Flux tube diagnostics based on the Stokes V profiles of infrared H-band lines.

Details Flux tube diagnostics based on the Stokes V profiles of infrared H-band lines. Flux tube diagnostics based on the Stokes V profiles of infrared H-band lines.

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991sopo.work..489m&link_type=abstract

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

Physics

Scientific paper

Stokes V profiles of the unblended Fe I lines in the wavelength range 1.5 - 1.8 μ (H-band) observed in the solar network are analysed. The data are consistent with an absence of stationary flows larger than 0.3 km s-1. The infrared Stokes V profiles are asymmetric in the same sense as lines in the visible, but tend to be of smaller magnitude, in particular the area asymmetry. The widths of the Stokes V profiles are consistent with kG field strengths. Finally, model calculations allow an upper limit of 2 to be set on the continuum intensity of small magnetic features relative to the quiet Sun.

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