Polarization of the white-light corona and its large-scale structure in the period of solar cycle maximum-Reference-Cited by-同舟云学术

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Polarization of the white-light corona and its large-scale structure in the period of solar cycle maximum

Published:1993-06 Issue:2 Volume:145 Page:279-290
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Badalyan O. G.,Livshits M. A.,S�kora J.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00690656.pdf

Reference17 articles.

1. Badalyan, O. G.: 1986,Astron. Astrophys. 169, 305.

2. Badalyan, O. G.: 1988,Physics of Solar Activity, Nauka, Moscow, p. 88.

3. Badalyan, O. G. and Livshits, M. A.: 1986,Solar Phys. 103, 385.

4. Clette, F., Cugnon, P., and Koeckelenbergh, A.: 1985,Solar Phys. 98, 163.

5. D�rst, J.: 1973,Astron. Mitt. Z�rich, No. 320, 1.

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