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The infrared sensor puts out a voltage depending on the difference between the case temperature and the sky temperature. The sensor voltage is denoted irvolts and the case temperature is related to ovolts. I determine the "cloud" calibration by observing the range of irvolts and ovolts over as wide a range of conditions as possible. Figure 3.10 is a graph of voltages measured over December 2006.
Figure 3.10:
Cloud Sensor Calibration
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The upper envelope is the clearest sky. The bottom represents cloud. The amplifier can only produce positive signals and there unfortunately seems to be a negative bias, which I will remove by installing a resistor in the future. However we can still continue. By assuming the "clear" value is the red in the graph and "cloudy" is 0 irvolts. We come up with the crazy formula that:
cloud=1 - (irvolts - (ovolts-2.820)*0.467)/0.3
where cloud ranges from
. The formula does a good job for clear skies and lousy for really cloudy ones. In other words if cloud
don't bother.
Figure 3.11 is a photo of the cloud sensor mounted on the roof.
Figure 3.11:
Photo of Cloud Sensor
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Next: Declination Axis
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Louis-Gregory Strolger
2012-01-09