Space Weather Forecasting: Active Times Ahead

  • Released Tuesday, August 16, 2005
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SOHO/MDI magnetograms combined with the Potential-Field Source-Surface (PFSS) model can be used to generate a model of magnetic field lines in the lower part of the solar corona. When these models are compared to the loops visible in TRACE imagery, a bad match (as in this case) indicates that the region will generate flare events over the next few days.

This movie zooms in to the solar surface then fades to a time varying magnetogram. The PFSS model is overlaid on the source magnetic field, then compared to the TRACE loops. Following the region for several days, we see a major flare event.

A magnetogram closeup view of an active region. White indicates north magnetic polarity, black is south.

A magnetogram closeup view of an active region. White indicates north magnetic polarity, black is south.

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NASA/Goddard Space Flight Center Scientific Visualization Studio

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This page was originally published on Tuesday, August 16, 2005.
This page was last updated on Wednesday, May 3, 2023 at 1:56 PM EDT.


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