Polarimetry with an imaging FTS

Details Polarimetry with an imaging FTS Polarimetry with an imaging FTS

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.344..197s&link_type=abstract

In ESA, Solar Physics and Astrophysics at Interferometric Resolution p 197-200 (SEE N93-10901 01-90)

Astronomy and Astrophysics

Astrophysics

Fourier Transformation, Imaging Spectrometers, Polarimetry, Solar Magnetic Field, Charge Coupled Devices, Demodulation, High Resolution, Modulation, Piezoelectricity, Solar Spectrometers

Scientific paper

The concept of an imaging Fourier Transform Spectrometer (FTS) polarimeter based on piezoelastic modulation and direct demodulation in partially masked Charge Coupled Devices (CCD's) is outlined. The currently operational FTS polarimeter at the McMath telescope as well as the detection scheme of the ETH polarimeter, based on partially masked CCD cameras, are outlined to illustrate its principle.

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