Ion-collision broadening of solar lines in the far-infrared and submillimeter spectrum

Details Ion-collision broadening of solar lines in the far-infrared and submillimeter spectrum Ion-collision broadening of solar lines in the far-infrared and submillimeter spectrum

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...181..134h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 181, no. 1, July 1987, p. 134-137.

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Far Infrared Radiation, Ionic Collisions, Solar Spectra, Spectral Line Width, Stark Effect, Submillimeter Waves, Computational Astrophysics, Ion Recombination, Solar Atmosphere

Scientific paper

The authors give new theoretical data for calculating the ion impact broadening of solar far-infrared and submillimeter lines. These are more accurate than, and should be preferred to data extrapolated directly from Griem's (1967) work on radio recombination lines. The variation of the line width as a function of the upper level of the transition has also been investigated. It may be a potentially important diagnostic tool for determining the physical conditions in the solar atmosphere.

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