| 摘要 |
A dark field infrared telescope. Energy from an infrared scene is focused by a lens (10) onto a thermoptic modulator (12) comprising an optical structure (16) containing a thin film of vanadium dioxide disposed to form the faceplate of a conventional cathode ray tube. The modulator, normally nonreflecting of infrared energy, may have reflecting spots written at selected coordinates thereon by an electron beam from the cathode ray tube. A reflecting spot written on the modulator optically couples a selected element of the scene imaged on the modulator to an infrared detector (52) maintained at low temperature. A retroreflecting mirror (30), cold spectral filter (46), field lens (47), cold field stop (48) and cold pupil stop (50) are provided ahead of the detector to produce a low background flux cavity with the detector at one end and the retroreflecting mirror at the other. In its unswitched state, the modulator is nonreflecting and the scene image is not coupled to the detector. The cold detector thus looks back upon itself and sees a "dark field." Under the control of the sensor microprocessor (22), the electron beam is synchronously switched on and off to modulate the detector signal. The detector signal is then synchronously demodulated by a signal processor (56) to reduce the noise of the detector and preamplifier. By reducing background flux and detector noise, the sensor approaches a signal shot noise or electronic noise limited condition.
|
