FARM converts helioseismic far-side phase shifts into magnetic flux and inserts far-side active regions into a surface flux transport model, improving modeled open-field areas in EUV comparisons during 2010-2024.
The polar field strength from F ARM is calculated by taking the mean of the magnetic fields from±60◦ to ±90◦
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Combined Surface Flux Transport and Helioseismic Far-side Active Region Model (FARM)
FARM converts helioseismic far-side phase shifts into magnetic flux and inserts far-side active regions into a surface flux transport model, improving modeled open-field areas in EUV comparisons during 2010-2024.