Stationary Reconnection Of 2.5D Magnetic Fields And Localized Non-Idealness In Incompressible MHD Flows

Details Stationary Reconnection Of 2.5D Magnetic Fields And Localized Non-Idealness In Incompressible MHD Flows Stationary Reconnection Of 2.5D Magnetic Fields And Localized Non-Idealness In Incompressible MHD Flows

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...3e..55n&link_type=abstract

Solar Active Regions and 3D Magnetic Structure, 26th meeting of the IAU, Joint Discussion 3, 16-17 August, 2006, Prague, Czech R

Computer Science

Scientific paper

We construct 2D potential magnetic fields for modelling pre-flare magnetic field structures. We ask the question how the application of magnetic shear components, i.e. components of the magnetic field in the invariant direction, could be a source of stationary reconnection. We also ask how this is coupled to the localized non-idealness which produces field aligned electric field components, indicating that magnetic reconnection takes place.

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