Solar Magnetoconvection and Small-Scale Dynamo Recent Developments in Observation and Simulation

被引：38

作者：

Borrero, J. M. ^{[1
]}

Jafarzadeh, S. ^{[2
]}

Schuessler, M. ^{[3
]}

Solanki, S. K. ^{[3
,4
]}

机构：

[1] Kiepenheuer Inst Sonnenphys, Schoneckstr 6, D-79104 Freiburg, Germany

[2] Univ Oslo, Inst Theoret Astrophys, POB 1029 Blindern, N-0315 Oslo, Norway

[3] Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany

[4] Kyung Hee Univ, Sch Space Res, Yongin 446701, Gyeonggi Do, South Korea

来源：

SPACE SCIENCE REVIEWS | 2017年 / 210卷 / 1-4期

基金：

新加坡国家研究基金会;

关键词：

Sun; Convection; Magnetic field; G-BAND BRIGHT; MAGNETIC-FLUX-TUBES; TO-LIMB VARIATION; STOKES-V ASYMMETRY; QUIET-SUN; CONVECTIVE INSTABILITY; PHOTOSPHERIC FACULAE; INTENSITY CONTRAST; MODEL-CALCULATIONS; INFRARED LINES;

D O I：

10.1007/s11214-015-0204-5

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A number of observational and theoretical aspects of solar magnetoconvection are considered in this review. We discuss recent developments in our understanding of the small-scale structure of the magnetic field on the solar surface and its interaction with convective flows, which is at the centre of current research. Topics range from plage areas in active regions over the magnetic network shaped by supergranulation to the ubiquituous 'turbulent' internetwork fields. On the theoretical side, we focus upon magnetic field generation by small-scale dynamo action.

引用

页码：275 / 316

页数：42

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