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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Astrophysics and Space Science Libraryhttp://image.papertrans.cn/o/image/704589.jpg

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https://doi.org/10.1007/978-94-011-3640-2Planet; Solar System; earth; solar

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The Present Status of the Munich Dust Counter Experiment on Board of the Hiten Spacecraftion has been launched on January 24th, 1990 from Kago-shima Space Center. Here the present status of the MDC experiment is summarized. The number of dust particles measured so far is presented together with first and preliminary results of flux calculations and spatial as well as directional distrib

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In-Situ Exploration of Dust in the Solar System and Initial Results from the Galileo Dust Detectorive areas (typically 0.01 m. for the highly sensitive impact ionization sensors) or low mass sensitivities ≥10.g of the large area penetration detectors) previous instruments recorded only a few 100 impacts during their lifetimes. Nevertheless, important information on the distribution of dust in in

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The NASA Solar Probe Mission: In Situ Determination of Interplanetary Out-of-the Ecliptic and Near-Sf dust within our solar system. Solar Probe will map the dust environment from the orbit of Jupiter (5 AU), to within 4 solar radii of the sun’s center. The region between 0.3 AU and 4 R. has never been visited before, so the 10 days that the spacecraft spends during each (of the two) orbit is purel

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