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The solar wind interaction with Comet P/Grigg-SkjellerupThe Giotto spacecraft is scheduled to intercept Comet P/Grigg-Skjellerup on July 10, 1992. The observed outgassing rate of this comet is over an order of magnitude smaller than Comet Giacobini-Zinner and over two orders of magnitude smaller than that of Comet Halley. Consequently, the new data obtained during the upcoming encounter will strengthen our understanding of how the solar wind interaction with comets depends upon the neutral gas production rate. In this brief note, we make predictions of the location of the flow transition regions - i.e., the bow shock and the ionopause, and discuss the expected level of wave turbulence.
Document ID
19930051398
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Flammer, K. R.
(NASA Headquarters Washington, DC United States)
Mendis, D. A.
(NASA Headquarters Washington, DC United States)
Shapiro, V. D.
(NASA Headquarters Washington, DC United States)
Shevchenko, V. I.
(California Univ. La Jolla, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1993
Publication Information
Publication: Earth, Moon, and Planets
Volume: 60
Issue: 1
ISSN: 0167-9295
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0167-9295
Accession Number
93A35395
Funding Number(s)
CONTRACT_GRANT: NAGW-1502
Distribution Limits
Public
Copyright
Other

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