A USRP2-based reconfigurable multi-constellation multi-frequency GNSS software receiver front end

被引:43
作者
Peng, Senlin [1 ]
Morton, Yu [2 ]
机构
[1] Virginia Tech, Dept Elect & Comp Engn, Blacksburg, VA 24061 USA
[2] Miami Univ, Dept Elect & Comp Engn, Oxford, OH 45056 USA
关键词
Multi-constellation multi-band; GNSS software receiver; USRP2; Ionosphere scintillation; IONOSPHERIC SCINTILLATION; CMOS RECEIVER; TRACKING;
D O I
10.1007/s10291-012-0263-y
中图分类号
TP7 [遥感技术];
学科分类号
081102 ; 0816 ; 081602 ; 083002 ; 1404 ;
摘要
We present a multi-constellation multi-band GNSS software receiver front end based on USRP2, a general purpose radio platform. When integrated with appropriate daughter boards, the USRP2 can be used to collect raw intermediate frequency (IF) data covering the entire GNSS family of signals. In this study, C++ class-based software receiver processing functions were developed to process the IF data for GPS L1, L2C, and L5 and GLONASS L1 and L2 signals collected by the USRP2 front end. The front end performance is evaluated against the outputs of a high end custom front end driven by the same local oscillator and two commercial receivers, all using the same real signal sources. The results show that for GPS signals, the USRP2 front end typically generates carrier-to-noise ratio (C/N (0)) at 1-3 and 1-2 dB below that of the high end front end and a NovAtel receiver, respectively. For GLONASS signals, the USRP2 C/N (0) outputs are comparable to those of a Septentrio receiver. The carrier phase noise from the USRP2 outputs is similar to those of the benchmarking devices. These results demonstrate that the USRP2 is a suitable front end for applications, such as ionosphere scintillation studies.
引用
收藏
页码:89 / 102
页数:14
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