Laboratory simulation experiments on the solid-state greenhouse effect in planetary ices     

Erika Kaufmann  Norbert I. Kömle  Günter Kargl 《Icarus》2006,185(1):274-286

Icy surfaces like the polar caps of Mars, comets, Edgeworth-Kuiper belt objects or the surface areas of many moons in the outer Solar System behave different than rock and soil surfaces when irradiated by solar light. The latter ones absorb and reflect incoming solar radiation immediately at the surface. In contrast, ices are partially transparent in the visible spectral range and opaque in the infrared. Due to this fact it is possible for the solar radiation to reach a certain depth and increase the temperature of the sub-surface layers directly. This internal temperature rise is called “solid-state greenhouse effect,” in analogy to the classical greenhouse effect in an atmosphere. It may play an important role in the energy balance of various icy bodies in the Solar System. Within the scope of a project conducted at the Space Research Institute of the Austrian Academy of Sciences in Graz the solid-state greenhouse effect was investigated experimentally and theoretically. A number of experiments with diverse materials, focussing mainly on layered samples with a surface cover consisting of transparent H₂O-ice, were performed. The samples were irradiated under cryo-vacuum conditions by a solar simulator. The temperature distributions inside the samples were measured and compared with the results of numerical model calculations. We found that the predicted sub-surface temperature maximum is very clearly measurable in glass beads samples with various particle size distributions, but can also be detected in transparent compact surface ice layers. However, in the latter case it is less distinct than originally expected. Measuring the effect by laboratory methods turned out to be a difficult task due to the shallow depth where the temperature maximum occurs.  相似文献   

Excitation of Radial P-Modes in the Sun and Stars     

Robert Stein  Dali Georgobiani  Regner Trampedach  Hans-Günter Ludwig  Åke Nordlund 《Solar physics》2004,220(2):229-242

P-mode oscillations in the Sun and stars are excited stochastically by Reynolds stress and entropy fluctuations produced by convection in their outer envelopes. The excitation rate of radial oscillations of stars near the main sequence from K to F and a subgiant K IV star have been calculated from numerical simulations of their surface convection zones. P-mode excitation increases with increasing effective temperature (until envelope convection ceases in the F stars) and also increases with decreasing gravity. The frequency of the maximum excitation decreases with decreasing surface gravity.  相似文献   

National flood discharge mapping in Austria   总被引：5，自引：0，他引：5  

Ralf Merz  Günter Blöschl  Günter Humer 《Natural Hazards》2008,46(1):53-72

This article presents the approach and the results of a study in which 30, 100 and 200 year return period flood discharges were estimated for 26,000 km of Austrian streams. Three guiding principles were adopted: combination of automatic methods and manual assessments by hydrologists to allow speedy processing and account for the local hydrological situation; combination of various sources of information including flood peak samples, rainfall data, runoff coefficients and historical flood data; and involvement of the Hydrographic Services to increase the accuracy and enhance the acceptance of results. The flood discharges for ungauged catchments were estimated by the Top-kriging approach with manual adjustment to the local flood characteristics. The adopted combination approach proved to be very efficient both in terms of the project time required and in terms of the accuracy and acceptability of the estimated flood discharges of given return periods.  相似文献   

Neuere Veröffentlichungen     

H. C. Freiesleben  Günter Dietrich  F. Lucht  H. G. Macht 《Ocean Dynamics》1953,6(1):40-41

Ohne Zusammenfassung  相似文献   

Neuere Veröffentlichungen     

Günter Dietrich  Walter Hansen  A. Schumacher  F. Errulat 《Ocean Dynamics》1952,5(2-3):153-156

Ohne Zusammenfassung  相似文献   

The geomagnetic field in 1996 according to measurements of the geomagnetic observatory wingst     

Günter Schulz 《Ocean Dynamics》1996,48(2):203-206

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Advances in the use of observed spatial patterns of catchment hydrological response   总被引：2，自引：0，他引：2  

Rodger B Grayson  Günter Blschl  Andrew W Western  Thomas A McMahon 《Advances in water resources》2002,25(8-12)

