Figure 4 from Inferring Solar Differential Rotation through Normal-mode Coupling Using Bayesian Statistics

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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 4.

Cross-spectrum for ℓ = 222 and Δℓ = 0, 2, 4. The upper panels correspond to m⁺, and the lower panels correspond to m⁻. The black curve shows observed data. The blue curve is the model before considering eigenfunction coupling, and the red curve corresponds to the model constructed using parameters estimated from MCMC.

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