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References: [ +subject:/^(?:^\s*(re|sv|fwd|fw)[\[\]\d]*[:>-]+\s*)*VLF\:\s+EbNaut\s+8270\.1\,\s+Sunday\s+Mar\s+20\s*$/: 9 ]

Total 9 documents matching your query.

1. Re: VLF: EbNaut 8270.1, Sunday Mar 20 (score: 1)
Author: "Markus Vester" <[email protected]>
Date: Sun, 20 Mar 2016 09:42:09 +0100
Another repeat will be running 9:00:02 until 10:25:22. 73, Markus From: Markus Vester Sent: Sunday, March 20, 2016 8:15 AM To: [email protected] Subject: Re: VLF: EbNaut 8270.1, Sunday Mar
/rsgb_lf_group-archives/html/rsgb_lf_group/2016-03/msg00284.html (14,155 bytes)

2. Re: VLF: EbNaut 8270.1, Sunday Mar 20 (score: 1)
Author: "Markus Vester" <[email protected]>
Date: Sun, 20 Mar 2016 11:51:00 +0100
Both EbNaut sequencies went out ok on 8270.1 Hz. I'll leave the carrier on 8270.0025 for a couple of hours to see whether the phase is stable now after the GPS antenna has been repositioned, and whet
/rsgb_lf_group-archives/html/rsgb_lf_group/2016-03/msg00290.html (15,354 bytes)

3. Re: VLF: EbNaut 8270.1, Sunday Mar 20 (score: 1)
Author: Paul Nicholson <[email protected]>
Date: Sun, 20 Mar 2016 12:45:56 +0000
And both came in ok here, 07:10:02 Eb/N0 = 2,0 dB from BER 33.8%, carrier 2.6 dB; 09:00:02 Eb/N0 = 1.7 dB from BER 34.2%, carrier 1.1 dB; Your messages almost always decode here, a very reliable sign
/rsgb_lf_group-archives/html/rsgb_lf_group/2016-03/msg00291.html (10,448 bytes)

4. Re: VLF: EbNaut 8270.1, Sunday Mar 20 (score: 1)
Author: "Markus Vester" <[email protected]>
Date: Sun, 20 Mar 2016 18:21:33 +0100
Very fine again Paul, thanks for the report. Looks like DJ8WX has also fired up on 8270.000 Hz this afternoon. Rotating the pointer on your directional spectrogram allows us to toggle between your lo
/rsgb_lf_group-archives/html/rsgb_lf_group/2016-03/msg00293.html (12,432 bytes)

5. Re: VLF: EbNaut 8270.1, Sunday Mar 20 (score: 1)
Author: Paul Nicholson <[email protected]>
Date: Sun, 20 Mar 2016 20:02:45 +0000
The phase doesn't look very steady Markus. Below are 10 minute averages, stepping 5 mins and the timestamp is the start time of each window. 2016-03-20_10:30:00 0.02 fT -94.4 deg 2016-03-20_10:35:00
/rsgb_lf_group-archives/html/rsgb_lf_group/2016-03/msg00295.html (13,948 bytes)

6. Re: VLF: EbNaut 8270.1, Sunday Mar 20 (score: 1)
Author: "Markus Vester" <[email protected]>
Date: Sun, 20 Mar 2016 22:15:18 +0100
Thanks Paul for the measurements. Hmm, it's a bit disappointing, especially as I don't know the cause for the variation. From here, it appeared that the PLL was nicely in lock every time I looked, an
/rsgb_lf_group-archives/html/rsgb_lf_group/2016-03/msg00296.html (16,507 bytes)

7. Re: VLF: EbNaut 8270.1, Sunday Mar 20 (score: 1)
Author: Markus Vester <[email protected]>
Date: Mon, 21 Mar 2016 09:39:12 -0400
Paul, maybe the explanation is that with 10 minute averages my signal is just too close to the noise. Plotting your data as complex numbers seems to show a fairly Gaussian distribution around a globa
/rsgb_lf_group-archives/html/rsgb_lf_group/2016-03/msg00304.html (17,133 bytes)

8. Re: VLF: EbNaut 8270.1, Sunday Mar 20 (score: 1)
Author: Paul Nicholson <[email protected]>
Date: Wed, 23 Mar 2016 20:55:05 +0000
You're right. I confirmed this by injecting an artificial carrier into the VLF recording at 8271.0025 at the same average strength as your signal, then running this signal through the same process. T
/rsgb_lf_group-archives/html/rsgb_lf_group/2016-03/msg00320.html (10,834 bytes)

9. Re: VLF: EbNaut 8270.1, Sunday Mar 20 (score: 1)
Author: "Markus Vester" <[email protected]>
Date: Wed, 23 Mar 2016 23:46:33 +0100
Thanks again Paul for the effort. The result does make sense now. The one-hour averages seem to show a slow trend towards negative (retarded) phase after 15 UT, which may be caused by decreasing sola
/rsgb_lf_group-archives/html/rsgb_lf_group/2016-03/msg00322.html (13,312 bytes)


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