The S2 baseband processing system for phase-coherent pulsar applications

Abstract

Abstract. The S2 baseband processing system (S2-BPS) is designed for a variety of pulsar measurements such as ultrafast signal fluctuations and pulse timing. Its key features are: the S2 recorder; the S2 Tape-to-Computer Interface (S2-TCI) which provides an efficient high data rate transfer from S2 tapes to computer; and the tightly coupled control interface to the computer which enables automated data transfer and processing. Developed originally for VLBI applications, the S2 recorder is based on the use of commercial VHS tape transports (VCR's), modified for use in digital high density, high data rate applications. A single S2 recorder "tape-set" of eight SVHS tapes provides up to 500 GBytes of data storage, and an unattended operating time of up to 8.5 hours at the maximum data rate of 128 Mbits/s or 16 MBytes/s, corresponding typically to 16 MHz bandwidth in two circular polarizations at 2-bit quantization, which generates a data rate of up to 1 GByte/minute. With 16 MHz individual record channels, a single S2 yields a sample time resolution of 31 ns. For more challenging applications, multiple S2's may be used for increased bandwidth and higher time resolutions. In this paper, we present an overview of the S2 baseband processing system and plans for future implementations of the system, and demonstrate first results of Vela pulsar recordings at Parkes in September 1995. We pay specific attention to the S2-TCI, a system designed to transfer S2 recorded data from tape to computer memory (RAM) via direct memory access (DMA). Computer data may be processed locally or sent to a more powerful "remote" (super) computer for processing.

DSPSR: Digital Signal Processing Software for Pulsar Astronomy

“…The Princeton Mark IV system, capable of continuously 2-bit sampling a 2 Â 10 MHz bandpass (Shrauner 1997;Stairs 1998;Stairs et al 2000), was in use at the Arecibo and Jodrell Bank observatories. At Parkes, baseband recorders included the Wide Bandwidth Digital Recording (WBDR) system, capable of recording a 2 Â 50 MHz bandpass (Jenet et al 1997); the S2 VLBI recorder, a 2 Â 16 MHz system (Wietfeldt et al 1998); and the Caltech Parkes Swinburne Recorder (CPSR; van Straten et al 2000;van Straten 2003), a 2 Â 20 MHz version of the Caltech Baseband Recorder (CBR) at Arecibo. Each of the above systems recorded the baseband signal to magnetic tape for transport and offline analysis on high-performance computing resources.…”

Removal of the GLONASS C/A Signal from OH Spectral Line Observations Using a Parametric Modeling Technique

“…The resulting bandpass was 8 MHz wide centered at 1610 MHz. The data were then extracted using the S2TCI system (Wietfeldt et al 1998) and demultiplexed. This data set and others are freely available .…”

Base Band Data for Testing Interference Mitigation Algorithms

“…In both cases, the data were recorded using three S2 recorders (Cannon et al 1997), allowing a total recording rate of 384 Mb s −1 . The data were extracted from the S2 tapes using the s2tci system (Wietfeldt et al 1998), demultiplexed and stored on DLT and CD media. Table 2 summarises the data collected.…”