Polarimetric studies of solar magneto-sensitive spectral lines.

Details Polarimetric studies of solar magneto-sensitive spectral lines. Polarimetric studies of solar magneto-sensitive spectral lines.

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991sopo.work..403y&link_type=abstract

Solar Polarimetry, Proceedings of the 11th Sacramento Peak Summper Workshop. Edited by L.J. November. Sunspot, NM: National Sola

Computer Science

Scientific paper

This paper presents a comprehensive account of a series of researches on solar magneto-sensitive spectral lines made by the author and his coworkers. On the basis of numerical solutions of the equations of transfer of polarized radiation in magnetic fields, the following characteristics of solar magneto-sensitive lines have been studied: (1) profiles of Stokes parameters, (2) temperature sensitivity, (3) magnetic intensification, (4) depth of formation, (5) Zeeman components and Seares' formulae, (6) monochromatic images, (7) line asymmetry and gradient of sunspot magnetic fields, (8) relation with Alfvén waves, (9) derivation of information of magnetic vector, (10) Faraday rotation and azimuth of the transverse magnetic field, (11) twist of magnetic lines of force in depth.

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