2022
DOI: 10.3847/1538-4357/ac6fe4
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Reconstruction of Photospheric Velocity Fields from Highly Corrupted Data

Abstract: The analysis of the photospheric velocity field is essential for understanding plasma turbulence in the solar surface, which may be responsible for driving processes such as magnetic reconnection, flares, wave propagation, particle acceleration, and coronal heating. Currently, the only available methods to estimate velocities at the solar photosphere transverse to an observer’s line of sight infer flows from differences in image structure in successive observations. Due to data noise, algorithms such as local … Show more

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