Structure and Data Processing of the Solar Stokes Spectral Telescope

Details Structure and Data Processing of the Solar Stokes Spectral Telescope Structure and Data Processing of the Solar Stokes Spectral Telescope

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007pnaoc...4..249l&link_type=abstract

Astronomical Research and Technology. Publications of National Astronomical Observatories of China (ISSN 1672-7673), Vol. 4, No.

Astronomy and Astrophysics

Astronomy

Polarization, Fourier Transformation, Flat Field, Dark Field

Scientific paper

The Solar Stokes Spectral Telescope at the Yunnan Observatory is a typical spectral vector magnetograph which can measure accurately the vector magnetic field of sunspots by using Stokes profiles, I, Q, U, and V, of magnetic-sensitive lines. By using abundant message contained in the four Stokes profiles, it can determine the polarization state of radiation from the sunspots and measure accurately the vector magnetic field within sunspots. The structure of the telescope is described first. In the following, the process of the polarization spectra collected by the telescope is introduced in detail.

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