Light-splitting light path structure of broad-spectrum solar spectral irradiance monitor
A solar spectrum and irradiance technology, applied in the field of spectral measurement, can solve problems such as aberration and low spectral resolution, achieve high resolution, improve diffraction efficiency, and reasonably control aberrations
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example 1
[0019] The solar spectrum irradiance monitor is designed for the 200-800nm band, and the first-order diffraction of 400nm-800nm and the second-order diffraction of 200nm-400nm are applied at this time. A planar grating with 600 line pairs / mm is selected, the curvature of the hyperbolic concave mirror is selected to be 356.10 mm, and its conic coefficient is -5.52; the curvature of the variable ellipsoidal concave mirror is selected to be 356.11 mm, and its conical coefficient is 0.66. The semi-off-axis angle α was set to 7°, the grating incident angle i was set to -2°, and the semi-off-axis angle β was set to 10.43°. The slit width is set to 50 microns, and the linear array detector is selected as two Hamamatsu ones with 2048 pixels, and the pixel size is 25 μm×2.5mm linear array CCD.
[0020] Corresponding to the above-mentioned solar spectrum irradiance monitor, the spectral resolution can be obtained in the 400nm-800nm band to be 0.45nm, and the spectral resolution ca...
example 2
[0022] Changing the incident angle i of the grating in Example 1 to -4°, the curvature of the hyperbolic concave mirror is 358.76 mm, and its conic coefficient becomes -5.69; the curvature of the variable ellipsoidal concave mirror is 358.77 mm, and its conic coefficient becomes 0.69. At this time, the spectral resolution obtained in the 400nm-800nm band is 0.43nm, and the spectral resolution obtained in the 200nm-400nm band is 0.22nm, and the modulation transfer function at the full-band cut-off frequency of the optical system is greater than 0.6, and the maximum dispersion spot in the whole band is uniform The square root radius is less than 1 / 3 of the cell width.
example 3
[0024] The solar spectrum irradiance monitor is designed for the 600nm-1000nm and 1200nm-2000nm bands. At this time, the first-order diffraction of 1200nm-2000nm and the second-order diffraction of 600nm-1000nm are applied. A planar grating with 300 line pairs / mm is selected, and the curvature of the hyperbolic concave mirror is selected through optimization design. The curvature is 322.87mm, and its conic coefficient is -3.01; . The semi-off-axis angle α was set to 6°, the grating incident angle i was set to -3°, and the semi-off-axis angle β was set to 8°. The slit width is set to 50 microns, and the linear array detector is selected as Goodrich’s one with 1024 pixels and a pixel size of 50 μm×2.5mm, and a Hamamatsu one with 2048 pixels and a pixel size of It is 25μm×2.5mm linear array CCD.
[0025] Corresponding to the above-mentioned solar spectrum irradiance monitor, the spectral resolution can be obtained in the 1200nm-2000nm band to be 0.87nm, and the spectral resolut...
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