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It has been previously observed that narrow lanes of transverse andlongitudinal magnetic field with opposite polarity are the site of large solarflares. We performed a comprehensive examination of the stokes asymmetries ofactive region NOAA 10930. The active region was observed just before, duringand after an X-class flare, which occurred during December 13, 2006 from 02:20to 06:18 UT. We observe a static fibril interacting with a rotating penumbra ofopposite polarity in the hours prior to the flare. Above the fibril wereseveral small sites of hot gas in the chromosphere. During and after the flare,the fibril and its corresponding flow and profiles were much less pronounced.We present a full analysis of magnetic and plasma properties of this activeregion.

Stokes Profiles at the Narrow Magnetic Lanes of Sun Spots