Energetic electron populations in solar flares

Details Energetic electron populations in solar flares Energetic electron populations in solar flares

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aipc..294..199w&link_type=abstract

High energy solar phenomena-A new era of spacecraft measurements. AIP Conference Proceedings, Volume 294, pp. 199-204 (1994).

Physics

4

Solar Electromagnetic Emission

Scientific paper

Millimeter-interferometer observations of flares are used to study the MeV-energy electrons accelerated in solar flares. The focus of this study is a remarkable similarity found in the time profiles of emission associated with the impulsive onset of a flare. In a large fraction of flares, the impulsive phase emission at millimeter wavelengths consists of a rapid rise (~5 seconds) linear in time to a sharp peak, followed by an exponential decay with a decay constant of order 15 seconds. The onset of millimeter emission may be delayed by several seconds with respect to the onset of hard X-rays. The implications of this homologous property are discussed briefly.

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