2.3.7 Near-Earth Fragmentation of Cosmic Dust-Reference-Cited by-同舟云学术

2.3.7 Near-Earth Fragmentation of Cosmic Dust

Published:1976 Issue: Volume:31 Page:290-295
ISSN:0252-9211
Container-title:International Astronomical Union Colloquium
language:en
Short-container-title:International Astronomical Union Colloquium

Author:

Fechtig H.,Hemenway C.

Abstract

AbstractCosmic dust fragmentation in near-earth space is strongly suggested by the high fluxes (~102/m2s) of submicron particles observed in the upper atmospheric collection experiments, the lower fluxes (~10-l/m2s) observed in near-earth space by the lower sensitivity detection experiments and the much lower fluxes (~10−4/m2s) observed in the deep-space experiments. Various possible fragmentation mechanisms are discussed.

Publisher

Cambridge University Press (CUP)

Reference13 articles.

1. Rosen J. , “The Vertical Distribution of Dust to 30 Kilometer”, JGR, V 69, 21, p. 4673–4676, Nov. 1, 1964.

2. Observations of the micrometeoroid flux from Prospero

3. Time variation of the Altitude Distribution of the Cosmic Dust Layer in the Upper Atmosphere;Hemenway;Space Research,1970

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