Evolution and advection of solar mesogranulation

Details Evolution and advection of solar mesogranulation Evolution and advection of solar mesogranulation

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992natur.356..322m&link_type=abstract

Nature (ISSN 0028-0836), vol. 356, March 26, 1992, p. 322-325. Research supported by USAF, NASA, NSF, et al.

Physics

51

Advection, Solar Granulation, Solar Physics, Convection Cells, Solar Magnetic Field

Scientific paper

A three-hour sequence of observations at the Pic du Midi observatory has been obtained which shows the evolution of solar mesogranules from appearance to disappearance with unprecedented clarity. It is seen that the supergranules, which are known to advect the granules with their convective motion, also advect the mesogranules to their boundaries. This process controls the evolution and disappearance of mesogranules.

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