Non-Force free mahnetic flux ropres with axial flow

Details Non-Force free mahnetic flux ropres with axial flow Non-Force free mahnetic flux ropres with axial flow

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsh51a1463b&link_type=abstract

American Geophysical Union, Fall Meeting 2006, abstract #SH51A-1463

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2101 Coronal Mass Ejections (7513), 7513 Coronal Mass Ejections (2101), 7524 Magnetic Fields

Scientific paper

Magnetic flux ropes are important to study various astrophysical systems, especially in coronal structures with sigmoidal forms and have implications for space weather. In this work, a mean-field formalism is developed to obtain non force-free steady-states using Hall-MHD equations in the presence of flows and resistive effects. It is observed that the governing equations at steady-state support a flux rope solution with non zero pressure and finite flow. The non force-free flux ropes are particularly interesting as they are observed in the Venus ionosphere and other regions of interplanetary space. The dynamo field necessary to sustain such a solution is obtained self-consistently

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