A Software for RFI Analysis of Radio Environment around Radio Telescope

Author:

Wang Yu1ORCID,Zhang Haiyan234ORCID,Wang Jian56ORCID,Huang Shijie23,Hu Hao23,Yang Cheng56ORCID

Affiliation:

1. Research Center for Intelligent Computing Platforms, Zhejiang Laboratory, Hangzhou 311100, China

2. National Astronomical Observatories of China, Chinese Academy of Sciences, Beijing 100101, China

3. National Key Laboratory of Radio Astronomy and Technology, Beijing 100101, China

4. Hebei Key Laboratory of Radio Astronomy Technology, Hebei 050081, China

5. School of Microelectronics, Tianjin University, Tianjin 300072, China

6. Qingdao Institute for Ocean Technology, Tianjin University, Qingdao 266200, China

Abstract

Radio astronomy uses radio telescopes to detect very faint emissions from celestial objects. However, human-made radio frequency interference (RFI) is currently a common problem faced by most terrestrial radio telescopes, and it is getting worse with the development of the economy and technology. Therefore, it is essential to monitor and evaluate interference during the planning, construction, and operation stages of the radio telescope and protect the quiet radio environment around the radio astronomical site. In this paper, we present a software for an RFI analysis of the radio environment around the telescope. In this software, information has been collected, including the location of the site; the technical specifications, such as aperture and the frequency range of the radio telescopes; and the terrain around the site. The software and its modules are composed of telescope, geographic, and meteorological databases, and analysis modules of terrestrial and space-based RFI. Combined with the propagation characteristics of radio waves, we can analyze and evaluate RFI on the ground and in space around the radio telescope. The feasibility of the software has been proved by the experimental implementation of the propagation properties and RFI source estimation. With this software, efficient technical support can be expected for protecting the radio environment around the telescope, as well as improving site selection for planned radio astronomical facilities.

Funder

National Key R&D Program of China

National Natural Science Foundation of China

Publisher

MDPI AG

Subject

General Physics and Astronomy

Reference32 articles.

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3. Katore, S.N., Raybole, P.A., Rai, S., Nayak, S., and Kumar, S. (2017, January 19–26). Tools for avoiding satellite interference at the upgraded GMRT. Proceedings of the 32nd URSI GASS, Montreal, QC, Canada.

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