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From: | Marcus Leech |
Subject: | Re: [Discuss-gnuradio] Re: USRP / DBSRX calibration |
Date: | Thu, 08 May 2008 12:03:23 -0400 |
User-agent: | Mozilla/5.0 (X11; U; Linux i686; en-US; rv:1.7.12) Gecko/20060130 Red Hat/1.7.12-1.4.2 |
Staffan Josefsson wrote:
The MAX2118 chip that is used to do the downconversion has a very high noise figure--10dB. The DBS_RX board has a GaAsFET amplifier in front of it. which has a roughly 0.9dBHi.I'm trying to estimate the noise temperature in the DBSRX and USRP as a part of a student project where we compare the USRP as an alternative for the receiver in a radio telescope. I tried to convert the -165dBm/Hz to Kelven but I'm not getting a sane value. I may be way out here but would be very pleased to find out what the noise temperature might be, in Kelvin.Thanks Staffan Josefsson
noise figure.Unless you have the DBS_RX right at the receive horn, you'll need your own LNA chain in front of the DBS_RX. Go with an LNA with the lowest noise figure you can afford. The LNAs produced by Radio Astronomy Supplies are pretty good, and there's a fellow in Switzerland who produces semi-custom LNAs for the 21cm band that are really well built. I use three LNAs in series in my system--all from Down East Microwave. My first LNA is attached directly to the feedhorn, followed by a ceramic filter cut for 1420Mhz, followed by another pair of LNAs--I did it this way because I had a lot of feedline to drive, and certainly you could get away with less front-end gain. But your first low-noise amplifier element had better be right at the feedhorn--no feedline (high-quality RF connectors between the feedhorn and the first LNA are OK, but keep them to an absolute minimum).
My overall system temperature with this setup was about 95K. -- Marcus Leech Mail: Dept 1A12, M/S: 04352P16 Security Standards Advisor Phone: (ESN) 393-9145 +1 613 763 9145 Strategic Standards Nortel Networks address@hidden
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