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DTIC ADA292318: A Turbulent Model of the Solar Granulation,
by Defense Technical Information Center
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The paper dealt with a new model for the development of
convective velocity fields at various spatial scales in
order to understand the differential rotation of the sun
which affects the solar dynamo responsible for the
magnetic activity as seen in its myriad forms. The new
model is based on inverse cascading of energy to take
into account the granulation phenomenon in its entirety.
(AN)
Date Published: 2018-03-22 17:39:46
Identifier: DTIC_ADA292318
Item Size: 2841370
Language: english
Media Type: texts
# Topics
DTIC Archive; Krishan, Vinod; ASIAN O...
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