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|    Message 237 of 3,036    |
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|    ARLP012    |
|    25 Mar 11 17:44:34    |
      SB PROP @ ARL $ARLP012       ARLP012 Propagation de K7RA              ZCZC AP12       QST de W1AW        Propagation Forecast Bulletin 12 ARLP012       From Tad Cook, K7RA       Seattle, WA March 25, 2011       To all radio amateurs               SB PROP ARL ARLP012       ARLP012 Propagation de K7RA              All solar indicators were lower again for the second consecutive       week. Average daily sunspot numbers declined over 28 points from       the week before to 40.9, and average daily solar flux was off over       18 points to 94.8.              But looking at solar images from the STEREO mission at       http://stereo.gsfc.nasa.gov we can see a great deal of activity       about to rotate toward us over the Sun's eastern horizon. The whole       "back" side of our Sun looks very busy.              The March 24 NOAA forecast for solar flux and planetary A index sees       solar flux for March 25 to April 3 at 110, 115, 120, 125, 125, 130,       130, 130, 120 and 115. Planetary A index for the same period is       predicted at 5 for March 25-29, 7 on March 30-31, and 5 on April       1-3.              This indicates improving HF propagation for the near term, with       geomagnetic indicators unsettled only very slightly compared to       recent very quiet conditions. Conditions should be good for the CQ       World Wide WPX SSB Contest this weekend, and there is a useful web       site devoted to this contest at http://www.cqwpx.com.              Geophysical Institute Prague has a forecast for geomagnetic       conditions quite different from NOAA, predicting quiet conditions       for March 25-27, unsettled to active on March 28, unsettled March       29-30, and quiet to unsettled March 31.              Carl Luetzelschwab, K9LA pointed out that the nanoTesla values for       each level of K index mentioned in last week's bulletin are actually       for the Boulder, Colorado magnetometer, and the values are different       for each observatory. He has a good description of how this all       works at his web site,       http://mysite.ncnetwork.net/k9la/Where_Do_the_K_and_A_Index_Come_From.pdf.              Jeff Hartley, N8II of Shepherdstown, West Virginia sent in a report       last Saturday, March 19. He wrote, "Despite the decline in solar       activity 12 meters has been consistently open to Europe every       weekday this week including some Russians, Latvia, and Lithuania. As       the flux has dropped off, the band has been opening later. The band       was wide open to Europe at 1230Z Monday (March 14), Thursday and       Friday (March 17-18) were good from about 1445Z to past 1600Z. 15       meters has been consistently good to Russia with loud signals (RL3A       S9+20-30dB) and even central Asia including UK6, UK8, and UN3M (S9)       worked 2 days and I even caught HS0ZDS on Wednesday right over the       pole. The low K indexes seem more important than the high flux for       anything close to the pole, no big surprise. VU4PB had a good signal       Thursday (March 17) on 17 meters from 1300-1500Z and quite a few USA       stations, including me, were getting thru the European pile for a       new one."              NASA has a video at http://www.youtube.com/watch?v=aTBgHd8exI4       explaining the very low sunspot activity over the past few years.              MIT Technology Review at       http://www.technologyreview.com/blog/arxiv/26568 has an article       about the double-peak of many sunspot cycles.              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 March 17 through 23 were 45, 35, 48, 47, 34, 31,       and 46, with a mean of 40.9. 10.7 cm flux was 90.1, 87.6, 88.8, 92,       101, 99.8, and 104.6, with a mean of 94.8. Estimated planetary A       indices were 3, 2, 4, 4, 4, 6, and 10, with a mean of 4.7. Estimated       mid-latitude A indices were 2, 2, 2, 4, 4, 5, and 9, with a mean of       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.              DO you offer a ham radio related service via fidonet? We       post a notice in the ls_arrl echo every 90 days describing       fidonet ham radio services and echomail conferences.              Send netmail to infoserv at fidonet 1:116/901 and describe       the service you offer. If an echomail conference not       available via the various backbone systems please tell those       interested wehre to link in. OTherwise, give the reader       enough information to get started using your service.                            ---        * Origin: RRN BBS: Your fidonet ham radio connection! (1:116/901)    |
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