The Zeeman broadening of high n solar recombination lines-Reference-Cited by-同舟云学术

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The Zeeman broadening of high n solar recombination lines

Published:1975-10 Issue:2 Volume:44 Page:371-382
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Greve A.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00153216.pdf

Reference14 articles.

1. Allen, C. W.: 1973, Astrophys. Quantities, 3rd ed., The Athlone Press, London.

2. Beekers, J. M.: 1970, in R. Howard (ed.), ?Solar Magnetic Fields?, IAU Symp. 43, 11.

3. Berger, P. S. and Simon, M.: 1972, Astrophys. J. 171, 191.

4. Chaisson, E. J. and Beichman, C. A.: 1975, Astrophys. J. 199, L39.

5. Dravskikh, A. F. and Dravskikh, Z. V.: 1969, Astron. Zh. 46, 455.

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1. Solar ALMA predictions: tutorial;Proceedings of the International Astronomical Union;2016-10

2. The Standard Solar Model;International Astronomical Union Colloquium;1990

3. The Standard Solar Model;Inside the Sun;1990

4. Solar structure from global studies of the 5-minute oscillation;Nature;1979-12

5. High n solar radio recombination lines;Solar Physics;1977-05

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