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- W2549033533 abstract "With the proliferation of autonomous small telescope networks, it is desirable to have a cloud detector that can be used to reduce time spent attempting to collect data when transient clouds are obscuring portions of the sky. The conventional method of cloud detection for a small telescope is to use a Boltwood Cloud Sensor or similar device. This type of device measures the amount of cloud cover by comparing the temperature of the sky to the ambient ground level temperature, where a large temperature di↵erence between the sky and the ground level indicates clear skies. This sky temperature measurement is based on a single IR detector sensing the average temperature of the entire sky. The Air Force’s Ground-based Electro-Optical Deep Space Surveillance (GEODSS) system employs a much more capable Infrared Cloud Imager (IRCI) for the purpose of cloud detection. IRCI uses the same IR temperature measurement technique as a Boltwood-type device but does so with an array of sensors dividing the sky into 104 zones.[1] This allows the GEODSS telescopes to continue to operate e ciently during partially clouded nights by adjusting the observation schedule to not look in sectors where clouds have been detected. Just like the Air Force’s GEODSS system, an autonomous network of small telescopes would benefit from a device capable of monitoring and reporting cloud cover by sector. IRCI is a complex and costly solution, so we chose to implement a commercial o↵-the-shelf (COTS) visible all-sky camera to perform a similar function." @default.
- W2549033533 created "2016-11-11" @default.
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- W2549033533 date "2015-01-01" @default.
- W2549033533 modified "2023-09-26" @default.
- W2549033533 title "Visible Cloud Imager for Autonomous Telescopes" @default.
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