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www.southgatearc.org
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Propagation de K7RAThe past couple of days have seen robust solar activity, with flares and strong solar wind. On Wednesday and Thursday, December 6 and 7, the planetary A index rose to 28, then 25. On December 5 a large X9 class solar flare emerged from the sun's eastern side, but it wasn't earth directed. This was from a large sunspot 930, which drove the sunspot number to
59 on the same day as the solar flare, the same Flare activity caused a 10.7 cm solar flux reading at Penticton, British Columbia to jump off the scale. The noon reading showed a solar flux of 573.4, and had to be adjusted downward to 103 for the day. Currently a forecast from NOAA and the U.S. Air Force calls for a planetary A index on December 8-12 of 30, 50, 40, 20 and 10. The predicted A index of 50 and 40 for December 9-10 does not bode well for the weekend contest. Even if the geomagnetic activity is this strong, there still should be some north-south trans-equatorial propagation on 10 meters. But here we see an average sunspot number of 52 for this week, 35 points higher than last week, and of course the downside is greater chance for solar flares. There is a new prediction for the sunspot cycle minimum. Until recently,
the minimum was predicted to have a smoothed sunspot number of 6 centered
on March and April 2007. The new forecast moves the minimum out a little
further and not as low, with a smoothed sunspot number of 7 for May 2007.
You can see the difference in the table on page 11 of the SEC Preliminary
Report and Forecast for this Last week's Propagation Forecast Bulletin ARLP050 mentioned a theory about cooling in the upper ionosphere causing greater density in lower layers. It turns out that data from different locations shows different results, and the net effect doesn't look strong or conclusive. If you do a web search for terms such as "long term ionosphere change" you'll find abstracts for several scientific papers on the subject. The most interesting thing I ran across (thanks to K9LA) was the map
on page 12 of the PDF at http://tinyurl.com/yyn4ut.
The hmF2 referred to in this document is the height of the densest portion
of the F2 layer, with positive trends at some ionosonde stations and negative
at others. The trend for change in height of the F2 layer is also very
slight. It comes Jon Jones, N0JK commented that recently in the CQ Worldwide CW Contest
even with solar activity so low, HC8N on 10 meters worked 1,838 stations
in 32 zones and 113 countries. Also, Dave Deatrick, WA8OLD way up in Northern
Michigan next to Sault Ste Marie, Ontario, remarks that he's had great
luck recently on 40 meters with a shortened dipole at 28 feet and 100
watts. He worked 5A7A, CN2R and If you would like to make a comment or have a tip for our readers, email the author at, k7ra@arrl.net. For more information concerning radio propagation, see the ARRL Technical
Information Service at, For a detailed explanation of the numbers used in this bulletin see, http://www.arrl.org/tis/info/k9la-prop.html. An archive of past propagation bulletins is at, http://www.arrl.org/w1aw/prop/. Monthly propagation charts between four USA regions and twelve overseas locations are at, http://www.arrl.org/qst/propcharts/. Sunspot numbers for November 30 through December 6 were 59, 58, 55, 46, 43, 59 and 44 with a mean of 52. 10.7 cm flux was 84.1, 84.2, 87.3, 86.5, 92.8, 102.4, and 103, with a mean of 91.5. Estimated planetary A indices were 28, 4, 2, 3, 1, 2 and 28 with a mean of 9.7. Estimated mid-latitude A indices were 15, 3, 1, 2, 1, 2 and 15, with a mean of 5.6.
Source: The American Radio Relay League
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