Figure 5 from Inferring Solar Differential Rotation through Normal-mode Coupling Using Bayesian Statistics

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 5.

Cross-spectrum for ℓ = 70 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.

Other Images in This Article

Copyright and Terms & Conditions