Involved people at OAB: D'Amico, Innocenti
The new pulsar data acquistion system was fully commissioned in 2001. This
system will be used at the italian 32mt dish in Medicina to observe
Pulsar radio sources. Long term timing observations of pulsars give
information about the interior structure of neutron stars and is useful in
the understanding of the evolution of neutron stars. In timing
observations, the radio frequency signal needs to be sampled in the time
and frequency domain, in order to dedisperse and detect the radio pulses.
The radio frequency signal is down converted from the sky frequency of 1.4
or 1.6 GHz into 4 IF bands, each one from 16 to 48 Mhz as required by the
front-end filter bank (two adjacent bands for each circular polarization).
Each IF band is splitted into 32 1MHz bw channels by the filter bank,
square law detected, pass-throw a programmable antialiasing filter, then
digitized at 1 bit and by a fast data link built with CERN S-LINK
interface; data acquired by a Pentium computer with Linux operating system
will be stored on DLT tapes for off-line analysis. Time tag of data
acquired is very important, so all operations are synchronized to UTC time
reference by GPS receiver and sampling rate clock generator is synch to
H-Maser reference.
The parameters of the data acquisition subsystem are:
2 x 64 x 1MHz filter bank (left and right polarization)
designed at Jodrell Bank Observatory GB
128 channel antialiasing filter 2 poles programmable (0.9KHz,
1KHz, 5 Khz, 10Khz)
128 channel low frequency integrator (0.5 Hz) for interference
monitoring system
128 channel 1 bit digitizer
Synch to H-maser UT clock, programmable sampling rate (10uS-100uS)
Femb board (digitizer to slink interface, Fpga xilinx based)
Fast link to Personal computer By E-Slink form Nowoczesna
Elektonica (LSC & LDC) & Pci to S-Link by Incaa
PentiumIII-500MHz 128MB ram, Linux OS Red Hat 6.1
Data storage on DLT tape unit (up to 20GB on a single tape)
GPS Motorola Oncore UT+
The system has been calibrated on a number of know pulsars, using the standard timing software for offline analysis, and has shown good performances, although some issues related to the interference clipping need to be solved.
This work is carried on in collaboration with A. Maccaferri (IRA/CNR).