The observation of the chromospheric fine structure by the 53-cm lyot coronagraph-Reference-Cited by-同舟云学术

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The observation of the chromospheric fine structure by the 53-cm lyot coronagraph

Published:1970-06 Issue:3 Volume:12 Page:379-390
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Nikolsky G. M.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00148021.pdf

Reference8 articles.

1. Beckers, J. M.: 1968, Solar Phys. 3, 367.

2. Bhavilai, R., Norton, G., and Giovanelli, R. G.: 1965, Astrophys. J., 141, 274.

3. Gnevyshev, M. N., Nikolsky, G. M., and Sazanov, A. A.: 1967, Solar Phys. 2, 233.

4. Lyot, B.: 1932, L'Astronomie 46, 272; Compt. Rend. Acad. Sci. (France) 194, 443.

5. Nikolsky, G. M. and Sazanov, A. A.: 1966, Astron. Zh. 43, 928.

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