Verification of the helioseismic Fourier-Legendre analysis for meridional flow measurements

Abstract

Measuring the Sun's internal meridional flow is one of the key issues of helioseismology. Using the Fourier-Legendre analysis is a technique for addressing this problem. We validate this technique with the help of artificial helioseismic data. The analysed data set was obtained by numerically simulating the effect of the meridional flow on the seismic wave field in the full volume of the Sun. In this way, a 51.2-hour long time series was generated. The resulting surface velocity field is then analyzed in various settings: Two $360^{\circ }\times 90^{\circ }$ halfspheres, two $120^{\circ }\times 60^{\circ }$ patches on the front and farside of the Sun (North and South, respectively) and two $120^{\circ }\times 60^{\circ }$ patches on the northern and southern frontside only. We compare two possible measurement setups: observations from Earth and from an additional spacecraft on the solar farside, and observations from Earth only, in which case the full information of the global solar oscillation wave field was available. We find that, with decreasing observing area, the accessible depth range decreases: the $360^{\circ }\times 90^{\circ }$ view allows us to probe the meridional flow almost to the bottom of the convection zone, while the $120^{\circ }\times 60^{\circ }$ view means only the outer layers can be probed. These results confirm the validity of the Fourier-Legendre analysis technique for helioseismology of the meridional flow. Furthermore these flows are of special interest for missions like Solar Orbiter that promises to complement standard helioseismic measurements from the solar nearside with farside observations.

5 pages, 2 figures

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• The Solar Orbiter Science Activity Plan: translating solar and heliospheric physics questions into action
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• Inversions for Deep Solar Meridional Flow Using Spherical Born Kernels
• Probing the Solar Meridional Circulation using Fourier Legendre Decomposition
• Validation of Spherical Born Approximation Sensitivity Functions for Measuring Deep Solar Meridional Flow
• Computing Helioseismic Sensitivity Kernels for the Sun's Large-Scale Internal Flows using Global-Scale Wave-Propagation Simulations