Properties and interactions of interplanetary dust : proceedings of the 85th colloquium of the international astronomical union, Marseille, France, July 9-12, 1984
著者
書誌事項
Properties and interactions of interplanetary dust : proceedings of the 85th colloquium of the international astronomical union, Marseille, France, July 9-12, 1984
（Astrophysics and space science library, v. 119）
D. Reidel , Sold and distributed in the U.S.A. and Canada by Kluwer Academic Publishers, c1985
大学図書館所蔵 全12件
注記
Includes index
内容説明・目次
内容説明
Investigation of the interplanetary dust cloud is characterized by contributions from quite different methods and fields, such as research on zodiacal light, meteors, micrometeoroids, asteroids, and comets. Since the earth's environment and interplanetary space became accessible to space vehicles these interrelations are clearly evident and extremely useful. Space measurements by micrometeoroid detectors, for example, provide individual and eventually detailed information on impact events, which however are limited in number and therefore restricted in statistical significance. On the other hand, zodiacal light measurements involve scattered light from many particles and therefore provide global information about the average values of physical properties and spatial distribution of interplanetary grains. Additional knowledge stems from lunar samples and from dust collections in the atmosphere and in deep sea sediments. All these sources of complementary information must be put together into a synoptical synthesis. This also has to take into account dynamical aspects and the results of laboratory investigations concerning physical properties of small grains. Such considerable effort is not merely an academic exercise for a few specialists interested in the solar dust cloud. Since this same cloud exclusively allows direct in-situ acess to investigate extraterrestrial dust particles over a wide range of sizes and materials, it provides valuable information for realistic treatment of dust phenomena in other remote cosmic regions such as in dense molecular clouds, circumstellar dust shells, and even protostellar or protoplanetary systems.
目次
I. Zodiacal Light and F-Corona: Observations.- II. Interplanetary Dust: Space and Ground Studies.- III. Interplanetary Dust: Laboratory Studies.- IV. Optical Studies of Dust.- V. Relations to Comets and Meteoroids.- VI. Dust — Plasma Interactions.- VII. Dynamics of Interplanetary Dust.- Final Discussion.- Summary and Conclusion of the Colloquium.- Index of Authors.- Index of Subjects.
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