Re: Topband: Pulleys for antennas in trees

2015-01-27 Thread Jim Brown

On Tue,1/27/2015 9:50 AM, Mel Crichton wrote:
So if using a pulley, please be sure the supporting branch is 
stout I had to replace the windshield of my truck to prove this 
point to me. I find it best to install inverted vee type (center 
supported) dipoles or very light inverted L's to minimize the sideways 
stress on the branch (sideways stress intensifies when the wind blows 
hard). And yes I have pulleys high in trees. 


Hi Mel,

I can't dispute your mechanical engineering and rigging thoughts, but I 
strongly prefer flat dipoles if I can rig them. So does N6BT, the 
excellent antenna engineer behind the original Force 12 antennas, who 
observes that the performance of the antenna will be dependent on its 
average height.


Quite a few years ago, I saw a piece in QST stating that a lag screw 
going horizontally into the trunk of tree was one of the least invasive 
ways to rig an antenna. That means, of course, that someone has to climb 
the tree. My wire antennas are mostly rigged that way.


Since the subject line is about pulleys, I'll link to the pulley I use. 
It's a really neat pulley, and is sold out here by stores who cater to 
arborists and tree climbers.


http://www.cmi-gear.com/collections/frontpage-2-service-line-pulleys/products/rp115

Here's a photo of the pulley and the lag screw.

k9yc.com/Pulley.JPG

I use the 5/16-in rope distributed by Synthetic Textiles. DX Engineering 
and HRO also sell it. I use the 5/16-in size because it's big enough to 
be able to grab it hard enough to put a lot of tension on it. It's a 
double-braid polyester rope with a black outer sheath that provides UV 
protection.


 http://www.synthetictextilesinc.com/supportham.html

My wires are up 130 ft in redwoods, so they need pretty robust rigging 
hardware. Not everyone needs stuff this robust. :) Another important 
rigging element for any wire in a tree is a weight below a pulley 
terminating one end of the antenna to provide some give for tree sway. 
There are many ways to skin this cat, including old window weights and 
cement in a bucket. I use big water jugs that I fill with dry sand. I'm 
typically using 70-90 pounds of tension.


73, Jim K9YC

_
Topband Reflector Archives - http://www.contesting.com/_topband


Re: Topband: K levels and skew path on 160

2015-01-27 Thread Tom W8JI

I was rereading the article by Cary Oler and Ted Cohen (N4XX), published in
1998, which provided a good primer for understanding, as much as we can,
propagation on Topband. In one section the impact of a high K index on the
auroral oval, and its subsequent impact on signals passing through the 
oval,
was discussed. My question is does the K index, especially at higher 
levels,
impact the SW or SSW skew path many of us were trying to use this morning 
to
work Ken, XW4ZW? Any information or observations will be appreciated. 
Best,


Steve,

From my location now, and when I was in Ohio, it was quite normal for any 
signal passing near or through the north magnetic pole to never make it 
through via the direct path. When signals were heard, they were always 
skewed in some other direction.


The only exception seems to be when sunspots and geomagnetic activity are 
very low. In this very last solar minimum, when sunspots were absent, many 
stations would appear via north. Of course that gave the northern NA 
stations nearly north of me a clear advantage, because they were closer.


My policy is to not worry about predicting or expecting anything, and I 
rarely even look at solar activity. I just listen in all dark directions 
when the station is almost on the opposite side of the world, especially 
when he is anywhere near the equator and far,far, away.   :)


73 Tom






_
Topband Reflector Archives - http://www.contesting.com/_topband


Re: Topband: Elimination of Treadmill RFI on 160 meters

2015-01-27 Thread Don Kirk
Hi Brad,

Great to hear you had similar results.

The 20VR1 and the 20DRGG5 filter appear to be of very similar design (two
stage filters, and component values not vastly different).  The 20VR1 looks
to be double the price of the 20DRGG5, but it might offset some of the
additional cost if it allows elimination of the additional Toroid core
choke.  Since all cases are different I would have to test the 20VR1 in my
application to see if it would indeed allow elimination of the Toroid core
choke, but I doubt I would be able to eliminate the Toroid core choke for
the following reason that Jim K9YC mentioned on another reflector : What
the power industry calls common mode is NOT what we call common mode.
They are talking about the voltage between neutral and the green wire. We
are talking about current that is flowing in the same direction on three
conductors.  In my case the additional Toroid core choke had a very
noticeable impact, and I now can't tell when the treadmill is on when using
the combination of both filters.