Over the past two decades there have been repeated calls for the collection of new data for use in developing hydrological science. The last few years have begun to bear fruit from the seeds sown by these calls, through increases in the availability and utility of remote sensing data, as well as the execution of campaigns in research catchments aimed at providing new data for advancing hydrological understanding and predictive capability. In this paper we discuss some philosophical considerations related to model complexity, data availability and predictive performance, highlighting the potential of observed patterns in moving the science and practice of catchment hydrology forward. We then review advances that have arisen from recent work on spatial patterns, including in the characterisation of spatial structure and heterogeneity, and the use of patterns for developing, calibrating and testing distributed hydrological models. We illustrate progress via examples using observed patterns of snow cover, runoff occurrence and soil moisture. Methods for the comparison of patterns are presented, illustrating how they can be used to assess hydrologically important characteristics of model performance. These methods include point-to-point comparisons, spatial relationships between errors and landscape parameters, transects, and optimal local alignment. It is argued that the progress made to date augers well for future developments, but there is scope for improvements in several areas. These include better quantitative methods for pattern comparisons, better use of pattern information in data assimilation and modelling, and a call for improved archiving of data from field studies to assist in comparative studies for generalising results and developing fundamental understanding.  相似文献   

Results of a 36-hour storm surge prediction of the North Sea for 3 January 1976 on the basis of numerical models     

Drof. Dr. Günter Fischer 《Ocean Dynamics》1979,32(3):89-99

Summary To explore the feasibility of forescasting North Sea storm surges by integrating numerically a combined atmospheric-oceanographic physical model, the severe storm and the resulting water levels occurring on 3 January 1976 were simulated as a first step into this direction. For this purpose, the atmospheric model was run with a resolution of 8 levels in the vertical and a horizontal grid spacing of 1.4° in latitude and 2.8° in longitude on the hemisphere. The initial conditions are based upon observations of 2 January 1976, 12 GMT, i.e. about 24 hours before the storm reached its greatest intensity in the southern parts of the North Sea.The surface wind predicted by the atmospheric model was converted into stress values through a bulk formula which then entered the vertically integrated North Sea model, to yield the desired water elevations in a 22 km-grid. Moreover, also the observed wind, stemming from a careful re-analysis of the storm situation, was handled in the same way. The numerically obtained results were compared with gauge measurements at a number of coastal stations.

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Ergebnisse einer 36stündigen Vorhersage der Nordsee-Sturmflut am 3. Januar 1976 aufgrund von numerischen Modellen

Zusammenfassung Zur Untersuchung der Möglichkeiten, Sturmfluten mit physikalischen Modellen der Atmosphäre und der Nordsee vorherzusagen, wurde als erster Schritt in dieser Richtung die schwere Sturmflut an der deutschen Nordseeküste vom 3. Januar 1976 nachgerechnet. Hierzu wurde das im Sonderforschungsbereich 94 entwickelte Atmosphärenmodell auf der Grundlage der hydro- und thermodynamischen Gleichungen mit einer Auflösung von 8 Flächen in der Vertikalen sowie 1,4° in der geographischen Breite und 2,8° in der geographischen Länge auf der gesamten Nordhalbkugel über 36 Stunden numerisch integriert. Als Eingangsdaten dienten die Beobachtungen vom 2. Januar 1976, 12 Uhr. dieser Termin liegt ca. 24 Stunden vor Eintritt des stärksten Sturmes im Bereich der Deutschen Bucht.Die auf diese Weise prognostizierte Windverteilung wurde über der Nordsee in Schubspannungswerte überführt, woraus das Nordseemodell mit den hydrodynamischen Gleichungen die Wasserstandswerte in einem 22-km-Netz berechnete. In entsprechender Weise wurde mit einem aus Beobachtungen während dieses Zeitraums gewonnenen Windfeld verfahren; diesem lag eine besonders sorgfältige, nachträglich angefertigte Analyse des Seewetteramts Hamburg zugrunde. Die so errechneten Wasserstände sind dann mit Pegelmessungen verglichen worden.

