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The termination shock: Physical processesA brief overview of the physics thought to determine the properties of the heliospheric termination shock is given and the central role of hot interstellar pick-up ions and cosmic rays is emphasized.
Document ID
19950053664
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1016/0273-1177(94)00129-O
Authors
Zank, G. P. (Univ. of Delaware, Newark, DE US, United States)
Cairns, I. H. (Univ. of Iowa, Iowa City, IA US, United States)
Webb, G. M. (Univ. of Arizona AZ, US, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1995
Publication Information
Publication: Advances in Space Research
Volume: 15
Issue: 9-Aug
ISSN: 0273-1177
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0273-1177
Accession Number
95A85263
Funding Number(s)
CONTRACT_GRANT: NAGW-2076
CONTRACT_GRANT: JPL-959167
CONTRACT_GRANT: NAGW-2040
CONTRACT_GRANT: NSF ATM-93-57861
CONTRACT_GRANT: NSG-7101
CONTRACT_GRANT: NAGW-3461
CONTRACT_GRANT: NAGW-3450
Distribution Limits
Public
Copyright
Other

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