Observational evidence for non-Maxwellian electron energy distributions in the solar transition region

Details Observational evidence for non-Maxwellian electron energy distributions in the solar transition region Observational evidence for non-Maxwellian electron energy distributions in the solar transition region

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...280l..35d&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 280, May 1, 1984, p. L35-L37. Research supported by

Astronomy and Astrophysics

Astrophysics

28

Electron Distribution, Electron Energy, Solar Electrons, Solar Spectra, Spectral Energy Distribution, Emission Spectra, Ion Production Rates, Silicon

Scientific paper

Calculations of Si III emission-line strengths, which incorporate the
non-Maxwellian electron energy distributions given by Shoub, are
compared with Skylab observations for the quiet Sun and a solar flare.
The good agreement provides plausible evidence for the existence of such
electron energy distributions in the lower solar transition region.

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