Rotational models of solar prominences and flares

Details Rotational models of solar prominences and flares Rotational models of solar prominences and flares

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985acaps...5..132y&link_type=abstract

(Acta Astrophysica Sinica, vol. 5, no. 1, 1985, p. 132-139) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 9, Sept. 1

Astronomy and Astrophysics

Astrophysics

Solar Flares, Solar Prominences, Solar Rotation, Angular Velocity, Balmer Series, Line Spectra, Solar Spectra, Stellar Models

Scientific paper

The effect of rotation on the spectral lines of solar active bodies (flares and prominences) is studied. For the two cases of the spin velocity being a constant and having a gradient, the Balmer line profiles and their variation from the center of the active body to the edge are calculated. Methods for finding the spin velocity from the inclination or shift of the lines and the velocity gradient from the curvature of the lines are developed and applied to observational data from the ring flare of April 27, 1981.

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