The Equatorial Glaciers of New Guinea—Results of the 1971–1973 Australian Universities' Expeditions to Irian Jaya: Survey, glaciology, meteorology, biology and palaeoenvironments : Edited by G. S. Hope, J. A. Peterson, U. Radok, and I. Allison. A. A. Balkema, Rotterdam, 1976, 244 pp. $14.80     

Ernst Lffler 《Quaternary Research》1979,11(3):388-389

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Geologic evolution of the westernmost part of the internal Betic zone (Betic Cordilleras,Southern Spain)     

Dr. Theodor Ernst Felder 《International Journal of Earth Sciences》1980,69(1):131-148

The Serranía de Ronda (western Betic Cordilleras, S-Spain) is formed by different tectonic units of the Betic internal domain. Stratigraphic correlations of the Permo-Triassic and Triassic sedimentary sequences imply that one part of the Mesozoic carbonates of the Rondaides (Dorsale bétique), namely the Cabrilla unit (Dorsale interne), is shearedoff from the frontal part of the Malaguides, and another part (Nieves unit, Dorsale externe) forms the Mesozoic cover of the alpujarride Casares unit. The first alpine compressional phases took place in the Paleogene; post-metamorphic movements followed in the time between the Upper Aquitanian and the Upper Tortonian. From geometrical considerations it can be concluded that the Malaguides originated paleogeographically from a more internal region than the Alpujarrides.

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Zusammenfassung Am Aufbau der Serranía de Ronda (westliche Betische Kordilleren, S-Spanien) nehmen verschiedene Einheiten der betischen Intemzonen teil. Stratigraphische Vergleiche der permotriadischen und triadischen Sedimentserien erlauben den Schluß, daß die mesozoischen Karbonate der Rondaiden (Dorsale bétique) zu einem Teil (Cabrilla-Einheit, Dorsale interne) von der frontalen Partie der Malagiden abglitten und zum anderen Teil (Nieves-Einheit, Dorsale externe) das abgescherte Mesozoikum der alpujarriden Casares-Einheit bilden. Die ersten alpinen Kompressionsphasen sind im Paleogen anzusetzen, da für mesozoische Deckenbewegungen beweiskräftige Argumente fehlen. Zwischen Oberaquitanian und Obertortonian fanden post-metamorphe Überschiebungen statt. Aus geometrischen Gründen wird angenommen, daß die Malagiden paläogeographisch internerer Herkunft sein müssen als die benachbarten Alpujarriden.

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Resumen La Serranía de Ronda (Cordilleras béticas occidentales, Prov. Málaga) está formado por diferentes unidades del conjunto bético interno. Correlaciones estratigráficas del Permo-Triásico y del Triásico de los diferentes unidades permiten la conclusión que los Rondáides (Dorsal bética) está por una parte (unidad de Cabrilla, Dorsal interna) el revestimiento mesozóico de la parte frontal de los mantos maláguides, y por otra parte (unidad de las Nievas, Dorsal externa) la parte mesozóica de la unidad alpujárride de Casares. Las primeras fases alpinas de compresión deben ser situadas en el Paleógeno. Las traslaciones post-metamórficas de mantos son de edad aquitaniense superior hasta pre-tortoniense superior. Con argumentación geométrica se puede concluir que los Maláguides son de un orígen paleográfico más interno que los Alpujárrides.

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( , . « » , (Dorsale bétique) ( , Dorsale interne) , ( , Dorsale externe) . .. , . - . , , .

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Sedimentation and structure of the Izu-Ogasawara (Bonin) Trench off Tokyo: new lights on the results of a diving campaign with the bathyscape “Archimede”     

Gilbert Bellaiche 《Earth and Planetary Science Letters》1980,47(1):124-130

Direct observations from submersible prove that in the explored areas, the Izu-Ogasawara Trench is devoid of any significant sediment cover. The effects of the tensional forces affecting the oceanic crust have been observed in the outer wall of this trench, especially near its foot between 8200 and 8500 m depth. They lead to a staircase morphology (with rock exposures) corresponding probably with vertical faulting parallel to the trend of the trench axis. The inner wall, at about 5000 m depth, shows large rock exposures that have been sampled. These rocks are volcanic lavas of the tholeiitic series (icelandites). The staircase morphology observed in this part of the overriding plate seems to prove the occurrence of distensive forces induced probably by the underthrusting of the oceanic crust. No indication of compressive stress has been registered in the whole investigated area.  相似文献   

Stratigraphisch-fazielle Identifizierung von Sedimenten auf chemisch-geologischem Wege     

Dozent Dr. Werner Ernst 《International Journal of Earth Sciences》1966,55(1):21-29

Zusammenfassung Die Bor-Gehalte des paralischen Oberkarbons sind vorwiegend von der ursprünglichen Salinität im Ablagerungsgebiet abhängig. Daneben scheint das Klima eine Auswirkung zu haben, die sich durch die Erhöhung der Bor-Gehalte vom Westfal B an und im Rotliegenden, Keuper und Tertiär bemerkbar macht.

