On the Thermal Interpretation of Hard X-Ray Bursts from Solar Flares-Reference-Cited by-同舟云学术

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On the Thermal Interpretation of Hard X-Ray Bursts from Solar Flares

Published:1974 Issue: Volume: Page:395-412
ISSN:
Container-title:Coronal Disturbances
language:
Short-container-title:

Author:

Brown John C.

Publisher

Springer Netherlands

Link

http://link.springer.com/content/pdf/10.1007/978-94-010-2257-6_48

Reference52 articles.

1. Abramowitz, M. and Segun, I. A.: 1965, Handbook of Mathematical Functions, Dover.

2. Batestone, R. M., Evans, K., Parkinson, J. H., and Pounds, K. A.: 1970, Solar Phys. 13, 389.

3. Beigman, I. L. and Vainshtein, L. A.: 1974, Astron. J. (USSR), in press.

4. Billings, D. E.: 1966, A Guide to the Solar Corona, Academic Press, N.Y.

5. Brown, J. C.: 1971, Solar Phys. 18, 489.

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1. A Deep Exposure in High Resolution X-Rays Reveals the Hottest Plasma in the ζ Puppis Wind;The Astrophysical Journal;2020-04-15

2. Global Energetics of Solar Flares. VIII. The Low-energy Cutoff;The Astrophysical Journal;2019-08-06

3. The Compatibility of Flare Temperatures Observed with AIA, GOES, and RHESSI;Solar Physics;2014-02-26

4. References;Electron and Proton Kinetics and Dynamics in Flaring Atmospheres;2012-08-03

5. Deducing Electron Properties from Hard X-ray Observations;Space Science Reviews;2011-08-11

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