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Résultats d'une prédiction d'onde de tempête de 36 heures de la mer du Nord pour le 3 janvier 1976 sur la base de modèles numériques

Résumé Afin d'étudier la possibilité de prévior les ondes de tempête en mer du Nord en intégrant numériquement un modèle physique combiné atmosphère-océan, la forte tempête du 3 janvier 1976 et des niveaux d'eau qui en ont résulté ont été simulés comme premier pas dans cette voie. Dans ce but, on a fait fonctionner le modèle atmosphérique avec une résolution de 8 niveaux dans le plan vertical et un réseau horizontal aux pas de 1,4° en latitude et de 2,8° en longitude sur l'hémisphère. Les conditions initiales sont basées sur les observations du 2 janvier 1976 à 12h GMT, c'est-à-dire environ 24 heures avant que la tempête n'atteignît sa plus forte intensité dans les parties méridionales de la mer du Nord.Le vent en surface prédit par le modèle atmosphérique était converti par l'intermédiaire d'une formule globale en valeurs de tensions qui étaient alors introduites dans le modèle de la mer du Nord intégré verticalement, pour obtenir les hauteurs d'eau désirées, dans un réseau de 22 km de côté. En outre, le vent observé, issu d'une nouvelle analyse soignée de la situation de tempête, était aussi traité de la même manière. Les résultats obtenus numériquement furent comparés aux mesures fournies par les marégraphes en un certain nombre de stations côtières.

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Hydrothermale Lösungen     

Dr. Günter Strübel 《International Journal of Earth Sciences》1968,58(1):259-273

Zusammenfassung Das hydrothermale Auflösungsverhalten der vorwiegend als Gangarten auf-tretenden Mineralphasen Fluorit (CaF₂), Baryt (BaSO₄), Cölestin (SrSO₄) und Anglesit (PbSO₄) läßt sich übersichtlich in einem Temperatur-Löslichkeitsdiagramm darstellen und mit dem bekannten, qualitativ ähnlichen System SiO₂-H₂O vergleichen.Gegenüber dem molekulardispers gelösten SiO₂ ergeben sich aber für die in Ionen dissoziierten Lösungen der schwerlöslichen Sulfate und des Fluorits beträchtliche Verschiebungen der Sättigungsgleichgewichte, insbesondere bei Anwesenheit von Elektrolyten als Lösungsgenossen.Diese Beeinflussung, die für die genetischen Verhältnisse der Minerallagerstätten von entscheidender Bedeutung ist, wird für 0,1–2,0 normale NaCl-Lösungen im NaCl-Konzentrations-Löslichkeits-Diagramm der Minerale Fluorit, Baryt, Cölestin und Anglesit isotherm bis zum Siedepunkt der wäßrigen Mischphasen untersucht.Ferner wird das Löslichkeitsverhalten in den ternären Systemen BaSO₄-NaCl-H₂O und SrSO₄-NaCl-H₂O für Baryt und Cölestin gegen 2,0n NaCl-Lösungen entlang der Grenzkurve des Dreiphasengebietes und für die Isochoren 0,326 bis 0,6 bis 600° C und 2000 Bar dargestellt und mit den entsprechenden Verhältnissen der reinen wäßrigen Systeme verglichen.Ein abweichendes inkongruentes Auflösungsverhalten von Alumosilikaten mit Schichtgitterstruktur läßt sich am Beispiel des Muskovits durch die experimentelle Bestimmung der nichtstöchiometrischen Molekularverhältnisse SiO₂/K₂O und SiO₂/Al₂O₃ in den gesättigten Lösungen für den hydrothermalen Existenzbereich des Muskovits nachweisen.