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The boron contents of the paralic Upper Carboniferous depend principally on the original salinity in the area of sedimentation. Besides, the climate appears to have an effect that manifests itself by increase in the boron contents from the Westphalian B on and in the Rotliegendes, Keuper and tertiary.

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Résumé Les teneurs en bore du Carbonifère supérieur pralique dépendent avant tout de la salinité originale de la région de sédimentation. Par ailleurs, le climat paraît avoir eu une influence qui se traduit par un accroissement des teneurs en bore dans le Westphalien B, le Rotliegende, le Keuper et le Tertiaire.

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Das Sockelstockwerk in den Randzonen der Urkontinente     

Prof. Dr. Ernst H. Ackermann 《International Journal of Earth Sciences》1965,54(2):796-812

The rocks of the cratonic foreland extend underneath many orogens, where they are subjected to “regeneration” during the geosynclinal phase and to superimposed structures during the folding of the orogen. Such structural and metamorphic alterations are now exposed in the “Sockelstockwerk” of certain orogenic belts in Africa, America, Australia and Europe. In this deep level, originally situated between the bottom of the geosyncline and the migmatite stockwerk, the following zones have been observed along the total length of the orogenic belt: border zone along the margin of the cratonic foreland: broad belt with superimposed structures of two (ore more) different orogenic deformations; main vergency fan, marking the central axis of the orogen. This fan often is a lineament with deep roots and a structure of continental importance.  相似文献   

Ergebnisse von Messungen über den Wärmehaushalt eines künstlich erwärmten Flusses     

Dr. Ernst Rudel 《Meteorology and Atmospheric Physics》1977,25(3):281-292

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An example of enhanced tephra deposition driven by topographically induced atmospheric turbulence     

Sebastian F. L. Watt  Jennie S. Gilbert  Arnau Folch  Jeremy C. Phillips  Xiaoming M. Cai 《Bulletin of Volcanology》2015,77(5):1-14

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A MEXICAN CORPORATE CAMPAIGN IN CONSERVATION     

Ernst Griffin  Howard W. Dennis 《The Professional geographer》1969,21(5):358-359

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Accelerating the convergence of coupled geomechanical‐reservoir simulations     

L. Jeannin  M. Mainguy  R. Masson  S. Vidal‐Gilbert 《国际地质力学数值与分析法杂志》2007,31(10):1163-1181

The pressure variations during the production of petroleum reservoir induce stress changes in and around the reservoir. Such changes of the stress state can induce marked deformation of geological structures for stress sensitive reservoirs as chalk or unconsolidated sand reservoirs. The compaction of those reservoirs during depletion affects the pressure field and so the reservoir productivity. Therefore, the evaluation of the geomechanical effects requires to solve in a coupling way the geomechanical problem and the reservoir multiphase fluid flow problem. In this paper, we formulate the coupled geomechanical‐reservoir problem as a non‐linear fixed point problem and improve the resolution of the coupling problem by comparing in terms of robustness and convergence different algorithms. We study two accelerated algorithms which are much more robust and faster than the conventional staggered algorithm and we conclude that they should be used for the iterative resolution of coupled reservoir‐geomechanical problem. Copyright © 2006 John Wiley & Sons, Ltd.  相似文献   

The initial responses of hot liquid water released under low atmospheric pressures: Experimental insights     

Alistair Simon Bargery  Alexander Barrett  Lionel Wilson  Jennie S. Gilbert 《Icarus》2010,210(1):488-506

Experiments have been performed to simulate the shallow ascent and surface release of water and brines under low atmospheric pressure. Atmospheric pressure was treated as an independent variable and water temperature and vapor pressure were examined as a function of total pressure variation down to low pressures. The physical and thermal responses of water to reducing pressure were monitored with pressure transducers, temperature sensors and visible imaging. Data were obtained for pure water and for solutions with dissolved NaCl or CO₂. The experiments showed the pressure conditions under which the water remained liquid, underwent a rapid phase change to the gas state by boiling, and then solidified because of removal of latent heat. Liquid water is removed from phase equilibrium by decompression. Solid, liquid and gaseous water are present simultaneously, and not at the 611 Pa triple point, because dynamic interactions between the phases maintain unstable temperature gradients. After phase changes stop, the system reverts to equilibrium with its surroundings. Surface and shallow subsurface pressure conditions were simulated for Mars and the icy satellites of the outer Solar System. Freezing by evaporation in the absence of wind on Mars is shown to be unlikely for pure water at pressures greater than c. 670 Pa, and for saline solutions at pressures greater than c. 610 Pa. The physical nature of ice that forms depends on the salt content. Ice formed from saline water at pressures less than c. 610 Pa could be similar to terrestrial sea ice. Ice formed from pure water at pressures less than c. 100 Pa develops a low thermal conductivity and a ‘honeycomb’ structure created by sublimation. This ice could have a density as low as c. 450 kg m⁻³ and a thermal conductivity as low as 1.6 W m⁻¹ K⁻¹, and is highly reflective, more akin to snow than the clear ice from which it grew. The physical properties of ice formed from either pure or saline water at low pressures will act to reduce the surface temperature, and hence rate of sublimation, thereby prolonging the lifespan of any liquid water beneath.  相似文献