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PSR-detection

Source (software & hardware) for PSR detection

Software

RFI analysis

  • CygnusRFI for frequency-domain search.
  • VIRGO for time-domain analysis.

PSR data acquisition & pre-processing

  • PSR channelizer (GNU Radio flowgraph that performs real-time digital signal processing and writes the data directly to a filterbank-formatted file for further processing & analysis with e.g. PRESTO). To be uploaded.

PSR data analysis

  • PRESTO for de-dispersion and folding (DM-search and P-search also used).
  • Potentially a variation of simpleReader in the future for further feature support.

Hardware

*Installed inside a custom-built double-shielded Faraday cage for EMI mitigation and EMC maximization.

RFI mitigation from hardware

For EMI suppresion (spurious emission reduction), two Faraday cages were considered: one that had a single layer of shielding, and one that had a double layer of shielding (custom-built with two fans for heat dissipation). For a sample frequency of 460 MHz, preliminary EMI tests (conducted with CygnusRFI) have given the following results: Preliminary EMI Test Results

The apparent inconsistency appears to be due to SDR noise floor variability with time (e.g. SDR temperature (T) is proportional to the system noise temperature (T_sys) and dT/dt ≠ 0). Therefore, because the measurements were taken at slightly different times (waiting for each measurement to finish), the noise floor varies (T ∝ T_sys ∧ dT/dt ≠ 0 ∴ dT_sys/dt ≠ 0)). Besides internal factors, T_ant variability (caused by DUT-unrelated RFI) may also have a significant impact.

Further EMC updates

Further preliminary EMI checks, this time on a different receiving computer candidate: EMI Check

Reference level

EMI Source (DUT under suspicion) out of the antenna's beam (equivalent to turning it off): EMI Check

EMI Source in front of the beam

EMI Check

Narrower span

EMI Check

Pulse profile span

EMI Check

More to be added soon...

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Source (software & hardware) for Pulsar detection

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