Line radiation cooling with partial redistribution in atmospheres with shocks.

Details Line radiation cooling with partial redistribution in atmospheres with shocks. Line radiation cooling with partial redistribution in atmospheres with shocks.

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...293..166h&link_type=abstract

Astronomy and Astrophysics 293, 166-171 (1995)

Astronomy and Astrophysics

Astrophysics

13

Methods: Numerical, Sun: Chromosphere, Shock Waves, Radiative Transfer, Stars: Atmospheres

Scientific paper

We investigate the energy loss by spectral line radiation assuming partial redistribution PRD in atmospheres permeated by acoustic shock waves. It is found that with PRD the emission is much reduced and much more concentrated in a narrow region behind the shocks compared to cases which assume complete redistribution CRD. A fast method to approximate the radiation losses for time-dependent calculations is proposed.

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