Dynamic Behavior of the Solar Atmosphere

Details Dynamic Behavior of the Solar Atmosphere Dynamic Behavior of the Solar Atmosphere

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997assl..225..261s&link_type=abstract

SCORe'96 : Solar Convection and Oscillations and their Relationship, Proceedings of a workshop, held in Aarhus, Denmark, May 27

Astronomy and Astrophysics

Astrophysics

2

Sun:Chromosphere, Radiation Transfer, Hydrodynamics, Shock Waves, Diagnostics

Scientific paper

We have studied the dynamics of acoustic and MHD waves in the solar atmosphere using a one-dimensional, non-LTE, radiation magneto-hydrodynamic code, with 6 level model atoms for hydrogen and singly ionized calcium. We drive waves by a piston through an initial atmosphere in radiative equilibrium. We report on the effects of radiative energy loss on the waves, the effects of shocks on line formation, and the behavior of typical diagnostics in a dynamic atmosphere.

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