Flare processes in a quiet prominence

Details Flare processes in a quiet prominence Flare processes in a quiet prominence

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15...82k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Jan. 1989, p. 82-88. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

3

Balmer Series, Solar Electrons, Solar Flares, Solar Prominences, Electron Density (Concentration), Emission Spectra, Line Of Sight, Line Spectra

Scientific paper

A novel method is proposed for determining the limits of electron concentration variations in a plasma along the line of sight from the precontinuum of the Balmer series. The characteristic value of n(e) for volumes responsible for hydrogen line emission is about 5 x 10 to the 10th/cu cm. It is concluded that, at small volumes of a quiet prominence, a powerful flarelike energy release takes place which manifests itself in a Balmer precontinuum.

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