Spectral coefficients of emission and absorption due to ion-atom radiation collisions in the solar atmosphere

Details Spectral coefficients of emission and absorption due to ion-atom radiation collisions in the solar atmosphere Spectral coefficients of emission and absorption due to ion-atom radiation collisions in the solar atmosphere

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26as..103...57m&link_type=abstract

Astronomy and Astrophysics Suppl. 103, 57-66 (1994)

Astronomy and Astrophysics

Astrophysics

10

Scientific paper

Spectral coefficients of spontaneous emission and absorption (for 365nm <= λ <= 820nm range) due to ion-atom radiation processes H^+^ + H(1s) <--> H^+^_2_(1{SIGMA}_g_) and H^+^ + H(1s) <--> H(1s) + H^+^ are presented. Calculations have been performed within semiclassical approach for standard solar photosphere and chromosphere models. The presented numerical results enable the inclusion of considered ion-atom radiative processes in the optical depth calculation for the layers mentioned. These results might be of interest as well for other astrophysical plasmas with dominant hydrogen component and temperatures around 6000 K.

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