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Prediction of energetic particle disturbancesThe prediction of fluxes of energetic particles of solar or magnetospheric origin is addressed. Topics include the prediction of the properties of the particle populations generated by magnetospheric storms and substorms, and the prediction of long term variations in the populations of magnetospheric particles.
Document ID
19800016215
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Paulikas, G. A. (Aerospace Corp. Los Angles, Calif., United States)
Baker, D. N. (LASL Noordwijk, Netherlands)
Barron, W. R. (AFGL Palo Alto, Calif., United States)
Domingo, V. (European Space Technol. Center Greenbelt, MD, United States)
Higbie, P. R. (LASL Greenbelt, MD, United States)
Imhof, W. L. (LMSC Laurel, Md., United States)
Lyons, L. R. (NASA Goddard Space Flight Center Munich, Germany)
Mcpherron, R. L. (NASA Goddard Space Flight Center)
Roelof, E. C. (APL/JHU)
Scholer, M. (Max-Planck-Inst. fuer Phys. und Astrophys.)
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
Space Radiation
Accession Number
80N24708
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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