Electron acceleration in current sheets of solar flares

Details Electron acceleration in current sheets of solar flares Electron acceleration in current sheets of solar flares

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17..835l&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, Sept. 1991, p. 835-840. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Current Sheets, Electron Acceleration, Solar Electrons, Solar Flares, Astronomical Models, Magnetic Field Reconnection, Solar Magnetic Field

Scientific paper

A model for electron acceleration in high-temperature turbulent current sheets is presented. In this model different processes of fast-particle generation in solar flares are found to have a common cause, namely, magnetic energy dissipation in a region of magnetic reconnection. The spectral index of 2-5 and the total number of electrons accelerated during the main phase of a flare are consistent with observational data.

Affiliated with

Also associated with

No associations

Rating

Electron acceleration in current sheets of solar flares does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Electron acceleration in current sheets of solar flares, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Electron acceleration in current sheets of solar flares will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1342122