Center-to-limb variation of Stokes profiles and the diagnostics of solar magnetic fluxtubes

Details Center-to-limb variation of Stokes profiles and the diagnostics of solar magnetic fluxtubes Center-to-limb variation of Stokes profiles and the diagnostics of solar magnetic fluxtubes

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...171..305s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 171, no. 1-2, Jan. 1987, p. 305-316.

Astronomy and Astrophysics

Astrophysics

61

Line Shape, Magnetic Flux, Solar Magnetic Field, Spatial Resolution, Spectrum Analysis, Stokes Law Of Radiation, Doppler Effect, Fourier Transformation, Polarization Characteristics, Solar Limb

Scientific paper

Simultaneous recordings of the Stokes I, Q, and V spectra have been performed with a Fourier transform spectrometer in 10 solar regions distributed over various center-to-limb distances, from disk center to the extreme limb. The observational material and the recording technique used are presented. The authors then evaluate the Stokes profile parameters for a small selected set of spectral lines to explore the potential of this qualitatively new data set for the diagnostics of spatially unresolved magnetic fluxtubes.

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