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LF: Re: Re: VLF...alpha long selective fade?

To: <[email protected]>
Subject: LF: Re: Re: VLF...alpha long selective fade?
From: "Markus Vester" <[email protected]>
Date: Thu, 15 Apr 2010 11:08:50 +0200
In-reply-to: <FF2804421368412F83680BDC35D7A58A@Black>
References: <000c01cadbca$b43bdfe0$6d01a8c0@DELL4> <FF2804421368412F83680BDC35D7A58A@Black>
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Jay,
 
one more remark on the interpretation of your observation: In your image, there is clearly a 1.66 Hz envelope structure. Given the 11.905 kHz sequence [ N . K E . . ], this must be a superposition of K (Krasnodar, presumably across the Atlantic) and E (Khabarovsk, more likely across the Pacific). Apparently the Krasnodar signal is experiencing a phase advance during the observation period, caused by sunrise over Europe and the Atlantic lowering the D-layer.
 
73, Markus
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 seconds apart would result in a 0.83 Hz periodic ripple in the spectral envelope.
 
As the transmitters are laid out on a ~ 6000 km baseline, the components 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. contracts towards zero).
...
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