Figure 8 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 8.

The red line corresponds to N₀. The gray region corresponds to 5% error from N₀. The gray points correspond to N_ℓ, and the solid black lines are from each MCMC simulation. The rightmost panel shows the histogram of all of the gray points, taken from all radial orders.

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