Strong Stokes V asymmetries of photospheric spectral lines: What can they tell us about the magnetic field structure?

Details Strong Stokes V asymmetries of photospheric spectral lines: What can they tell us about the magnetic field structure? Strong Stokes V asymmetries of photospheric spectral lines: What can they tell us about the magnetic field structure?

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...357..351g&link_type=abstract

Astronomy and Astrophysics, v.357, p.351-358 (2000)

Astronomy and Astrophysics

Astrophysics

26

Line: Formation, Line: Profiles, Polarization, Radiative Transfer, Sun: Magnetic Fields

Scientific paper

In an attempt to identify the mechanism responsible for the extremely
asymmetric Stokes V profiles which were recently observed we analyzed
several simple atmospheric configurations with separated layers of mass
flow and magnetic field. We found that under appropriate conditions the
models are capable of producing the observed one-lobe profiles.

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