Experimental Astronomy

, Volume 1, Issue 5, pp 329–343

A polarimetric spectral imager using acousto-optic tunable filters

Authors

  • WM. Hayden Smith
    • Department of Earth and Planetary SciencesWashington University
  • K. M. Smith
    • Department of Earth and Planetary SciencesWashington University
Article

DOI: 10.1007/BF00454329

Cite this article as:
Hayden Smith, W. & Smith, K.M. Exp Astron (1990) 1: 329. doi:10.1007/BF00454329

Abstract

We report laboratory and telescopic observations with a polarimetric spectral imager based on an acousto-optic tunable filter (AOTF) where we demonstrate simultaneous acquisition of orthogonally polarized images at a spectral resolving power on the order of 103 and at a Rayleigh criterion spatial resolution of 100 line pairs per mm. This matches the spatial resolution of most digital arrays. An AOTF is shown to be usable as a fast shutter with a contrast of over 104 on a sub-millisecond time scale while providing an high transmittance of about 75% (both polarizations summed) when illuminated by white light. The polarization contrast between the orthogonally polarized images exceeds 104 across the field of view, permitting accurate measurement of the polarization parameters of incident light. These characteristics are now being used in a program of high spatial resolution imaging in narrow spectral bands. Some peculiarities and limitations of AOTFs are indicated.

Key words

narrow band imagingpolarimetry

Copyright information

© Kluwer Academic Publishers 1991