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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 8.

Inversion results for meridional flows. Shown are (from left to right) target flows (flow profile from the simulation convolved with target kernels), inverted flows from forward-modeled travel times (δτFwd) and measured travel times (δτMeas), as well as inversion errors for the inversion of measured travel times. Gray dashed lines indicate locations at r/R = 0.7, 0.8, 0.9, and 1.0 and multiples of 15° distance from the equator.

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