EPJ Web of Conferences
Volume 89, 2015AtmoHEAD 2014: Atmospheric Monitoring for High Energy AstroParticle Detectors
|Number of page(s)||3|
|Section||Instruments and Methods|
|Published online||26 March 2015|
All Sky Camera for the CTA Atmospheric Calibration work package
1 Institute of Physics Academy of Sciences, Czech Republic
2 University and INFN Padova, via Marzolo 8, 35131 Padova, Italy
3 Department of Physics, Universitat Autónoma de Barcelona, Campus UAB, 08193 Bellaterra, Spain
a e-mail: firstname.lastname@example.org
Published online: 26 March 2015
The All Sky Camera (ASC) is a passive non-invasive imaging system for rapid night sky atmosphere monitoring. By design, the operation of the ASC will not affect the measurement procedure of the CTA observatory, for which we discuss its application in this report. The data collected should enable improved productivity and increased measurement time for the CTA observatory. The goal of ASC is to identify cloud position, atmosphere attenuation and time evolution of the sky condition, working within the CTA Central Calibration Facilities (CCF) group. Clouds and atmosphere monitoring may allow near-future prediction of the night-sky quality, helping scheduling. Also, in the case of partly cloudy night sky the cameras will identify the uncovered regions of the sky during the operation time, and define potential observable sources that can be measured. By doing so, a higher productivity of the CTA observatory measurements may be possible.
© Owned by the authors, published by EDP Sciences, 2015
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