A procedure for investigating solar flare mechanisms by means of the hydrogen lines

Details A procedure for investigating solar flare mechanisms by means of the hydrogen lines A procedure for investigating solar flare mechanisms by means of the hydrogen lines

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pazh....4..415o&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 4, Sept.-Oct. 1978, p. 415-419.) Soviet Astronomy Letters, vol. 4, Sept.-Oct. 1978, p.

Astronomy and Astrophysics

Astronomy

1

H Lines, Hydrogen, Plasma Turbulence, Solar Flares, Solar Spectra, Stellar Models

Scientific paper

Hydrogen line profiles observed in solar flares are analyzed on the basis of a systematic theory in which all significant noise effects are incorporated in analytic form. The results obtained provide direct confirmation of the hypothesis of turbulent flare plasma, which is the basis for most theoretical flare models. Quantitative analysis of several flares indicates strong low-frequency turbulence that develops to a level of the order of 0.1.

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