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From: | Lamar Owen |
Subject: | Re: [Discuss-gnuradio] Pulsar detection success |
Date: | Mon, 25 Sep 2006 01:01:11 -0400 |
User-agent: | KMail/1.9.4 |
On Monday 25 September 2006 00:45, Marcus Leech wrote: > I got word from Lamar Owen this evening that PARI were successful in > using my gnuradio-based pulsar monitor > software along with the excellent USRP + TV_RX hardware to detect and > monitor the pulsar B0950+08, which > has a pulse rate of 3.95Hz. I can't be sure from the trace, but I > *think* they detected the much-weaker inter-pulse > as well. I'll post some captures of the screen.. hmm, if the list will take attachments, here are the clearest traces.... All are of B0950+08, one of the brightest pulsars in the sky, and one with a low dispersion measure. The receive antenna was PARI's East 26 meter radio telescope (see the PARI website for pictures and such) with a cross-dipole-in-a-bucket standard feed at the prime focus, centered on 327MHz. The coax run from the dipole to the first LNA is about three feet; the first LNA is an Angle Linear unit, driving a second broadband Minicircuits amp. This drives the 400+ foot RG214 cable run down to the control room, where it is a straight patch through a lightning arrestor panel to the TVRX input. PC is a Dell PowerEdge 2850 dual Xeon 3.0GHz; CPU utilization at 2MHz bandwidth is around 60% of one CPU. Time to go to bed... -- Lamar Owen Director of Information Technology Pisgah Astronomical Research Institute 1 PARI Drive Rosman, NC 28772 (828)862-5554 www.pari.edu
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