Polarization of Photospheric Lines from Turbulent Dynamo Simulations
We employ the magnetic and velocity fields from turbulent dynamo simulations to synthesize the polarization of a typical photospheric line. The synthetic Stokes profiles have properties in common with those observed in the quiet Sun. The simulated magnetograms present a level of signal similar to that of the Inter-Network regions. Asymmetric Stokes
Sánchez Almeida, J. et al.
Fecha de publicación:
3
2003