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- W29121086 abstract "An examination of the relation of track densities from solar energetic particles in interplanetary dust grains (IDP's) to the orbital elements of source bodies is made and the positive and negative aspects of using track densities to determine the origin of IDP's are reported. It is found from calculations that predicted track densities for a particle of given size are related logarithmically to the minimum semimajor axis of the source body. Consequently, although track densities measurements may not be capable of distinguishing cometary from asteroidal sources, they should give information on the minimum semimajor axis of the originating bodies." @default.
- W29121086 created "2016-06-24" @default.
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- W29121086 date "1994-01-01" @default.
- W29121086 modified "2023-09-27" @default.
- W29121086 title "Solar energetic particle track densities as an indicator of the origin of interplanetary dust" @default.
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