Spectral type solar radiance measuring instrument
A technology for measuring solar radiation and illuminance, which is used in spectrum surveys and other directions, and can solve problems such as unseen patents or literature reports, inconsistent spectral distributions of sensor spectral characteristics, and potential safety hazards for long-distance optical fiber laying.
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Embodiment 1
[0059] Embodiment 1 The specific implementation of the instrument of the present invention will be described below with reference to the accompanying drawings.
[0060] Based on the spectrum type solar irradiance measuring instrument of the present invention, its principle block diagram is as figure 1 shown. The instrument of the present invention adopts optical dispersion method, and based on spectral measurement, array detector and ARM microprocessor as the core technology, it constitutes a spectral solar radiation illuminance measuring instrument.
[0061] The instrument includes: optical receiving unit, optical coupling unit, fiber optic spectrometer module unit, GPS module unit, constant temperature control unit and housing and other units. The optical receiving unit is located on the top of the housing to receive and process the light radiation signal from the sun; the optical coupling unit connects the output interface of the optical receiving unit and the input interf...
Embodiment 2
[0078] Embodiment 2 illustrates the working principle of the spectral solar irradiance measuring instrument of the present invention.
[0079] Working principle and working process of the present invention comprise:
[0080] Step 1: Start the instrument, and the instrument will automatically initialize. Use the built-in GPS module unit to determine the local time;
[0081] Step 2: If the time is within the range of local sunrise to sunset, the instrument starts the constant temperature control unit. When the temperature tends to be stable, set the integration time of the array detector to the minimum value, open the shutter of the optical system, and the light radiation of all wavelengths emitted from the sun at a certain moment enters the diffuse transmission plate through the double protective cover, and passes through the diffuse transmission plate The uniform mixing of the incident light eliminates the directional error (that is, the cosine effect);
[0082] Step 3: The...
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