Electron Acceleration in the Corona

Details Electron Acceleration in the Corona Electron Acceleration in the Corona

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005soph..229..213s&link_type=abstract

Solar Physics, Volume 229, Issue 2, pp.213-226

Physics

5

Scientific paper

The series of nine impulsive, highly collimated beams of near-relativistic electrons seen by ACE/EPAM on 26 and 27 June 2004 occurred at a quiet time with respect to solar flare and CME production. However, they were accompanied by decametric type III radio bursts observed by WIND/WAVES, which had progressively higher starting frequencies, suggestive of coronal acceleration. There were no CMEs seen by SOHO/LASCO in association with any of the type III bursts except possibly the first. The energy spectrum of the electrons was soft, typically E-4.5 but extended up to at least ˜200 keV. We suggest that the source region for these events is in the high corona. We discuss this result in the context of solar electron acceleration at other times.

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