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21. RE: LF: AW: 477.7 kHz CW (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Sun, 18 Jan 2015 22:30:15 +0000
Hi Joe, I just tuned to 477.7 and your signal is visible but not (yet) audible. QRN is worse than last nght. 73, Rik OR7T ________________________________________ Van: owner-rsgb_lf_group@blacksheep.
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-01/msg00386.html (12,591 bytes)

22. RE: LF: AW: 477.7 kHz CW (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Sun, 18 Jan 2015 22:35:11 +0000
VO1NA now popping out of the noise, 429 for a short period. 73, Rik OR7T ________________________________________ Van: [email protected] [[email protected]] namens R
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-01/msg00387.html (13,062 bytes)

23. RE: LF: AW: 477.7 kHz CW (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Sun, 18 Jan 2015 23:05:24 +0000
Hello Joe, your signal was audible for some minutes, but after that down in the noise again. I have to get out of bed at 05:30 UTC tomorrow, so I'm QRT now. 73, Rik OR7T _____________________________
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-01/msg00390.html (14,237 bytes)

24. RE: LF: OP8 477KHz 500K + in last 24 H (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Fri, 23 Jan 2015 17:32:05 +0000
Hi Stefan, I'm afraid you don't understand how excellent the deep search function of opera is: even if your ERP is 0 W your signal is detected thousands km away. SNR has become irrelevant. We just ha
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-01/msg00410.html (125,532 bytes)

25. LF: RE: CQ OR7TK (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Fri, 23 Jan 2015 22:56:08 +0000
CQ OR7T K Van: [email protected] [[email protected]] namens Graham [[email protected]] Verzonden: vrijdag 23 januari 2015 23:28 Aan: [email protected]
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-01/msg00418.html (9,399 bytes)

26. LF: RE: comparison OP8 477KHZ opds(DF6NM)--OPERA 1.5.6 LAST NIGHT (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Sat, 24 Jan 2015 10:06:03 +0000
Hello Dionysios, thanks for the very interesting comparisation. If the decodes from Costas are removed (at 7km his signal must be S9+++) it looks like this: sv8rv km07ks Opera-8 477khz correlation (D
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-01/msg00427.html (13,397 bytes)

27. LF: RE: RL aerial (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Thu, 29 Jan 2015 07:53:45 +0000
Hello Joe, I just simulated the antenna with MMANA-GAL and it resulted in Z = 1.57-j185.5 Ohm. So the antenna C would be about 1.8 nF. However a 50 uH loading coil point to 2.2 nF antenna capacitance
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-01/msg00480.html (18,995 bytes)

28. LF: RE: Distance record (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Fri, 6 Feb 2015 17:36:16 +0000
Hello Fausto, what are you looking for: - QSO or just one-way copy? - mode? Just to give you an idea, my distance records on MF (2-way QSO): CW = 1849km (9H9ES) QRSS3 = 4073km (VX9MRC) JT9-2 = 1851km
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-02/msg00056.html (11,617 bytes)

29. LF: RE: WSPR 630m (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Tue, 17 Feb 2015 09:53:15 +0000
Hello Roelof, I had half a dozen decodes of WG2XJM too. But this is still peanuts compared to the 2009-2011 winters where I could often copy the US stations as early as 22 UTC and as late as 7 UTC. L
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-02/msg00182.html (17,401 bytes)

30. RE: LF: Todays monitor size (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Sat, 28 Feb 2015 12:48:43 +0000
Hi Stefan, not sure that all devices will adapt the picture size automatically, but it requires only a few lines of _javascript_ code to adapt the picture size to the monitor resolution. 73, Rik ON7Y
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-02/msg00274.html (12,873 bytes)

31. LF: RE: MF (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Fri, 6 Mar 2015 11:11:01 +0000
Hello Fausto, CW activity is dropping compared to mid-winter but I still hear many stations. Heard the past days: DL: DJ6CB, DF5QG, DL6TY PA: PA3FUN, PA0HTT, PE5T G: G3XIZ, G3KEV GW: GW3UEP SM: SM4WI
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-03/msg00053.html (13,755 bytes)

32. RE: LF: Activity etc. - DG3LV discussion -One year later (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Fri, 13 Mar 2015 09:23:28 +0000
Hi Stefan, Tobias, all, so far I made 130 QSO's on 472kHz: CW: 88 (68%) JT9: 35 (27%) QRS: 4 (3%) WSQ: 3 (2%) But is the average distance for CW os "only" 477km while it is 1180km for the other modes
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-03/msg00152.html (16,595 bytes)

33. LF: RE: EI0CF (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Wed, 18 Mar 2015 09:15:37 +0000
Hi Fausto, [email protected] 73, Rik ON7YD - OR7T Van: [email protected] [[email protected]] namens Fausto Coletti [[email protected]] Verzonden: woensdag 18
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-03/msg00220.html (11,813 bytes)

34. RE: LF: Eclipse/137.777 kHz (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Fri, 20 Mar 2015 16:39:48 +0000
Hi Peter, I am not sure that the morning dip is related to the eclips, the propagation path didn't cross the eclips line at any time. Looking at the graphs, knowing there was an eclpis but not knowin
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-03/msg00248.html (19,193 bytes)

35. RE: LF: TXing WSPR on 630m on a Raspberry Pi, Stefan in QRP... (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Fri, 27 Mar 2015 09:29:00 +0000
Hi Stefan, solid signal here, best decode was at -8dB! 73, Rik ON7YD - OR7T Van: [email protected] [[email protected]] namens DK7FC [[email protected]] Verzonde
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-03/msg00302.html (17,350 bytes)

36. RE: LF: Re: TXing WSPR on 630m on a Raspberry Pi, Stefan in QRP... (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Fri, 27 Mar 2015 13:43:28 +0000
Hi Stefan, all, And i wrote an email to PE1NNZ and asked to a modification of the C-program to generate a signal with 4x higher FSK shift. Then it it would be possible to use that version for OMs hav
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-03/msg00312.html (16,966 bytes)

37. RE: LF: Re: TXing WSPR on 630m on a Raspberry Pi, Stefan in QRP... (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Fri, 27 Mar 2015 15:26:46 +0000
Hi Stefan, sri, no RF output. Just a audio signal (+/- 1500Hz) via the sound card. It is intended to be used with a HF TRX (most of them will not transmit below 1.8MHz) and then divide the (attenuate
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-03/msg00316.html (16,442 bytes)

38. LF: only today ... (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Wed, 1 Apr 2015 11:55:01 +0000
completely off topic, but good: http://home.web.cern.ch/about/updates/2015/04/cern-researchers-confirm-existence-force 73, Rik ON7YD - OR7T
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-04/msg00003.html (11,522 bytes)

39. RE: LF: only today ... (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Wed, 1 Apr 2015 13:44:59 +0000
Joe, give it a try! But be aware that the top-load will collapse at 01-04-2015 23:59:59 UTC ;-) 73, Rik Van: [email protected] [[email protected]] namens jcraig@mun.
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-04/msg00006.html (18,369 bytes)

40. LF: RE: Schumann Frequenz (score: 1)
Author: Rik Strobbe <[email protected]>
Date: Fri, 17 Apr 2015 13:48:09 +0000
Hello Uwe the Schumann resonance is determined by 1. radius of the earth 2. speed of light 3. density of the ionosphere As 1. and 2. can be considered constant a raise of the Schumann resonance (by 3
/rsgb_lf_group-archives/html/rsgb_lf_group/2015-04/msg00121.html (14,751 bytes)


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