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|    ARLP047    |
|    29 Nov 10 20:15:48    |
      SB PROP @ ARL $ARLP047       ARLP047 Propagation de K7RA              ZCZC AP47       QST de W1AW        Propagation Forecast Bulletin 47 ARLP047       From Tad Cook, K7RA       Seattle, WA November 29, 2010       To all radio amateurs               SB PROP ARL ARLP047       ARLP047 Propagation de K7RA              Average daily solar flux declined this week over 36 points compared       to last week, to 24.6. Our reporting week, which ran until November       24, showed the daily sunspot number declining from 40 to 11, but on       November 25 the sunspot number rose to 22.              Sunspot group 1125 disappeared on November 17, and on November 20       sunspot group 1124 was gone, after ten days of visibility. 1126 was       gone on November 23 (after 11 days), and 1127 is still visible after       ten days. On November 25 new sunspot group 1128 arose near the       eastern horizon, and may provide some needed propagation juice for       this weekend's CQ World Wide CW DX Contest.              Solar flux during this week went from a high of 86.5 to 74.8, and       the predicted solar flux for November 26-30 is 78, 78, 79, 80 and       80. Solar flux is predicted at 78 for December 1-3, then 85 on       December 4-11 and 90 on December 12-14. Perhaps this bodes well for       the ARRL 10 meter Contest, December 11-12. That contest is also       during a time when ionization from meteors may enhance 10 meter       propagation.              The above solar flux forecast is from NOAA and USAF, and they say       planetary A index should be stable for the next couple of weeks,       with the index at five for November 26 through December 10.       Geophysical Institute Prague has a different outlook. They also say       that for the next week, look for quiet conditions November 26,       quiet-to-unsettled November 27, unsettled November 28,       quiet-to-unsettled November 29, and quiet November 30 through       December 2.              This weekend the STEREO mission (see http://stereo.gsfc.nasa.gov/)       will achieve 97.3% coverage. This means that only 2.7% of the Sun       is now not visible to us, and that is in the area on the side of the       Sun facing away from Earth. STEREO will achieve 98.7% coverage by       the end of this year, and should finally achieve 100% coverage some       time on February 6, 2011.              Things are still looking up in terms of increasing sunspot activity.       The first 25 days in November had an average daily sunspot number of       38, compared to 18, 23.1, 28.2, 35.7 and 35 for June through       October. If this average continues through the next five days,       November will have the highest monthly average of daily sunspot       numbers since May, 2006 when it was 39.6.              A brief report from Pete Heins, N6ZE of Thousand Oaks, California       (DM04): On November 19 at 0056 UTC with 100 watts and a vertical he       worked VP8LP in the Falkland Islands, with S5 reports both       directions. VP8LP was working mostly W6, W7 and VE7. For details       on Pete's VHF exploits, see http://www.qrz.com/db/n6ze.              Larry Jones, K5ZRK of Sandersville, Mississippi lives on the edge of       the Tallahala Swamp. He wrote, "I operate only 30 and 60 meters. On       60 meters I have a separate receive antenna. The morning of November       17 while in QSO with Les, KG4QZV (in Rome, Georgia, about 300 miles       away), after Les un-keyed I heard a very distinct echo off his       signal. We were on 5.3465 MHz. The echo had less signal strength       than Les's originating signal. I have only heard this happen once       before on 60 meters and I chase the gray line on this band every       day. Is this long path or diversity reception? I might also note       that the gray line was very productive this same morning."              Hard to say what was causing that echo, but at 186,000 miles per       second, a 30 ms echo could emerge if the signal traveled 2700 miles,       bounced, and covered the same distance back. Seems unlikely to be       long path, but perhaps that gray line was propagating that signal a       long distance, and propagating the echo back.              Read more about Larry's QRP activity on 30 and 60 meters at       http://www.qrz.com/db/k5zrk.              Some readers who read this bulletin in the html version on the ARRL       web site had trouble linking to the PDF provided by Dean Straw, N6BV       last week. Try the text version at       http://www.arrl.org/w1aw-bulletins-archive/ARLP046/2010 and       right-click and save via the link provided for the PDF of "Seeing       the HF Propagation Big Picture."              Carl Luetzelschwab, K9LA has a piece on HF circular polarization in       his Propagation column in the current issue of World Radio at       http://www.worldradiomagazine.com.              Thanks to K1SFA for posting this bulletin to the ARRL web site from       her home on Friday, November 26. The email version won't propagate       until Monday, November 29.              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 web page at       http://arrl.org/propagation-of-rf-signals. For an explanation of the       numbers used in this bulletin, see       http://arrl.org/the-sun-the-earth-the-ionosphere. An archive of past       propagation bulletins is at       http://arrl.org/w1aw-bulletins-archive-propagation. Find more good       information and tutorials on propagation at       http://mysite.ncnetwork.net/k9la/index.html.              Monthly propagation charts between four USA regions and twelve       overseas locations are at http://arrl.org/propagation.              Instructions for starting or ending email distribution of ARRL       bulletins are at http://arrl.org/bulletins.              Sunspot numbers for November 18 through 24 were 40, 37, 24, 25, 23,       12, and 11, with a mean of 24.6. 10.7 cm flux was 86.5, 84, 79.8,       77.6, 74.8, 75.3 and 75.8 with a mean of 79.1. Estimated planetary A       indices were 5, 2, 2, 3, 4, 8 and 4 with a mean of 4. Estimated       mid-latitude A indices were 4, 2, 2, 2, 4, 7 and 3 with a mean of       3.4.       NNNN       /EX              ---        ========              IF you have questions or concerns regarding the accuracy       of information posted, or the opinions expressed, contact the content       originators directly. All publications retransmitted as       fidonet echomail without alteration other than the removal of       email header and other control information which       is not part of the actual publication.              Providing emergency communications assistance to your       neighbors and community isn't just a good thing to do, it's       the first and foremost activity recognized in the U.s. rules       governing amateur radio in 47 CFR section 97.1. IF you enjoy       amateur radio remember that this is an obligation you       tacitly agreed to when you acquired your license.                            ---        * Origin: RRN BBS: Your fidonet ham radio connection! 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