Spacecraft measurements of solar energetic particles

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

Solar energetic particles (SEPs) are accelerated in the solar atmosphere during flares and coronal mass ejections. They can escape from the Sun and propagate through interplanetary space, where they can be measured by particle detectors on board spacecraft. Key to understanding the acceleration and propagation of these particles are: 1) combined analysis of SEP data and solar flare/CME observations and 2) easy comparison of SEP data from different spacecraft/instruments. This paper will demonstrate the importance of the multi-spacecraft and multi-instrument approach by showing new results from the analysis of SEP data from Ulysses and Wind.

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