太阳对流区的磁场

IF 23 1区物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS

Living Reviews in Solar Physics Pub Date : 2009-12-14 DOI:10.12942/lrsp-2009-4

Yuhong Fan

{"title":"太阳对流区的磁场","authors":"Yuhong Fan","doi":"10.12942/lrsp-2009-4","DOIUrl":null,"url":null,"abstract":"<p>Active regions on the solar surface are generally thought to originate from a strong toroidal magnetic field generated by a deep seated solar dynamo mechanism operating 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. Understanding this process of active region flux emergence is therefore a crucial component for the study of the solar cycle dynamo. This article reviews studies with regard to the formation and rise of active region scale magnetic flux tubes in the solar convection zone and their emergence into the solar atmosphere as active regions.</p>","PeriodicalId":687,"journal":{"name":"Living Reviews in Solar Physics","volume":"6 1","pages":""},"PeriodicalIF":23.0000,"publicationDate":"2009-12-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.12942/lrsp-2009-4","citationCount":"70","resultStr":"{\"title\":\"Magnetic Fields in the Solar Convection Zone\",\"authors\":\"Yuhong Fan\",\"doi\":\"10.12942/lrsp-2009-4\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>Active regions on the solar surface are generally thought to originate from a strong toroidal magnetic field generated by a deep seated solar dynamo mechanism operating 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. Understanding this process of active region flux emergence is therefore a crucial component for the study of the solar cycle dynamo. This article reviews studies with regard to the formation and rise of active region scale magnetic flux tubes in the solar convection zone and their emergence into the solar atmosphere as active regions.</p>\",\"PeriodicalId\":687,\"journal\":{\"name\":\"Living Reviews in Solar Physics\",\"volume\":\"6 1\",\"pages\":\"\"},\"PeriodicalIF\":23.0000,\"publicationDate\":\"2009-12-14\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.12942/lrsp-2009-4\",\"citationCount\":\"70\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Living Reviews in Solar Physics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.12942/lrsp-2009-4\",\"RegionNum\":1,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Living Reviews in Solar Physics","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.12942/lrsp-2009-4","RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}

引用次数: 70

摘要

太阳表面的活动区域通常被认为是由在太阳对流区底部运行的深层太阳发电机机制产生的强环形磁场产生的。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。因此，了解这一活跃区域通量出现的过程是研究太阳周期发电机的关键组成部分。本文综述了太阳对流区活动区域尺度磁通管的形成和上升以及它们作为活动区域出现在太阳大气中的研究。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

Magnetic Fields in the Solar Convection Zone

查看原文本刊更多论文

Magnetic Fields in the Solar Convection Zone

Active regions on the solar surface are generally thought to originate from a strong toroidal magnetic field generated by a deep seated solar dynamo mechanism operating 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. Understanding this process of active region flux emergence is therefore a crucial component for the study of the solar cycle dynamo. This article reviews studies with regard to the formation and rise of active region scale magnetic flux tubes in the solar convection zone and their emergence into the solar atmosphere as active regions.

求助全文

通过发布文献求助，成功后即可免费获取论文全文。去求助

来源期刊

Living Reviews in Solar Physics Earth and Planetary Sciences-Space and Planetary Science

CiteScore

41.90

自引率

1.40%

发文量

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.