Concentration of magnetic fields in the deep convection zone

Autor: G. W. Simon, N. O. Weiss
Rok vydání: 1968
Zdroj: Symposium - International Astronomical Union. 35:108-111
ISSN: 0074-1809
Popis: The strong magnetic fields observed between supergranules indicate that there must be subphotospheric convection in cells with a preferred diameter of about 30000 km. Orthodox mixing length theory assumes that the dimensions of cells are limited by the density scale-height. This is adequate for explaining granules but cannot account for supergranulation. A model is therefore proposed in which cellular motions extend over several scale-heights. In addition to granules and supergranules this model predicts a third characteristic scale of motion, with giant cells around 300000 km in diameter. These cells may produce a pattern of magnetic fields like that suggested by Bumba and Howard for complexes of activity.
Databáze: OpenAIRE