Return-Path: Received: (qmail 4897 invoked from network); 5 Aug 1999 10:19:06 +0100 Received: from magnus.plus.net.uk (HELO magnus.force9.net) (195.166.128.27) by guiness.force9.net with SMTP; 5 Aug 1999 10:19:06 +0100 Received: (qmail 17070 invoked from network); 5 Aug 1999 09:22:11 -0000 Received: from unknown (HELO post.thorcom.com) (212.172.148.70) by magnus.plus.net.uk with SMTP; 5 Aug 1999 09:22:11 -0000 Received: from majordom by post.thorcom.com with local (Exim 3.02 #1) id 11CJVn-0003dQ-00 for rsgb_lf_group-outgoing@blacksheep.org; Thu, 05 Aug 1999 10:08:31 +0100 Received: from mserv1c.u-net.net ([195.102.240.33]) by post.thorcom.com with esmtp (Exim 3.02 #1) id 11CJVm-0003dL-00 for rsgb_lf_group@blacksheep.org; Thu, 05 Aug 1999 10:08:30 +0100 X-Priority: 3 X-MSMail-Priority: Normal Received: from rsgb.u-net.com ([195.102.80.225] helo=rsgb.org.uk) by mserv1c.u-net.net with smtp (Exim 2.10 #34) id 11CKPY-0003HZ-00 for rsgb_lf_group@blacksheep.org; Thu, 5 Aug 1999 10:06:10 +0000 Received: from miked.rsgbhq [192.168.2.30] by rsgb.org.uk [192.168.2.132] with SMTP (MDaemon.v2.7.SP5.R) for ; Thu, 05 Aug 1999 09:57:24 +0100 From: "Mike Dennison" X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 Organization: Radio Society of Great Britain To: rsgb_lf_group@blacksheep.org Date: Thu, 5 Aug 1999 09:59:55 +0100 MIME-Version: 1.0 Content-Type: text/plain; charset=US-ASCII; format=flowed Content-Transfer-Encoding: 8bit Subject: Re: LF: eclipse In-reply-to: <199908050140_MC2-7FCF-5F5A@compuserve.com> X-Mailer: Pegasus Mail for Win32 (v3.01d) X-MDaemon-Deliver-To: rsgb_lf_group@blacksheep.org X-Return-Path: miked@mail.rsgbhq Message-ID: Precedence: bulk Reply-To: rsgb_lf_group@blacksheep.org Sender: G3YMC wrote: > The RSGB's programme for studying propogation on the eclipse was in April > 99 RadComm. This suggested various monitoring programmes for 73 and 128 > (sic!) kHz. > Oops - our trusty proof readers didn't spot that one until too late! One of things the article said was that the effects of the eclipse may last a while, especially as the zone of totality changes with the Earth moving. The thing to do it to monitor something consistent (obviously regular amateur skeds would be best, but commercial signals would do) over a period of days, and LF is especially useful for that is under normal conditions the signal strengths are remarkably consistent. So although most of us will either be at work, or enjoying the eclipse away from home, information on DCF's signal in the mornings and evenings will still be useful - even if it does not reveal any changes. Because the totality region moves south-south-east from the UK, I imagine that HBG on 75kHz and the Greek RTTY on 135.8kHz would be more useful than DCF which is too far north. Similarly, observations across the line of totality are thought to be useful, so monitoring DCF from Italy could be the thing to do. That is my understanding of the recommendations - feel free to correct me if I have it wrong. I shall probably arrange to ask my wife to run Spectrogram on 135.8kHz for an hour around eclipse time. I will then record morning and evening signal strengths on as many DX signals (amateur and professional) as I can hear. It would be useful for as many stations as possible to put out a call whenever possible from Monday morning to Thursday morning. It may be especially helpful if anyone can transmit on 73kHz (I will try to do so, despite needing to work most of the weekend - see this group and my web site for an announcement). Mike, G3XDV (IO91VT) http://www.dennison.demon.co.uk/activity.htm