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FAST 数字后端及超宽带百万通道频谱仪算法仿真

张夏 俞欣颖 段然 李菂 蒿杰 金乘进

天文学进展2016,Vol.34Issue(2):249-257,9.
天文学进展2016,Vol.34Issue(2):249-257,9.DOI:10.3969/j.issn.1000-8349.2016.02.08

FAST 数字后端及超宽带百万通道频谱仪算法仿真

FAST Digital Backend and Algorithm Simulation for Broadband Million Channel Spectrometer

张夏 1俞欣颖 2段然 3李菂 1蒿杰 1金乘进4

作者信息

  • 1. 中国科学院 国家天文台,北京 100012
  • 2. 中国科学院大学,北京 100049
  • 3. 贵州大学大数据与信息工程学院,贵阳 550025
  • 4. 中国科学院 射电天文重点实验室,南京 210008
  • 折叠

摘要

Abstract

The National Astronomical Observatories of the Chinese Academy of Sciences (NAOC) will soon finish the Five-hundred-meter Aperture Spherical Radio Telescope (FAST), which will be the most sensitive single-dish radio telescope in the low frequency radio bands between 70 MHz and 3 GHz. To take advantage of its giant aperture, the ongoing self-developing brand-new broadband receiver China Reconfigurable ANalog-Digital backEnd (CRANE) is expected to ensure that it would achieve the best possible overall performance. <br> In hardware, CRANE includes developed parts — FAST Digital Backend (FDB), 3 Gbits/s, 12-bit Analog-to-Digital Converter (FAST3212ADC) — and developing part —Analog Front-end Board (AFB). In its firmware, FPGA-based digital signal processing al-gorithms such as Digital Down Converter (DDC) and Fast Fourier Transform(FFT) will be applied to realize channelization on FDB. CRANE plans to build million channel spectrome-ter which measures a frequency precisely on FDB. We utilize two cascaded FFT to optimize the FFT for large-scale operation. However, the resolution of the first FFT unit would cause the distortion of the output results. The simulation on Matlab shows that final frequency can be restored.

关键词

射电望远镜/超宽带接收机/百万通道频谱仪/仿真设计

Key words

radio telescope/broadband receiver/million channel spectrometer/simulation design

分类

天文与地球科学

引用本文复制引用

张夏,俞欣颖,段然,李菂,蒿杰,金乘进..FAST 数字后端及超宽带百万通道频谱仪算法仿真[J].天文学进展,2016,34(2):249-257,9.

基金项目

国家自然科学基金(11373045);天文联合基金(U1531139);973项目(2012CB821800,2015CB857103) (11373045)

天文学进展

OA北大核心CSCDCSTPCD

1000-8349

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