Flaring Solar Hale Sector Boundaries

Details Flaring Solar Hale Sector Boundaries Flaring Solar Hale Sector Boundaries

2010-10-13

arxiv.org/abs/1010.2710v2

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

11 pages; 4 figures

Scientific paper

Magnetic fields and the occurrence of flares and microflares are strongly
concentrated near that portion (the Hale boundary) in each solar hemisphere
where the change in magnetic sector polarity is the same as that between
leading and following sunspot polarities in active regions.

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