Determination of the horizontal velocity field in the solar atmosphere: Method validation using 3D MHD model

arXiv:2607.19169 · astro-ph.SR · Submitted 2026-07-21 · Read on arXiv

Andrii Prysiazhnyi, Oleksandra Baran

astro-ph.SR

Submitted: 2026-07-21

Comments: 15 pages with 13 figures

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Accuracy — 6× in this paper · explained in 1 episode
• Sparsity — 3× in this paper · explained in 4 episodes
• Active Regions — 2× in this paper · explained in 1 episode
• U-net architecture — 2× in this paper · explained in 3 episodes
• Michelson Doppler Imager — 1× in this paper
• Robustness — 1× in this paper · explained in 5 episodes
• Solar Dynamics Observatory — 1× in this paper

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