A Simplified Method for Computing Radiative Energy Loss Due to Spectral Lines. II. 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.
Document Details
- Document Type
- Technical Report
- Publication Date
- Mar 26, 1974
- Accession Number
- ADA005390
Entities
People
- Richard C. Canfield
Organizations
- Air Force Cambridge Research Laboratories