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The spatial distribution of large cometary meteoroids in the inner solar systemA model of the spatial density distribution of large (m greater than 10(exp -3) g) cometary meteoroids in the inner solar system is obtained assuming that they have orbits closely associated with that of their parent comet. Distributions of the orbital parameters of the Taurid, Quadrantid and Perseid meteoroid streams are used in developing the model.
Document ID
19930010019
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Mcbride, Neil (Sheffield Univ.)
Hughes, David W. (Sheffield Univ.)
Date Acquired
September 6, 2013
Publication Date
January 1, 1992
Publication Information
Publication: Lunar and Planetary Inst., Asteroids, Comets, Meteors 1991
Subject Category
Astrophysics
Accession Number
93N19208
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19930009924Collected WorksAsteroids, Comets, Meteors 199119930009924Collected WorksAsteroids, Comets, Meteors 1991
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