P.S. I sent an e-mail to the manufacturer of our Treadmill, and they never
responded.  I am now going to call them on the phone in an attempt to get
in touch with their design engineers, and likely will also file a complaint
with the FCC regarding treadmills in general.  There are a couple more
treadmills near my home that generate very strong RFI, but fortunately they
normally use their Treadmills during the day, and I operate mostly at night.

73,
Don (wd8dsb)




On Tue, Jan 27, 2015 at 1:26 PM, Brad Rehm bradr...@gmail.com wrote:

 Don,

 FWIW, today, W5UJE and I dealt with a treadmill problem similar to yours
 by installing a commercial line filter between the line and the treadmill
 electronics.  A Corcom/TE Connectivity 20VR1 filter reduced the 40m and 75m
 noise at his receiver from S9+10db to less than S2 (his noise floor this
 morning).  The 20 Amp rating was needed because the manufacturer's
 published current requirement for the treadmill was 15 Amps.

 In measurements we'd made earlier, we found that this was a common-mode
 problem and that the noise spurs were about 20 kHz apart when the treadmill
 was operating under a moderate load.  The spectrum scope on his radio
 showed 20 kHz-spaced broadband noise up through 29 MHz, peaking between 1.8
 and 15 MHz.  The line filter we chose offers 10-20 dB of supperssion below
 50 kHz and 60-80 dB of suppression between 300 kHz and 29 MHz.  No
 additional filtering with torroids or capacitors was needed.

 In other words, our results were similar to yours, and one wonders how
 manufacturers can say these things meet Part 15 requirements for conducted
 emissions.

 Brad  KV5V

 On Mon, Jan 26, 2015 at 7:22 PM, Don Kirk wd8...@gmail.com wrote:

 Treadmill combination filter update.

 Today I replaced the 10 amp commercial filter with the 20 amp version of
 the filter, and the results are similar.  Below are a few measurements on
 160 meters and 80 meters showing how effective the combination of the two
 filters are (14 turn toroid choke, and commercial filter model 20DRGG5
 made
 by Delta) in reducing my treadmill RFI.

 *1.8068 Mhz*
 No Filters : 19db over S9
 With Filters : S7 which is my noise floor

 *1.8291 Mhz*
 No Filters : 15db over S9
 With Filters : S7 which is my noise floor

 *3.5250 Mhz*
 No Filters : 28db over S9
 With Filters : S6 which is my noise floor


 *3.5475 Mhz*
 No Filters : 25db over S9
 With Filters : S6 which is my noise floor

 The 3.5250 Mhz readings indicate the filter is knocking the signal down at
 least 46db (and probably more).

 73,
 Don (wd8dsb)


_
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Re: Topband: K levels and skew path on 160

2015-01-27 Thread donovanf
From mid-November through mid-February, daylight over Antarctica 
and the Southern Ocean prevents the 160 meter long path from 
propagating due south (+/- about 20 degrees). 

Except for sunspot minimum, short path propagation transiting only 
the northern hemisphere to southeast Asia is very uncommon from the 
eastern USA. 

160 and 80 meter propagation from eastern USA to southeast Asia is 
most likely to follow the SSE evening and SSW sunrise gray lines, 
although as Tom says, its best to listen for the actual path. 

From 1145-1300Z (the likely times for long path propagation to southeast 
Asia during eastern USA morning) the gray line passes approximately 
through HC8, so the long path is likely to be SSW or possibly SW 

Because the southern magnetic pole is just off the coast of Antarctica and 
directly south of Australia, the SSW long path crosses through the auroral 
belt and this long path is significantly affected by geomagnetic activity. 

From 2300-2330Z (the most likely times for southeast Asia long path in 
eastern USA evening) the grey line crosses Uruguay, so the long path to 
southeast Asia is likely to be SSE or possibly SE. Because the southern 
magnetic pole is on the opposite side of Antarctica, the SSE long path is 
much less affected by geomagnetic conditions than the 1145-1300Z SSW 
long path. 

