Current sheet creation by a super-Alfvénic jet in a bipolar field

Details Current sheet creation by a super-Alfvénic jet in a bipolar field Current sheet creation by a super-Alfvénic jet in a bipolar field

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..161..165p&link_type=abstract

Solar Physics, Volume 161, Issue 1, pp.165-181

Physics

14

Scientific paper

Energy accumulation in a current sheet (CS) can occur during the injection of a fast plasma jet in a perpendicular magnetic field. A similar situation can occur in the solar corona when a flux of plasma appears under a magnetic arch. The flare can be produced at the CS disruption. The CS creation during plasma jet interaction with the magnetic field is demonstrated by numerical MHD simulation. The choice of dimensionless parameters Re, Rem,β, II, which are suitable for simulation of coronal phenomena, is discussed. When jet injection ceases, the CS evolution produces an unstable state and fast magnetic energy dissipation is observed.

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