The modeling of the solar upper photosphere and lower chromosphere based upon ATM data
Abstract
The use of the solar H I Lyman spectral line as a diagnostic of the lower to middle chromosphere is discussed. Quiet sun Lyman profiles from the photographic spectra were subjected to data reduction and appropriate theoretical modelling was accomplished. Apollo telescope mount data was utilized.
- Publication:
-
NASA STI/Recon Technical Report N
- Pub Date:
- July 1982
- Bibcode:
- 1982STIN...8312033H
- Keywords:
-
- Apollo Telescope Mount;
- Atmospheric Models;
- Chromosphere;
- Photosphere;
- Skylab Program;
- Autoionization;
- Digital Data;
- H Lines;
- Lyman Spectra;
- Photographs;
- Solar Physics