73 
Frank 
W3LPL 



- Original Message -

From: Tom W8JI w...@w8ji.com 
To: Steven R Daniel, D.D.S. n...@comcast.net, topband@contesting.com 
Sent: Tuesday, January 27, 2015 7:21:00 PM 
Subject: Re: Topband: K levels and skew path on 160 

I was rereading the article by Cary Oler and Ted Cohen (N4XX), published in 
 1998, which provided a good primer for understanding, as much as we can, 
 propagation on Topband. In one section the impact of a high K index on the 
 auroral oval, and its subsequent impact on signals passing through the 
 oval, 
 was discussed. My question is does the K index, especially at higher 
 levels, 
 impact the SW or SSW skew path many of us were trying to use this morning 
 to 
 work Ken, XW4ZW? Any information or observations will be appreciated. 
 Best, 

Steve, 

From my location now, and when I was in Ohio, it was quite normal for any 
signal passing near or through the north magnetic pole to never make it 
through via the direct path. When signals were heard, they were always 
skewed in some other direction. 

The only exception seems to be when sunspots and geomagnetic activity are 
very low. In this very last solar minimum, when sunspots were absent, many 
stations would appear via north. Of course that gave the northern NA 
stations nearly north of me a clear advantage, because they were closer. 

My policy is to not worry about predicting or expecting anything, and I 
rarely even look at solar activity. I just listen in all dark directions 
when the station is almost on the opposite side of the world, especially 
when he is anywhere near the equator and far,far, away. :) 

73 Tom 






_ 
Topband Reflector Archives - http://www.contesting.com/_topband 

_
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Re: Topband: Elimination of Treadmill RFI on 160 meters

2015-01-27 Thread Brad Rehm
Don,

You make a good point about the difference between our definition of CM
noise and the definition implied in Part 15.  If the external torroid made
a difference for you, then it's important and worth having.

We can't be too optimistic about the manufacturer's interest in fixing this
kind of problem.  He won't be willing to install a $50 or even $25 filter
to satisfy a few hams who have EMC complaints.  At the same time, because
the products you and I have dealt with responded so well when we added
filters, we have to wonder if and how the Part 15 compliance testing was
done.

In the EMC lab where I worked, we tested them under load (with someone
walking on the treadmill or with a fixed load applied), but some labs might
be tempted to test only the uP controller.  It's hard to imagine how this
could be justified, because the belt is usually driven with square
pulses.  RF noise from these can be hard to suppress.

I didn't think to check the label for the machine I worked on, but I wonder
if you've looked for an FCC compliance mark on your treadmill.  If it has
one, it might be interesting to go to the FCC URL and look at the report
that was filed for it.  And BTW, if the treadmill was manufactured in the
far east, the mark could be bogus or filtering could have been deleted
after the initial testing was done.  This kind of thing isn't all that
unusual.

73,
Brad  KV5V

On Tue, Jan 27, 2015 at 4:05 PM, Don Kirk wd8...@gmail.com wrote:

 Hi Brad,

 Great to hear you had similar results.

 The 20VR1 and the 20DRGG5 filter appear to be of very similar design (two
 stage filters, and component values not vastly different).  The 20VR1 looks
 to be double the price of the 20DRGG5, but it might offset some of the
 additional cost if it allows elimination of the additional Toroid core
 choke.  Since all cases are different I would have to test the 20VR1 in my
 application to see if it would indeed allow elimination of the Toroid core
 choke, but I doubt I would be able to eliminate the Toroid core choke for
 the following reason that Jim K9YC mentioned on another reflector : What
 the power industry calls common mode is NOT what we call common mode.
 They are talking about the voltage between neutral and the green wire. We
 are talking about current that is flowing in the same direction on three
 conductors.  In my case the additional Toroid core choke had a very
 noticeable impact, and I now can't tell when the treadmill is on when using
 the combination of both filters.

 P.S. I sent an e-mail to the manufacturer of our Treadmill, and they never
 responded.  I am now going to call them on the phone in an attempt to get
 in touch with their design engineers, and likely will also file a complaint
 with the FCC regarding treadmills in general.  There are a couple more
 treadmills near my home that generate very strong RFI, but fortunately they
 normally use their Treadmills during the day, and I operate mostly at night.

