Thermally Driven Rossby-Mode Dynamo for Solar Magnetic-Field Reversals

Details Thermally Driven Rossby-Mode Dynamo for Solar Magnetic-Field Reversals Thermally Driven Rossby-Mode Dynamo for Solar Magnetic-Field Reversals

May 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968sci...160..760g&link_type=abstract

Science, Volume 160, Issue 3829, pp. 760-763

Physics

9

Scientific paper

There is increasing interest in the possible existence of large eddies or "Rossby waves" in Sun's convection zone and photosphere. It is shown that many flows of this type, driven by an equator-pole temperature difference, act as hydromagnetic dynamos to produce magnetic fields that periodically reverse. The periods and field amplitudes agree with solar phenomena within an order of magnitude.

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