Hello Markus , Wolf and LF'rs ,
If I can allow myself , how I found best in SL against the sferics, it
is a fast AGC behind a narrow filter! to see my configuration at :
http://jpmere.online.fr/Grabber/Setup/Setup.htm . Many Thank Wolf for
your very good software .
73's Jean-Pierre f1afj
Wolf DL4YHF a écrit :
Hello Markus,
Just a suggestion...
Instead (or in addition to?) of the "old" noiseblanker (inside SL's
"DSP" blackbox), try the noise-limiter in the FFT-based filter, with a
small FFT size for the filter. I tried it a few weeks ago at the club
and found it worked even better than the classic noiseblanker. The
trick is to set the limiter values (in the FFT filter control panel)
just a few dB's above your usual noise level. Then everything above
that level will be cut off, before transforming the signal back into
the time domain. Note that this must happen with a low FFT size (256
points or less) to let it react fast enough for sferics. After this,
the signal will be fed to the main spectrum analyser which of course
runs with a larger FFT size (16384 points, plus decimation).
This "spectral limiter" also works nice for other kinds of local QRM
which is "normally not there", and would otherwise spoil the
spectrogram. Of course, when the noise is very strong, it will deafen
the receiver.
If you like, I can search for some screen shots taken in dual-channel
mode (with and without limiter+blanker). They must be somewhere on the
club's "LF computer" ;-)
Cheers,
Wolf .
[email protected] schrieb:
Dear John and LF,
yes my grabber seems to be plagued a lot. Most of the QRN is
currently emanating from the Mediterranan sea area. I believe the
unilateral directivity of the K9AY E-H-loops does help a lot for
Hartmurt and Jean-Pierre. However up to now my own attempts on
H-field reception have always resulted in decreased SNR due to all
sorts of local QRM.
The QRN was probably emphasized a little by the increased dynamic
headroom which was required here to cope with the Budapest telegrams.
Apparently these have also affected the software noise blanker
performance, which I have tried to improve now by inserting a
bandpass filter before the trigger.
Judging by the fat CFH trace last night, LF propagation looks quite
favorable in the aftermath of the recent period of geomagnetic
activity. On the 100 kHz monitor, all stations from the the Far East
Loran chains (including Minami Torishima island) were well visible
this evening.
73 and best wishes
de Markus, DF6NM
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