Return-Path: Received: from mtain-dc02.r1000.mx.aol.com (mtain-dc02.r1000.mx.aol.com [172.29.64.130]) by air-dc05.mail.aol.com (v128.1) with ESMTP id MAILINDC051-86014bc6d364298; Thu, 15 Apr 2010 04:50:44 -0400 Received: from post.thorcom.com (post.thorcom.com [193.82.116.20]) by mtain-dc02.r1000.mx.aol.com (Internet Inbound) with ESMTP id BC72638000099; Thu, 15 Apr 2010 04:50:42 -0400 (EDT) Received: from majordom by post.thorcom.com with local (Exim 4.14) id 1O2KlH-0003XU-CS for rs_out_1@blacksheep.org; Thu, 15 Apr 2010 09:49:23 +0100 Received: from [193.82.116.32] (helo=relay1.thorcom.net) by post.thorcom.com with esmtp (Exim 4.14) id 1O2KlG-0003XL-QT for rsgb_lf_group@blacksheep.org; Thu, 15 Apr 2010 09:49:22 +0100 Received: from imr-da03.mx.aol.com ([205.188.105.145]) by relay1.thorcom.net with esmtp (Exim 4.63) (envelope-from ) id 1O2Kl7-0007xt-S5 for rsgb_lf_group@blacksheep.org; Thu, 15 Apr 2010 09:49:22 +0100 Received: from mtaout-da05.r1000.mx.aol.com (mtaout-da05.r1000.mx.aol.com [172.29.51.133]) by imr-da03.mx.aol.com (8.14.1/8.14.1) with ESMTP id o3F8n25b008992 for ; Thu, 15 Apr 2010 04:49:02 -0400 Received: from Black (g229148092.adsl.alicedsl.de [92.229.148.92]) by mtaout-da05.r1000.mx.aol.com (MUA/Third Party Client Interface) with ESMTPA id C7B6CE000201 for ; Thu, 15 Apr 2010 04:49:00 -0400 (EDT) Message-ID: From: "Markus Vester" To: References: <000c01cadbca$b43bdfe0$6d01a8c0@DELL4> In-Reply-To: <000c01cadbca$b43bdfe0$6d01a8c0@DELL4> Date: Thu, 15 Apr 2010 10:48:34 +0200 MIME-Version: 1.0 X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Windows Mail 6.0.6000.16480 X-MimeOLE: Produced By Microsoft MimeOLE V6.0.6000.16669 X-AOL-VSS-INFO: 5400.1158/57478 X-AOL-VSS-CODE: clean X-Spam-Score: 0.0 (/) X-Spam-Report: autolearn=disabled,HTML_MESSAGE=0.001 Subject: LF: Re: VLF...alpha long selective fade? Content-Type: multipart/mixed; boundary="----=_NextPart_000_002C_01CADC89.32006F40" X-Spam-Checker-Version: SpamAssassin 2.63 (2004-01-11) on post.thorcom.com X-Spam-Level: X-Spam-Status: No, hits=0.6 required=5.0 tests=HTML_20_30,HTML_MESSAGE, MISSING_OUTLOOK_NAME 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-global-disposition: G X-AOL-VSS-INFO: 5400.1158/57478 X-AOL-VSS-CODE: clean x-aol-sid: 3039ac1d40824bc6d3621e1f X-AOL-IP: 193.82.116.20 ------=_NextPart_000_002C_01CADC89.32006F40 Content-Type: multipart/alternative; boundary="----=_NextPart_001_002D_01CADC89.32009650" ------=_NextPart_001_002D_01CADC89.32009650 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: quoted-printable Dear Jay, thanks for posting this interesting screenshot. The fine structure in the spectrum is superposition of the three sourc= es, transmitting coherently on the same frequency but occupying differ= ent time slots 0.6 s apart. The scheme of the 3.6 s repeating frames= is currently: 0 3.6 s +-----------+=20 |K E N N*. .| 14.881 kHz |. N E K . .| 12.649 kHz |N . K E . .| 11.905 kHz +-----------+ K =3D Krasnodar (West) N =3D Novosibirsk (Center)=20 E =3D Khabarovsk (Far East) * second dash from N on 14.881 has alternating phase The mechanism is similar to selective fading, but the delay involved= is not from propagation but from the (much longer) transmitter delay.= If you were for example getting only N and K, the two dashes 1.2 seco= nds apart would result in a 0.83 Hz periodic ripple in the spectral en= velope. As the transmitters are laid out on a ~ 6000 km baseline, the componen= ts will have different diurnal phase variations, resulting in a slow= movement of the minima in the spectrogram. If the later component is= lagging more, the ripple pattern moves down in frequency (ie. contrac= ts towards zero). The plot appended here shows the three signals separated in time domai= n, as observed here on Mar. 20. The idea behind this was to get more= data for a simple model for propagation loss, and I was expecting som= ething along the lines of 1/sqrt(r) and -2 to -3 dB/Mm.=20 But the pattern appears to be much more complex. For example, at 11.9= and 12.6 kHz, nighttime fieldstrength from Novosibirsk at 5 Mm actual= ly exceeds that from Krasnodar at 2 Mm (ie. the red and green thin lin= es go above the thick lines). This is not the case at 14.8 kHz (blue).= Also, the 8 Mm path from Khabarovsk exhibits an unexpectedly deep day= time minimum. There are more plots in http://df6nm.bplaced.net/VLF/Alp= ha/ , showing that level and phase patterns are essentially repeating= every day. The results seem to indicate that a fieldstrength prediction for long= ranges would seem feasible in principle, but one would have to includ= e interference between groundwave and multiple waveguide modes. There= may be favourable and unfavourable combinations of distance and frequ= ency, which (unlike at HF) are rather fixed and will not be averaged= out by slight ionospheric movements. This is also pointed out by an= older dual-frequency observation of DHO at 475 km: http://freenet-homepage.de/df6nm/vlf/vlf_DHO_dualfreq.htm . Kind regards, Markus (DF6NM) ----- Original Message -----=20 From: jrusgrove@comcast.net=20 To: rsgb_lf_group@blacksheep.org=20 Sent: Wednesday, April 14, 2010 2:04 PM Subject: LF: VLF...alpha long selective fade?=20 Been monitoring / plotting the alpha stations over the past couple= weeks while working to improve=20 the VLF receiving setup. The following very slow 'selective fade' ha= s been seen every night that=20 I've looked (4 times) so it's not a one off occurrence. Anyone care= to speculate on what would cause=20 this? Full screen here: http://www.w1vd.com/capture/alphafade1.jpg . Conde= nsed version as an attachment. Jay W1VD WD2XNS WE2XGR/2=20 ------=_NextPart_001_002D_01CADC89.32009650 Content-Type: text/html; charset="iso-8859-1" Content-Transfer-Encoding: quoted-printable
Dear Jay,
 