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The behaviour of solubility for some minerals, which were for the most part found as vein minerals, was determined experimentally and is represented by summarizing diagrams.In the temperature-solubility diagram the hydrothermal solubility of fluorite, barite, celestine and anglesite is compared to the solubility of quartz and muskovite for the boundary curve of the three-phase region and for some isochores. As opposed to SiO₂, which is molecularly dispersed in solution, the ionic solutions of the systems CaF₂-H₂O, BaSO₄-H₂O, SrSO₄-H₂O and PbSO₄-H₂O show considerable displacement of the saturation equilibrium when other components are present in the solution.This influence on the solubility, significant for the genetic relations of mineral deposits, was quantitatively analyzed for 0.1–0.2 n-NaCl solutions. The results are isothermally shown in the NaCl-concentration solubility diagram within the boundaries of room temperature and the boiling point of the aqueous mixed phases.In the tenary systems BaSO₄-NaCl-H₂O and SrSO₄-NaCl-H₂O, the hydro-thermal solubility of barite and celestine in 2.0 n-NaCl solutions is also shown for the range of the boundary curve of the three-phase region and for the isochores 0.326–0.6 up to a temperature of 600° C and a pressure of 2000 bar. These solubilities are then compared with the diagrams of solubility for pure aqueous solutions.The irregular and incongruent behaviour of the solubility of aluminium-silicates of a layered-lattic structure is demonstrated for the system KAl₂(OH)₂-AlSi₂O₁₀-H₂O in the presence of muscovite by experimental determination of the non-stoechiometric molecular proportions of SiO₂K₂O and SiO₂ Al₂O₃. Such determination was conducted in saturated solutions for the hydrothermal range of the existence of muscovite.The geological importance of the knowledge of hydrothermal data of solubility and their application to the process of the hydrothermalmagmatic series and hydrothermalmetamorphosis is discussed.

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Résumé Le comportement de dissolution expérimentalement déterminé de certains minéraux trouvés surtout en filons est exposé en le résumant par diagrammes.La solubilité hydrothermique de fluorine, barytine, célestine et anglésite est comparée pour la courbe limitante (de la région triphasée) et pour les isochores 0,326–0,6 g.cm³ du diagramme température-solubilité avec le comportement de dissolution du quartz et de la muscovite. Les solutions ioniques des systèmes CaF₂H₂O, BaSO₄-H₂O, SrSO₄-H₂O et PbSO₄-H₂O montrent, comparées au SiO₂ dissous en dispersion moléculaire, de différences importantes d'équilibres de saturation en présence d'associés de solution.Cette influence sur la solubilité qui est d'une importance décisive pour les conditions génétiques des gisements de minéraux, a été examinée quantitativement pour les solutions 0,1–0,2—normales de NaCl. La présentation s'est faite isothermiquement dans le diagramme de concentration-solubilité de NaCl entre la température de chambre et le point d'ébullition des phases mixtes aqueuses.Dans les systèmes ternaires BaSO-NaCl-H₂O et SrSO₄-NaCl-H₂O la solubilité hydrothermique de barytine et de célestine en des solutions 2,0-normales de NaCl est présentée également pour l'espace des courbes limitantes de la région triphase et pour les isochores 0,326–0,6 jusqu'à 600° C et 2000 Bar. Elle est comparée avec les courbes de solubilité de systèmes purement aqueux. Le comportement de dissolution divergeant incongruent des silicates d'alumine à structure stratifiée en treillis est démontré pour le systême KAl₂(OH)₂-AlSi₃O₁₀-H₂O par exemple de la muscovite en déterminant expérimentalement les proportions moléculaires non-stochiométriques SiO₂ K₂O et SiO₂Al₂O₃ dans les solutions saturées pour la domaine d'existence hydrothermique de la muscovite.Importance géologique de la connaissance des dates de solubilité hydrothermique et leur application sur les événements des conséquences hydrothermiques-magmatiques et sur les événements de la métamorphose hydrothermique sont discutées.

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y 600° 2000 . (CaF₂), ( SO₄), . (SrSO₄) (PbSO₄) - Sio₂-₂.

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Verteilung des im Oberflächenwasser gelösten anorganischen Phosphats in der Irminger See im Mai und Juni 1963     

Günter Weichart 《Ocean Dynamics》1965,18(5):210-218

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