Remote sensing of the temperature of a greybody or blackbody radiator is effected by passing its
radiation (24) through a modulated
infrared filter
spectrometer. The
infrared filter comprises, in sequence, a
band pass filter (20), a first polariser (21) which polarises the
radiation, an electro-optical element (22) which splits the polarised
radiation into two orthogonally polarised components, and a second polariser (23). A lens (28) images the radiation leaving the second polariser onto a
detector (27). The electrical
signal from the
detector (27) is input to a numerical
analyser. The electro-optical element (22), typically comprising a
birefringent crystal assembly (25) and a birefringent trim plate (26), is configured so that the net optical
delay of the orthogonally polarised components passed through it is such that the recombined components are at or near a peak or trough in their interferogram. A sinusoidally varying
voltage is applied to the electro-optical element to modulate the net
delay of the components passed through the electro-optical element. The numerical
analyser is programmed to compute the
harmonic amplitude ratio (the ratio of
signal amplitudes at the fundamental and second
harmonic of the frequency of the modulating
voltage) of the
signal that it receives from the
detector (27). The
harmonic amplitude ratio is a function of the temperature of the radiator, which can be estimated by reference to a calibration look-up table.