Study of Magnetic Motions in the Solar Photosphere and Their Implications for Heating the Solar Atmosphere
Abstract
Dynamic modeling of CO line formation, and the development of a two-dimensional radiative transfer code that includes the effects of partial frequency redistribution, are described.
- Publication:
-
Smithsonian Astrophysical Observatory Report
- Pub Date:
- April 1996
- Bibcode:
- 1996sao..rept.....N
- Keywords:
-
- Radiative Transfer;
- Solar Atmosphere;
- Photosphere;
- Chromosphere;
- Carbon Monoxide;
- Line Spectra;
- Solar Magnetic Field;
- Atmospheric Models;
- Atmospheric Heating;
- Frequency Distribution;
- Inhomogeneity;
- Lyman Alpha Radiation;
- Lyman Beta Radiation;
- Hydrogen;
- Solar Spectra;
- Molecular Spectra;
- Solar Temperature;
- Time Dependence;
- Dynamic Models;
- Stellar Activity;
- Applications Programs (Computers);
- Solar Physics