Center-to-limb variation of the Stokes V asymmetry in solar magnetic flux tubes.

Details Center-to-limb variation of the Stokes V asymmetry in solar magnetic flux tubes. Center-to-limb variation of the Stokes V asymmetry in solar magnetic flux tubes.

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991sopo.work..468b&link_type=abstract

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

Computer Science

2

Scientific paper

The center-to-limb-variation of synthetic Stokes V line profiles of the
spectral line Fe I 5250.22 Å is presented and compared with
observations. These synthetic profiles are calculated using models that
contain the main features of the current basic pictures of small scale
magnetic fields on the Sun.

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