Book reviews     

Dieter Richter  Axel Borsdorf  Olusegun Areola  Risto Laulajainen  L. Wahlstroem  Reinhard Stewig  Jonathan B. Laronne  Gösta A. Eriksson  Cesar N. Caviedes  John Gunn  Karl Mauder  G. Kunkel  John T. Pierce  Leszek A. Kosinski  G.orge H. Kakiuchi  Reiner Herrmann  W. M. Sackinger 《GeoJournal》1982,6(6):581-588

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A new method for reconstructing type III trajectories     

M. J. Reiner  R. G. Stone 《Solar physics》1986,106(2):397-401

A local density approximation (LDA) method is developed for reconstructing the trajectories of type III radio bursts through the interplanetary medium. The method uses the measured source directions and the measured frequency drift rates of the type III burst to determine the locations of the radio source in the interplanetary medium at consecutive frequency levels. The technique is used to reconstruct the trajectory of an actual type III burst and the results are compared to the trajectory obtained from the global density law method. The LDA method represents an improvement in that it utilizes more observed data on the type III burst and that it takes full account of the local density variations at the source locations.  相似文献   

Primary fluids entrapped at blueschist to eclogite transition: evidence from the Tianshan meta-subduction complex in northwestern China   总被引：5，自引：1，他引：5  

Jun Gao  Reiner Klemd 《Contributions to Mineralogy and Petrology》2001,142(1):1-14

Orthopyroxene and olivine exposed along the rim of a harzburgite xenolith from La Palma (Canary Islands) show polycrystalline selvages and diffusion zones that result from contact with mafic, alkaline, silica-undersaturated melts during at least 10-100 years before eruption. The zoned selvages consist of a fine-grained reaction rim towards the xenolith and a coarser grained, cumulate-like layer towards the melt contact. The diffusion zones are characterized by decreasing magnesium number from about 89-91 in the xenolith interior to 79-85 at the rims, and clearly result from Fe-Mg exchange with surrounding mafic melt. The width of the diffusion zones is 80-200 µm in orthopyroxene and 1,020-1,730 µm in olivine. Orthopyroxene also shows decreasing Al₂O₃ and Cr₂O₃ and increasing MnO and TiO₂ towards the reaction rims. Textural relations and comparisons with dissolution experiments suggest that orthopyroxene dissolution by silica-undersaturated melt essentially ceased after days to weeks of melt contact, possibly because of decreasing temperature and formation of the reaction rims. The short dissolution phase was followed by prolonged growth of diffusion zones through cation exchange between xenolith minerals and melt across the reaction rims, and by the growth of cumulus crystals. The observations indicate that orthopyroxene xenocrysts and harzburgite xenoliths can survive in mafic, silica-undersaturated, subliquidus magmas at 1,050-1,200 °C and 200-800 MPa for tens of years. Modeling and comparison of the diffusion zones indicate that the average Fe-Mg interdiffusion coefficient D_FeMg in orthopyroxene is 2 log units lower than that in olivine; at 1,130 °C and QFM-buffered oxygen fugacity, D_FeMg^opx = 3 ×10 ^{- 19}  m²  s^{- 1}D_{FeMg}^{opx} = 3 \times 10^{ - 19} \,{\rm m}^2 \,{\rm s}^{{\rm - 1}} . The new data overlap well with recently published data for D_FeMg in diopside, and indicate that D_FeMg ^opxD_{FeMg\,}^{opx} (as predicted by previous authors) may be extrapolated to higher temperatures and oxygen fugacities. It is suggested that D_FeMg ^opx D_{FeMg\,}^{opx} and D_FeMg in Mn-poor ferromagnesian garnet are similar within 0.5 log units at temperatures between 1,050 and 1,200 °C.  相似文献   

Comment on the paper “On estimating gravity anomalies—A comparison of least squares collocation with conventional least squares techniques”     

Reiner Rummel  Richard H. Rapp 《Journal of Geodesy》1978,52(4):297-297

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Approximation for Steady Interface Beneath a Well Pumping Fresh Water Overlying Salt Water     

