Differential rotation and convection in the Sun
We show that the differential rotation profile of the solar convection zone, apart from inner and outer boundary layers, can be reproduced with great accuracy if the isorotation contours correspond to characteristics of the thermal wind equation. This requires that there be a formal quantitative rel...
| Κύριοι συγγραφείς: | , , , |
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| Μορφή: | Journal article |
| Έκδοση: |
2009
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