Return-Path: Received: from rly-mc11.mx.aol.com (rly-mc11.mail.aol.com [172.21.164.95]) by air-mc02.mail.aol.com (v125.7) with ESMTP id MAILINMC021-da74b01b4e63a8; Mon, 16 Nov 2009 15:24:22 -0500 Received: from post.thorcom.com (post.thorcom.com [193.82.116.20]) by rly-mc11.mx.aol.com (v125.7) with ESMTP id MAILRELAYINMC117-da74b01b4e63a8; Mon, 16 Nov 2009 15:24:08 -0500 Received: from majordom by post.thorcom.com with local (Exim 4.14) id 1NA86J-0008GY-Pd for rs_out_1@blacksheep.org; Mon, 16 Nov 2009 20:23:03 +0000 Received: from [193.82.116.32] (helo=relay1.thorcom.net) by post.thorcom.com with esmtp (Exim 4.14) id 1NA86J-0008GP-B7 for rsgb_lf_group@blacksheep.org; Mon, 16 Nov 2009 20:23:03 +0000 Received: from smtp818.mail.ird.yahoo.com ([77.238.189.18]) by relay1.thorcom.net with smtp (Exim 4.63) (envelope-from ) id 1NA86I-0002hh-Fm for rsgb_lf_group@blacksheep.org; Mon, 16 Nov 2009 20:23:03 +0000 Received: (qmail 71388 invoked from network); 16 Nov 2009 20:22:56 -0000 DomainKey-Signature: a=rsa-sha1; q=dns; c=nofws; s=s1024; d=btinternet.com; h=Received:X-Yahoo-SMTP:X-YMail-OSG:X-Yahoo-Newman-Property:Message-ID:From:To:References:Subject:Date:MIME-Version:Content-Type:Content-Transfer-Encoding:X-Priority:X-MSMail-Priority:X-Mailer:X-MimeOLE; b=whPSxUtrV3Bjd1ZbFmMjzaL30TnBQL4chRKHUEHrCN8hPhBzfqqHtR3irsd0pOgffTSwr1Shl4po9Fr+bn5hcSD7AYZ/FI0aU+TRl/Xrv+86YtW+MDEOoPGXObtNSgVb5S+bZYZCsMQReSovflFyaUk9hE5Z2asZcTt6scdFE18= ; Received: from unknown (HELO lark) (alan.melia@213.122.7.126 with login) by smtp818.mail.ird.yahoo.com with SMTP; 16 Nov 2009 20:22:55 -0000 X-Yahoo-SMTP: KHdpK2OswBBXlm4uxknbEiS4uYdJoGknHN90u4K8__lTafnafZg- X-YMail-OSG: tg9KkGEVM1lvPP3Pw.CciqwijFRBBQ0naE4sOidnMlmOKGkuJvNgUpT4Orhgl0qtV4yHth1jccwMIRmESn89BUikYWlIPzuKqt8b.8QaSPY7ykRamGslyutMmdWS9cQ2iGnQLduixbq1F7QY0vqxMFoVDghEZ_nwqPOdjkrbcn3v_1zwq4ZY9TcevcSxyO7f4JWEtWh2nIY7bJtw91aRFse_CEA23IfMhj4gwjCH1v.S4b2g_XzfNnO6tAwa7plhBznJyhqu8MoZWiqcOqzcT_1d2a.wvGa0YvMltzqHmx8ODUGxOK4TWT3UQ_VflLUJTqvnnTR7FdLnpfSbltz5kdytrz2.ytA- X-Yahoo-Newman-Property: ymail-3 Message-ID: <002e01ca66fa$9edc5f20$0900a8c0@lark> From: "Alan Melia" To: References: <626551.33117.qm@web63607.mail.re1.yahoo.com> Date: Mon, 16 Nov 2009 20:21:20 -0000 MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1106 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 X-Karma: unknown: DomainKey-Status: good (testing) X-Spam-Score: 0.3 (/) X-Spam-Report: autolearn=disabled,MAILTO_TO_SPAM_ADDR=0.276 Subject: LF: Re: LEONIDS and propagation Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Spam-Checker-Version: SpamAssassin 2.63 (2004-01-11) on post.thorcom.com X-Spam-Level: * X-Spam-Status: No, hits=1.1 required=5.0 tests=MAILTO_TO_SPAM_ADDR autolearn=no version=2.63 X-SA-Exim-Scanned: Yes Sender: owner-rsgb_lf_group@blacksheep.org Precedence: bulk Reply-To: rsgb_lf_group@blacksheep.org X-Listname: rsgb_lf_group X-SA-Exim-Rcpt-To: rs_out_1@blacksheep.org X-SA-Exim-Scanned: No; SAEximRunCond expanded to false X-AOL-IP: 193.82.116.20 Hi Andy observations over several months by some of the VLF group suggest that whilst there are some radio effects from meteors at low frequencies they are very weak and difficult to be sure of. In general there is no known mechanism for extensive ionisation which can be detected at LF.......however that doesnt say you shouldn't listen for it !!.....just dont be surprised if it is a bit "underwhelming" :-)) The best bet for observing effects are are reflections between 20 and 150Mhz. In Europe, the Graves satellite radar on 140.050 is a good way to watch pings with something like Argo or Spectrum Lab. I guess you could then try to correlate those with LF effects. See a recent paper on Renato's web site www.vlf.it Alan G3NYK ----- Original Message ----- From: "Andy - KU4XR" To: ; ; "Part-15 Yahoo" ; "600 meter group" Sent: Monday, November 16, 2009 5:29 PM Subject: LF: LEONIDS and propagation > ******* Quoting from SPACE.com ******* > > > Circle Nov. 17 on your calendar, for early that morning a moderate to possibly very strong showing of annual Leonid meteor shower is likely. > > The very strong display will favor those living across most of central and eastern Asia. In this region, meteor rates might briefly rise to a few hundred per hour (the time frame for the most intense activity is anticipated sometime around 21:40 GMT). > > A far more modest, but still potentially enjoyable display of a few dozen Leonid meteors per hour is expected to favor North America. In the United States and Canada, eastern observers will be particularly well-positioned for maximum activity, expected sometime between 3:30 and 5:30 a.m. EST, when the radiant of the Leonid shower will be well up in the dark southeastern sky. > > Hello all: > > Probable " D " and " E " layer ionization during meteor shower peak. > interesting propagation could take place at MF anf LF. The effectes will be seen into the VLF regions for those who monitor utility stations. > This would be a good opportunity for GRABBERS to be online if possible, and for WSPR stations to transmit, the WSPR spot database will show the results of any out of the ordinary propagational enhancements, as well as the GRABBERS. > QRSS signals will show the effects of the ionization trails in various > regions as they show up on various grabbers, or by direct captures of > a signal. > WSPR and WOLF modes will possibly show any changes in signals thru > the received data at the monitoring station. > Sporadic enhancement and reception of NDB's may be noticable. > > Good luck to all those who will be trying the PING mode, may you have > lots of QSO's. > > 73 all :::: > > > > Andy - KU4XR - EM75xr - Friendsville, TN. > LOWfer Beacon " XR " @ 185.29866 KHz ( QRSS-60 ) > Coordinates: N: 35* 43' 54" - W: 84* 3' 16" > http://www.myspace.com/beaconxr > > > >