Six mixed f/g modes in a solar model yield OLA kernels that can measure core rotation at two radii with precision sufficient to discriminate Fuller versus Eggenberger transport scenarios.
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On the feasibility of inverting the rotation of the solar core with mixed f/g modes
Six mixed f/g modes in a solar model yield OLA kernels that can measure core rotation at two radii with precision sufficient to discriminate Fuller versus Eggenberger transport scenarios.