Abstract

Astronomers have traditionally monitored cloud cover visually. However, this technique is difficult under dark conditions, insensitive to thin cirrus, and impossible for remote telescope use. A sensitive camera operating in the thermal infrared escapes these problems. Unfortunately, commercially available cameras have smaller than desired fields of view, are not intended for continuous operation, and are expensive. Consequently, a single channel all- sky scanner has been constructed to continuously monitor observatory cloud cover and motions. Operating at a wavelength of 10 microns, it produces a 135 degree(s) X 135 degree(s) image with a resolution of 0.9 degrees. These data are suitable for returning to remote observers and for archiving with astronomical data.

Keywords

SkyScannerCloud computingRemote sensingTelescopeCover (algebra)CirrusObservatoryComputer scienceCloud coverImage resolutionComputer graphics (images)PhysicsAstronomyComputer visionArtificial intelligenceGeographyEngineeringOperating system

Affiliated Institutions

Related Publications

Publication Info

Year
1994
Type
article
Volume
2199
Pages
852-857
Citations
17
Access
Closed

External Links

Social Impact

Social media, news, blog, policy document mentions

Citation Metrics

17
OpenAlex

Cite This

Charles L. H. Hull, Siriluk Limmongkol, Walter A. Siegmund (1994). <title>Sloan Digital Sky Survey cloud scanner</title>. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE , 2199 , 852-857. https://doi.org/10.1117/12.176257

Identifiers

DOI
10.1117/12.176257