A time-dependent model of magnetic field annihilation.

Details A time-dependent model of magnetic field annihilation. A time-dependent model of magnetic field annihilation.

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jplph..49...17h&link_type=abstract

Journal of Plasma Physics, Vol. 49, Part 1, p. 17 - 27

Physics

Plasma Physics

3

Scientific paper

Quasi-periodic variations in the electric field intensity near the dayside magnetopause are studied within a planar, dissipative MHD model of a stagnation-line flow embedded in a rectilinear magnetic field. The model is based on an exact time-dependent solution of the resistive MHD equations applied to a Parker-type diffusion region of field-line merging. The results lead to the prediction of certain relations between physical parameters of the solar-wind plasma, and these are compared with actual measurements.

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