Return-Path: Received: (qmail 4582 invoked from network); 29 Jan 2000 13:33:50 -0000 Received: from unknown (HELO post.thorcom.com) (212.172.148.70) by dimple.core.plus.net.uk with SMTP; 29 Jan 2000 13:33:50 -0000 Received: from majordom by post.thorcom.com with local (Exim 3.02 #1) id 12EXs7-0000WL-00 for rsgb_lf_group-outgoing@blacksheep.org; Sat, 29 Jan 2000 13:25:03 +0000 Received: from mail.sci.fi ([195.74.0.41] helo=pyyhe.saunalahti.fi ident=root) by post.thorcom.com with esmtp (Exim 3.02 #1) id 12EXs5-0000WG-00 for rsgb_lf_group@blacksheep.org; Sat, 29 Jan 2000 13:25:02 +0000 Received: from DCXLIII.hdyn.saunalahti.fi (DCXLIII.hdyn.saunalahti.fi [195.74.25.43]) by pyyhe.saunalahti.fi (8.9.1/8.9.1) with SMTP id PAA06800 for ; Sat, 29 Jan 2000 15:35:29 +0200 (EET) X-Priority: 3 X-MSMail-Priority: Normal From: "Paul Keinanen" To: rsgb_lf_group@blacksheep.org Subject: Re: LF: Long integration times X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 Date: Sat, 29 Jan 2000 15:26:50 +0200 Message-ID: References: <38920EA4.B3A3F5A9@bellatlantic.net> <3892A61A.C049A749@virgin.net> In-reply-to: <3892A61A.C049A749@virgin.net> X-Mailer: Forte Agent 1.7/32.534 MIME-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 8bit Precedence: bulk Reply-To: rsgb_lf_group@blacksheep.org X-Listname: rsgb_lf_group Sender: On Sat, 29 Jan 2000 08:34:34 +0000, Stewart Bryant wrote: >For some time I have been thinking of setting up a remote receiver >in a quite location linked back to a more conveniently located >transmitter location. This would be an interesting extension. There >are however some licensing issues. > >The obvious first stage would be to use a radio link, but that would >require licensing. Unfortunately the obvious band to use would be >70cms (quiet, low occupancy, reasonable range cheap equipment) >but it will be very difficult to get a permit, and then on top of that >an NoV will be required to relay the signals. > >The alternative would be to use the Internet or the telephone, but >ironically our administration which is ostensibly promoting the linking >of amateur radio and the Internet has just changed our license to >require government approval to connect our stations to an public >network. I have not seen the wording of your regulations, so this is just a guess, but did't you say you only wanted to move the receiver to a remote location. Assume that you have connected the receiver to a modified answering machine and you are calling your answering machine to listen to the signal and tune the receiver using the answering machine control functions. I don't understand how that remote receiver could be considered an amateur radio station (although the receiver can tune one or more amateur bands) since no transmitter is present at the remote location. There may be regulations against connected modified answering machines to the telephone network, but a computer with a receiver and auto answer modem could be constructed from type approved parts, but unfortunately, after introduction of the computer to a quiet place, it would no longer be a quiet place :-). >One approach that we could take is to record the sampled signals >for a long period with GPS timing markers, and post analyse. There >may be some stuff we can borrow from the SETI folks here. If you have two or more reception sites, you could do some aperture synthesis by postprocessing received data in a similar way as radio telescopes are used in VLBI. This requires accurate timing marks at each receiver site in order to generate various antenna patterns. A long time ago, there was a long discussion in some sci.space... newsgroup with the title "Amateur VLBI" or something similar about the feasibility of establishing a continent wide VLBI network to get some usable angular resolution for upper HF/VHF with small backyard antennas. The problem with only a few (2-3) antennas several wavelength distance from each other is that it will produce a combined radiation pattern with a lot of narrow "fingers", i.e. several very narrow peaks and nulls in the radiation pattern. With more stations, the undesired peaks can be suppressed and only a single strong and narrow peak will remain. Unfortunately this requires a lot of stations. In VLBI, the rotation of the Earth will constantly change the positions relative to the source and assuming the emission of the source does not change, the new relative position is considered a new synthesised station and with properly phase and amplitude settings the received signal is added into the correlator. For LF reception and beam synthesis, there is not much point in having very narrow beams, so several stations within a 10 km radius could be used to generate a beam of about 5 degrees, with a radical reduction of (far field) noise, mainly QRN, coming from other direction, thus increasing the SNR. With such a small geographical area, synchro- nisation would not bee too difficult, even the power grid or a local TV station would be sufficient to provide common phase reference to all receivers. For larger geographical areas any geostationary TV- transponder visible on all ground stations could be used. With the received signal recorded on one channel of the sound card and the reference signal on the other channel, there is no need to synchronise the sampling rate at each station, thus existing hardware can be used. While most of these ideas above are not feasible in practice, I hope they will inspire someone else to find more practical solutions. Paul OH3LWR