The stream of secondary particles in the circumlunar space
A mathematical model which permits one to calculate a circumlunar cloud ofsecondary particles by a known meteorite stream on the Moon surface is considered. The cloudcharacteristics in the sphere of the Moon gravitation are presented. The article gives a review ofworks executed on the Calculus Department of Tomsk State University in 1977-80.
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Keywords
первичный поток метеороидов, кратерообразование, поток вторичных частиц, размеры, масса, скорость, энергия частиц, primary meteoroid stream, cratering, secondary particles stream, size, mass, velocity, energy of particlesAuthors
Name | Organization | |
Krivyakova Eleonora Nonovna | National Research Tomsk State University | eleon@sibmail.com |
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