On solar hydrogen lines in the far-infrared and submillimeter spectrum

Details On solar hydrogen lines in the far-infrared and submillimeter spectrum On solar hydrogen lines in the far-infrared and submillimeter spectrum

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...112l...3h&link_type=abstract

Astronomy and Astrophysics, vol. 112, no. 2, Aug. 1982, p. L3-L5.

Astronomy and Astrophysics

Astrophysics

10

Chromosphere, H Lines, Infrared Spectra, Pressure Broadening, Solar Spectra, Far Infrared Radiation, H Alpha Line, Rydberg Series, Submillimeter Waves

Scientific paper

Strength of H n-alpha lines, where n ranges from 5 to 20 have been evaluated, using a recent model of the solar chromosphere. It is found that they are much stronger than coronal ions lines, formed by the process of dielectronic recombination; and their wavelength dependence is strongly affected by pressure broadening. Observation of these lines may provide useful diagnostics of the physical conditions in the chromosphere, as well as valuable information on the behavior of atoms in high Rydberg states.

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