Cells of solar photospheric background magnetic fields and coronal mass ejections

Details Cells of solar photospheric background magnetic fields and coronal mass ejections Cells of solar photospheric background magnetic fields and coronal mass ejections

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sosyr..40..437s&link_type=abstract

Solar System Research, Volume 40, Issue 5, pp.437-440

Physics

91.25.Fd

Scientific paper

The cells of photospheric background magnetic fields during Carrington rotation 2009 in October November 2003 are considered. The small number of large sunspots and the high activity on the Sun in this period allow the correspondence between the activity of background field cells (flares) and the appearance of coronal mass ejections (CMEs) observed with the LASCO coronagraphs to be established without statistical analyses. The sunspots of opposite polarities in one background field cell are shown to serve as the legs of the same CME. The separation between them is close to 30°.

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