Laboratory observations of spontaneous magnetic reconnection

被引:90
作者
Egedal, J. [1 ]
Fox, W. [1 ]
Katz, N. [1 ]
Porkolab, M. [1 ]
Reim, K. [1 ]
Zhang, E. [1 ]
机构
[1] MIT, Plasma Sci & Fus Ctr, Cambridge, MA 02139 USA
关键词
D O I
10.1103/PhysRevLett.98.015003
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Detailed measurements of spontaneous magnetic reconnection are presented. The experimental data, which were obtained in the new closed Versatile Toroidal Facility magnetic configuration, document the profile evolution of the plasma density, magnetic flux function, reconnection rate, and the current density during a spontaneous reconnection event in the presence of a strong guide magnetic field. The reconnection process is at first slow, which allows magnetic stress to build in the system while the current channel becomes increasingly narrow and intense. The onset of a fast reconnection event occurs as the width of the current channel approaches the ion-sound-Larmor radius rho(s). During the reconnection event magnetically stored energy is channeled into energetic ion outflows and a rapid increase in the electron temperature.
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页数:4
相关论文
共 16 条
[1]   PLASMA INSTABILITY AT AN X-TYPE MAGNETIC NEUTRAL POINT [J].
BAUM, PJ ;
BRATENAHL, A ;
KAO, M ;
WHITE, RS .
PHYSICS OF FLUIDS, 1973, 16 (09) :1501-1504
[2]   Current singularities: Drivers of impulsive reconnection [J].
Bhattacharjee, A ;
Germaschewski, K ;
Ng, CS .
PHYSICS OF PLASMAS, 2005, 12 (04) :1-11
[3]  
Birn J, 2001, J GEOPHYS RES-SPACE, V106, P3715, DOI 10.1029/1999JA900449
[4]   Catastrophe model for fast magnetic reconnection onset [J].
Cassak, PA ;
Shay, MA ;
Drake, JF .
PHYSICAL REVIEW LETTERS, 2005, 95 (23)
[5]  
CASSAK PA, COMMUNICATION
[6]  
DUNGEY JW, 1953, PHILOS MAG, V44, P725
[7]   Dynamical plasma response during driven magnetic reconnection [J].
Egedal, J ;
Fasoli, A ;
Nazemi, J .
PHYSICAL REVIEW LETTERS, 2003, 90 (13) :4
[8]   Magnetic reconnection and current sheet formation in 3D magnetic configurations [J].
Frank, AG .
PLASMA PHYSICS AND CONTROLLED FUSION, 1999, 41 :A687-A697
[9]  
Hastie RJ, 1998, ASTROPHYS SPACE SCI, V256, P177
[10]   A LOOP TOP HARD X-RAY SOURCE IN A COMPACT SOLAR-FLARE AS EVIDENCE FOR MAGNETIC RECONNECTION [J].
MASUDA, S ;
KOSUGI, T ;
HARA, H ;
OGAWARA, Y .
NATURE, 1994, 371 (6497) :495-497