The Observation of 10–50 KeV Solar Flare X-rays by the OGO Satellites and their Correlation with Solar Radio and Energetic Particle Emission-Reference-Cited by-同舟云学术

The Observation of 10–50 KeV Solar Flare X-rays by the OGO Satellites and their Correlation with Solar Radio and Energetic Particle Emission

Published:1968 Issue: Volume: Page:490-509
ISSN:
Container-title:Structure and Development of Solar Active Regions
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Author:

Arnoldy R. L.,Kane S. R.,Winckler J. R.

Publisher

Springer Netherlands

Link

http://link.springer.com/content/pdf/10.1007/978-94-011-6815-1_74.pdf

Reference29 articles.

1. Acton, L. W. (1964) Nature, 204, 64–65.

2. Anderson, K. A., Winckler, J.R. (1962) J, geophys. Res., 67, 4103–4117.

3. Arnoldy, R.L., Kane, S.R., Winckler, J.R. (1967 a) Solar Phys., 2, 171.

4. Arnoldy, R.L., Kane, S.R., Winckler, J.R. 1967 b) University of Minnesota Technical Report CR-97. Also, to be published in Astrophysical Journal, February, 1968.

5. Bruzek, A. (1964) AAS-NASA Symposium on the Physics of Solar Flares, Scientific and Technical Information Division, NASA, Washington, D.C., 301–322.

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