The solar magnetic field

作者:

DOI: 10.1088/0034-4885/69/3/R02

关键词:

摘要: The magnetic field of the Sun is underlying cause many diverse phenomena combined under heading solar activity. Here we describe as it threads its way from bottom convection zone, where built up by dynamo, to surface, manifests itself in form sunspots and faculae, beyond into outer atmosphere and, finally, heliosphere. On transports energy surface subsurface layers corona, heats gas accelerates wind.

参考文章(672)
Jon A Linker, Z Mikić, Doug A Biesecker, Robert J Forsyth, Sarah E Gibson, Alan J Lazarus, A Lecinski, Pete Riley, Adam Szabo, Barbara J Thompson, None, Magnetohydrodynamic modeling of the solar corona during Whole Sun Month Journal of Geophysical Research: Space Physics. ,vol. 104, pp. 9809- 9830 ,(1999) , 10.1029/1998JA900159
D. S. Brown, E. R. Priest, The topological behaviour of 3D null points in the Sun's corona Astronomy and Astrophysics. ,vol. 367, pp. 339- 346 ,(2001) , 10.1051/0004-6361:20010016
E. N. Parker, A solar dynamo surface wave at the interface between convection and nonuniform rotation The Astrophysical Journal. ,vol. 408, pp. 707- 719 ,(1993) , 10.1086/172631
Ward B Manchester IV, Tamas I Gombosi, Ilia Roussev, Darren L De Zeeuw, IV Sokolov, Kenneth G Powell, Gábor Tóth, Merav Opher, Three‐dimensional MHD simulation of a flux rope driven CME Journal of Geophysical Research. ,vol. 109, ,(2004) , 10.1029/2002JA009672
Y. Fan, G. H. Fisher, A. N. McClymont, Dynamics of emerging active region flux loops The Astrophysical Journal. ,vol. 436, pp. 907- ,(1994) , 10.1086/174967
Robert F. Howard, Axial tilt angles of sunspot groups Solar Physics. ,vol. 136, pp. 251- 262 ,(1991) , 10.1007/BF00146534
N. Seehafer, Electric current helicity in the solar atmosphere Solar Physics. ,vol. 125, pp. 219- 232 ,(1990) , 10.1007/BF00158402
E. N. Frazier, J. O. Stenflo, On the small-scale structure of solar magnetic fields Solar Physics. ,vol. 27, pp. 330- 346 ,(1972) , 10.1007/BF00153105