thanks for posting this interesting= =20 screenshot.
 
The fine structure in the=20 spectrum is superposition of the three sources, transmi= tting=20 coherently on the same frequency but occupying different time slo= ts 0.6 s=20 apart. The scheme of the 3.6 s repeating frames is currently:
 
0    &n= bsp;     3.6=20 s
+-----------+ |K E=20 N N*. .|  14.881 kHz
|. N E K . .|  12.649=20 kHz
|N . K E . .|  11.905=20 kHz
+-----------+
 
K =3D Krasnodar (West)
N =3D Novos= ibirsk (Center)=20
E =3D Khabarovsk (Far East)
 * second dash from N on 14.881= has=20 alternating phase
The mechanism is similar=20 to selective fading, but the delay involved is not from prop= agation=20 but from the (much longer) transmitter delay. If you were for exa= mple=20 getting only N and K, the two dashes 1.2 seconds apart would resu= lt in a=20 0.83 Hz periodic ripple in the spectral envelope.
 
As the transmitters are laid out on= a ~ 6000 km=20 baseline, the components will have different diurnal phase variations,= resulting=20 in a slow movement of the minima in the spectrogram. If the later= component=20 is lagging more, the ripple pattern moves down in frequency (ie. contr= acts=20 towards zero).
 
The plot appended here shows the=  three=20 signals separated in time domain, as observed here on Mar.= =20 20. The idea behind this was to get more data=  for=20 a simple model for propagation loss, and I was expecting som= ething=20 along the lines of 1/sqrt(r) and -2 to -3 dB/Mm.
 
But the pattern appears to be&nb= sp;much more=20 complex. For example, at 11.9 and= 12.6 kHz,=20 nighttime fieldstrength from Novosibirsk at 5 Mm actually exceeds that= from=20 Krasnodar at 2 Mm (ie. the red and green thin lines go above the thick= lines).=20 This is not the case at 14.8 kHz (blue). Also, the 8 Mm path from Khab= arovsk=20 exhibits an unexpectedly deep daytime minimum. There are more plots in http:/= /df6nm.bplaced.net/VLF/Alpha/ , showing that=20 level and phase patterns are essentially repeating every day.
 
The results seem to indicate that a= fieldstrength=20 prediction for long ranges would seem feasible in principle, but one= would have=20 to include interference between groundwave and multiple waveguide mode= s.=20 There may be favourable and unfavourable combinations of dis= tance and=20 frequency, which (unlike at HF) are rather fixed and will not be avera= ged out by=20 slight ionospheric movements. This is also pointed out by an= =20 older dual-frequency observation of DHO at 475 km:
 
Kind regards,
Markus (DF6NM)
 
 
----- Original Message -----
Sent: Wednesday, April 14, 20= 10 2:04=20 PM
Subject: LF: VLF...alpha long= selective=20 fade?

Been monitoring /= plotting the=20 alpha stations over the past couple weeks while working to improve=
the VLF=20 receiving setup. The following very slow 'selective fade' has been= seen every=20 night that
I've looked (4 times) so it's not a one off occurrenc= e. Anyone=20 care to speculate on what would cause
this?

Full screen= here: http= ://www.w1vd.com/capture/alphafade1.jpg=20 . Condensed version as an attachment.

Jay W1VD  WD2XNS&n= bsp;=20 WE2XGR/2
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