The contribution of ion-atom radiative collisions to the opacity of the solar atmosphere

Details The contribution of ion-atom radiative collisions to the opacity of the solar atmosphere The contribution of ion-atom radiative collisions to the opacity of the solar atmosphere

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...276..187m&link_type=abstract

Astronomy and Astrophysics, Vol. 276, p. 187 (1993)

Astronomy and Astrophysics

Astrophysics

13

Atomic Processes, Molecular Processes, Sun: Photosphere, Sun: Chromosphere

Scientific paper

We investigate the contribution to the opacity of the solar atmosphere of some processes other than formation and photodissociation of the H- ion. We show that positive-ion-atom radiative collision processes are not negligible at certain layers of the photosphere and of the chromosphere, although they make only a negligible contribution to the solar continuous optical emission emergent intensity.

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