Magnetic Flux Transport at the Solar Surface

	Magnetic Flux Transport at the Solar Surface
	Jiang, J.1 ; Hathaway, D. H.2; Cameron, R. H.3; Solanki, S. K.3,4; Gizon, L.3,5; Upton, L.6,7
刊名	SPACE SCIENCE REVIEWS
	2014-12-01
卷号	186 期号:1-4 页码:491-523
关键词	Sun: magnetic fields Sun: photosphere Flux transport Meridional flow Differential rotation Diffusion
英文摘要	After emerging to the solar surface, the Sun's magnetic field displays a complex and intricate evolution. The evolution of the surface field is important for several reasons. One is that the surface field, and its dynamics, sets the boundary condition for the coronal and heliospheric magnetic fields. Another is that the surface evolution gives us insight into the dynamo process. In particular, it plays an essential role in the Babcock-Leighton model of the solar dynamo. Describing this evolution is the aim of the surface flux transport model. The model starts from the emergence of magnetic bipoles. Thereafter, the model is based on the induction equation and the fact that after emergence the magnetic field is observed to evolve as if it were purely radial. The induction equation then describes how the surface flows-differential rotation, meridional circulation, granular, supergranular flows, and active region inflows-determine the evolution of the field (now taken to be purely radial). In this paper, we review the modeling of the various processes that determine the evolution of the surface field. We restrict our attention to their role in the surface flux transport model. We also discuss the success of the model and some of the results that have been obtained using this model.
收录类别	SCI
语种	英语
WOS记录号	WOS:000347409800017
内容类型	期刊论文
源URL	[http://ir.bao.ac.cn/handle/114a11/6513]
专题	国家天文台_太阳物理研究部
作者单位	1.Chinese Acad Sci, Key Lab Solar Act, Natl Astron Observ, Beijing 100012, Peoples R China 2.NASA MSFC, Huntsville, AL 35812 USA 3.Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany 4.Kyung Hee Univ, Sch Space Res, Yongin 446701, Gyeonggi Do, South Korea 5.Univ Gottingen, Inst Astrophys, D-37077 Gottingen, Germany 6.Vanderbilt Univ, Nashville, TN 37235 USA 7.Univ Alabama, Huntsville, AL 35899 USA
推荐引用方式 GB/T 7714	Jiang, J.,Hathaway, D. H.,Cameron, R. H.,et al. Magnetic Flux Transport at the Solar Surface[J]. SPACE SCIENCE REVIEWS,2014,186(1-4):491-523.
APA	Jiang, J.,Hathaway, D. H.,Cameron, R. H.,Solanki, S. K.,Gizon, L.,&Upton, L..(2014).Magnetic Flux Transport at the Solar Surface.SPACE SCIENCE REVIEWS,186(1-4),491-523.
MLA	Jiang, J.,et al."Magnetic Flux Transport at the Solar Surface".SPACE SCIENCE REVIEWS 186.1-4(2014):491-523.