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The high-energy proton fluxes in the SAA observed with REM aboard the MIR orbital stationDuring two years, from November 1994 to 1996, the particle detector REM measured the highly energetic electron and proton environment at the outside of the MIR orbital station. Using mission averaged data we investigate various aspects of the proton fluxes in the SAA. Comparison with the radiation belt model AP8 reveal important differences. c2002 Elsevier Science Ltd. All rights reserved.
Document ID
20040105371
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1016/S1350-4487(02)00079-3
Authors
Buhler, P. (Paul Scherrer Institute Villigen, PSI, Switzerland)
Zehnder, A.
Kruglanski, M.
Daly, E.
Adams, L.
Date Acquired
August 21, 2013
Publication Date
October 1, 2002
Publication Information
Publication: Radiation measurements
Volume: 35
Issue: 5
ISSN: 1350-4487
Subject Category
Aerospace Medicine
Distribution Limits
Public
Copyright
Other
Keywords
long duration
Mir Project
manned
Flight Experiment

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