On the characteristics of the basic framework of solar active regions and the magnetohydrodynamical structure of the convection zone-Reference-Cited by-同舟云学术

On the characteristics of the basic framework of solar active regions and the magnetohydrodynamical structure of the convection zone

Published:1973-11 Issue:1 Volume:33 Page:131-143
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Yoshimura Hirokazu

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00152385.pdf

Reference46 articles.

1. Alfvén, H.: 1950, Tellus 2, 74.

2. Ambro?, P., Bumba, V., Howard, R., and Sýkora, J.: 1971, in R. Howard (ed.), ?Solar Magnetic Fields? IAU Symp. 43, 696.

3. Babcock, H. W.: 1961, Astrophys. J. 133, 572.

4. Brunner, W.: 1930, Astron. Mitt. Zürich, No. 124, 67.

5. Bruzek, A.: 1967, Solar Phys. 2, 451.

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