 73,
 Don (wd8dsb)




 On Tue, Jan 27, 2015 at 1:26 PM, Brad Rehm bradr...@gmail.com wrote:

 Don,

 FWIW, today, W5UJE and I dealt with a treadmill problem similar to yours
 by installing a commercial line filter between the line and the treadmill
 electronics.  A Corcom/TE Connectivity 20VR1 filter reduced the 40m and 75m
 noise at his receiver from S9+10db to less than S2 (his noise floor this
 morning).  The 20 Amp rating was needed because the manufacturer's
 published current requirement for the treadmill was 15 Amps.

 In measurements we'd made earlier, we found that this was a common-mode
 problem and that the noise spurs were about 20 kHz apart when the treadmill
 was operating under a moderate load.  The spectrum scope on his radio
 showed 20 kHz-spaced broadband noise up through 29 MHz, peaking between 1.8
 and 15 MHz.  The line filter we chose offers 10-20 dB of supperssion below
 50 kHz and 60-80 dB of suppression between 300 kHz and 29 MHz.  No
 additional filtering with torroids or capacitors was needed.

 In other words, our results were similar to yours, and one wonders how
 manufacturers can say these things meet Part 15 requirements for conducted
 emissions.

 Brad  KV5V

 On Mon, Jan 26, 2015 at 7:22 PM, Don Kirk wd8...@gmail.com wrote:

 Treadmill combination filter update.

 Today I replaced the 10 amp commercial filter with the 20 amp version of
 the filter, and the results are similar.  Below are a few measurements on
 160 meters and 80 meters showing how effective the combination of the two
 filters are (14 turn toroid choke, and commercial filter model 20DRGG5
 made
 by Delta) in reducing my treadmill RFI.

 *1.8068 Mhz*
 No Filters : 19db over S9
 With Filters : S7 which is my noise floor

 *1.8291 Mhz*
 No Filters : 15db over S9
 With Filters : S7 which is my noise floor

 *3.5250 Mhz*
 No Filters : 28db over S9
 With Filters : S6 which is my noise floor


 *3.5475 Mhz*
 No Filters : 25db over S9
 With Filters : S6 which is my noise floor

 The 3.5250 Mhz readings 

Re: Topband: Elimination of Treadmill RFI on 160 meters

2015-01-27 Thread Tom W8JI

are talking about current that is flowing in the same direction on three
conductors.  In my case the additional Toroid core choke had a very
noticeable impact, and I now can't tell when the treadmill is on when 
using

the combination of both filters.

P.S. I sent an e-mail to the manufacturer of our Treadmill, and they never
responded.  I am now going to call them on the phone in an attempt to get
in touch with their design engineers, and likely will also file a 
complaint

with the FCC regarding treadmills in general.  There are a couple more
treadmills near my home that generate very strong RFI, but fortunately 
they
normally use their Treadmills during the day, and I operate mostly at 
night.


The FCC requires testing of power line conducted emissions with a line 
sample unit that connects from each conductor to ground. One LISN is 
specified to go from each current-carrying conductor to ground. The safety 
ground, since it does not carry current, is grounded.


The flaw in this system is that differential voltages between current 
carrying wires are not measured, and anything on the safety ground isn't 
measured.  Noise voltage is only measured from individual current carrying 
conductors to ground, and the safety ground is grounded and not measured.


Filters inside devices and many outside filters often route the noise right 
out on the safety ground, in differential to the equipment case (if large it 
acts like a groundplane) or other connecting wired systems like a Telco line 
or data interface cable.


Since the FCC mandates the safety ground and other grounds be grounded to 
the test equipment RF measurement groundplane, that path or ground loop 
paths are not measured. This allows some pretty ratty stuff to pass FCC 
tests.


The FCC should have created a better test, instead of assuming all grounds 
in the real world were common-connected with near zero impedance.


