天文研究与技术-国家天文台台刊
天文研究與技術-國傢天文檯檯刊
천문연구여기술-국가천문태태간
Astronomical Research & Technology-Publications of National Astronomical Observatories of China
2015年
4期
473-479
,共7页
吴俊霖%金乘进%朱岩%岳友岭%甘恒谦%赵欣
吳俊霖%金乘進%硃巖%嶽友嶺%甘恆謙%趙訢
오준림%금승진%주암%악우령%감항겸%조흔
Zoom-FPB%ROACH%Xilinx System Generator%接收机数字后端
Zoom-FPB%ROACH%Xilinx System Generator%接收機數字後耑
Zoom-FPB%ROACH%Xilinx System Generator%접수궤수자후단
Zoom-PFB%ROACH%Xilinx System Generator%Digital backend of a radio receiver
简述了基于ROACH和Xilinx System Generator平台的接收机数字后端系统的设计与实现。介绍了Zoom-PFB算法原理,讨论了该算法的核心部分低通滤波和抽取的现场可编程门阵列( Field-Programmable Gate Array, FPGA)实现。针对谱线观测局部高精度分辨率的需要,给出了将400 MHz带宽分为带宽25 MHz的16个通道,对其中任一通道做通道数为6 k、频率分辨率为4 kHz的频谱细化系统的具体设计方案。在实验室条件下,对该数字后端的性能进行了分析和测试,并以4.5m口径X/Y结构天线进行银道面中性氢谱线观测检验其应用效果,验证了方案的可行性。
簡述瞭基于ROACH和Xilinx System Generator平檯的接收機數字後耑繫統的設計與實現。介紹瞭Zoom-PFB算法原理,討論瞭該算法的覈心部分低通濾波和抽取的現場可編程門陣列( Field-Programmable Gate Array, FPGA)實現。針對譜線觀測跼部高精度分辨率的需要,給齣瞭將400 MHz帶寬分為帶寬25 MHz的16箇通道,對其中任一通道做通道數為6 k、頻率分辨率為4 kHz的頻譜細化繫統的具體設計方案。在實驗室條件下,對該數字後耑的性能進行瞭分析和測試,併以4.5m口徑X/Y結構天線進行銀道麵中性氫譜線觀測檢驗其應用效果,驗證瞭方案的可行性。
간술료기우ROACH화Xilinx System Generator평태적접수궤수자후단계통적설계여실현。개소료Zoom-PFB산법원리,토론료해산법적핵심부분저통려파화추취적현장가편정문진렬( Field-Programmable Gate Array, FPGA)실현。침대보선관측국부고정도분변솔적수요,급출료장400 MHz대관분위대관25 MHz적16개통도,대기중임일통도주통도수위6 k、빈솔분변솔위4 kHz적빈보세화계통적구체설계방안。재실험실조건하,대해수자후단적성능진행료분석화측시,병이4.5m구경X/Y결구천선진행은도면중성경보선관측검험기응용효과,험증료방안적가행성。
In this paper we describe design and implementation of a digital backend system for a radio-telescope receiver based on a ROACH system and a Xilinx System Generator.The system incorporates a Zoom-PFB algorithm.We first discuss principles of a Zoom-PFB algorithm and approaches to use an FPGA to realize the key parts of a Zoom-PFB, the low-bandpass filtering and decimation.To meet the demand of high-resolution observation of parts of spectra around a spectral line, we have designed the backend system by dividing its 400MHz bandwidth into 16 bands, each of which extends 25MHz and is further divided into 6k channels with a frequency resolution of about 4kHz.We have analyzed the specifications of the system and have carried out tests for its performance under laboratory conditions.We have also verified the feasibility of our design by using the system to observe the 21cm hydrogen line from the Galactic plane.The observation is through a radio telescope of a 4.5m antenna of the X/Y structure.