As part of a feasibility study for a far-infrared Fourier-transform spacebo
rne spectrometer, the criteria that drive the choice of the instrument conf
iguration have been identified as broadband operation, dual input and outpu
t ports, optics of the interferometer with full tilt compensation, and meas
urement of both planes of polarization of the source on a single detector.
Despite the fact that some of these requirements are apparently difficult t
o reconcile, a new configuration of the polarizing interferometer that meet
s all the above requirements has been identified. The considerations that l
ed to the design of this new configuration are discussed. (C) 1994 Optical
Society of America.