Forced magnetic reconnection in a sheared force-free magnetic field brings about relaxation of the system to a state of lower magnetic energy. The resulting energy release becomes strongly amplified when the field is close to the tearing instability threshold, which makes the linear theory [Vekstein and Jain, Phys. Plasmas 5, 1506 (1998)] not applicable in this case. In the present Brief Communication the reconnective energy release in the marginally stable magnetic field is derived by exploring the quasilinear theory of tearing modes.
REFERENCES
1.
H.
Furth
, J.
Killeen
, and M. N.
Rosenbluth
, Phys. Fluids
6
, 459
(1963
).2.
3.
4.
5.
6.
7.
E. R. Priest, Solar Magnetohydrodynamics (Riedel, Dordrecht, 1984), Chap. 6.
8.
9.
10.
11.
12.
13.
R. B.
White
, D. A.
Monticello
, M. N.
Rosenbluth
, and B. V.
Waddell
, Phys. Fluids
20
, 800
(1977
).
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© 2004 American Institute of Physics.
2004
American Institute of Physics
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