The Formation of One-Lobed Stokes V Profiles in an Inhomogeneous Atmosphere

Details The Formation of One-Lobed Stokes V Profiles in an Inhomogeneous Atmosphere The Formation of One-Lobed Stokes V Profiles in an Inhomogeneous Atmosphere

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aspc..236..371p&link_type=abstract

Advanced Solar Polarimetry -- Theory, Observation, and Instrumentation -- 20TH NSO/Sac Summer Workshop, ASP Conference Proceedin

Mathematics

Logic

10

Sun: Magnetic Fields, Sun: Granulation, Sun: Spectral Lines

Scientific paper

We assess the diagnostic potential of the observed pathological Stokes V profiles that differ strongly from the customary, nearly antisymmetric two-lobed shape. In particular, we consider the formation of one-lobed Stokes V profiles using the results of an MHD simulation. We find that the majority of one-lobed profiles is produced in regions of weak horizontal field with significant cancellation caused by mixed polarity along the line of sight. A minority of one-lobed profiles originates close to strong magnetic field concentrations with strong gradients of velocity and magnetic field strength.

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