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Identification of the hard X-ray pulse in the flare of September 11-12, 1968

Vorpahl, J. and Zirin, H. (1970) Identification of the hard X-ray pulse in the flare of September 11-12, 1968. Solar Physics, 11 (2). pp. 285-290. ISSN 0038-0938. https://resolver.caltech.edu/CaltechAUTHORS:20200701-072523716

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Abstract

A hard X-ray pulse in the 11–12 September 1968 flare is identified with the formation of a brilliant kernel. Each stage in the X-ray event corresponds to a definite phase in flare development.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/bf00155227DOIArticle
https://ui.adsabs.harvard.edu/abs/1970SoPh...11..285V/abstractADSArticle
Additional Information:© 1970 Kluwer Academic Publishers. Provided by the NASA Astrophysics Data System. Received 16 October 1969; Issue Date February 1970. We wish to express our thanks to Professor Kinsey Anderson for making available for study his data from the OGO-5 Experiment, and to Dr. Sharad Kane for his continued help in understanding and interpreting the records. The University of California, Berkeley Experiment, as well as J. V., is supported by NASA Contract NAS5-9094, and the Cal Tech Photoheliograph, as well as Harold Zirin, by NASA Grant No. NGL 05-002-071, and by NSF Grant No. 1472.
Funders:
Funding AgencyGrant Number
NASANAS5-9094
CaltechUNSPECIFIED
NASANGL 05-002-071
NSF1472
Subject Keywords:Flare; Definite Phase
Issue or Number:2
Record Number:CaltechAUTHORS:20200701-072523716
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200701-072523716
Official Citation:Vorpahl, J., Zirin, H. Identification of the hard X-ray pulse in the flare of September 11–12, 1968. Sol Phys 11, 285–290 (1970). https://doi.org/10.1007/BF00155227
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:104176
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:01 Jul 2020 17:19
Last Modified:01 Jul 2020 17:19

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