Validating a magnetic reconnection model for the magnetopause

Eos ◽  
2012 ◽  
Vol 93 (3) ◽  
pp. 40-40
Author(s):  
Colin Schultz
Keyword(s):  
Magnetic Reconnection ◽  
Reconnection Model

scholarly journals Theory of Flares and MHD Jets

1998 ◽  
Vol 188 ◽  
pp. 9-12 ◽  
Author(s):  
Kazunari Shibata
Keyword(s):  
Numerical Modeling ◽  
Magnetic Reconnection ◽  
Solar Flares ◽  
Model Application ◽  
Reconnection Model

Recent development on the theory and numerical modeling of solar flares and jets is reviewed with emphasis on the magnetic reconnection model. Application to protostellar flares and jets is also discussed.

scholarly journals Magnetic annihilation in colliding-wind binary systems

1995 ◽  
Vol 163 ◽  
pp. 523-524
Author(s):  
M. Jardine ◽  
H.R. Allen ◽  
A.M.T. Pollock
Keyword(s):  
Particle Acceleration ◽  
Radio Emission ◽  
Magnetic Reconnection ◽  
Stagnation Point ◽  
Binary Systems ◽  
Nonthermal Radio ◽  
Nonthermal Radio Emission ◽  
Reconnection Model

We investigate the possibility that a stagnation-point magnetic reconnection model may account for the particle acceleration necessary for the generation of nonthermal radio emission in the Wolf-Rayet binary systems exemplified by WR140.

scholarly journals Large solar-type magnetic reconnection model for magnetar giant flare

2008 ◽  
Vol 4 (S259) ◽  
pp. 123-124
Author(s):  
Youhei Masada
Keyword(s):  
Solar Flare ◽  
Magnetic Reconnection ◽  
Radiative Heat ◽  
Energy Transport ◽  
Magnetic Energy ◽  
Baryonic Matter ◽  
Solar Type ◽  
Mass Ejection ◽  
Giant Flare ◽  
Reconnection Model

AbstractWe construct a magnetic reconnection model for magnetar giant flare in the framework of solar flare/coronal mass ejection theory. As is the case with the solar flare, the explosive magnetic reconnection plays a crucial role in the energetics of the magnetar flare. A key physics controlling the energy transport in the system, on the other hand, is the radiative process unlike that in the solar flare. After the release of the magnetic energy via the magnetic reconnection, the radiative heat flux drives the baryonic evaporation. Our model can predict that the baryonic matter evaporated in the preflare stage would be the origin of the radio emitting ejecta observed in association with the giant flare on 2004 December 27 from SGR1806-20.

Magnetic reconnection model for X-ray flare loop interaction

1995 ◽  
Vol 226 (1) ◽  
pp. 31-46 ◽  
Author(s):  
Zhen-Da Zhang ◽  
Xiao-Qing Li ◽  
R. N. Smartt
Keyword(s):  
Magnetic Reconnection ◽  
Flare Loop ◽  
X Ray ◽  
Reconnection Model

scholarly journals Solar-Type Magnetic Reconnection Model for Magnetar Giant Flares

2010 ◽  
Vol 62 (4) ◽  
pp. 1093-1102 ◽  
Author(s):  
Youhei Masada ◽  
Shigehiro Nagataki ◽  
Kazunari Shibata ◽  
Toshio Terasawa
Keyword(s):  
Magnetic Reconnection ◽  
Solar Type ◽  
Reconnection Model

Magnetic reconnection model of X-ray plasmas in the Galactic center

2000 ◽  
Vol 25 (3-4) ◽  
pp. 505-508
Author(s):  
T. Yokoyama ◽  
S. Tanuma ◽  
T. Kudoh ◽  
K. Shibata
Keyword(s):  
Magnetic Reconnection ◽  
Galactic Center ◽  
X Ray ◽  
Reconnection Model
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