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   

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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The Relationship Between Shoreline Armoring and Adjacent Submerged Aquatic Vegetation in Chesapeake Bay and Nearby Atlantic Coastal Bays     

Christopher J. Patrick  Donald E. Weller  Micah Ryder 《Estuaries and Coasts》2016,39(1):158-170

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The summer radiation and heat budget of the Arctic and Antarctic     

G. Wendler  G. Weller 《Theoretical and Applied Climatology》1989,40(1-2):53-60

Summary For two pairs of arctic and antarctic stations, one coastal and one mountainous, an intercomparison between the summer radiation and surface energy budgets was carried out. The station pairs were similar in both latitude and altitude. It was found that the global radiation was larger for both antarctic stations. This is the result of a smaller Earth-Sun distance and cleaner atmosphere in Antarctica. Cloudiness, and for the arctic mountainous station substantial screening of the sun, also contributed. Further, large differences were found in the albedo. In the Arctic, the summer surfaces considered were bare tundra and melting snow, with respective albedos of 20 and 59%, while in Antarctica the surfaces considered were melting and dry snow, with albedos of 67 and 83% respectively.This results in a less positive radiation balance at both antarctic stations, despite the higher incoming global radiation. In turn, less sensible heat transfer from the surface to air results in lower temperatures in the Antarctic. The reduced rate of evaporation in Antarctica results in a drier atmosphere and less cloudy conditions.

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Zusammenfassung Für jeweils zwei arktische und antarktische Stationen, von denen jeweils eine an der Küste, eine in den Bergen liegt, wurden Vergleiche in bezug auf sommerliche Strahlungs- und Oberflächenenergiebilanz angestellt. Die Stationen liegen auf vergleichbarer Höhe und Breite. Es hat sich gezeigt, daß die Gesamt-Einstrahlung in den antarktischen Stationen größer war, aufgrund geringerer Erde-Sonnen-Distanz und der reineren Atmosphäre. Bewölkung und vor allem die für die arktischen Gebirgsstationen ausschlaggebende Sonnenabschirmung tragen auch zu dieser Differenz bei. Weiters wurden starke Albedounterschiede beobachtet. In der Arktis waren die Beobachtungsoberflächen im Sommer offene Tundra und schmelzender Schnee mit einer Albedo von 20 bzw. 59%, während die Antarktisoberflächen, nasser und trockener Schnee, eine Albedo von 67 bzw. 83% aufwiesen.Dies ergibt eine weniger positive Strahlungsbilanz für die beiden antarktischen Stationen trotz höherer Gesamteinstrahlung. Infolgedessen bewirkt die geringere Wärmeabgabe des Bodens an die Luft niedere Temperaturen in der Antarktis. Geringere Verdunstung ergibt somit geringere Bewölkung und eine trockenere Atmosphäre über der Antarktis.

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With 5 Figures  相似文献   

Preliminary results from the long-term upper-ocean study (LOTUS)     

Melbourne G. Briscoe  Robert A. Weller 《Dynamics of Atmospheres and Oceans》1984,8(3-4)

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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   

The measurement of radiative and conductive heat transfer in ice and snow     

Dr. Peter Schwerdtfeger  Gunter Weller 《Theoretical and Applied Climatology》1967,15(1-2):24-38

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