Published May 1971
| Published
Journal Article
Open
On K-line central reversals
- Creators
-
Pasachoff, Jay M.
- Zirin, Harold
Abstract
The double reversal at the center of the spatially-averaged profiles of the H and K resonance lines in the solar atmosphere has been used as a probe to give the distribution of temperature and density with height. Details of the interpretations depend on the mechanism assumed for the formation of the central reversals. The non-LTE theory of stellar atmospheres has succeeded in explaining a symmetric double reversal; the history of this effort has recently been reviewed by Linsky and Avrett (1970).
Additional Information
© 1971 Kluwer Academic Publishers. Provided by the NASA Astrophysics Data System. Received 11 February 1971; Issue Date May 1971. This work was partially supported by NASA Grant NGR 05-002-034 and by NSF Grant No. GA 24015.Attached Files
Published - 1971SoPh___18___27P.pdf
Files
1971SoPh___18___27P.pdf
Files
(110.8 kB)
| Name | Size | Download all |
|---|---|---|
|
md5:8b2513b291abc5d22bfbc74c1eedb12a
|
110.8 kB | Preview Download |
Additional details
- Eprint ID
- 104171
- Resolver ID
- CaltechAUTHORS:20200630-152052528
- NGR 05-002-034
- NASA
- GA 24015
- NSF
- Created
-
2020-06-30Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field