Abstract:<p>In-situ observations of solar energetic particle events are determined by a combination of acceleration, injection, and transport processes which are often hard to disentangle. However, the energy spectrum of impulsive electron events is believed to carry the imprint of the flare acceleration process which can be studied by analyzing the hard X-ray (HXR) spectrum of the flare.</p><p>Using STEREO/SEPT electron data of the whole STEREO mission we have identified 64 so… Show more
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