Published March 1982
| Published
Journal Article
Open
The Hα/Hβ ratio in solar flares
Abstract
We have measured the ratio of Hα to Hβ central intensities in the peak kernels of 14 flares, using simultaneous filtergrams. The ratio is typically one with some scatter. By contrast, in stellar flares the ratio is about 0.8.
Additional Information
© 1982 Kluwer Academic Publishers. Provided by the NASA Astrophysics Data System. Received 7 November, 1980; in revised form 16 April, 1981. This work was supported by NASA under grant NGL 05-002-034 and the Atmospheric Sciences section of the NSF under ATM76-21132.Attached Files
Published - 1982SoPh___76__387Z.pdf
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Additional details
- Eprint ID
- 103812
- Resolver ID
- CaltechAUTHORS:20200610-085821380
- NGL 05-002-034
- NASA
- ATM76-21132
- NSF
- Created
-
2020-06-10Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field