Hi Markus, it would seem that the majority of the
"hot" precipitated electrons enter the ionosphere at the dawn and dusk edges
where the magnetosphere is distorted by the solar wind pressure. I believe they
enter at high latitudes and diffuse towards the equator. So I am guessing that
if there are any gradients they are pole towards the equator. Certainly there is
evidence from Laurence and Scott VE7TIL that they see propagation collapse
almost immediately after a geomag shock. I dont have any data for worldwide
distribution. In fact the only plottable data is that for the N.Atlantic path to
CFH. The plots from Scott suggest that the decay of the attenuation after a
shock is around 5-6dB/hour . This suggests that when the Equatorial Ring
Current is exhausted the global ionosphere returns to the simple
photo-dissociation model with solar UV activation (what a load of pretentious
rot I just wrote :-)) ) I mean we get an absorbing daylight D-region again
which disappears as soon as it becomes dark. The solar eclipse plots of a few
yeas ago suggest the free daytime electrons recombine in seconds due to the
relatively high pressure 50 to 100km altitude (it would still make you gasp a
bit though :-)) ) and their relatively low energy (just above the
ionisation level)
I wonder if your Loran data would give any
information on worldwide distribution? However I believe most of the Loran
chains are in the Northern Hemisphere (not sure if there are any around
VK/ZL
The Dst is not a measure of electrons in the
D-layer, rather it is a measure of the potential gradient driving the
exchange between the Ring Current and the Ionosphere . Thus very
low Dst indicates a high potential to drive lots of excess free electrons
into the D-region. The Dst recovery as the ring is depleted is approximately
logarithmic as one would expect for a diffusion process. I did wonder whether
measurements of total electron density would give any ideas. but I could not
make any progress with that, probably because most of the electrons will be in
the higher levels of the F-layer.
Interestingly when a big storm occurs the excess
electrons have the same effect as a flare in daytime ! They enhance the daytime
signal level for one or perhaps at most two days. The are much hotter that the
flare generated electrons so the effect lasts longer but is much weaker than the
absorption effect at night.
We may get some more ideas when the data from the
latest satellite (that found the 3rd Van Allan belt) finishes surveying the
region. I have seen it suggested that there are up to 7(I think it was) ion
filled rings reaching up to nine Earth diameters out.
Unfortunately a good Dst doesnt guarantee good
signals.....there is something else at work. It may just be multipath but I
cant get any useful data yet. Maybe I need phase data.
Best Wishes
Alan
G3NYK
----- Original Message -----
Sent: Tuesday, April 09, 2013 7:49
PM
Subject: Re: LF: Best results so far from
Germany to Tasmania
Edgar, Stefan,
this is an outstanding result! Great to
see what is possible on LF, given a good antenna, a quiet location,
and patience paired with persistence.
Did you by chance have a look at the best SNR in
the spectrum plot? The fat parts of the trace might have
been 12 or even 15 dB, in a 7.5 mHz FFT. This would put
it within easy reach of an Opera-32 correlation detection,
and possibly even close to a WSPR-15 decode.
Alan, I assume that DST would affect attenuation
globally, without preference for one direction or another. Or could an
eastern path be better during one night, versus westward in
another?
Best 73,
Markus (DF6NM)
Sent: Tuesday, April 09, 2013 2:09 PM
Subject: LF: Best results so far from Germany to
Tasmania
LF,
Last
evening there was excellent LF propagation from EU to VK. Edgar J. Twining
(SWL) was watching the LF DX window for several weeks now. The season on that
path in spring (EU) 2013 was very poor and we already thought that the season
is over. However yesterday the path was open for a exceptional long time and
the S/N was very good! Transmissions were done in DFCW-180. I've been on air
for several days now and such a result is most probably possible for 1 time in
the year or maybe 2 years.
These are the results:
My signal: https://dl.dropbox.com/u/19882028/LF/DK7FC%20WR%20ver%20spectrum%20-18.PNG
DCF39:
https://dl.dropbox.com/u/19882028/LF/DCF39%20WR%20ver%20spectrum%20-14.PNG
DCF39
plot: https://dl.dropbox.com/u/19882028/LF/DCF39%20WR%20ver%20plot%202013-04-08%2021-30.jpg
The
path is 16806 km, http://no.nonsense.ee/qthmap/?qth=QE37PD&from=jn49ik00wd
It
shows once again that it is always worth to transmit and to receive/watch for
exceptional conds(x) on the bands!
Many thanks to Edgar for his
continuous patience and interest to receive on 137 kHz from the other side of
the world!
73, Stefan/DK7FC