Reiner G. Haubold 《Ground water》1975,13(3):254-259

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Photochemical,advective and turbulent effects on the meridional distribution of ozone     

Dr. Reiner Gebhart 《Meteorology and Atmospheric Physics》1968,17(4):301-335

Summary A time-dependent study of the formation, distribution and destruction of atmospheric ozone is made for a meridional plane between 15 km and 45 km under the assumption of zonal symmetry. Included are time-effects of photochemistry, advection and turbulence, using presently available information on theoretical and observational data. The attempt is made to investigate the important part played by pure photochemistry, by the various transport processes and by the combination of both.In the photochemical calculations the equations of a pure oxygen photochemistry and solar ultraviolet energy data obtained from recent rocket observations are used.Murgatroyd andSingleton's results of a possible meridional circulation andPrabhakara's pattern of large-scale eddy diffusion, derived from the spread of radioactive tungsten in the stratosphere, are assumed to be the basic transport meachanisms.Several combinations of these non-photochemical processes are tested in the model and compared with recent observations.The relatively largest seasonal variations of the O₃-concentration take place in the upper stratosphere with a maximum concentration in the high-latitude winter-hemisphere. In the midstratosphere the maximum concentration appears over the equatorial latitudes following the sun's position. In the lower stratosphere the highest O₃-concentrations are over the polar latitudes throughout the year.The seasonal variation of the total ozone at middle and high latitudes can be explained by photochemical effects, the increase of total ozone with increasing latitude by the combined effects of photochemistry and transport processes only. With an advective transport of 70% ofMurgatroyd andSingleton's circulation we have reasonably well reproduced an observed spring distribution of O₃ in the northern hemisphere.

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Zusammenfassung Die Bildung, Ausbreitung und Zerstörung des atmosphärischen Ozons wird in einem meridionalen Profil zwischen 15 km und 45 km unter der Annahme zonaler Symmetrie als nichtstationäres Problem untersucht. Die Einflüsse der Photochemie, der Advektion und der Turbulenz werden als Funktionen der Zeit behandelt. Es wird versucht, die Bedeutung der photochemischen Einflüsse, der verschiedenen Transportprozesse sowie der Kombination beider in einem numerischen Modell zu studieren; gegenwärtig verfügbare theoretische und experimentelle Daten finden Verwendung.In den photochemischen Berechnungen werden die Gleichungen der reinen Sauerstoff-Photochemie und mit Raketen ermittelte Daten der verfügbaren Sonnenenergie verwendet.Murgatroyds undSinlgetons Ergebnisse einer möglichen meridionalen Zirkulation und die vonPrabhakara benützten Werte der großräumigen Turbulenz, die aus der Verbreitung des radioaktiven Wolframs abgeleitet worden sind, werden als Transportmechanismen betrachtet. Verschiedene Kombinationen dieser Transportgrößen werden im Modell getestet und mit neueren Beobachtungen verglichen.Die relativ größten jahreszeitlichen Schwankungen der Ozonkonzentration treten in der oberen Stratosphäre auf mit einer maximalen Konzentration in der Winterhemisphäre hoher Breiten. In der mittleren Stratosphäre befindet sich das Maximum über den äquatorialen Breiten. In der unteren Stratosphäre findet man die höchsten Ozonkonzentrationen während des ganzen Jahres über den polaren Breiten.Der Jahresgang des Gesamtgehaltes an Ozon über mittleren und hohen Breiten kann durch photochemische Einflüsse erklärt werden, die Zunahme des Gesamtozons mit zunehmender Breite nur durch ein Zusammenwirken von photochemischen und Transport-Prozessen. Mit 70% der Advektion vonMurgatroyd undSingleton haben wir eine beobachtete Frühjahrsverteilung des Ozons in der nördlichen Hemisphäre mit guter Annäherung reproduziert.

