Variability of the integrated solar K line emission

Author:

Bumba V.,Růžičková-Topolová B.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference5 articles.

1. Bumba, V. and Howard, R.: 1965a, Astrophys. J. 141, 1502.

2. Bumba, V. and Howard, R.: 1965b, Astrophys. J. 141, 1492.

3. Bumba, V., Howard, R., and Smith, S. F.: 1965, Goddard Symp. on Magnetic Stars.

4. Simon, G. W. and Leighton, R. B.: 1964, Astrophys. J. 140, p. 1120.

5. Valníček, B., Letfus, V., Blaha, M., Švestka, Z., and Seidl, Z.: 1959, Bull. Astron. Inst. Czechoslovakia 10, 149.

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1. Rotations of the sun and stars and their activity;Kinematics and Physics of Celestial Bodies;2009-06

2. The HeI λ10830 Å Line as an Indicator of the Chromospheric and Coronal Activity of the Sun;International Astronomical Union Colloquium;1991

3. The Mg 280-nm doublet as a monitor of changes in solar ultraviolet irradiance;Journal of Geophysical Research;1986

4. VII. The Sun as a Star;Transactions of the International Astronomical Union;1985

5. The relationship between solar activity and the H and K line cores in integrated sunlight;Solar Physics;1978-04

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