Time-development of proton energy spectra in solar energetic particle events

Computer Science

Scientific paper

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Scientific paper

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.

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