Acceleration of ultrarelativistic electrons in solar flares

Details Acceleration of ultrarelativistic electrons in solar flares Acceleration of ultrarelativistic electrons in solar flares

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..383b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, May 1985, p. 383-389) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, May-June

Astronomy and Astrophysics

Astronomy

1

Electron Acceleration, Electron Energy, Relativistic Electron Beams, Solar Flares, Energy Spectra, Solar Magnetic Field, Synchrotron Radiation

Scientific paper

The role of synchrotron losses in the process of acceleration of electrons in the vicinities of magnetic-field zero points in solar flares is considered and typical energies of accelerated particles are estimated. Experimental data are obtained that evidence in favour of acceleration of ultrarelativistic electrons (up to 1 GeV) in the solar flare of April 29, 1973 and steepening of the energy spectrum of electrons. The synchrotron losses are suggested to be a possible cause of the spectrum steepening.

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