Abstract Solar energetic particle events often consist of two components: a ‘prompt’ component of particles accelerated in the flare or by a coronal shock, and an ‘energetic storm particle’ component accelerated by an interplanetary shock. In events observed by two or more spacecraft the time-development of the proton spectrum, together with the analysis of the intensity and anisotropy time profiles, allows one to distinguish between these components.
Time-development of proton energy spectra in solar energetic particle events
Advances in Space Research ; 13 , 9 ; 363-366
1993-01-01
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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