On-orbit polarization measuring system of satellite-borne imaging spectrometer
An imaging spectrometer and measurement system technology, applied in the field of space optics, can solve the problems of reducing imaging quality, measurement accuracy error, etc., and achieve the effects of improving measurement accuracy, simple structure, and light weight
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specific Embodiment approach 1
[0010] Specific implementation mode 1. Combination figure 1 and figure 2 Description of the present embodiment, an on-orbit polarization measurement system of a spaceborne imaging spectrometer, uses Brewster prism 5 as a light splitting and polarization element to realize on-orbit polarization measurement of a spaceborne imaging spectrometer; the system includes an aperture stop 1, Telescope 2, entrance slit 3, collimating mirror 4, Brewster prism 5, focusing mirror 6, plane folding mirror 7 and focal plane detector 8. The system is arranged in an orderly manner according to the xyz right-handed space coordinate system, the z-axis direction is defined as the optical axis direction, the x-axis is perpendicular to the yz plane, the yz plane is the meridian plane of the system, the length direction of the incident slit 3 is along the x-axis direction, and the incident slit 3 is along the x-axis direction. The slit width direction is along the y-axis direction. The incident lig...
specific Embodiment approach 2
[0015] Specific Embodiment 2. This embodiment is an embodiment of the on-orbit polarization measurement system of a spaceborne imaging spectrometer described in Specific Embodiment 1:
[0016] The on-orbit polarization measurement system of the spaceborne imaging spectrometer described in this embodiment is used in conjunction with the imaging spectrometer for atmospheric detection to measure the polarization characteristics of incident light, thereby correcting the polarization response of the imaging spectrometer. The working band of the on-orbit polarization measurement system of the spaceborne imaging spectrometer is 320-500nm, and the atmospheric scattered light radiation with a field angle of 1.8°×0.045° is imaged on the incident slit through the aperture diaphragm and off-axis parabolic telescope. The diameter of the aperture is Φ31mm, the focal length of the off-axis parabolic telescope is 240.269mm, the off-axis distance is 35mm, the size of the incident slit is 7.55mm...
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