Alfven resonances, forced magnetic reconnection and model of solar flares

被引：0

作者：

Uberoi, C ^{[1
]}

机构：

[1] Indian Inst Sci, Dept Math, Bangalore 560012, Karnataka, India

来源：

PLASMA PHYSICS AND CONTROLLED FUSION | 2003年 / 45卷 / 06期

关键词：

D O I：

10.1088/0741-3335/45/6/308

中图分类号：

O35 [流体力学]; O53 [等离子体物理学];

学科分类号：

070204 ; 080103 ; 080704 ;

摘要：

This paper briefly reviews the surface-wave-induced-magnetic reconnection (SWIMR) model based on the Alfven resonance theory near the neutral point. Extending this model to magnetosonic waves it is seen that it not only has features of formation of current sheets and plasmoids as in the incompressible case but in addition energy considerations show the triggering of solar flares by the catastrophic loss of equilibrium. The similarity of SWIMR model to the emerging flux and plasmoid induced magnetic reconnection model for solar flares is discussed. This article was scheduled to appear in issue 5 of Plasma Phys. Control. Fusion. To access this Special issue please follow this link: http://www.iop.org/EJ/toc/0741-3335/45/5.

引用

页码：949 / 955

页数：7

共 50 条

[31] Oblique shocks in the magnetic reconnection jet in solar flares
Tanuma, Syuniti
Shibata, Kazunari
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2007, 59 (02) : L1 - L5
[32] MHD simulations of magnetic reconnection in the solar corona and flares
Yokoyama, T
OBSERVATIONAL PLASMA ASTROPHYSICS: FIVE YEARS OF YOHKOH AND BEYOND, 1998, 229 : 161 - 170
[33] MHD simulations of magnetic reconnection in solar flares and jets
Yokoyama, T
MAGNETIC RECONNECTION PROCESSES IN THE SOLAR ATMOSPHERE, 2000, 26 (03): : 511 - 520
[34] Magnetic reconnection plasmoid model for Sagittarius A* flares
Aimar, N.
Dmytriiev, A.
Vincent, F. H.
El Mellah, I.
Paumard, T.
Perrin, G.
Zech, A.
ASTRONOMY & ASTROPHYSICS, 2023, 672
[35] A window into magnetic reconnection: IRIS observations of the consequences of reconnection during solar flares
Reeves, Katharine K.
FRONTIERS IN ASTRONOMY AND SPACE SCIENCES, 2022, 9
[36] Magnetic Reconnection in Solar Flares and the Near-Sun Solar Wind
J. F. Drake
S. K. Antiochos
S. D. Bale
Bin Chen
C. M. S. Cohen
J. T. Dahlin
Lindsay Glesener
F. Guo
M. Hoshino
Shinsuke Imada
M. Oka
T. D. Phan
Katherine K. Reeves
M. Swisdak
Space Science Reviews, 2025, 221 (2)
[37] Solar coronal heating by forced magnetic reconnection: Multiple reconnection events
Jain, R
Browning, P
Kusano, K
PHYSICS OF PLASMAS, 2005, 12 (01) : 1 - 12
[38] Reconnection, substorms and solar flares
Axford, WI
PHYSICS AND CHEMISTRY OF THE EARTH PART C-SOLAR-TERRESTIAL AND PLANETARY SCIENCE, 1999, 24 (1-3): : 147 - 151
[39] PARTICLE-ACCELERATION AND MAGNETIC RECONNECTION IN SOLAR-FLARES
TSUNETA, S
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1995, 47 (05) : 691 - 697
[40] Reconnection, substorms and solar flares
Phys Chem Earth, 1-3 (147-151):

← 1 2 3 4 5 →