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Difficulties in the Simultaneous Measurement of All Stokes Parameters

  • E. Wiehr (a1)

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Telescopic phase retardation in connection with the polarizer behind a polarimeter's KDP-crystal strongly influences the Zeeman pattern, since the circular polarized parts of the two σ-components are strengthened and weakened respectively. This influence depends on the hour angle if the solar image rotates with respect to the polarizer (e.g. for Coudé telescopes).

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References

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Jäger, F. W. and Oetken, L.: 1963, Publ. Astron. Obs. Potsdam No. 103, Vol. 31, p. 30.
Wiehr, E.: 1969, Solar Phys. 9, 225.
Wiehr, E.: 1971, Solar Phys. 18, 226.

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