Solar Emission Lines Produced in the Wake of a Shock Wave - Part Two - Line Profiles

Details Solar Emission Lines Produced in the Wake of a Shock Wave - Part Two - Line Profiles Solar Emission Lines Produced in the Wake of a Shock Wave - Part Two - Line Profiles

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...110..163f&link_type=abstract

Astronomy and Astrophysics, Vol.110, P. 163, 1982

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We consider the influence of the passage of a shock wave on the profiles of lines in its wake. The time dependent equations are solved following a fluid particle which has undergone the shock compression and the profiles of the C IV λ1548.20 and O V λl2l8.35 limes are evaluated. For the steady-state atmosphere, we employ hole model of Pineau des Forêts (1979: Astron. Astrophys. 78,159). Comparison of the computed line profiles with existing observations proves inconclusive and further observations are suggested which would provide a more direct test of the model.

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