Weak Emission Lines in the Wings of Solar H and K
β Scribed by W. Livingston; L. Wallace; O. R. White
- Book ID
- 106533041
- Publisher
- Springer
- Year
- 2011
- Tongue
- English
- Weight
- 386 KB
- Volume
- 270
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Enhancement of the violet K2 emission peak results when the atmospheric layers at heights where Ka forms are moving downward with velocities of 10-20 km/sec or when the K2 layers and those immediately below are moving upward with velocities of 3-7 km/sec. Evidence favoring the former alternative is
Calculations are made for the center-limb variations of the K2 and Kz components of the solar Ca Ii K line using an optically thick model of the chromosphere. The center-limb variations are shown to require an increase of Doppler width with height in the chromosphere and to depend critically upon th