File:144F2.png: Difference between revisions

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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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Latest revision as of 14:35, 1 November 2024

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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