Figure 3 from Validation of Spherical Born Approximation Sensitivity Functions for Measuring Deep Solar Meridional Flow

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Validation of Spherical Born Approximation Sensitivity Functions for Measuring Deep Solar Meridional Flow

Authors: Vincent G. A. Böning, Markus Roth, Jason Jackiewicz, and Shukur Kholikov

2017 The Astrophysical Journal 838 53.

Provider: AAS Journals

Caption: Figure 3.

Comparison of the same power spectra as in Figure 2, integrated over frequency. The observational power spectra from simulated data (blue solid line) and model power spectra (red dashed, matched) are nearly identical. Unmatched power spectra are also shown (green dots).

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