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4.8 Evolution and Detectability of Interplanetary Dust Streams

Published online by Cambridge University Press:  12 April 2016

Lubor Kresák
Lubor Kresák*
Affiliation:
Astronomical Institute, Slovak Academy of Sciences, Bratislava, Czechoslovakia

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Sudden enhancements in responses recorded by micrometeoroid detectors flown on spacecrafts have been repeatedly attributed to encounters with streams of cometary debris similar to, or identical with, the meteor streams known from ground-based observations. Por measurements made in the Earth-Moon environment, spacecraft effects, atmospheric fragmentation of larger particles, and possibly lunar ejecta can be misinterpreted as interplanetary streams. For deep space observations it is necessary to inquire whether a compact dust stream can persist under the dispersive and destructive effects which increase rapidly with decreasing particle size.

Type
4 Meteors and their Relation to Interplanetary Dust
Information
International Astronomical Union Colloquium , Volume 31: Interplanetary Dust and Zodiacal Light , 1976 , pp. 391 - 395
Copyright
Copyright © Springer-Verlag 1976

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