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arXiv · 2201.00178

Imaging the Sun's near-surface flows using mode-coupling analysis

Prasad Mani·Chris Hanson·Shravan Hanasoge
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Abstract

The technique of normal-mode coupling is a powerful tool with which to seismically image non-axisymmetric phenomena in the Sun. Here we apply mode coupling in the Cartesian approximation to probe steady, near-surface flows in the Sun. Using Doppler cubes obtained from the Helioseismic and Magnetic Imager onboard the Solar Dynamics Observatory, we perform inversions on mode-coupling measurements to show that the resulting divergence and radial vorticity maps at supergranular length scales ($\sim$30 Mm) near the surface compare extremely well with those obtained using the Local Correlation Tracking method. We find that the Pearson correlation coefficient is $\geq$ 0.9 for divergence flows, while $\geq$ 0.8 is obtained for the radial vorticity.

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Prasad Mani, Chris Hanson, Shravan Hanasoge. 2022-01-01. Imaging the Sun's near-surface flows using mode-coupling analysis. https://doi.org/10.3847/1538-4357%2Fac474e

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