Comparison of solar horizontal velocity fields from SDO/HMI and Hinode data
Th. Roudier, M. Rieutord, V. Prat, J.M. Malherbe, N. Renon, Z. Frank,, M. Svanda, T. Berger, R. Burston, L. Gizon

TL;DR
This study compares high-resolution horizontal velocity measurements of the Sun's surface from SDO/HMI and Hinode data, validating and calibrating the velocity fields to improve solar surface dynamics analysis.
Contribution
It introduces a method to correct SDO/HMI horizontal velocity measurements using Hinode data and derives detailed velocity components including solar differential rotation.
Findings
High-precision measurement of solar differential rotation (+-0.037 km/s)
Validation of SDO/HMI velocity fields against Hinode data
Derivation of spherical velocity components from surface flow measurements
Abstract
The measurement of the Sun's surface motions with a high spatial and temporal resolution is still a challenge. We wish to validate horizontal velocity measurements all over the visible disk of the Sun from Solar Dynamics Observatory/ Helioseismic and Magnetic Imager (SDO/HMI) data. Horizontal velocity fields are measured by following the proper motions of solar granules using a newly developed version of the Coherent Structure Tracking (CST) code. The comparison of the surface flows measured at high spatial resolution (Hinode, 0.1 arcsec) and low resolution (SDO/HMI, 0.5 arcsec) allows us to determine corrections to be applied to the horizontal velocity measured from HMI white light data. We derive horizontal velocity maps with spatial and temporal resolutions of respectively 2.5 Mm and 30 min. From the two components of the horizontal velocity Vx and Vy measured in the sky plane and…
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