The Rotation Of The Deep Solar Layers

Details The Rotation Of The Deep Solar Layers The Rotation Of The Deep Solar Layers

2003-09-30

arxiv.org/abs/astro-ph/0309806v1

Astrophys.J.597:L77-L80,2003

Astronomy and Astrophysics

Astrophysics

accepted in ApJ Letters 5 pages, 2 figures

Scientific paper

10.1086/379698

From the analysis of low-order GOLF+MDI sectoral modes and LOWL data (l > 3), we derive the solar radial rotation profile assuming no latitudinal dependance in the solar core. These low-order acoustic modes contain the most statistically significant information about rotation of the deepest solar layers and should be least influenced by internal variability associated with the solar dynamo. After correction of the sectoral splittings for their contamination by the rotation of the higher latitudes, we obtain a flat rotation profile down to 0.2 solar radius.

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