A 1-D code for radiation hydrodynamics problems.
Abstract
In order to properly calculate the effects of waves in the chromosphere it is necessary to solve simultaneously the equation of hydrodynamics, radiative transfer and statistical equilibrium. Efficient methods in radiative transfer are beeing combined with methods to treat the dynamical equations capable of resolving shocks. There is no complete code finished yet and this report is more of a progress report centered on methodology rather than a presentation of physically relevant results.
- Publication:
-
Flux Tubes in the Solar Atmosphere
- Pub Date:
- 1989
- Bibcode:
- 1989ftsa.conf...93C
- Keywords:
-
- Solar Chromosphere: Radiative Transfer;
- Solar Chromosphere: Hydrodynamics