Small-Scale Solar Magnetic Fields

被引：138

作者：

de Wijn, A. G. ^{[1
]}

Stenflo, J. O. ^{[2
]}

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

Tsuneta, S. ^{[4
]}

机构：

[1] Univ Corp Atmospher Res, Boulder, CO 80307 USA

[2] ETH, Inst Astron, CH-8093 Zurich, Switzerland

[3] Max Planck Inst Sonnensyst Forsch, D-37191 Katlenburg Lindau, Germany

[4] Natl Astron Observ, Mitaka, Tokyo 1818588, Japan

来源：

SPACE SCIENCE REVIEWS | 2009年 / 144卷 / 1-4期

关键词：

Sun; Photosphere; Magnetism; Small scale; G-BAND BRIGHT; INTERNETWORK QUIET SUN; DOPPLER IMAGER MAGNETOGRAMS; EPHEMERAL ACTIVE REGIONS; I-4607 ANGSTROM LINE; TO-LIMB VARIATION; FLUX TUBES; PHOTOSPHERIC NETWORK; OPTICAL TELESCOPE; INFRARED LINES;

D O I：

10.1007/s11214-008-9473-6

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

As we resolve ever smaller structures in the solar atmosphere, it has become clear that magnetism is an important component of those small structures. Small-scale magnetism holds the key to many poorly understood facets of solar magnetism on all scales, such as the existence of a local dynamo, chromospheric heating, and flux emergence, to name a few. Here, we review our knowledge of small-scale photospheric fields, with particular emphasis on quiet-sun field, and discuss the implications of several results obtained recently using new instruments, as well as future prospects in this field of research.

引用

页码：275 / 315

页数：41

共 183 条

[1] The magnetic connection between the convection zone and corona in the quiet sun [J].