Higher PFSS grid resolution improves high-speed stream onset and duration predictions, and the optimal source surface height varies per Carrington rotation, with coronal hole observations helping to constrain it.
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What Causes Errors in Wang-Sheeley-Arge Solar Wind Modeling at L1 ?
Higher PFSS grid resolution improves high-speed stream onset and duration predictions, and the optimal source surface height varies per Carrington rotation, with coronal hole observations helping to constrain it.