The hydrogen Balmer, Paschen, and Brackett series lines in quiescent prominences
Abstract
To calculate the Balmer, Paschen, and Brackett line intensities, we solved the statistical equilibrium equations for a twenty level plus continuum atom of hydrogen.
- Publication:
-
Solar Physics
- Pub Date:
- August 1986
- DOI:
- 10.1007/BF00158499
- Bibcode:
- 1986SoPh..106..315R
- Keywords:
-
- Balmer Series;
- H Lines;
- Paschen Series;
- Solar Prominences;
- Spectral Energy Distribution;
- Continuum Modeling;
- Equilibrium Equations;
- Stellar Models;
- Solar Physics;
- Optical Depth;
- Line Intensity;
- Thermal Conduction Coefficient;
- Radiative Rate;
- Series Line