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Coronal Mass Ejections and Solar Proton Events During the Great March 1989 DisturbancesThe great active region of March 1989 was the most prolific in X- rays in the preceding 15 years, and produced very large bright optical solar flares. The accompanying solar energetic particle event was one of the four most intense episodes since 1963. These increases in particle fluxes are compared to the major X-ray and optical flares and to the major coronal mass ejections in order to test hypothesis.
Document ID
20060037613
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Feynman, J.
Date Acquired
August 23, 2013
Publication Date
October 1, 1995
Publication Information
Publication: Journal of Geophysical Research
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
Keywords
Corona Coronal Mass Ejections Solar Flares Sun

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