The prominence radiation theory

Details The prominence radiation theory The prominence radiation theory

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...45..319i&link_type=abstract

Solar Physics, vol. 45, Dec. 1975, p. 319-338.

Physics

Radiation Sources, Solar Prominences, Solar Radiation, Solar Spectra, Continuous Spectra, Diffuse Radiation, Line Spectra, Resonance Scattering

Scientific paper

The present work is a review of papers related to the theory of prominence radiation. Special attention is paid to stationary equations and the theory of radiation diffusion in the lines and continua of hydrogen, helium, and metals. It is concluded that prominences are low-temperature formations (7000 K) of low density and that the chemical composition of prominences and that of the solar atmosphere are the same. The prominence radiation in the lines of hydrogen, helium, and metals is due mainly to quasi-resonance scattering of the photospheric radiation.

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