Differential rotation in fully convective stars
Under the assumption of thermal wind balance and effective entropy mixing in constant rotation surfaces, the isorotational contours of the solar convective zone may be reproduced with great fidelity. Even at this early stage of development, this helioseismology fit may be used to put a lower bound o...
| Main Authors: | , |
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| Format: | Journal article |
| Language: | English |
| Published: |
2010
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