Energetic electron injection into the high corona during the gradual phase of flares: Evidence against acceleration by a large scale shock

Details Energetic electron injection into the high corona during the gradual phase of flares: Evidence against acceleration by a large scale shock Energetic electron injection into the high corona during the gradual phase of flares: Evidence against acceleration by a large scale shock

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aipc..294..187k&link_type=abstract

High energy solar phenomena-A new ear of spacecraft measurements. AIP Conference Proceedings, Volume 294, pp. 187-192 (1994).

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7

Solar Electromagnetic Emission

Scientific paper

Large scale coronal shock waves are observed by their radio signature associated with many solar flares. In this contribution it is demonstrated that such coronal shock waves are inefficient accelerators of electrons observed both in the downstream region (<1 R0 above the photosphere) and the upstream region (>~10 R0), as compared to other, though unspecified, mechanisms which act in the lower solar atmosphere.

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