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H2O(+) structures in the inner plasma tail of comet AustinWe present images of comet Austin 1989c1 in the light of H2O(+) from which the contribution of the dust continuum and the gas coma was completely removed. We describe the behavior of the H2O(+) plasma in the inner coma where it is reliably observed for the first time.
Document ID
19930009985
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Jockers, Klaus (Max-Planck-Inst. fuer Aeronomie Katlenburg-Lindau, Germany)
Bonev, T. (Bulgarian Academy of Sciences Sofia., United States)
Geyer, E. H. (Observatorium Hoher List Daun, Germany)
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
93N19174
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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