73 Tom 


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Topband: K levels and skew path on 160

2015-01-27 Thread Steven R Daniel, D.D.S.
I was rereading the article by Cary Oler and Ted Cohen (N4XX), published in
1998, which provided a good primer for understanding, as much as we can,
propagation on Topband. In one section the impact of a high K index on the
auroral oval, and its subsequent impact on signals passing through the oval,
was discussed. My question is does the K index, especially at higher levels,
impact the SW or SSW skew path many of us were trying to use this morning to
work Ken, XW4ZW? Any information or observations will be appreciated. Best,
Steve, NN4T

_
Topband Reflector Archives - http://www.contesting.com/_topband


Re: Topband: Elimination of Treadmill RFI on 160 meters

2015-01-27 Thread Jim Brown

On Tue,1/27/2015 3:19 PM, Brad Rehm wrote:

You make a good point about the difference between our definition of CM
noise and the definition implied in Part 15.  If the external torroid made
a difference for you, then it's important and worth having.


Exactly. The commercial filter addresses only differential mode. The 
ferrite choke is necessary to suppress what we (and Part 15) call common 
mode.


Several years ago, I put some good quality line filters in electrical 
boxes for use on Field Day and California QSO Party county expeditions 
with our Yamaha generators. They didn't do much -- to kill the moderate 
trash, I had to to wind multiple turns of the line cord  through a big 
ferrite core. I used a big 1-in i.d. Fair-Rite #31 clamp-on that's a 
couple of inches long (the biggest they make). Depending on the diameter 
of the line cord I had used, I was able to get either three or four 
turns through it. That was enough to kill 20-10M, which is what we heard 
in the tri-banders that were close to the generator, and for the 80/40 
dipoles that were much further away. If the 80/40 antennas had been 
closer we would likely have needed more turns.


Did the commercial line filters do any good?  I don't know -- but they 
certainly didn't hurt, and the boxes I put them in have a bunch of 
outlets on them for power distro. :)  OTOH, one of the guys used to 
bring his big RV with a noisy generator on-board. All I used there was 
as many turns as I could get through a small stack of 1.4-in i.d. #31 
toroids as close as I could get them to the generator, and it did the job.


73, Jim K9YC


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Re: Topband: K levels and skew path on 160

2015-01-27 Thread JC


-Original Message-
From: Topband [mailto:topband-boun...@contesting.com] On Behalf Of
donov...@starpower.net
Sent: Tuesday, January 27, 2015 3:28 PM
To: topband@contesting.com
Cc: n...@comcast.net

Because the southern magnetic pole is just off the coast of Antarctica and
directly south of Australia, the SSW long path crosses through the auroral
belt and this long path is significantly affected by geomagnetic activity. 

From 2300-2330Z (the most likely times for southeast Asia long path in
eastern USA evening) the grey line crosses Uruguay, so the long path to
southeast Asia is likely to be SSE or possibly SE. Because the southern
magnetic pole is on the opposite side of Antarctica, the SSE long path is
much less affected by geomagnetic conditions than the 1145-1300Z SSW long
path. 


Frank

Your observations match my observations since 2009 when I started to work
with Horizontal polarized receiver antenna for 80/160. 2010 and 2011 the
SSE/SSW path was open most of the days. Peter (XU7ACY) was very active and I
heard  him from October to March over 60 days out of 180 days on 160m, and
every single day on 80m at the same operating time you mentioned.

I did try to correlate the openings with K and AL and it is not directly
related. The only index for magnetic storm that was correlated was Dst.  Dst
index is an index of magnetic activity derived from a network of
near-equatorial geomagnetic observatories that measures the intensity of the
globally symmetrical equatorial electrojet (the ring current).
I started to follow Dst because Alan Melia G3NYK long wave propagation page.
Alan noticed the LF  ( 500KHz) propagation could be good after few days of
Dst above zero, it means low activity of magnetic storm.

K, AL and Dst and all related with solar wind speed, predictions are
available from Colorado and Kyoto.

http://lasp.colorado.edu/space_weather/dsttemerin/dsttemerin.html


http://wdc.kugi.kyoto-u.ac.jp/dst_realtime/presentmonth/index.html

The Dst can be useful when is positive for 5 or more days, indicating good
condition possibility. Activity is more important than possibility, without
activity propagation does not matter. So when a flare or CME hit the
magnetic ring, two things happen, first there is a very good improvement on
the propagation for few hours followed by a depression and degradation of
propagation, that depression last for several days and a good recovery can
take over a week. After the impact the attenuation is high above normal and
the impact on 160m is significate, but not much on 80m.

