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Measurement of light pollution at the Iranian National Observatory

Published online by Cambridge University Press:  01 August 2006

S. Sona Hosseini  and
Sadollah Nasiri
S. Sona Hosseini
Affiliation:
Zanjan University, Iran email: s.sona.h@gmail.com
Sadollah Nasiri
Affiliation:
Zanjan University, Iran email: s.sona.h@gmail.com IASBS, Iran email: nasiri@iasbs.ac.ir
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Abstract

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The problem of light pollution became important mainly since 1960, by growth of urban development and using more artificial lights and lamps at the nighttimes. Optical telescopes share the same range of wavelengths as are used to provide illumination of roadways, buildings and automobiles. The light glow that emanates from man made pollution will scatter off the atmosphere and affects the images taken by the observatory instruments. A method of estimating the night sky brightness produced by a city of known population and distance is useful in site testing of the new observatories, as well as in studying the likely future deterioration of existing sites. Now with planning the Iranian National Observatory that will house a 2-metre telescope and on the way of the site selection project, studying the light pollution is propounded in Iran. Thus, we need a site with the least light pollution, beside other parameters, i.e. seeing, meteorological, geophysical and local parameters. The seeing parameter is being measured in our four preliminary selected sites at Qom, Kashan, Kerman and Birjand since two years ago using an out of focus Differential Image Motion Monitor. These sites are selected among 33 candidate sites by studying the meteorological data obtained from the local synoptic stations and the Meteosat. We measured and used the Walker's law to estimate the Sky brightness for three of these sites

The data obtained using an 8-inch Meade telescope with a ST7 CCD camera for above sites are consistent with the estimated values of the light pollution mentioned above.

Keywords

Light pollutionsky brightnessIranian National Observatory
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Special Session SPS5: Astronomy for the developing world , August 2006 , pp. 183 - 188
Copyright
Copyright © International Astronomical Union 2007

References

Berry, R.L., 1976, J. Roy. Astron. Soc., Canada 70, 97-115.Google Scholar
Cinzano, P. J., 2000, Italian Astro. Soc., 71, N. 1, 1-280.Google Scholar
Darudi, A., Nasiri, S., 2005, Iran. J. Phys. Research, Vol.5, No. 3, 121-128.Google Scholar
Garstang, R.H., 1988, The Observatory, 108.Google Scholar
Garstang, R.H., 1991, ASPC, 1-14.Google Scholar
Information Sheet 20, 1994, reported by International Dark Sky Association (IDA).Google Scholar
Landolt, A. U., 1983, Astro. J., 83, 3.Google Scholar
Tear, S. W., 2000, NASA Astrophys. Data System.Google Scholar
Tomas, R. W. L., Modali, S. B. and Roose, R. G., 1973, Bull. Am. Astron. Soc. 5, 391.Google Scholar
Treanor, P.J., 1973, The Observatory, 93, 117–120.Google Scholar
Walker, M.F., 1970, Publ. Astron. Soc. Pacific, 82, 672–698.CrossRefGoogle Scholar
Yocke, M.A., Hogo, H. and Henderson, D., 1986, Publ. Astron. Soc. Pacific 98, 889–893.CrossRefGoogle Scholar