Formation of Eruptive Magnetic Configurations in the Corona via Reconnection

Details Formation of Eruptive Magnetic Configurations in the Corona via Reconnection Formation of Eruptive Magnetic Configurations in the Corona via Reconnection

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh22a06t&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH22A-06

Mathematics

Logic

7509 Corona, 7513 Coronal Mass Ejections, 7524 Magnetic Fields, 7835 Magnetic Reconnection, 7843 Numerical Simulation Studies

Scientific paper

Using numerical simulations we examine how reconnection causes the formation of eruptive magnetic configurations in the corona. We describe the topology of the global velocity field which results from the co-rotational flows imposed at the photospheric boundary. Such velocity profile is shown to force the magnetic field lines to twist, reconnect and expand outwards forming configurations that posess features present in CME observations. The topological changes caused by reconnection are discussed in detail.

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