After a good success with HWF in Florida, some friends in South America, and
Brazil started to use the HWF for long path. I get very serious trying to
understand the physics behind 50% openings on LP and I collect data from
previous QSO on 80 and 160m when directive RX antenna systems was used. 

For my surprise all opening on the South Hemisphere long path were actually
NNW NNE. That result indicate that the actual signal SSE SSW  get refracted
at the equator region and travel inside the darkness. 

Robert DU7ET was a good example of this kind of propagation long path , we
had QSO's every month from Jan to July 2013. For me all openings were SSW
but from my friends on Brazil the path was NNW. 

Based on the observations my conclusion (still a work in progress) is that
the signal does not reach the south pole auroral belt. It's run along the
equator, That s why I am calling this propagation mode TELP , Trans
Equatorial Long Path.

Carl K9LA did a nice paper with the ray traces from my location to XU7 , and
at 40 degree there is a refraction  bending SSW signal to W. It can explain
the same bending for reflated signals NNW to W from Brazil.

Dst also can show how bad the propagation was Dec 2014 to middle Jan 2015.
Ove several years the Dst  was in between 0 and -20 but during the last two
month Dst was between -20 and -40 with very deeps near -100.

I would say that TELP I open on 80m almost every day, we just don't have
much activity to understand it better.

Regards
JC
N4IS




- Original Message -

From: Tom W8JI w...@w8ji.com
To: Steven R Daniel, D.D.S. n...@comcast.net, topband@contesting.com
Sent: Tuesday, January 27, 2015 7:21:00 PM
Subject: Re: Topband: K levels and skew path on 160 

I was rereading the article by Cary Oler and Ted Cohen (N4XX), 
published in  1998, which provided a good primer for understanding, as 
much as we can,  propagation on Topband. In one section the impact of a 
high K index on the  auroral oval, and its subsequent impact on signals 
passing through the  oval,  was discussed. My question is does the K 
index, especially at higher  levels,  impact the SW or SSW skew path 
many of us were trying to use this morning  to  work Ken, XW4ZW? Any 
information or observations will be appreciated.
 Best,

Steve, 

From my location now, and when I was in Ohio, it was quite normal for any
signal passing near or through the north magnetic pole to never make it

Re: Topband: Elimination of Treadmill RFI on 160 meters

2015-01-27 Thread Jim Brown

On Tue,1/27/2015 4:08 PM, Tom W8JI wrote:
The flaw in this system is that differential voltages between current 
carrying wires are not measured, and anything on the safety ground 
isn't measured.  Noise voltage is only measured from individual 
current carrying conductors to ground, and the safety ground is 
grounded and not measured.


Exactly right, Tom. A common design/manufacturing defect is that the 
green wire fails to make contact with the shielding enclosure, but 
instead goes to common on a circuit board, which may or may not ever 
find the chassis. This defect, which is the power system equivalent of a 
Pin One Problem, puts noise on the green wire. You may remember that we 
corresponded several years ago about Astron power supplies, in which a 
very common defect is that the green wire is soldered to the mounting 
lug of a terminal strip, which is insulated from the chassis by paint. 
The same mounting lug is the point where V- is bonded, so it never finds 
the chassis either. AND, wiring for both V- and the green wire act as 
antennas for both TX and RX.


I have long suspected that similar defects are at least partially 
responsible for noise conducted onto coax and AC lines from consumer 
products of all sorts.


73, Jim K9YC


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Re: Topband: K levels and skew path on 160

2015-01-27 Thread donovanf
Hi JC, 

Thanks for your interesting email. You may be correct that SSE/SSW 
long path propagation may not extend very far into the southern 
hemisphere. I wasn't aware of the NNE/NNW observations by 
our southern hemisphere friends. It also appears that SSE/SSW long 
path is more reliable for more southerly locations in the USA than it is 
for higher latitude locations. 

Unfortunately there usually isn't enough activity in southeast asia for us to 
make regular observations, you were fortunate to be able to have long 
term observations with XU7ACY and DU7ET . 

