Reconnection of Magnetic Field Lines in a Non-Stationary Case

Details Reconnection of Magnetic Field Lines in a Non-Stationary Case Reconnection of Magnetic Field Lines in a Non-Stationary Case

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60.1138s&link_type=abstract

Astronomicheskii Zhurnal, Vol.60:6, P.1138, 1983

Astronomy and Astrophysics

Astronomy

14

Scientific paper

An asymptotic solution of the time-dependent magnetic-field-line reconnection problem with travelling shock waves was obtained by the method of the "frozen-in" coordinates. There were studied three phases: the phase of growth when the magnetic-field energy is being converted into kinetic and internal energy of a plasma, the phase of separation, and the phase of outflow when the two field reversal regions (confined by slow shock waves) carry away the energy converted at the phase of growth.

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