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Radial gradient of cosmic ray intensity from a comparative study of data from Voyager 1 and 2 and IMP 8The IMP 8 satellite and Voyager 1 and 2 space probes obtained cosmic ray measurements during the late 1977 to mid-1982 period. Comparisons of 27-day averages of the data show that a positive radial intensity gradient existed on the average during this period, and that the cosmic ray intensity decrease toward solar maximum in 1980-1981 proceeds in a stepwise fashion. The cosmic ray minimum reached in late 1980/early 1981 appears almost simultaneously at 1 AU and at 10 AU, with and without propagation time delay effects, between IMP 8 and the Voyager spacecraft. These data are generally consistent with a heliolatitudinal gradient of 0 + or - 1 percent/deg. Attention is given to the implications of these results in the overall context of cosmic ray modulation theory.
Document ID
19840053290
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Venkatesan, D.
(Calgary, University Calgary, Alberta, Canada)
Decker, R. B.
(Calgary Univ. Alberta Canada)
Krimigis, S. M.
(Johns Hopkins University Laurel, MD, United States)
Date Acquired
August 12, 2013
Publication Date
June 1, 1984
Publication Information
Publication: Journal of Geophysical Research
Volume: 89
ISSN: 0148-0227
Subject Category
Space Radiation
Accession Number
84A36077
Funding Number(s)
CONTRACT_GRANT: NASA TASK I
CONTRACT_GRANT: NAGW-154
CONTRACT_GRANT: N00024-78-C-5384
Distribution Limits
Public
Copyright
Other

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