PA1ASB has been active recently on VLF and on his site he has a grabber showing what signals he has/is copying around 8.270kHz which is the new favoured spot. This is below 8.3kHz and so falls in the unallocated part of the spectrum as 8.970kHz is now within the spectrum reserved for sferics research. Most amateur VLF TX stations are now operating around 8.270kHz. Here in the UK I believe it is legal for ANYONE to TX below 8.300kHz as long as no harmful interference is caused to allocated services above 8.300kHz. This is my view, not a legal statement. I have asked OFCOM to clarify.
Also of note on these pages are the .SDR configuration files for Spectrum Lab software. It is ESSENTIAL to use Spectrun Lab or very similar software to detect anything at any range. See http://www.qsl.net/pa1sdb/index.htm . I suggest that, if you want to build a VLF amateur RX, to base your configuration files on those given on these pages.
My own experience is that 420uHz or less bandwidth is essential to see any trace of amateur VLF signals integrated over many hours. 42uHz is better. In both cases you have to lock to a VLF MSK signal, Russian Alpha beacons or GPS for excellent stability. This is all sorted out with the .SDR file automatically. You may be surprised how stable a RX you can make very simply.
Showing posts with label spectrum laboratory. Show all posts
Showing posts with label spectrum laboratory. Show all posts
29 Jan 2014
5 Mar 2013
More analysis with Spectrum Lab software
Spectran is a very easy package to use but it has its limitations when analysing weak audio signals. A more powerful package is DL4YHF's Spectrum Laboratory which is an extremely powerful piece of software. The problem is that if I've not used it for months it takes me hours to remember how to drive it. A secret is to store ".usr" configuration files so one can go back instantly to a set of settings e.g. a given frequency to analyse with a specified bandpass filter and bandwidth.
Anyway, to cut a long story, this evening I set up some config files to allow me to look again at the recordings of my 8.9775kHz VLF earth-mode signals made during recent drive around tests locally. Although the original analysis was done at 180mHz bandwidth I can now replay the recordings and look in bandwidths down to 34mHz. What happens then is that signals present but too weak to see now appear above the noise floor as a faint line. The net result is that the signals can be detected in some of the "in between" locations that were not apparent from the 180mHz (wider!) bandwidth analysis.
I intend to use Spectrum Laboratory and narrow bandwidths for the over-the-horizon 481THz optical tests if Spectran proves not up to the job. However, when bandwidths are very narrow there is a time-lag before the trace appears on the screen. This is less than ideal when trying to align weak optical signals with beamwidths measured in a degree or less. What is needed is an accurate beam heading and then allow the trace to build on the screen. I don't have enough experience yet to know how much beamwidth spread a cloud or free space dust scattered optical signal gets. When looking for G4HJW's signal over the horizon in clear skies last year the alignment was quite critical, but his signal was audible in headphones so the optics could be peaked by ear before analysing with Spectran or Spectrum Lab. I had more luck with my own QRSS3 signal over the horizon on a shorter path, managing to align by eye on visible landmarks enough to see the trace on the PC and then peak it.
Faint line at 8.9775kHz visible at greater range (43mHz bandwidth) |
I intend to use Spectrum Laboratory and narrow bandwidths for the over-the-horizon 481THz optical tests if Spectran proves not up to the job. However, when bandwidths are very narrow there is a time-lag before the trace appears on the screen. This is less than ideal when trying to align weak optical signals with beamwidths measured in a degree or less. What is needed is an accurate beam heading and then allow the trace to build on the screen. I don't have enough experience yet to know how much beamwidth spread a cloud or free space dust scattered optical signal gets. When looking for G4HJW's signal over the horizon in clear skies last year the alignment was quite critical, but his signal was audible in headphones so the optics could be peaked by ear before analysing with Spectran or Spectrum Lab. I had more luck with my own QRSS3 signal over the horizon on a shorter path, managing to align by eye on visible landmarks enough to see the trace on the PC and then peak it.
Labels:
spectran,
spectrum laboratory,
vlf
10 Feb 2013
8.97kHz VLF amateur activity
DJ8WX's VLF signal received by G3ZJO (frequency is Hz) |
Labels:
dj8wx,
g3zjo,
spectrum laboratory,
vlf
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