A Fokker-Planck description of the trapping and precipitation of fast electrons in solar flares

Details A Fokker-Planck description of the trapping and precipitation of fast electrons in solar flares A Fokker-Planck description of the trapping and precipitation of fast electrons in solar flares

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...234..487m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 234, no. 1-2, Aug. 1990, p. 487-495. Research supported by Rutherford Appleton

Astronomy and Astrophysics

Astrophysics

19

Electron Precipitation, Fokker-Planck Equation, Solar Corona, Solar Flares, Solar X-Rays, Trapped Particles, Chromosphere, Electron Distribution

Scientific paper

The Fokker-Planck model is used in an attempt to determine the steady
state population of nonthermal electrons in a flaring coronal loop. The
electron precipitation rate and the ratio of footprint to coronal hard
X-ray emission are obtained numerically. The apparent absence of large
Doppler shifts in soft X-ray line spectra is examined in detail.

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