File:137fig16.png

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Distribution of RHESSI flares on each day a sector boundary was mapped back to central meridian for part of solar cycle 23, March 2002 to March 2008. The red boxes show where flares are expected based on association with strong magnetic fields: at the Hale boundary. The circles show that hardly any flares occur near a non-Hale boundary.

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current18:57, 3 October 2010Thumbnail for version as of 18:57, 3 October 2010758×352 (141 KB)Hhudson (Talk | contribs) (Distribution of RHESSI flares on each day a sector boundary was mapped back to central meridian for part of solar cycle 23, March 2002 to March 2008. The red boxes show where flares are expected based on association with strong magnetic fields: at the Hal)

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