Cloud detection system for the Mt Kent observatory

Abstract

The extent of cloud cover is crucial for astronomers when making ground based optical astronomical observations. This information is important to astronomers in determining if the sky is suitable for observing and to what extent the cloud cover may affect their data. Normally, estimation of cloud cover is done visually by the astronomer, however in the case of the Mt Kent Observatory this is not possible as the telescope is designed to be operated remotely and there will not be an astronomer on site every night of the year to make these observations.