Solar-blind ultraviolet light detecting device
A detection device and ultraviolet light technology, which are applied in measurement devices, photometry, optical radiation measurement, etc., can solve the problems of low sensitivity of ultraviolet light detectors, limit solar-blind ultraviolet light detection, and low emission power, etc., and achieve improved detection. Sensitivity, great economic value, low dark current effect
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Embodiment 1
[0018] like figure 1 As shown, a solar-blind ultraviolet light detection device is provided with a filter 1 at the incident window at the front end of the wide-field collector 2, and the rear end of the wide-field collector 2 is connected to the incident light window of the integrating sphere 4; inside the integrating sphere 4 Place the quantum tailoring fluorescent glass 3. The two sides of the quantum tailoring fluorescent glass 3 correspond to the incident window and the exit window of the integrating sphere 4 respectively. The detection windows of the photomultiplier tubes 5 are closely connected.
[0019] The filter 1 of the present invention will filter all the light in the non-detection wavelength region, and only keep the light in the desired detection wavelength range, that is, the transmission wavelength range of the filter 1 can be adjusted to limit the detection wavelength range, but the transmission of the filter The wavelength range should be included in the wav...
Embodiment 2
[0024] The difference between embodiment 2 and embodiment 1 is that the quantum tailoring fluorescent glass 3 whose substrate is silicate is selected in this embodiment, the stimulated emission light is monochromatic light and the peak value of the stimulated emission spectral power curve is at 640nm, and its Stimulated emission spectrum such as figure 2 Shown in the Ex2 curve. The remaining features of embodiment 2 are the same as embodiment 1.
[0025] As described in Embodiment 1, the fluorescent glass is cut and polished to a size that can fit inside the integrating sphere 4 , and the edge is attached to the inner surface of the integrating sphere 4 . Attach a low-pass filter with a cutoff wavelength of 280 nm to the outer surface of the incident window of the integrating sphere 4 . response curve as Figure 4 The photomultiplier tube 5 shown is placed in the exit window of the integrating sphere 4 , and its detection window is close to the outer surface of the exit wi...
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