Expected detection of the 2(2)P3/2-2(2)S1/2 hydrogen line in the radio emission spectrum of the quiet sun

Details Expected detection of the 2(2)P3/2-2(2)S1/2 hydrogen line in the radio emission spectrum of the quiet sun Expected detection of the 2(2)P3/2-2(2)S1/2 hydrogen line in the radio emission spectrum of the quiet sun

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65..199d&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Jan.-Feb. 1988, p. 199-202. In Russian.

Astronomy and Astrophysics

Astronomy

1

Emission Spectra, Line Shape, Solar Radio Emission, Solar Spectra, Fine Structure, Spectrum Analysis

Scientific paper

The results of six independent series of spectral observations of the solar radio emission are briefly presented. All these observations showed the existence of the 22P3/2-22S1/2 hydrogen fine-structure emission line in the spectrum of radio emission of the quiet Sun. The line intensity in maximum is 1.55% of the continuum, the profile of the line coincides with the theoretical one quite well.

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