Analyses of Hinode Magnetic Field Observations Using a 3D MHD Model

Details Analyses of Hinode Magnetic Field Observations Using a 3D MHD Model Analyses of Hinode Magnetic Field Observations Using a 3D MHD Model

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..397..167g&link_type=abstract

First Results From Hinode ASP Conference Series, Vol. 397, Proceedings of the conference held 20-24 August, 2007, at Trinity Col

Astronomy and Astrophysics

Astronomy

Scientific paper

A data-driven 3D MHD model (Wu et al. 2006) is used to investigate the sources of solar eruptive events. As an example, the Hinode data on 12 December 2006 (AR 10930) have been used to deduce the physical parameters before and after the observed flare. These parameters including the main length of strong magnetic shear and strong transverse field L_{ss} and current helicity. The 3D magnetic field lines are drawn and show the field topology before the flare. These are very preliminary results, and further study is needed for correlation between an active region configuration and an eruptive phenomenon.

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