Stability of the photometric observations of the solar corona and variations of its intensity in the solar cycle 21-Reference-Cited by-同舟云学术

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Stability of the photometric observations of the solar corona and variations of its intensity in the solar cycle 21

Published:1984-01 Issue:1 Volume:90 Page:177-184
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Gnevyshev M. N.,Mikhailutsa V. P.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00153793.pdf

Reference5 articles.

1. Gnevyshev, M. N.: 1963, Astron. Zh. 40, 401.

2. Gnevyshev, M. N.: 1966, Soviet Phys. Uspekhi 90, 291.

3. Gnevyshev, M. N.: 1967, Solar Phys. 1, 108.

4. Gnevyshev, M. N.: 1977, Solar Phys. 51, 175.

5. Letfus, V. and Sýkora, J.: 1982, Atlas of the Green Corona Synoptic Charts for the Period 1947?1976, Bratislava, p. 9.

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1. On the existence of the east-west asymmetry in the optical observations of the solar corona;Geomagnetism and Aeronomy;2010-12

2. Temperature of Polar Corona of the Sun According to Kislovodsk Observations During 1957–2002;Solar Physics;2006-08

3. The proportion of hot and cold regions in the polar solar corona during 1957–2002;Astronomy Reports;2005-11

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