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Inferring Solar Differential Rotation through Normal-mode Coupling Using Bayesian Statistics

  • Authors: Samarth G. Kashyap, Srijan Bharati Das, Shravan M. Hanasoge, Martin F. Woodard, and Jeroen Tromp

2021 The Astrophysical Journal Supplement Series 253 47.

  • Provider: AAS Journals

Caption: Figure 2.

Cross-spectral signal for = 200, Δ = 2, and n = 0. (a), (b) Observed cross-spectrum corresponding to m+ and m. (c), (d) Derotated cross-spectrum corresponding to m+ and m. (e), (f) ﹩{D}_{n}^{{\ell },{\rm{\Delta }}{\ell },\pm }﹩. The baseline is indicated by the dashed blue line. The blue dots represent observations from the five 72-day time series, and the red curve corresponds to the expectation value of the cross-spectrum.

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