Pankin - ICTP
Pankin - ICTP
Pankin - ICTP
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Summary<br />
Model for accretion disk in solar corona is developed<br />
and implemented in resistive MHD code<br />
Evolution of single and multiple magnetic loops in the<br />
corona driven by Keplerian shear flow in the disk is<br />
reported<br />
There are indications that the evolution of magnetic<br />
loop is associated with reconnection of magnetic<br />
field lines in corona and<br />
produces angular momentum transport towards<br />
the central object for inner spot<br />
ICTMB, Trieste, Italy, August 2007
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