The Solar and the Lunar RFI Test for the 40m Radio Telescope

Details The Solar and the Lunar RFI Test for the 40m Radio Telescope The Solar and the Lunar RFI Test for the 40m Radio Telescope

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008pnaoc...5...43g&link_type=abstract

Astronomical Research and Technology. Publications of National Astronomical Observatories of China (ISSN 1672-7673), Vol. 5, No.

Astronomy and Astrophysics

Astronomy

40M Radio Telescope, Radio Frequency Interference, Data Acquisition Subsystem

Scientific paper

In this paper, the noise temperatures of the Sun and the Moon are measured using the calibrations of the standard radio sources and the standard noise. The authors' conclusions are: (1) If the 40m antenna is pointed to the Sun with the angle >=2°, it will not interfere the DAS (Data Acquisition Subsystem). (2) The lunar noise temperature for 40m telescope is 87.1K, that means, DAS can work normally even when 40m antenna pointing to the Moon exactly.

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