A digital baseband recorder for radio pulsar observations
Using the Kunming 40-m radio telescope at Yunnan Observatory, a Pulsar coherent de-dispersion experiment has been carried out which uses a dual polarization receiver operating at s-band and a VLBA back-end: Mark5B+, whose highest sampling rate is 64MHz The data processing system is based on the C programs on Linux. Some pulsar profiles had been carried out using the DBBC and Mark5B+ record system. In this paper we will discuss the application of the DBBC platform in pulsar observation domain and the algorithm of de-dispersion. The main purposes for the instrument are studies of pulsar mode changing, pulsar timing, scintillation monitoring, glitches, GPs (Giant Pulsars), etc
PuLstzrs Mark5B+ Coherent De-dispersion FFT
Long-Fei Hao Min Wang Esamdin Ali
Yunnan Observatory, CAS NAOC Kunming 650011, China Urumqi Observatory, CAS NAOC Urumqi 830011, China
国际会议
2010 2nd International Conference on Signal Processing System(2010年信号处理系统国际会议 ICSPS 2010)
大连
英文
70-73
2010-07-05(万方平台首次上网日期,不代表论文的发表时间)