Two Fundamental MHD Problems in Solar Physics

Details Two Fundamental MHD Problems in Solar Physics Two Fundamental MHD Problems in Solar Physics

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..369..587s&link_type=abstract

New Solar Physics with Solar-B Mission ASP Conference Series, Vol. 369, proceedings of the conference held 8-11 November, 2005 a

Physics

Scientific paper

Two fundamental MHD problems in solar physics are discussed. The first one is the so-called Parker problem, namely the behavior of magnetic fields when their fieldline footpoints are moved around by flows. The expected incapability of settling the field into static equilibrium is a theoretical basis for the microflare model of coronal heating. The second one is the so-called Aly-Sturrock conjecture, stating that the magnetic field stressed by footpoint motions attains energy but may never exceed the energy of the open field. This is thought to be an anti-CME theorem.

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