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Cosmic ray modulation and merged interaction regionsBeyond several AU, interactions among shocks and streams give rise to merged interaction regions in which the magnetic field is turbulent. The integral intensity of . 75 MeV/Nuc cosmic rays at Voyager is generally observed to decrease when a merged interaction region moves past the spacecraft and to increase during the passage of a rarefaction region. When the separation between interaction regions is relatively large, the cosmic ray intensity tends to increase on a scale of a few months. This was the case at Voyager 1 from July 1, 1983 to May 1, 1984, when the spacecraft moved from 16.7 to 19.6 AU. Changes in cosmic ray intensity were related to the magnetic field strength in a simple way. It is estimated that the diffusion coefficient in merged interaction regions at this distance is similar to 0.6 x 10 to the 22nd power sq cm/s.
Document ID
19850026521
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Burlaga, L. F.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Goldstein, M. L.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Mcdonald, F. B.
(NASA Headquarters Washington, DC United States)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 4
Subject Category
Space Radiation
Report/Patent Number
SH-4.1-11
Report Number: SH-4.1-11
Accession Number
85N34834
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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