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Long term magnetospheric particle variations (1 day T infinity), appendix 2Effects of solar variations on energetic particle propagation are discussed, as well as prediction techniques for such particles within the magnetosphere. Magnetic field models, magnetic energy stored in the tail, magnetic monitoring measurements in the geostationary orbit and at certain ground based stations are important elements concerning improving such techniques.
Document ID
19800016217
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Vette, J. I. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Hills, H. K. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Paulikas, G. A. (Aerospace Corp. Los Angeles, Calif., United States)
Sawyer, D. A. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Stassinopoulos, E. G. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Teague, M. J. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 10, 2013
Publication Date
December 1, 1979
Publication Information
Publication: NASA. Marshall Space Flight Center Solar-Terrest. Predictions Proc., Vol. 2
Subject Category
Geophysics
Accession Number
80N24710
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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IDRelationTitle19800016185Collected WorksSolar-terrestrial Predictions Proceedings. Volume 2: Working Group Reports and Reviews
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