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Effects of a wavy neutral sheet on cosmic ray anisotropiesThe first results of a three-dimensional numerical code calculating cosmic ray anisotropies is presented. The code includes diffusion, convection, adiabatic cooling, and drift in an interplanetary magnetic field model containing a wavy neutral sheet. The 3-D model can reproduce all the principal observations for a reasonable set of parameters.
Document ID
19850026536
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Kota, J. (Arizona Univ. Tucson, AZ, United States)
Jokipii, J. R. (Arizona Univ. Tucson, AZ, 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-4.2-11
Report Number: SH-4.2-11
Accession Number
85N34849
Funding Number(s)
CONTRACT_GRANT: NSF INT-84-00591
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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