DSA-2000候选站点调查移动RFI监测站的设计

V. Prayag, G. Hellbourg, M. Virgin
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引用次数: 0

摘要

DSA-2000射电望远镜目前被设计成最快和最灵敏的天文测量仪器。该设计的一个重要因素是望远镜未来的射频干扰(RFI)环境。仔细的选址和RFI风险评估对于确保满足望远镜的规格非常重要。为此,已经开发了一个移动RFI监测站,以提供候选望远镜站点RFI环境的准确图像。本文介绍了这个监测站和欧文斯谷射电天文台获得的初步结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Design of a mobile RFI monitoring station for DSA-2000 candidate sites surveys
The DSA-2000 radio telescope is currently being designed to become the fastest and most sensitive astronomical survey instrument. An important factor in this design is the future Radio Frequency Interference (RFI) environment of the telescope. A careful site selection and RFI risks assessment are important to ensure that the specifications of the telescope are met. To this end, a mobile RFI survey station has been developed to provide an accurate picture of the RFI environment of a candidate telescope site. This paper presents this monitoring station and preliminary results captured at the Owens Valley Radio Observatory.
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