File:144F2.png

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HMI time-series observations of the flare, using standard data interpolated for helioseismology. The middle of the three vertical lines shows the "precursor" time frame, with a clear negative excursion in either footpoint region.

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Date/TimeThumbnailDimensionsUserComment
current17:33, 19 January 2011Thumbnail for version as of 17:33, 19 January 20111,154×1,184 (21 KB)Hhudson (Talk | contribs) (HMI time-series observations of the flare, using standard data interpolated for helioseismology. The middle of the three vertical lines shows the "precursor" time frame, with a clear negative excursion in either footpoint region.)

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