Annotation
An expression that explicitly describes variations in the internal energy of the plasma that flows through a discontinuity is derived based on the complete system of boundary conditions for the MHD equations on the discontinuity surface. The dependence of the plasma heating on the magnetic field density and configuration in the vicinity of the discontinuity surface (i.e., on the MHD flow type) is studied. The conditions of plasma heating at discontinuities in a self-consistent analytical model of magnetic reconnection are discussed.
Received: 2012 December 2
Approved: 2013 March 27
PACS:
95.30.Qd Magnetohydrodynamics and plasmas
96.60.Iv Magnetic reconnection
96.60.Q- Solar activity
96.60.qe Flares
96.60.Iv Magnetic reconnection
96.60.Q- Solar activity
96.60.qe Flares
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
L.S. Ledentsov, B.V. Somov
Sternberg Astronomical Institute, Moscow State University, Universitetskii pr. 13, Moscow, 119991, Russia
Sternberg Astronomical Institute, Moscow State University, Universitetskii pr. 13, Moscow, 119991, Russia