Optical and Thermal Properties of Interplanetary Dust
作者： A. Chantal Levasseur-Regourd , Ingrid Mann , René Dumont , Martha S. Hanner
DOI: 10.1007/978-3-642-56428-4_2
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摘要: This chapter reviews our understanding of the interplanetary dust, from its optical and thermal properties. The dust cloud, although extremely low thickness, is indeed visible through faint evanescent glow zodiacal light. Two types physical processes playa role in emission light by cloud: scattering solar particles, prevailing domain, radiation, infrared domain.
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