Smiling in the rain: Seven reasons to be positive about uncertainty in hydrological modelling   总被引：1，自引：0，他引：1  

John M. Juston  Anna Kauffeldt  Beatriz Quesada Montano  Jan Seibert  Keith J. Beven  Ida K. Westerberg 《水文研究》2013,27(7):1117-1122

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Olivine-rich exposures in the South Pole-Aitken Basin     

Satoru Yamamoto  Ryosuke Nakamura  Tsuneo Matsunaga  Yoshiko Ogawa  Yoshiaki Ishihara  Tomokatsu Morota  Naru Hirata  Makiko Ohtake  Takahiro Hiroi  Yasuhiro Yokota  Junichi Haruyama 《Icarus》2012,218(1):331-344

The distribution and the geological context of the olivine-rich exposures in the South Pole-Aitken (SPA) Basin on the Moon were investigated based on the spectral data obtained from the Spectral Profiler (SP) and Multiband Imager (MI) onboard the Japanese lunar explorer Kaguya/SELENE. The olivine-rich exposures are found only in the peak rings or central peaks of the Schrödinger basin and Zeeman crater, which are located in the outer region of the SPA Basin and not in the center region. On a localized scale, the olivine-rich materials are exposed on landslide features on the crater walls or sloped wall of the central peaks or the peak rings. Another observational finding is the co-existence of olivine-rich and plagioclase-rich materials on a kilometer scale spanning most of the olivine-rich sites in the Schrödinger basin. Pyroxene-rich materials are found in fresh craters outside the peak rings or the central peaks with olivine-rich materials. Based on these results, the following scenario are proposed: (1) the impact to form the SPA Basin melted a large amount of the lunar upper mantle and crust, and distributed the melted materials to the outer region; (2) local differentiation of melted materials hid the olivine-rich materials in the center region of the SPA Basin; (3) later impacts that formed the Schrödinger and Zeeman craters excavated and exposed the olivine-rich materials to the surface again; and (4) space weathering and regolith gardening obscured the olivine-rich spectra at the exposure sites, but recent, small scale impacts or landslides on the sloped wall exposed fresh olivine-rich materials, allowing the identification of the olivine-rich exposures by spectral remote-sensing. This suggests that several, different scale events play an important role in forming the surface distributions of originally deep-seated materials on the Moon, as well as on other planetary bodies.  相似文献   

Adsorption of polar aromatic hydrocarbons on synthetic calcite   总被引：1，自引：0，他引：1  

Lene Madsen  Laila Grahl-Madsen  Christian Grøn  Ida Lind  John Engell 《Organic Geochemistry》1996,24(12):1151-1155

The wettability of hydrocarbon reservoirs depends on how and to what extent the organic compounds are adsorbed onto the surfaces of calcite, quartz and clay. A model system of synthetic calcite, cyclohexane and the three probe molecules: benzoic acid, benzyl alcohol and benzylamine, have been studied by adsorption experiments. The results clearly demonstrate the differences in the adsorption behaviour between probes with different functional groups of varying polarity and acidity. The maximum adsorption decreases in the order: benzoic acid, benzyl alcohol and benzylamine. The order of magnitude of ΔG° for the adsorption process implies the formation of a strong bond between the calcite surface and the adsorbate molecules.  相似文献   

Beitrag zur Petrographie desmittleren Muschelkalkes Süddeutschlands     

Ida Valeton 《Contributions to Mineralogy and Petrology》1954,4(1-2):207-216

Zusammenfassung Der primare klastische Anteil des mittleren Muschelkalks besitzt ein Maximum in den Korngrößen von 6–20, Ø , das über weite Strecken konstant bleibt. Der Mineralgehalt besteht aus Quarz, Feldspat, Glimmer und vielleieht Kaolinit.Bei der Diagenese warden Quarz und Feldspat teils korrodiert, teils wurden Quarz und Albit neu gebildet. In Randgebieten entstand Glaukonit vermutlich aus Glimmern.Durch Grundwassereinwirkung bildete rich ein zweites Maximum zwischen 0–2 Ø aus. Dabei ist in diesen Korngrößen eine Zunahme an Illit und Kaolinit und das Neuauftreten von Montmorillonit zu verzeichnen.Bei der Verwitterung verschwand das Maximum zwischen 6–20 Ø zugunsten eines Maximums zwischen 0–2 Ø . Damit verschwand auch der primäre Mineralgehalt fast völlig. Die Fraktionen unter 2 Ø setzen sich aus einem illitähnlichen Mineral zusammen.Durch Grundwassertätigkeit und Oberflächenverwitterung wurde also nicht nur der lösliche Anteil des mm ausgelaugt, sondern es sind auch deutliche Veränderungen des klastischen Anteils wahrzunehmen.Herrn Professor Dr.Carl W. Correns zum 60. Geburtstag gewidmet.  相似文献   

Analysis of stick-slip and earthquake mechanism     

Yoshiaki Ida 《Physics of the Earth and Planetary Interiors》1975,11(2):147-156

A mathematical model of a sliding system that contains a frictional surface embedded in an elastic specimen and machine is proposed to analyze the frictional behavior observed in laboratory and field. It is shown that stick-slip occurs if the slope of the velocity-stress relation on the sliding surface exceeds a critical value at a certain point between static and kinetic frictions. This condition, coupled with Amontons' law and other subsidiary relations, predicts the effects of normal stress, gouge thickness, temperature, and loading rate etc. on the stick-slip instability, consistent with known experimental evidence. The elastic-wave radiation associated with stick-slip is governed by Brune's source time function, in which rise time and effective stress are proportional to fault dimension and stress drop, respectively.  相似文献