On the relationship between magnetic fields and supergranule velocity fields

Details On the relationship between magnetic fields and supergranule velocity fields On the relationship between magnetic fields and supergranule velocity fields

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..117..343w&link_type=abstract

(Solar Cycle Workshop, Meeting, 2nd, Lake Tahoe, CA, May 1987) Solar Physics (ISSN 0038-0938), vol. 117, no. 2, 1988, p. 343-358

Physics

37

Solar Granulation, Solar Magnetic Field, Sunspots, Velocity Distribution, Convective Flow, Grain Boundaries, Late Stars

Scientific paper

The author studied the size, correlation lifetime and horizontal velocity amplitude of supergranules in regions with different magnetic activity. He found that the supergranule velocity cells have similar scale, correlation lifetime and horizontal velocity amplitude in the unipolar enhanced magnetic network regions and in the mixed-polarity quiet Sun. However, the correlation lifetime of magnetic structure is much longer in the enhanced network. The author investigated the velocity pattern of moving magnetic features (MMF) surrounding a decaying sunspot.

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