Probing Coronal Magnetic Connectivity on Local and Global Scales

Details Probing Coronal Magnetic Connectivity on Local and Global Scales Probing Coronal Magnetic Connectivity on Local and Global Scales

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011spd....42.1831l&link_type=abstract

American Astronomical Society, SPD meeting #42, #18.31; Bulletin of the American Astronomical Society, Vol. 43, 2011

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Scientific paper

Magnetic reconnection and other magnetohydrodynamic interactions between an erupting flux rope and the overlying global magnetic field of the solar corona play an important role in predicting and interpreting possible interactions with magnetic clouds at 1AU. I employ coronal dimming signatures as a diagnostic analogue of the open or closed nature and subsequent evolution of the local magnetic field. In addition, potential field source surface models will yield insight into the global overlying magnetic topology. Existing statistical data on coronal dimming, several detailed case studies, and mathematical models of the flux rope / global field interaction will yield crucial insight into the eruption process, a critical component to space weather predictions.

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