CaltechAUTHORS
Published March 1982 | Version Published
Journal Article Open

The Hα/Hβ ratio in solar flares

Creators

  • 1. ROR icon California Institute of Technology

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.

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Published - 1982SoPh___76__387Z.pdf

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Additional details

Identifiers

Eprint ID
103812
Resolver ID
CaltechAUTHORS:20200610-085821380

Related works

Describes
https://ui.adsabs.harvard.edu/abs/1982SoPh...76..387Z/abstract (URL)

Funding

NASA
NGL 05-002-034
NSF
ATM76-21132

Dates

Created
2020-06-10
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Updated
2021-11-16
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