Expansion, radiation and condensation of vapor cloud, created by high-velocity impact onto a target in vacuum

The results of numerical simulations of small meteoroid impacts against the rocky lunar surface are presented which give an estimate of impact luminous efficiency. The obtained values of luminosity can considerably differ from the real ones because of the influence of regolith. Specific features of...

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Bibliographic Details
Published in:International journal of impact engineering Vol. 23; no. 1; pp. 651 - 662
Main Authors: Nemtchinov, I.V., Shuvalov, V.V., Artemieva, N.A., Kosarev, I.B., Trubetskaya, I.A.
Format: Journal Article
Language:English
Published: Elsevier Ltd 01-12-1999
Online Access:Get full text
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Summary:The results of numerical simulations of small meteoroid impacts against the rocky lunar surface are presented which give an estimate of impact luminous efficiency. The obtained values of luminosity can considerably differ from the real ones because of the influence of regolith. Specific features of impacts into the regolith are discussed and a simple model discribing the shock wave structure in the porous target is proposed.
ISSN:0734-743X
1879-3509
DOI:10.1016/S0734-743X(99)00111-6