Re: Topband: solarwind and 160 prop

2013-01-24 Thread Jim GM
I had seen when those factors a long with a full moon or new moon that
pulls the magnetic field more, What else helps use here in Wisconsin is the
Solar Wind when it comes out of the South.

All the other factors have to aline and if the sun just does not cooperate
we are just SOL.

-- 
Jim K9TF
_
Topband Reflector


Re: Topband: solarwind and 160 prop

2013-01-23 Thread donovanf
Wolf,

The web page for the National Space Weather Prediction Center's 
Wang-Sheeley-Arge solar wind model displays predictions and observations of 
solar wind speed and the polarity of the interplanetary magnetic field at earth.

http://www.swpc.noaa.gov/ws

73
Frank
W3LPL





 Original message 
Date: Wed, 23 Jan 2013 06:24:17 +0100
From: Dr. Wolf Ostwald df...@t-online.de  
Subject: Topband: solarwind and 160 prop  
To: topband@contesting.com

hi reflectees !
As we all know, the effects of the solar wind are strongly determining 
160m propagation. It seems that solely watching A and K indexes plus the 
SFI is not helping much in propagation predictions, at least not for 
160. We all tried that and failed in it. Now is the critical factor 
whether the polarity of the arriving solar wind, developing the 
interplanetary mag field , fits the earth mag field or not. becuase if 
it does, the influence is by far greater than without it.
Question is, where do i find that info ?? I think this might stir up 
some geophysicist - hopefully. Surely the information derived that way 
is not as easy to grasp as a simple number, but it may be the only way 
to further the cause.
73 de wolf  df2py

_
Topband Reflector
_
Topband Reflector


Re: Topband: solarwind and 160 prop

2013-01-23 Thread Arthur Delibert

Check out this website:

http://www.swpc.noaa.gov/SWN/

--Art Delibert, KB3FJO



 Date: Wed, 23 Jan 2013 06:24:17 +0100
 From: df...@t-online.de
 To: topband@contesting.com
 Subject: Topband: solarwind and 160 prop
 
 hi reflectees !
 As we all know, the effects of the solar wind are strongly determining 
 160m propagation. It seems that solely watching A and K indexes plus the 
 SFI is not helping much in propagation predictions, at least not for 
 160. We all tried that and failed in it. Now is the critical factor 
 whether the polarity of the arriving solar wind, developing the 
 interplanetary mag field , fits the earth mag field or not. becuase if 
 it does, the influence is by far greater than without it.
 Question is, where do i find that info ?? I think this might stir up 
 some geophysicist - hopefully. Surely the information derived that way 
 is not as easy to grasp as a simple number, but it may be the only way 
 to further the cause.
 73 de wolf  df2py
 
 _
 Topband Reflector
  
_
Topband Reflector


Re: Topband: solarwind and 160 prop

2013-01-23 Thread N1BUG

Hi Wolf,

I'm not sure if I understand your question. If you are looking for 
real time solar wind monitoring, you might start here:


http://www.aurorasentry.com

I have assembled a collection of solar, solar wind, and geomagnetic 
real time data, originally to forecast and track VHF and UHF radio 
reflection from aurora. The site needs updating. I haven't had time 
for it in a while.


Of particular interest is the ACE MAG  SWEPAM plot which you can 
find on the Solar Wind  Dst portion of that site, or directly here:


http://www.swpc.noaa.gov/ace/MAG_SWEPAM_24h.html

The red Bz trace in the top panel is the north-south orientation 
of the interplanetary magnetic field. It couples most heavily with 
Earth's magnetic field (producing geomagnetic disturbance) when it 
is south oriented. Note that there are versions of this plot 
available for time spans of 2, 6, or 24 hours, 3 or 7 days.


While on the subject, I never have liked, and still do not, the ever 
popular NOAA POES Auroral Activity plots:


http://www.swpc.noaa.gov/pmap/index.html

These have to me proven very unreliable for the intended purpose of 
correlating to VHF auroral propagation, but also do not track as 
well with intensity of real time auroral disturbances at MF and HF. 
Much better I think, but not yet adopted by hams, is OVATION Auroral 
Forecast:


http://helios.swpc.noaa.gov/ovation/

or

OVATION Prime Real-Time:

http://www.ngdc.noaa.gov/stp/ovation_prime/

Unfortunately this one lacks a good map overlay and takes some 
practice to read it correctly.


73,
Paul N1BUG


On 01/23/2013 12:24 AM, Dr. Wolf Ostwald wrote:

 Now is the critical factor
whether the polarity of the arriving solar wind, developing the
interplanetary mag field , fits the earth mag field or not. becuase if
it does, the influence is by far greater than without it.
Question is, where do i find that info ??



--
Paul Kelley, N1BUG
RFI Committee chair,
Piscataquis Amateur Radio Club
http://www.k1pq.org
_
Topband Reflector


Re: Topband: solarwind and 160 prop

2013-01-23 Thread Bill Cromwell
On Wed, 2013-01-23 at 09:39 -0500, Bill Tippett wrote:

---snip---
  There are many other factors affecting 160, and probably many
 we do not fully understand.  
---snip---
 
 73,  Bill  W4ZV


Hi Bill,

We probably know just enough to be dangerous. I often refer to the
propagation fairies - like the tooth fairy, etc. It's partly mystery.
That's why all of us have QSOs that should be impossible ( a gift from
the propagation fairies) or fail to make QSOs that should be easy
(tricks played by those same fairies). One attraction of ham radio is
the bundle of surprises we get when we turn on the radios. As Tim The
Toolman says - OY!?

73,

Bill  KU8H

_
Topband Reflector


Re: Topband: solarwind and 160 prop

2013-01-23 Thread Steve London

On 01/23/2013 07:39 AM, Bill Tippett wrote:



Weather Events in the Upper Atmosphere

D-region Winter Anomaly is a period of enhanced radio wave absorption
usually occurring in late winter and thought to be associated with a sudden
stratospheric warming

http://www.albany.edu/faculty/rgk/atm101/weather.htm


I see something called D-region Bite-Out in this link. That's a new one 
for me, and defined as:


D-region Bite-Out is a daytime depletion of electron density as the 
result of electrons attaching to polar mesopheric cloud ice particles


Seems like that would be good for 160 meters. Is it measurable ?

73,
Steve, N2IC
_
Topband Reflector


Re: Topband: solarwind and 160 prop

2013-01-23 Thread Shoppa, Tim
I have a hard time differentiating between low activity and poor DX 
conditions sometimes.

From the east coast of the US in the past week or two, I have not heard much 
EU at all, but domestic conditions are just fine as evidenced by two NAQP's 
past two weekends and there have been several Central American/South American 
stations on 160 with truly excellent (very very impressively loud) signals.

Tim N3QE
_
Topband Reflector


Topband: solarwind and 160 prop

2013-01-22 Thread Dr. Wolf Ostwald

hi reflectees !
As we all know, the effects of the solar wind are strongly determining 
160m propagation. It seems that solely watching A and K indexes plus the 
SFI is not helping much in propagation predictions, at least not for 
160. We all tried that and failed in it. Now is the critical factor 
whether the polarity of the arriving solar wind, developing the 
interplanetary mag field , fits the earth mag field or not. becuase if 
it does, the influence is by far greater than without it.
Question is, where do i find that info ?? I think this might stir up 
some geophysicist - hopefully. Surely the information derived that way 
is not as easy to grasp as a simple number, but it may be the only way 
to further the cause.

73 de wolf  df2py

_
Topband Reflector