A self-consistent model for the storm radio emission from the Sun-Reference-Cited by-同舟云学术

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A self-consistent model for the storm radio emission from the Sun

Published:1991-03 Issue:1 Volume:132 Page:173-193
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Thejappa G.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00159137.pdf

Reference36 articles.

1. Benz, A. O. and Thejappa, G.: 1988, Astron. Astrophys. 202, 267.

2. Benz, A. O. and Wentzel, D. G.: 1981, Astron. Astrophys. 94, 100.

3. Breizmann, B. N.: 1986, Soviet J. Plasma Phys. 12, 942.

4. Daigne, G., Lantos-Jarray, M. F., and Pick, M.: 1970, in R. Howard (ed.), IAU Symp. 43, 609.

5. Elgaroy, O.: 1977, Solar Noise Storms, Pergamon Press, Oxford.

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3. Axion quark nuggets. Dark matter and matter–antimatter asymmetry: Theory, observations and future experiments;Modern Physics Letters A;2021-05-31

4. Impulsive radio events in quiet solar corona and axion quark nugget dark matter;Physical Review D;2020-12-21

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