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