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Kilometer-Square Area Radio Synthesis Telescope Karst Project

Published online by Cambridge University Press:  25 May 2016

B. Peng
Affiliation:
Beijing Astronomical Observatory, China
R. Nan
Affiliation:
Beijing Astronomical Observatory, China

Extract

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One way to realize the Large radio Telescope with a collecting area approaching one square kilometer, continuously covering a frequency range between 200 MHz and 2 GHz, is to construct a passive spherical reflector array of about 30 individual unit telescopes, each ∼ 300 m diameter(Butcher 1995). Valleys amid the hills of southwest China would be ideal for such LT concept. We refer to this effort as the Kilometer-square Area Radio Synthesis Telescope project. Site surveying and Radio Interference monitoring looks promising. Engineering considerations are summarized.

Type
Part 2. Survey Projects
Copyright
Copyright © Kluwer 1998 

References

Butcher, H., 1995. Astron NFRA. Issue no.9 page 57.Google Scholar
Duan, B., Zhao, Y., Wang, J. and Xu, G., 1996. Proc. of the 3rd Meeting of the Large Telescope Working Group and of a Workshop on Spherical Radio Telescope, eds: Strom, Richard, Peng, Bo and Nan, Rendong 85102.Google Scholar
Guo, Y., Shu, X. and Yan, H., 1996. Proc. of the LTWG-3 & W-SRT. eds: Strom, Richard, Peng, Bo and Nan, Rendong 175177.Google Scholar
Mao, Y. and Jiao, Y.Y., 1996. Proc. of the LTWG-3 & W-SRT. 8184.Google Scholar
Peng, B., Strom, R., Nan, R., Nie, Y., Piao, T., Kang, L., Yan, Y. and Wu, S., 1996. Proc. of the LTWG–3 & W–SRT. 144151.Google Scholar
Wang, J., Xu, G., Duan, B., and Li, H., 1996. Proc. of the LTWG–3 & W-SRT. 158159.Google Scholar
Xiong, J. & Xie, S., 1996. Proc. of the LTWG–3 & W-SRT. 116122.Google Scholar