Radiative transfer across a magnetic flux tube

Details Radiative transfer across a magnetic flux tube Radiative transfer across a magnetic flux tube

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..135..275a&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 135, Oct. 1991, p. 275-297.

Physics

5

Magnetic Flux, Polarized Light, Radiative Transfer, Solar Magnetic Field, Line Of Sight, Solar Instruments, Telescopes

Scientific paper

The Stokes' parameters of a solar magnetic flux tube are simulated as seen with high resolution. Observing with a line-of-sight not parallel to the axis of the flux tube (assumed vertical and axisymmetric) it is possible to see differences between different configurations of the magnetic field inside the flux tube (presence, and in what direction, of an azimuthal component of the field). Furthermore, along such a line-of-sight, the polarization profiles of any atomic line are strongly absorbed at the line center. A strategy is proposed to infer the structure of the magnetic field from observations at high spatial resolution.

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