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Effect of the Coriolis force and slowly varying flow on the Kelvin-Helmholtz instability

✍ Scribed by D. N. Vyas; R. Singh; Krishna M. Srivastava

Publisher
Springer Netherlands
Year
1983
Tongue
English
Weight
466 KB
Volume
90
Category
Article
ISSN
0004-640X

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If the solar dynamo operates at the bottom of the convection zone, then the magnetic flux created there has to rise to the surface. When the convection zone is regarded as passive, the rising flux is deflected by the Coriolis force to emerge at rather high latitudes, poleward of typical sunspot zone