Abstract
Spectra of solar intensity oscillations in the degree range ℓ = 20–98 were obtained with a 92% duty cycle over a 50 hour period from the geographic South Pole. The spectra have been analyzed for frequency shifts caused by solar internal rotation as functions of latitude and depth. The results have been published elsewhere and some of the intermediate steps in producing the results are illustrated here.KeywordsFrequency ShiftSolar RotationSpherical Harmonic CoefficientNASA Goddard SpaceNational Solar ObservatoryThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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