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Evidence for non-potential magnetic fields in the quiet Sun
Authors:Woodard  MF  Chae  Jongchul
Institution:(1) Big Bear Solar Observatory, New Jersey Institute of Technology, 40386 North Shore Lane, USA
Abstract:A comparison of BBSO Hagr centerline filtergrams and videomagnetograms was made to investigate the existence of non- potential magnetic fields in the quiet Sun near magnetic network. We use the fibril structure in the Hagr images as a proxy for the horizontal chromospheric magnetic field which we compare with the horizontal field obtained by potential extrapolation of the observed, line-of-sight photospheric field. The quiet-Sun field was found to be consistently and significantly non-potential in each of the three fields of view studied. A transient extreme ultraviolet (EUV) brightening, known as a blinker, occurred during the observations of a region where the field is highly non-potential, suggesting a connection between magnetic reconnection and non-potentiality.
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