Real time prediction, detection and co-existing with satellite interference at GMRT

P. Raybole, S. Sureshkumar, S. Katore, S. Rai
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引用次数: 10

Abstract

Modern radio telescopes were designed for wider bandwidth to use the interference free bands for radio astronomy. Many intentional radiations are directional and line of site, pointing can be avoided to prevent receiver saturation. About 35000 Satellites are in space to provide voice and data service, navigation, GPS, weather, military and various space programs. These satellite footprints are larger to cover wide area and produce interference to radio telescopes. These satellites are geo stationary, geo synchronous, low, and medium orbiting satellites whose locations and orbits have been characterized with the precise servo system of GMRT antennas. The individual satellite signals have been characterized for its frequency, power level and beam width using GMRT antenna and receiver. The antenna control and monitoring system of GMRT observatory is programmed to produce an alarm whenever the antenna beam is nearing a satellite. The software tools provide prediction of these satellite cross over with any scheduled radio astronomy observation, real time location of the antenna beam with adjacent line of site satellites on the sky and tools to post process the old astronomical data for flagging the duration of satellite signal overlap or saturation. The soft tools will be used to apply digital filtering techniques to mitigate these satellite signals in real time or during post processing. The paper presents the detail characterization of satellite interference to GMRT and the software tools developed to co-exist with satellite interference with detail analysis of the loss of signal or data for any given astronomical observation.
GMRT实时预测、探测并与卫星干扰共存
现代射电望远镜被设计为更宽的带宽,以利用无干扰的波段进行射电天文学研究。许多有意的辐射是定向的,可以避免指向以防止接收器饱和。大约有35000颗卫星在太空中提供语音和数据服务、导航、GPS、天气、军事和各种太空计划。这些卫星足迹较大,覆盖范围广,对射电望远镜产生干扰。这些卫星包括地球静止轨道、地球同步轨道、低轨道和中轨道卫星,它们的位置和轨道都以GMRT天线的精确伺服系统为特征。利用GMRT天线和接收机对单个卫星信号的频率、功率电平和波束宽度进行了表征。GMRT天文台的天线控制和监测系统被编程为在天线波束接近卫星时产生警报。这些软件工具可以预测这些卫星与任何预定的射电天文观测的交叉,实时定位天线波束与天空中相邻的站点卫星的位置,以及对旧的天文数据进行后期处理的工具,以标记卫星信号重叠或饱和的持续时间。软工具将用于应用数字滤波技术来实时或在后处理期间减轻这些卫星信号。本文介绍了卫星干扰对GMRT的详细特征,以及为与卫星干扰共存而开发的软件工具,并详细分析了任何给定天文观测的信号或数据损失。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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