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Titlebook: Origin and Evolution of Interplanetary Dust; Proceedings of the 1 A. C. Levasseur-Regourd,H. Hasegawa Conference proceedings 1991 Springer

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書(shū)目名稱Origin and Evolution of Interplanetary Dust
副標(biāo)題Proceedings of the 1
編輯A. C. Levasseur-Regourd,H. Hasegawa
視頻videohttp://file.papertrans.cn/705/704589/704589.mp4
叢書(shū)名稱Astrophysics and Space Science Library
圖書(shū)封面Titlebook: Origin and Evolution of Interplanetary Dust; Proceedings of the 1 A. C. Levasseur-Regourd,H. Hasegawa Conference proceedings 1991 Springer
描述THE THE KYOTO KYOTO COLLOQUIUM COLLOQUIUM It It has has almost almost become become a a tradition tradition to to periodically periodically review review the the progress progress of of our our knowledge knowledge of of interplanetary interplanetary dust dust at at an an interdisciplinary interdisciplinary level. level. After After the the Honolulu Honolulu (1967), (1967), Heidelberg Heidelberg (1975), (1975), Ottawa Ottawa (1979) (1979) and and Marseilles Marseilles (1984) (1984) meetings, meetings, it it was was decided decided to to hold hold a a meeting meeting specially specially devoted devoted to to the the Origin Origin and and Evolution Evolution of of Interplanetary Interplanetary Dust Dust in in Kyoto, Kyoto, Japan Japan on on 27-30 27-30 August August 1990. 1990. This This colloquium colloquium was was certainly certainly appropriate appropriate in in location, location, timing timing and and objective. objective. The The choice choice of of the the location location was was most most appropriate, appropriate, not not only only because because of of the the charm charm of of the the beautiful beautiful city city of of Kyoto, Kyoto, but but also also because because of o
出版日期Conference proceedings 1991
關(guān)鍵詞Planet; Solar System; earth; solar
版次1
doihttps://doi.org/10.1007/978-94-011-3640-2
isbn_softcover978-94-010-5616-8
isbn_ebook978-94-011-3640-2Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media Dordrecht 1991
The information of publication is updating

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Aqueous Alteration in Hydrated Interplanetary Dust Particles in considerable detail. Evidence was found that a significant proportion of the hydrated IDPs have been processed by aqueous alteration, and the nature of the alteration resembles that of similarly affected meteorites. The mineralogical and chemical data provide important clues to the possible origins of IDPs.
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The Munich Dust Counter — A Cosmic Dust Experiment on Board of the Muses-A Mission of Japanis an impact ionization detector designed to determine mass and velocity of cosmic dust. Here a short overview over the MUSES-A mission is given to show the measurement situation of the MDC experiment. The measurement principle of the instrument together with a discussion of the scientific objectives and the design of the experiment is summarized.
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Condensation Experiments of Mg-Silicate Mineralses below about 1000°C, whiskers of forsterite and enstatite (MgSiO.) were formed by vapor-liquid-solid growth mechanism. These whiskers are different from enstatite whiskers in interplanetary dust, which were probably formed at small super coolings
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In-Situ Exploration of Dust in the Solar System and Initial Results from the Galileo Dust Detectorct ionization detectors (10. g) together with a large sensitive area (0.1 m.). The Galileo spacecraft was launched on October 18, 1989 and is on its solar system cruise towards Jupiter. Initial measurements of the dust flux from 0.7 to 1.2 AU are presented.
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