Hi Stefan - thats good news.
Typically I found (averaging) HGA22 5-10dB stronger than DCF39 in North and Central China and still the same variation in Malaysia (E+W), Indonesia and Singapore. With some of those paths still being affected by the sun; my most Northern sub "Polar" point was typically Perm/Kiev. For Eu to Japan your just about hitting the Arctic circle on the Gt Circle so more affected by these pesky Protons. Over here in Okie I dont see much difference and think DCF39 is a little stronger but not dont any quantative measurement over ds/dt.
The overnight screen in Alaska looked a lot more "active" than the bland flat screen days with high Proton count. Fingers crossed for continued improvement in the Dst.
ZL1BPU DDS
Again thanks for those pointing me to the ZL1BPU AVR prog software - Im on line with the "new" DDS using a 16.8MHz ref and seeing how clean it is to run at 475kHz...looks like occasional sluggishness from the AVR chip running directly from the so may square up with a 4046 from the TCXO. Getting about 15V Pk to Pk after the T3 LFP - with the TC4426 into 50ohms though the sine is a little noiser than I would like.
http://www.qsl.net/k0lr/ZL1BPU%20Exciter/K0LR-version.htm
Laurence KL7UK
remote from Sunny Okie
Date: Mon, 6 Feb 2012 11:45:33 +0100
From:
[email protected]To:
[email protected]Subject: Re: LF: Re: over the N pole improving
Hi Alan,
Yes, the path seems to improve.
I just got a hint that JA7NI reported to have seen my signal again:
| DK7FC |
136.1 |
04 Jan 22:41 |
JA7NI |
"M"at my grabber |
...taken from the DX cluster
Unfortunately i missed to watch his grabber to the stated time. Maybe he will send me a capture...
