Abstract
An all sky camera using commercial parts has been assembled at Cerro Tololo Inter-American Observatory to monitor a wide range of atmospheric effects of interest to astronomers, including thin cirrus and contrails which are otherwise invisible on moonless nights, air glow variations, light pollution in the Sodium and Mercury bands, and aircraft lights. To enhance the visibility of clouds, raw images are divided by the corresponding clear sky image, inferred from images taken at the corresponding sidereal time on previous nights. Frames are taken every 30 seconds so that subsequent animation is smooth enough for the eye to pick out motion of clouds at or below the noise floor.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Roger Smith, 2000, Cloud monitoring with CCDs, Optical Detectors for Astronomy II, P. Amico & J. W. Beletic (eds), p. 345–350
http://www.ctio.noao.edu/sitetests/WorkShop2002/meeting.html
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2004 Springer Science + Business Media, Inc.
About this paper
Cite this paper
Smith, R., Walker, D., Schwarz, H.E. (2004). The Tololo all Sky Camera. In: Amico, P., Beletic, J.W., Beletic, J.E. (eds) Scientific Detectors for Astronomy. Astrophysics and Space Science Library, vol 300. Springer, Dordrecht. https://doi.org/10.1007/1-4020-2527-0_46
Download citation
DOI: https://doi.org/10.1007/1-4020-2527-0_46
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-1788-9
Online ISBN: 978-1-4020-2527-3
eBook Packages: Springer Book Archive