at least two major events of reverse zoning (i.e. Fe-rich zones followed by Fe-poor ones). Resorption surfaces in Fe-poor zones are common and prove that short-term fluctuations occurred in the paleobrine composition and/or paleotemperature.

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Nachweis komplexer zonierung und resorption im breunnerit mittels Rückstreuelektronenbilder

Zusammenfassung Breunnerit-Proben von der Typlokalität evaporitischer Magnesitlagerstätten (ehemaliger Salzbergbau Hall in Tirol/Österreich) wurden an Hand von Rückstreuelektronen(BSE)-Bildern und energiedispersiven Röntgenanalysen (EDS) untersucht. Während Durch- und Auflichtmikroskopie lediglich eine zweiphasige Kristallisationsgeschichte erkennen ließen, konnte mittels BSE-Bildern eine detaillierte Rekonstruktion der spätdiagenetischen bzw. anchimetamorphen Breunneritbildung durchgeführt werden. Ein genereller Trend zu Fe-reicheren, häufig oszillierend-zonierter Mischkristalle der Reihe Magnesit-Siderit konnte erkannt werden, der jedoch von mindestens zwei invers zonierten Phasen unterbrochen wurde. Resorptionserscheinungen in den Fe-ärmeren Zonen sind verbreitet und belegen kurzfristige Fluktuationen in der Paläofluid-Zusammensetzung und/oder dessen Paläotemperatur.

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With 5 Figures  相似文献   

Identification and age of neoformed Paleozoic feldspar (adularia) in a Precambrian basement core from Scioto County,Ohio, USA     

Teresa M. Mensing  Gunter Faure 《Contributions to Mineralogy and Petrology》1983,82(4):327-333

Fourteen core samples of Precambrian granitic gneisses from a well drilled in the Green Township, Scioto County, Ohio were studied to determine the origin of alkali feldspar in these rocks. The well intersected the basement at a depth of 1,700 m and penetrated 11.3m of Precambrian crystalline rocks. Petrographically the samples in the upper 6.4 m of the basement core show evidence of severe alteration by the presence of hematite, limonite and chlorite and by the absence of plagioclase. Alkali feldspars from this part of the core are turbid, have a low 2 V of about 10°, are highly enriched in K, have low Na and Rb concentrations, lack cathode luminescence, and form a straight line on a Rb-Sr isochron diagram yielding a date of 599±69 Ma. Core samples from below 6.4 m appear relatively fresh and unaltered. Alkali feldspar from this portion of the core is orthoclase, shows uniform blue luminescence and gives a Rb-Sr date of 1,162±11 Ma. These results indicate that feldspars in the lowest part of the core are primary minerals that crystallized during the Grenville Orogeny, whereas the K-feldspar in the top of the core is of low-temperature secondary origin. The formation of this feldspar is explained as a consequence of chemical weathering of primary feldspar during late Precambrian time to clay minerals that were later reconstituted under low-temperature hydrothermal conditions as K-feldspar (adularia) by reactions with brines derived from the overlying Mt. Simon Formation of Cambrian age.Laboratory for Isotope Geology and Geochemistry (Isotopia), Contribution No. 68  相似文献   

Lithospheric thickness beneath the southern Kenya Rift: implications from basalt geochemistry     

Anton P. Roex  Andreas Späth  Robert E. Zartman 《Contributions to Mineralogy and Petrology》2001,142(1):89-106

