Opposite Polarities in the Development of Some Regularities in the Distribution of Large-Scale Magnetic Fields-Reference-Cited by-同舟云学术

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Opposite Polarities in the Development of Some Regularities in the Distribution of Large-Scale Magnetic Fields

Published:1971 Issue: Volume:43 Page:696-709
ISSN:0074-1809
Container-title:Symposium - International Astronomical Union
language:en
Short-container-title:Symp. - Int. Astron. Union

Author:

Ambrož P.,Bumba V.,Howard R.,Sýkora J.

Abstract

When viewed separately in the two polarities, the large-scale pattern of magnetic fields on the Sun gives an appearance reminiscent of a very large cellular structure. These structures and their relation to ‘active longitudes’ are discussed.

Publisher

Cambridge University Press (CUP)

Reference19 articles.

1. On the problem of active longitudes of sunspots and flares

2. On the possible existence of a 29-day period in the sunspot number series 1940-1964

3. Proton Flare Project, 1966

4. ‘Structure and Development of Solar Active Regions’;Švestka;IAU Symp.,1968b

Cited by 6 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Giant longitude zones on the sun;Solar Physics;1989

2. About the Relation between the Limb Effect of the Redshift on the Sun and the Large-Scale Distribution of Solar Activity;Basic Mechanisms of Solar Activity;1976

3. Studies of solar magnetic fields;Solar Physics;1974-10

4. Studies of solar magnetic fields;Solar Physics;1974-09

5. On the characteristics of the basic framework of solar active regions and the magnetohydrodynamical structure of the convection zone;Solar Physics;1973-11

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