The instrument mounts on front of the OTA, pointing towards what the telescope is observing. Its narrow, 5 degree, field of view will ensure that the observed area is in very close vicinity of telescopic FOV. In the event that a cloud starts to encroach towards the observed area, it will become very evident by observing the IR measured temperature and the standard deviation charts.
In addition, by observing the magnitude of the Sky temperature variance it is possible to gage the seeing and track its changes in real time: Since seeing is produced by the inhomogeneities of the real part of the air’s dielectric, and since both temperature and water vapor density affect this parameter, we would expect that the variability of the Sky mid-IR temperature would correlate with the low-altitude component of the atmospheric seeing.
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