NLFF Model of a Coronal Sigmoid

Details NLFF Model of a Coronal Sigmoid NLFF Model of a Coronal Sigmoid

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsp31a..05s&link_type=abstract

American Geophysical Union, Spring Meeting 2008, abstract #SP31A-05

Physics

7509 Corona, 7524 Magnetic Fields

Scientific paper

Between Feb 10 and 12, 2007, the X-ray telescope on Hinode produced some very high-cadence and high- resolution observations of a prominent coronal sigmoid. Here we show our results from computing a NLFF model of the sigmoid and compare it qualitatively to the XRT and TRACE observations. In addition we include some preliminary qualitative and quantitative results from 2.5D flux emergence simulation. We also discuss the future goals of this project.

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