The H-alpha/H-beta ratio in solar flares

Details The H-alpha/H-beta ratio in solar flares The H-alpha/H-beta ratio in solar flares

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...76..387z&link_type=abstract

Solar Physics, vol. 76, Mar. 1982, p. 387-392.

Physics

3

Astronomical Photography, Chromosphere, H Alpha Line, H Beta Line, Solar Flares, Cinematography, Optical Thickness, Solar Atmosphere, Solar Temperature, Stellar Flares

Scientific paper

The present investigation involves the study of an extensive body of data accumulated of simultaneous H-alpha and H-beta cinematography of flares. The data were obtained with two telescopes simultaneously photographing flares in H-alpha and H-beta. The results of measurements in a number of flares are presented in a table. The flares were selected purely by optical quality of the data. That the measured ratios are not too different from those in stellar flares is suggested by the last two columns of the table. These columns show that a variety of possible line width ratios could give an integrated intensity ratio of less than unity.

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