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Résumé On examine ici la formation, la propagation et la destruction de l'ozone atmosphérique dans un profil méridien entre 15 et 45 km d'altitude. Pour cela, on admet une symétrie zonale et qui'il s'agit d'un problème non stationnaire. On considére les influences de la photochimie, de l'advection et de la turbulence en fonction du temps. On essaie d'étudier au moyen d'un modèle numérique l'importance des influences de la seule photochimie, des différents processus de transport ainsi que la combinaison des deux phénomènes. Dans ce but, on utilise les valeurs théoriques et expérimentales disponibles actuellement.Dans le calcul photochimique, on utilise aussi bien les équations de la photochimie pure de l'oxygène que des valeurs de l'énergie solaire disponible, obtenues au moyen de mesures effectuées avec des fusées. Comme mécanismes de transport, on prend en considération les résultats des études deMurgatroyd etSingleton sur une circulation méridionale possible ainsi que les valeurs de la turbulence des grands espaces utilisées parPrabhakara. Ces dernières découlent de la dissémination du wolfram radioactif. On fait figurer dans le modèle diverses combinaisons de ces grandeurs de transport et on compare les résultats ainsi obtenus aux observations les plus récentes.Les variations saisonnières relativement les plus importantes de la concentration d'ozone se rencontrent dans la stratosphère supérieure. La concentration maximale se situe dans les hautes latitudes de l'hémisphère hivernal. Dans la stratosphère moyenne, le maximum se rencontre au voisinage de l'équateur. Dans la basse stratosphère, on note les plus fortes concentrations d'ozone au voisinage des pôles et cela durant toute l'année.On peut expliquer par des influences photochimiques les fluctuations annuelles de la teneur globale en ozone dans les latitudes moyennes et élevées. L'augmentation de la teneur totale de l'ozone avec la latitude ne s'explique que par les effets conjugués des processus photochimiques et de transport. On a assez bien pu reproduire une répartition de l'ozone observée au printemps sur l'hémisphère nord en utilisant le 70% de l'advection calculée selonMurgatroyd etSingleton.

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With 18 Figures

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This investigation was begun while the author was on leave at the National Center for Atmospheric Research in Boulder, Colorado, USA.  相似文献   

On the significance of the shortwave CO2-absorption in investigations concerning the CO2-theory of climatic change     

Dr. Reiner Gebhart 《Theoretical and Applied Climatology》1967,15(1-2):52-61

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Sky radiation,polarization and twilight radiation in Greenland   总被引：1，自引：0，他引：1  

Kurt Bullrich  Reiner Eiden  Wolfram Nowak 《Pure and Applied Geophysics》1966,64(1):220-242

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Sustaining productive ecosystems in face of risk     

Reiner Schwarz 《GeoJournal》2004,59(3):219-225

Ecosystems lacking human induced energy input from outside are in danger to degrade if man requires any sustainable yield. The risk of failure strongly depends on the amount of exploitation. This is shown by a simple one dimensional analytical feed-back model. Natural fluctuations determine the degradation probability of productive ecosystems. The stability behaviour of the latter is demonstrated by an analytical model in the two dimensional phase space. Full quantitative evaluation of the risk needs simulation experiments. One is carried out in the thorn shrub savannah rangelands at a site in Namibia where a fully calibrated simulation model shows that the less a sustainable yield is required, the more the breakdown is delayed. In this case of highly fluctuating rainfall any sustainability sensu strictu does not exist. This revised version was published online in August 2006 with corrections to the Cover Date.  相似文献   

Authigenic carbonates in sediments from the Gulf of Mexico     

Reiner Botz  Eckhard Faber  Michael J. Whiticar  James M. Brooks 《Earth and Planetary Science Letters》1988,88(3-4)

The carbon isotopic composition of diagenetic dolomite and calcite in some sediments of the Gulf of Mexico varies between “normal-marine” (δ¹³C ca. 0‰) and −14.6‰ which suggests that biogenic CO₂ contributed to the carbonate formation. The δ¹³O values of dolomite and coexisting calcite are very similar but variable down-core.Dolomite and calcite precipitated early from pore water where SO₄²⁻ was not reduced. However, during (and after?) SO₄²⁻ reduction dolomite and calcite still formed and there are at least two generations of carbonate minerals present.  相似文献