Gaussian separation reveals that optimization and CFIT NLFFF models reproduce some coronal current signatures from magnetogram data for AR 11429 but the CFIT model alters a flux rope signature along the lower PIL.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
method 1
citation-polarity summary
fields
astro-ph.SR 2years
2026 2verdicts
UNVERDICTED 2roles
method 1polarities
use method 1representative citing papers
Non-Gaussian Si IV profiles are common (~60%) in the solar transition region and strongly depend on the angle between the magnetic field and line of sight, with k-like shapes more prevalent at large angles.
citing papers explorer
-
Validating Coronal Magnetic Field Models Using Gaussian Separation
Gaussian separation reveals that optimization and CFIT NLFFF models reproduce some coronal current signatures from magnetogram data for AR 11429 but the CFIT model alters a flux rope signature along the lower PIL.
-
Anisotropic non-Maxwellian velocity distributions in the solar transition region
Non-Gaussian Si IV profiles are common (~60%) in the solar transition region and strongly depend on the angle between the magnetic field and line of sight, with k-like shapes more prevalent at large angles.