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tachocline

   Also found in: Wikipedia 0.03 sec.
tachocline [′takĀ·ə‚klīn]
(astronomy)
A zone of radial shear in the interior of the sun that is located at the base of the convection zone at a distance from the sun's center equal to about 0.7 of the sun's radius, and represents an abrupt transition from the rotation rates in the convection zone to those in the underlying layers.


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