Published May 1969
| Published
Journal Article
Open
Two prominence eruptions and the problem of emission
- Creators
- Zirin, Harold
Chicago
An error occurred while generating the citation.
Abstract
Two flare unconnected eruptions on January 15 and 29, 1968, are discussed. The first is a filament which turns bright and erupts upward, reappearing an hour later. The second is a large eruptive arch seen against the disk. The arch is bright at the top of its trajectory, turns dark, but produces chromospheric emission at the point of impact. The emission at the top of the arch is ascribed to the velocity shift of the illuminating chromospheric Ha line. It is shown that such emission will occur only if the motion is transverse to the line of sight and the prominence is optically thin.
Additional Information
© 1969 Kluwer Academic Publishers. Provided by the NASA Astrophysics Data System. Received 28 October 1968; Issue Date May 1969. This research was supported by the National Science Foundation under Grant 1472, the Advanced Research Projects Agency under the Office of Naval Research Grant N00014-67-C-0140, and the National Aeronautics and Space Administration under Grant NGR 05 002 034.Attached Files
Published - 1969SoPh____7__243Z.pdf
Files
1969SoPh____7__243Z.pdf
Files
(2.8 MB)
| Name | Size | Download all |
|---|---|---|
|
md5:c41bcefa413fcae3d32a136266c37655
|
2.8 MB | Preview Download |
Additional details
- Eprint ID
- 104180
- Resolver ID
- CaltechAUTHORS:20200701-083125302
- NSF
- 1472
- Advanced Research Projects Agency (ARPA)
- Office of Naval Research (ONR)
- N00014-67-C-0140
- NASA
- NGR 05 002 034
- Created
-
2020-07-01Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field