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convection zone

   Also found in: Wikipedia 0.01 sec.
convection zone
A region of turbulent plasma between a star's core and its visible photosphere at the surface, through which energy is transferred by convection. In the convection zone, hot plasma rises, cools as it nears the surface, and falls to be heated and rise again.


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This energy is then radiated to the convection zone, where mixing transfers the energy to the photosphere.
On tau Bootis, notes Cameron, the convection zone is thinner and the relative difference in rotation between the equator and the pole is greater.
This allows product to be conveyed horizontally through numerous precision-controlled convection zones and results in an oven that occupies approximately one-tenth of the footprint of legacy tunnel oven technology.
 
 
 
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