The Life Cycle of Active Region Magnetic Fields

被引：13

作者：

Cheung, M. C. M. ^{[1
,2
]}

van Driel-Gesztelyi, L. ^{[3
,4
,5
]}

Pillet, V. Martinez ^{[6
]}

Thompson, M. J. ^{[7
]}

机构：

[1] Lockheed Martin Solar & Astrophys Lab, 3251 Hanover St, Palo Alto, CA 94304 USA

[2] Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan

[3] Univ Coll London, Mullard Space Sci Lab, Holmbury St Mary, Dorking RH5 6NT, Surrey, England

[4] Hungarian Acad Sci, Res Ctr Astron & Earth Sci, Konkoly Observ, Budapest, Hungary

[5] Univ Paris Diderot, Observ Paris, LESIA, CNRS,UPMC, F-92195 Meudon, France

[6] Natl Solar Observ, 3665 Discovery Dr, Boulder, CO 80303 USA

[7] Natl Ctr Atmospher Res, POB 3000, Boulder, CO 80307 USA

来源：

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

基金：

美国国家科学基金会; 匈牙利科学研究基金会;

关键词：

Sun; Active region; MHD; Magnetic fields; Sunspots; SOLAR CONVECTION ZONE; VECTOR MAGNETOGRAPH DATA; EMERGING FLUX TUBES; DIFFERENTIAL ROTATION; TORSIONAL OSCILLATION; MAIN-SEQUENCE; COOL STARS; EMERGENCE; HELICITY; SUN;

D O I：

10.1007/s11214-016-0259-y

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a contemporary view of how solar active region magnetic fields are understood to be generated, transported and dispersed. Empirical trends of active region properties that guide model development are discussed. Physical principles considered important for active region evolution are introduced and advances in modeling are reviewed.

引用

页码：317 / 349

页数：33

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