Thanks 

73 
Frank 
W3LPL 



- Original Message -

From: JC n...@comcast.net 
To: donov...@starpower.net, topband@contesting.com 
Cc: n...@comcast.net 
Sent: Wednesday, January 28, 2015 2:45:05 AM 
Subject: RE: Topband: K levels and skew path on 160 



-Original Message- 
From: Topband [mailto:topband-boun...@contesting.com] On Behalf Of 
donov...@starpower.net 
Sent: Tuesday, January 27, 2015 3:28 PM 
To: topband@contesting.com 
Cc: n...@comcast.net 
 
Because the southern magnetic pole is just off the coast of Antarctica and 
directly south of Australia, the SSW long path crosses through the auroral 
belt and this long path is significantly affected by geomagnetic activity. 
 
From 2300-2330Z (the most likely times for southeast Asia long path in 
eastern USA evening) the grey line crosses Uruguay, so the long path to 
southeast Asia is likely to be SSE or possibly SE. Because the southern 
magnetic pole is on the opposite side of Antarctica, the SSE long path is 
much less affected by geomagnetic conditions than the 1145-1300Z SSW long 
path. 
 

Frank 

Your observations match my observations since 2009 when I started to work 
with Horizontal polarized receiver antenna for 80/160. 2010 and 2011 the 
SSE/SSW path was open most of the days. Peter (XU7ACY) was very active and I 
heard him from October to March over 60 days out of 180 days on 160m, and 
every single day on 80m at the same operating time you mentioned. 

I did try to correlate the openings with K and AL and it is not directly 
related. The only index for magnetic storm that was correlated was Dst. Dst 
index is an index of magnetic activity derived from a network of 
near-equatorial geomagnetic observatories that measures the intensity of the 
globally symmetrical equatorial electrojet (the ring current). 
I started to follow Dst because Alan Melia G3NYK long wave propagation page. 
Alan noticed the LF ( 500KHz) propagation could be good after few days of 
Dst above zero, it means low activity of magnetic storm. 

K, AL and Dst and all related with solar wind speed, predictions are 
available from Colorado and Kyoto. 

http://lasp.colorado.edu/space_weather/dsttemerin/dsttemerin.html 


http://wdc.kugi.kyoto-u.ac.jp/dst_realtime/presentmonth/index.html 

The Dst can be useful when is positive for 5 or more days, indicating good 
condition possibility. Activity is more important than possibility, without 
activity propagation does not matter. So when a flare or CME hit the 
magnetic ring, two things happen, first there is a very good improvement on 
the propagation for few hours followed by a depression and degradation of 
propagation, that depression last for several days and a good recovery can 
take over a week. After the impact the attenuation is high above normal and 
the impact on 160m is significate, but not much on 80m. 

After a good success with HWF in Florida, some friends in South America, and 
Brazil started to use the HWF for long path. I get very serious trying to 
understand the physics behind 50% openings on LP and I collect data from 
previous QSO on 80 and 160m when directive RX antenna systems was used. 

For my surprise all opening on the South Hemisphere long path were actually 
NNW NNE. That result indicate that the actual signal SSE SSW get refracted 
at the equator region and travel inside the darkness. 

Robert DU7ET was a good example of this kind of propagation long path , we 
had QSO's every month from Jan to July 2013. For me all openings were SSW 
but from my friends on Brazil the path was NNW. 

Based on the observations my conclusion (still a work in progress) is that 
the signal does not reach the south pole auroral belt. It's run along the 
equator, That s why I am calling this propagation mode TELP , Trans 
Equatorial Long Path. 

Carl K9LA did a nice paper with the ray traces from my location to XU7 , and 
at 40 degree there is a refraction bending SSW signal to W. It can explain 
the same bending for reflated signals NNW to W from Brazil. 

Dst also can show how bad the propagation was Dec 2014 to middle Jan 2015. 
Ove several years the Dst was in between 0 and -20 but during the last two 
month Dst was between -20 and -40 with very deeps near -100. 

I would say that TELP I open on 80m almost every day, we just don't have 
much activity to understand it better. 

Regards 
JC 
N4IS 




- Original Message - 

From: Tom