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The Hα/Hβ ratio in solar flares

Zirin, Harold and Liggett, Margaret and Patterson, Alan (1982) The Hα/Hβ ratio in solar flares. Solar Physics, 76 (2). pp. 387-392. ISSN 0038-0938. https://resolver.caltech.edu/CaltechAUTHORS:20200610-085821380

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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.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/bf00170993DOIArticle
https://ui.adsabs.harvard.edu/abs/1982SoPh...76..387Z/abstractADSArticle
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.
Funders:
Funding AgencyGrant Number
NASANGL 05-002-034
NSFATM76-21132
Subject Keywords:Flare; Central Intensity; Solar Flare; Stellar Flare; Peak Kernel
Issue or Number:2
Record Number:CaltechAUTHORS:20200610-085821380
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200610-085821380
Official Citation:Zirin, H., Liggett, M. & Patterson, A. The Hα/Hβ ratio in solar flares. Sol Phys 76, 387–392 (1982). https://doi.org/10.1007/BF00170993
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:103812
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:10 Jun 2020 16:13
Last Modified:10 Jun 2020 16:13

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