Magnetic Fields in the Solar Convection Zone

IF 23 1区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Yuhong Fan
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引用次数: 152

Abstract

Recent studies of the dynamic evolution of magnetic flux tubes in the solar convection zone are reviewed with focus on emerging flux tubes responsible for the formation of solar active regions. The current prevailing picture is that active regions on the solar surface originate from strong toroidal magnetic fields generated by the solar dynamo mechanism at the thin tachocline layer at the base of the solar convection zone. Thus the magnetic fields need to traverse the entire convection zone before they reach the photosphere to form the observed solar active regions. This review discusses results with regard to the following major topics:

Abstract Image

太阳对流区的磁场
本文综述了近年来太阳对流区磁通管动态演化的研究进展,重点介绍了太阳活动区形成中新出现的磁通管。目前流行的观点是,太阳表面的活动区域起源于太阳对流区底部薄速斜层上太阳发电机机制产生的强环形磁场。因此,磁场需要穿过整个对流区,才能到达光球层,形成观测到的太阳活动区。本次审查讨论了以下主要主题的结果:
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Living Reviews in Solar Physics
Living Reviews in Solar Physics Earth and Planetary Sciences-Space and Planetary Science
CiteScore
41.90
自引率
1.40%
发文量
3
审稿时长
20 weeks
期刊介绍: Living Reviews in Solar Physics is a peer-reviewed, full open access, and exclusively online journal, publishing freely available reviews of research in all areas of solar and heliospheric physics. Articles are solicited from leading authorities and are directed towards the scientific community at or above the graduate-student level. The articles in Living Reviews provide critical reviews of the current state of research in the fields they cover. They evaluate existing work, place it in a meaningful context, and suggest areas where more work and new results are needed. Articles also offer annotated insights into the key literature and describe other available resources. Living Reviews is unique in maintaining a suite of high-quality reviews, which are kept up-to-date by the authors. This is the meaning of the word "living" in the journal''s title.
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