Geochemical data are reported for samples from the flanks and floor of the southern Kenya Rift Valley in the Lake Magadi area, and from two central volcanoes located within the rift valley. Rift lavas include samples of Singaraini and Ol Tepesi basalts on the eastern flank, Kirikiti basalts from the western flank, and plateau trachytes from the rift valley floor. Central volcano samples are from Ol Esayeiti and Lenderut located on the eastern flank. The rift basalts are mildly ne-normative, moderately evolved (Mg#=0.39-0.62) alkali basalts and show an overall range in differentiation. Incompatible trace element abundances are moderately elevated (Nb=17-51; Zr=93-274; La=17-55 ppm) and show strongly coherent variations and constant inter-element ratios (e.g. Zr/Nb=4.2-5.5; Nb/Ta=17.5ǂ.4; (La/Sm)_n=7.3ǃ.1); isotope ratios are restricted in range (⁸⁷Sr/⁸⁶Sr=0.70393-0.70436; ¹⁴³Nd/¹⁴⁴Nd=0.51272-0.51280; ²⁰⁶Pb/²⁰⁴Pb=19.87-19.92; ²⁰⁷Pb/²⁰⁴Pb=15.68-15.70; ²⁰⁸Pb/²⁰⁴Pb=39.56-39.71). Central volcano lavas are more alkaline in character and include basanite (Ol Esayeiti; Mg# >60) and hawaiite to benmoreite (Lenderut; Mg#=0.48-0.38). Incompatible element ratio are similar to those of the rift basalts, although the chondrite normalised REE patterns are steeper (La/Sm)_n=17.4ǃ.2). ⁸⁷Sr/⁸⁶Sr (0.70358, 0.70391), ¹⁴³Nd/¹⁴⁴Nd (0.51280, 0.51267), ²⁰⁶Pb/²⁰⁴Pb (19.96,20.17), ²⁰⁷Pb/²⁰⁴Pb (15.66,15.76) and ²⁰⁸Pb/²⁰⁴Pb (39.80,40.00) ratios of Ol Esayeiti basanites are similar to the rift basalts, whereas the Lenderut lavas have unusually low¹⁴³Nd/¹⁴⁴Nd (0.512388-0.512453) ratios for their ⁸⁷Sr/⁸⁶Sr (0.70370-0.70481) ratios, and distinctly less radiogenic and variable Pb isotope compositions (²⁰⁶Pb/²⁰⁴Pb=17.93-19.01; ²⁰⁷Pb/²⁰⁴Pb=15.43-15.58; ²⁰⁸Pb/²⁰⁴Pb=37.91-39.14). An integrated model is developed in which the geochemical signature of the lavas is attributed to variable degrees of melting to depths within the garnet stability field, and in the presence of residual amphibole. The stability fields of these phases in P-T space indicates that the lavas must have formed within the sub-continental lithosphere rather than within the underlying ambient asthenosphere or a rising mantle plume. The subcontinental lithospheric mantle must therefore extend to a depth of at least 75 km beneath the Lake Magadi area, which contrasts with recent gravity models for the area, which infer that lithospheric mantle is absent beneath this section of the southern Kenya Rift.  相似文献   

Statistical characteristics of the vertical ozone distribution in mid-latitudes     

Spänkuch  D.  Döhler  W.  Kubasch  H. 《Pure and Applied Geophysics》1973,106(1):1208-1218

Summary The correlation matrix for the vertical ozone distribution and the temperature-ozone cross-correlation matrix, which was calculated from ozone soundings made over Berlin between 1967 and 1970, the statistical structure of the vertical ozone profile (correlation coefficients, average profiles, average standard deviation, relative variability) was derived for the three ozone seasons. The partial ozone pressure does not at all heights follow a normal distribution (e. g. at tropopause level). Generally, the correlation between tropospheric and stratospheric ozone is rather poor. In some layers the highest correlation coefficients, i.e. –0.3 and +0.4, occur in autumn (October to December) and in winter and spring (January to April). The correlation between the ozone amounts of various stratospheric layers is distinct in autumn, less distinct in summer (May to September) and entirely missing from January to April. Conspicuous cross-correlations between temperature and ozone have been found for all three seasons. a) With a negative correlation between tropospheric temperature and middle tropospheric to middle stratospheric ozone (maximum up to –0.8); b) with a rather strong positive correlation between the ozone amount and the temperature in the lower stratosphere (maximum up to +0.84); c) with a positive correlation between the ozone amount of the middle stratosphere and the temperature of the middle stratosphere (maximum up to +0.8). The highest correlation coefficients occur in autumn.  相似文献