Return-Path: Received: (qmail 893 invoked from network); 16 Apr 2002 11:48:33 -0000 Content-Transfer-Encoding: 8bit Received: from unknown (HELO murphys-inbound.services.quay.plus.net) (212.159.14.225) by excalibur.plus.net with SMTP; 16 Apr 2002 11:48:33 -0000 X-Priority: 3 X-MSMail-Priority: Normal Received: (qmail 22255 invoked from network); 16 Apr 2002 11:48:29 -0000 Received: from unknown (HELO post.thorcom.com) (212.172.148.70) by murphys.services.quay.plus.net with SMTP; 16 Apr 2002 11:48:29 -0000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 Received: from majordom by post.thorcom.com with local (Exim 3.33 #2) id 16xSts-0003yP-00 for rsgb_lf_group-outgoing@blacksheep.org; Tue, 16 Apr 2002 14:21:36 +0100 Received: from hestia.herts.ac.uk ([147.197.200.9]) by post.thorcom.com with esmtp (Exim 3.33 #2) id 16xStr-0003yK-00 for rsgb_lf_group@blacksheep.org; Tue, 16 Apr 2002 14:21:35 +0100 Received: from gemini ([147.197.200.44] helo=gemini.herts.ac.uk) by hestia.herts.ac.uk with esmtp (Exim 3.22 #1) id 16xRMv-0004z4-00 for rsgb_lf_group@blacksheep.org; Tue, 16 Apr 2002 12:43:29 +0100 Received: from [147.197.232.252] (helo=rsch-15.herts.ac.uk) by gemini.herts.ac.uk with esmtp (Exim 3.33 #1) id 16xRMv-0000y2-00 for rsgb_lf_group@blacksheep.org; Tue, 16 Apr 2002 12:43:29 +0100 Message-ID: <5.1.0.14.0.20020416115856.00aa6008@gemini.herts.ac.uk> X-Sender: mj9ar@gemini.herts.ac.uk X-Mailer: QUALCOMM Windows Eudora Version 5.1 Date: Tue, 16 Apr 2002 12:37:52 +0100 To: rsgb_lf_group@blacksheep.org From: "James Moritz" Subject: RE: LF: Phase meter for propagation experiment In-reply-to: <01C1E536.029E0670.g4jnt@thersgb.net> MIME-Version: 1.0 Content-Type: text/plain; charset=us-ascii; format=flowed Precedence: bulk Reply-To: rsgb_lf_group@blacksheep.org X-Listname: rsgb_lf_group Sender: At 11:01 16/04/2002 +0100, you wrote: >Not sure if the Doppler shift due to orbital wobble will affect the >modulation >in the same way it does carrier frequency. Are there any physicists out >there >who can confirm this ? > >Andy G4JNT > > Dear Andy, LF Group, I'm not a physicist, but it seems to me that however the line sync is modulated onto the satellite signal, a change in the path length to and from the satellite will change the path delay, and so the arrival time of the sync pulse, by 3.3ns per metre. At 15.625kHz, this will cause a change in relative phase of 2pi * 3.3ns/64us, which is 3.3*10e-4 radians per metre of path length. So if the path length changes by 40m/s as Stewart states, the rate of phase change will be 0.013rad/s, or 2.1 millihertz. Multiplied up to 136k, this would be about 0.02Hz as Stewart calculates. How fast is the ionosphere supposed to be moving around? my OCXO reference seems to be stable within a few parts in 10^9 over a short period of time on a good day, and this amounts to a fraction of a metre per second equivalent. So if the effective height of the ionosphere changes by a few 10s of km in a few hours, the frequency/phase change should be detectable without locked oscillators. Cheers, Jim Moritz 73 de M0BMU