Optical device for wide waveband plane grating dispersion type imaging spectrometer
A technology of imaging spectrometer and planar grating, which is applied in the field of imaging spectrometer, can solve the problems of large residual aberration and large astigmatism, and achieve the effects of wide spectral range, cost reduction and good imaging quality
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specific Embodiment approach 1
[0011] Specific implementation mode 1. Combination figure 1 with figure 2 Describe this embodiment, the optical device of the broadband planar grating dispersion imaging spectrometer, the device includes a front optical system and a Czerny-Turner spectral imaging system, and the front optical system includes an aperture stop 1 and an off-axis parabolic mirror 2; The Czerny-Turner spectral imaging system is composed of an entrance slit 3, a spherical collimator mirror 4, a plane grating, a plane mirror, a toroidal focusing mirror, and an area array focal plane detector; 1 and off-axis parabolic mirror 2 on the focal plane of the pre-optical system, the outgoing light passing through the incident slit 3 is projected onto the spherical collimator 4, collimated by the spherical collimator 4 and projected onto the plane grating 5 , the diffracted light emitted from the plane grating 5 is deflected by the plane mirror 6 and projected onto the toroidal focusing mirror 7, and then f...
specific Embodiment approach 2
[0012] Specific embodiment two, combine figure 2 with image 3 As shown, this embodiment is an embodiment of the optical device of the broadband plane grating dispersion imaging spectrometer described in the first embodiment, including a front optical system composed of an aperture stop 1 and an off-axis parabolic mirror 2 and an incident A spectral imaging system composed of a slit 3, a spherical collimator mirror 4, a plane grating 5, a plane mirror 6, a toroidal focusing mirror 7 and an area focal plane detector 8.
[0013] The device of the present invention is mounted on a satellite platform to detect ground targets, and the working band is 350nm-750nm. Combined with 3, the X direction is the cross-track direction, that is, the length direction of the incident slit 3, the Y direction is the satellite running direction, that is, the width direction of the incident slit 3, and the Z direction is the satellite height direction; the corresponding ground width of the X direc...
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