Antia, H. M. ; Basu, S. ; Chitre, S. M. (2009) What is new with zonal flows? Astronomical Society of the Pacific Conference Series, 416 . pp. 265-268. ISSN 1050-3390
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Abstract
We have used available helioseismic data for the solar cycle 23 to undertake a detailed study of temporal variations in solar rotation. We concentrate mainly on variation of the radial and latitudinal gradients of rotation. We find that the temporal variations of the rotation-rate gradients is about 20% or more than their average value, i.e., much larger than the relative variation in the rotation rate itself. These variations may play an important role in solar dynamo models.
Item Type: | Article |
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Source: | Copyright of this article belongs to Astronomical Society of the Pacific. |
ID Code: | 75698 |
Deposited On: | 24 Dec 2011 15:12 |
Last Modified: | 12 Jul 2012 08:41 |
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