A simplified method for computing radiative energy loss due to spectral lines. 2: Programs for solar flare models
Abstract
The paper lists FORTRAN-IV programs that implement a simplified method for computing radiative loss rates due to spectral lines. As it is planned to apply these techniques to solar flare models, the programs are set up to take into account Lyman alpha, Balmer-alpha and H-, the principal contributors to radiative energy loss in solar flares.
- Publication:
-
Environmental Research Papers Air Force Cambridge Research Labs
- Pub Date:
- March 1974
- Bibcode:
- 1974erp..reptQ....C
- Keywords:
-
- Computer Programming;
- Energy Dissipation;
- Line Spectra;
- Models;
- Radiative Transfer;
- Solar Flares;
- Balmer Series;
- Computer Programs;
- Fortran;
- Lyman Spectra;
- Prediction Analysis Techniques;
- Solar Radiation