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Z-rich solar particle event characteristics 1972-1976It is found in the reported investigation that Z-rich solar particle events usually have large and prolonged anisotropies in addition to an extremely variable charge composition that varies not only from event to event but also throughout the event. These observations suggest that one can no longer regard the event-averaged composition of solar particle events at low energies as providing an unbiased global sample of the solar atmospheric composition. The variability from event to event and among classes of events is just too great. However, the tendency for the Z-rich events to be associated with both the low-speed solar wind at or just before the onset of solar wind streams and with active regions located in the western hemisphere, indicates that charge composition studies of solar particle events can yield a better knowledge of the flare acceleration process as well as the inhomogeneous nature of magnetic field structure and particle composition in the solar atmosphere.
Document ID
19780068570
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Zwickl, R. D.
(Kansas Univ. Lawrence, KS, United States)
Roelof, E. C.
(Kansas Univ. Lawrence, KS, United States)
Gold, R. E.
(Kansas Univ. Lawrence, KS, United States)
Krimigis, S. M.
(Johns Hopkins University Applied Physics Laboratory, Laurel, Md., United States)
Armstrong, T. P.
(Kansas, University Lawrence, Kan., United States)
Date Acquired
August 9, 2013
Publication Date
October 1, 1978
Publication Information
Publication: Astrophysical Journal
Subject Category
Solar Physics
Accession Number
78A52479
Funding Number(s)
CONTRACT_GRANT: N00017-72-C-4401
CONTRACT_GRANT: AF TASK 10
CONTRACT_GRANT: NSF ATM-76-81099
CONTRACT_GRANT: NASA TASK I
Distribution Limits
Public
Copyright
Other

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