Models of solar magnetic fluxtubes - Constraints imposed by Fe I and II lines

Details Models of solar magnetic fluxtubes - Constraints imposed by Fe I and II lines Models of solar magnetic fluxtubes - Constraints imposed by Fe I and II lines

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...148..123s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 148, no. 1, July 1985, p. 123-132.

Astronomy and Astrophysics

Astrophysics

65

Line Spectra, Magnetic Flux, Metallicity, Solar Activity, Solar Magnetic Field, Solar Spectra, Faculae, Iron, Photosphere, Polarimetry, Solar Temperature, Spectrum Analysis, Statistical Analysis, Stokes Law Of Radiation

Scientific paper

The diagnostic contents of the Stokes I and V profiles of about 50 unblended Fe II lines have been explored and used to set new constraints on the temperature structure of magnetic fluxtubes. The simultaneous use of Fe I and II lines makes it possible to determine the temperature in both the upper and lower fluxtube photosphere. The Fe II lines further make it possible to obtain model-insensitive values of the magnetic filling factors. Empirically determined effective Lande factors of most of the unblended iron lines in the visible part of the solar spectrum are presented and compared with the corresponding LS coupling values.

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