Asymmetric variations of the coronal green line intensity-Reference-Cited by-同舟云学术

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Asymmetric variations of the coronal green line intensity

Published:1988 Issue:2 Volume:115 Page:367-384
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Tritakis V. P.,Mavromichalaki H.,Petropoulos B.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00148734.pdf

Reference43 articles.

1. Antonucci, E.: 1974, Solar Phys. 34, 471.

2. Bumba, V. and Howard, R.: 1969, Solar Phys. 7, 28.

3. Cant�, A. M., Godoli, G., and Poletto, G.: 1970, Astron. Astrophys. 120, L1.

4. Cuperman, S. and Sternlieb, A.: 1972, Solar Phys. 25, 493.

5. Dollfus, A.: 1971, in C. J. Macris (ed.), Physics of Solar Corona, Astrophysics and Space Science Library, Vol. 27, p. 97.

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