Return-Path: Received: (qmail 5609 invoked from network); 5 Mar 2000 11:56:02 -0000 Received: from unknown (HELO post.thorcom.com) (212.172.148.70) by grants.core.plus.net.uk with SMTP; 5 Mar 2000 11:56:02 -0000 Received: from majordom by post.thorcom.com with local (Exim 3.02 #1) id 12RZVq-0004Wk-00 for rsgb_lf_group-outgoing@blacksheep.org; Sun, 05 Mar 2000 11:47:54 +0000 Received: from smtp1.xs4all.nl ([194.109.127.48]) by post.thorcom.com with esmtp (Exim 3.02 #1) id 12RZVp-0004Wf-00 for rsgb_lf_group@blacksheep.org; Sun, 05 Mar 2000 11:47:53 +0000 Received: from v3q4v1 (dc2-isdn879.dial.xs4all.nl [194.109.151.111]) by smtp1.xs4all.nl (8.9.3/8.9.3) with SMTP id MAA16096 for ; Sun, 5 Mar 2000 12:47:37 +0100 (CET) From: "M. Sanders \(PA3BSH\)" To: rsgb_lf_group@blacksheep.org Subject: LF: RE: CFH plots Date: Sun, 5 Mar 2000 12:40:18 +0100 Message-ID: <000101bf8697$94cb5340$61976dc2@v3q4v1> MIME-Version: 1.0 Content-Type: text/plain; charset=iso-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook 8.5, Build 4.71.2232.26 Importance: Normal X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 In-reply-to: Precedence: bulk Reply-To: rsgb_lf_group@blacksheep.org X-Listname: rsgb_lf_group Sender: Hi All, You can download the software at: http://www.veron.nl/tech/prog/eclipse.htm /// > Thanks are due to ON5OO for writing the monitoring software. Does anyone > have a good copy of the original EXE file? The one I posted on my site > is corrupt and I deleted all other copies - doh! > > -- > Mike, G3XDV /// Congratulatins on the results on 73kHz! The flares seem to have a more or less similar effect on de D-layer as was seen during the '99 eclipse. I am convinced now there are two effects that work independently. 1) Reflection against the bottom of the D-layer. The D-layer lowers when the intensity of the radiation increases. This gives an increase in signal strength because the reflection improves when the angle of indecense decreases. 2) Total internal refraction of LF signals in the D-layer. The ionisation in the D-layer increases and so the signals passing through attennuate. This causes a decrease in signal strength. Both effects are combined in the reflection coefficient formula for 'sky wave' propagation. Observations during the eclipse have shown there is a time difference between the effects 1) and 2). The height appears to change rapidly and the ionisation process appears to take some time before propagation is affected. This time difference causes both the significant increase and decrease of the signals we observe (and we can use the increase for DX communications of course!!). Best 73's and good luck on lf, Michael Sanders, PA3BSH