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|    Message 706 of 3,036    |
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|    ARLP022    |
|    01 Jun 12 23:51:06    |
      SB PROP @ ARL $ARLP022       ARLP022 Propagation de K7RA              ZCZC AP22       QST de W1AW        Propagation Forecast Bulletin 22 ARLP022       From Tad Cook, K7RA       Seattle, WA June 1, 2012       To all radio amateurs               SB PROP ARL ARLP022       ARLP022 Propagation de K7RA              Average daily sunspot numbers sank more than 28 points this week       (nearly 26%) to 81.9. Average daily solar flux declined more than 16       points to 111.6. This is for the seven days of May 24-30, and is       compared to the previous seven days, May 17-23.              No new sunspots appeared over the five days of May 26-30, but on May       31, three new sunspot groups appeared. One day earlier the sunspot       number was 78, while the total relative sunspot area was 400. On May       31 those numbers dropped to 73 and 330, even with the new spots.              On May 30, sunspot groups 1486, 1488, 1490 and 1492 were in place.       By May 31, 1486 and 1488 disappeared, and new sunspot groups 1493,       1494 and 1495 emerged. But the total area of all visible spots was       less than the day before.              You can track the fading of sunspot groups and the emergence of new       ones at http://www.swpc.noaa.gov/ftpmenu/forecasts/SRS.html. The       dates shown are always for the new UTC day, the one following the       day for which the data is shown. So the report marked June 1 is       actually displaying data gathered on May 31.              In this report the area for each sunspot group is listed, and this       is expressed in millionths of a solar hemisphere. The total sunspot       area for the day, along with the sunspot number, is displayed along       with solar flux resolved to whole numbers at       http://www.swpc.noaa.gov/ftpdir/indices/DSD.txt.              The short term outlook is revised from the one given in yesterday's       ARRL Letter, with solar flux peaking around 125 on June 2-7, hitting       a minimum of 105 on June 27-28, then peaking at 120 on July 1-12.              The latest prediction has solar flux at 120 on June 1, 125 on June       2-7, 120 on June 8-15, 115 on June 16-18, 110 on June 19-26, and       105, 105, 110 and 115 on June 27-30, then 120 on July 1-12.              Predicted planetary A index is 5 on June 1-2, then 10, 15, 18, 15       and 10 on June 3-7, 5 on June 8-11, 8 on June 12-13, 5 on June       14-17, and 15, 12 and 8 on June 18-20, and 5 on June 21-25.              With the start of a new month, we can revisit our moving averages       for sunspot numbers. We've been observing a three-month moving       average, based on whole calendar months, so the latest average is       for March, April and May 2012. About a month ago we were reporting       for the months of February, March and April. It is a simple       arithmetic - with an accent on the third, rather than second       syllable - average, with a total of all sunspot numbers divided by       the number of days in the period.              So over September 1 through November 30, 2011, there were 91 days       and the sum of all daily sunspot numbers for that period was 10,808,       yielding an average daily sunspot number of 118.8 when the sunspot       number total is divided by the number of days. The next period       covered October 1 through December 31, 2011, with a total sum of all       daily sunspot numbers of 10,913 divided by 92 days, giving us an       average daily sunspot number of 118.6. That period in Fall 2011 had       the highest sunspot numbers seen so far in Cycle 24.              The three month moving averages of daily sunspot numbers for the       three month periods ending January 2010 through May 2012 were 15,       22.4, 25.7, 22.3, 18.5, 16.4, 20.4, 23.2, 28.9, 33, 35.6, 31, 30.1,       35.3, 55.7, 72.3, 74.4, 65.9, 61.5, 63, 79.6, 98.6, 118.8, 118.6,       110, 83.3, 73.7, 71.2, and 87.3. As you can see, the numbers are up       slightly over the past few months.              The monthly average sunspot numbers for February through May 2012       are 50.1, 78, 84.5 and 99.4.              Go to       http://phys.org/news/2012-05-science-nugget-solar-particles-infiltrating.html       to read an article on Ground Level Enhancements, or GLE, a rare       event in which a sudden rise in neutrons coincides with an energetic       solar flare or coronal mass ejection. A GLE detected on May 17 was       the first GLE of the current solar cycle.              Dave Blood, W1AFC of Oberlin, Ohio had some comments on WA8MEA's       recent query on LUF and MUF. Dave wrote, "MUF is affected by solar       UV light mostly and therefore is governed by the daily solar flux       levels. The LUF, as mentioned, is set by daytime absorption in the       D-region at about 100 km heights (hence by the number of radio wave       passes through it (up and down) and the number of ionospheric hops       supported by the F-region at 300 km heights). The absorption is       altered by the instantaneous X-ray radiation from the Sun and this       can vary up and down highly during solar flare activity. Radio       'Blackout' conditions occur when the absorption is so high that the       LUF exceeds MUF for any propagation path distance for long periods       from 20 minutes to several hours."              Dave worked for Raytheon for several decades on over-the-horizon       radar from 1960-1992. Dave has been a ham for 60 years.              Rick McCurdy, WA1GTP is in FN31si in Ivoryton, Connecticut. He       wrote, "On May 23 at 1550 UTC I received RADAR on 432.100, first       time in years! Heading was WSW from (Essex) New London/New Haven       CT area. Very few openings on 6 meters but April 30 worked short E       skip to VE2DLC, FN58rk, 527 miles. Also Florida openings May 24, not       much else."              We received another geomagnetic forecast from F.K. Janda, OK1HH. He       predicts quiet to active conditions on June 1, quiet on June 2,       quiet to unsettled June 3-4, quiet to active June 5, active June       6-7, quiet to active June 8-9, quiet to unsettled June 10, quiet       June 11-12, quiet to active June 13, mostly quiet June 14, quiet to       unsettled June 15-16, quiet to active June 17, mostly quiet June 18,       active June 19, and quiet to unsettled June 20-21.              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://myplace.frontier.com/~k9la/.              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 May 24 through 30 were 96, 86, 70, 83, 87, 73,       and 78, with a mean of 81.9. 10.7 cm flux was 115.5, 117.2, 110,       110.7, 110.3, 106.3 and 111, with a mean of 111.6. Estimated       planetary A indices were 8, 6, 4, 4, 6, 6, and 6, with a mean of       5.7. Estimated mid-latitude A indices were 11, 8, 5, 3, 3, 5, and 5,       with a mean of 5.7.       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.              We invite you to use and support the ham-fdn!       The ham-fdn is coordinated by Mark LEwis at fidonet 1:3634/12. Contact him       for further       information about ham-fdn file echoes. Announcements of newly       hatched ham-fdn files can be seen in the echoes ham and ham_tech.              THe ham-fdn is distributed by the International FIlegate project.       Ham-fdn file echoes are available from major hubs. Bbs users with an       interest in these file echoes should ask your sysop to carry them.              Users and sysops with materials appropriate for distribution       via the ham-fdn should contact the coordinator for submission       guidelines at the above shown address. IF you have access to       shareware programs that would be useful to radio amateurs,       or other files which may be appropriate use the back channel       area to submit them. IF you are not sure how to accomplish this       contact the fdn coordinator, or ask your local bbs sysop.                     ---        * Origin: RRN BBS: Your fidonet ham radio connection! (1:116/901)    |
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