On a limitation of Zeeman polarimetry and imperfect instrumentation in representing solar magnetic fields with weaker polarization signal

no code implementations • 18 Jan 2021 • Alexei A. Pevtsov, Yang Liu, Ilpo Virtanen, Luca Bertello, Kalevi Mursula, K. D. Leka, Anna L. H. Hughes

Full disk vector magnetic fields are used widely for developing better understanding of large-scale structure, morphology, and patterns of the solar magnetic field.

Solar and Stellar Astrophysics