Supergranulation rotation

Details Supergranulation rotation Supergranulation rotation

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000soph..193..333b&link_type=abstract

Solar Physics, v. 193, Issue 1/2, p. 333-343 (2000).

Physics

31

Scientific paper

Simple convection models estimate the depth of supergranulation at approximately 7500 km which suggests that supergranules would rotate at the rate of the plasma in the outer 1% of the solar radius. The supergranulation rotation obtained from MDI dopplergrams shows that supergranules rotate faster than the outer 5% of the convection zone and show zonal flows matching results from inversions of f-mode splittings. Additionally, the rotation rate depends on the size scale of the features.

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