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|    Message 273 of 3,036    |
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|    ARLP017    |
|    29 Apr 11 15:51:40    |
      SB PROP @ ARL $ARLP017       ARLP017 Propagation de K7RA              ZCZC AP17       QST de W1AW        Propagation Forecast Bulletin 17 ARLP017       From Tad Cook, K7RA       Seattle, WA April 29, 2011       To all radio amateurs               SB PROP ARL ARLP017       ARLP017 Propagation de K7RA              Geomagnetic conditions are quiet this week, but may become slightly       unsettled over this weekend. Average daily sunspot numbers were       down over 18 points to 74.9, while average daily solar flux was off       less than four points to 113.4.              Predicted solar flux values for today and tomorrow, April 29-30 are       110, May 1-8 is 105, 110 on May 9 and 115 on May 10. The next peak       in solar flux is May 11-13 with a value of 120. This is actually       higher than the flux values over the last month, except for one day,       April 15, at 129. Over the last three days five new sunspot groups       emerged. Daily sunspot numbers fell over April 22-27, then rose to       71 on April 28.              Predicted planetary A index for April 29 to May 3 is 5, 10, 12, 10       and 8, then 5 on May 4-7, then 8, 15, 15, 7 and 5 on May 8-12. So       the two periods in the short term with unsettled to active       geomagnetic conditions are May 1 and May 9-10.              Geophysical Institute Prague predicts quiet conditions on April 29,       unsettled to active on April 30, unsettled May 1-2, quiet to       unsettled May 3, and quiet May 4-5.              Angel Santana, WP3GW of Trujillo Alto, Puerto Rico feels that the       good old days are back for twenty meters. He wrote, "On World       Amateur Radio Day at 0304-0630 UTC on 20 meters, worked 22 stations       from Europe and the Pacific, including VK, ZL, FO and NH7 all on SSB       (and so on to get my WARD Award). When working Europe it looked like       it was 3-4pm local time, something I have not experienced for a long       time! Then on this past holiday weekend I deliberately lost sleep to       see how the band was, and it worked the same way: worked a P29, SV1       and a few more Europeans, and also looking at PSK31, wow, seeing the       same activity, something not seen two months ago. Propagation is       really turning on, making 20 meters the 24 hour band again. Plus on       Easter Day at 0845 UTC worked T31A in 40 meters, a new DXCC country       for me! Right now at 0850 UTC April 26th I am hearing ON4UN working       lots of VKs."              Rol Anders, K3RA of Elkridge, Maryland (southwest of Baltimore) also       likes 20 meters lately. He wrote, "On Easter Sunday morning (April       24), there was an excellent long path opening on 12 meters to VR2       and BV from 1200-1230z. I worked VR2XMT on phone with my antenna on       the long path, then tuned down to CW and heard BU2AQ working Asiatic       Russians and Eastern Europeans. He was moderately strong and very       solid. I could not hear the stations he was working, but they were       all given 599 reports by BU2AQ. I heard no other USA stations       calling him for the first 10 minutes or so. A PY was trying,       unsuccessfully, but neither he nor I could break the Asia/Europe       'wall.' Eventually several other stations in the US heard him, but       we all failed to break through. He started to fade at 1225z in       Maryland. However, around 1230z, some W8s and W4s got through, and       he worked a number of them, but by that time he was very weak in       Maryland.              "Also, I am hearing a return of the LP on 20 to SE Africa around       1200z. I haven't heard that opening for years.              "Isn't it great to have 20 meters being an all-day DX band again?"              Rich Dowty, W7EET of St. Paul, Oregon sent info on an interesting       tool called "PSK Reporter." See the web site at       http://pskreporter.info and also their map utility at       http://pskreporter.info/pskmap.html. The map displays stations using       digital modes on HF who are tied into the reporting network. The       user can click on any of the balloons to display a callsign for a       monitor at that location, then enter that call in a query above the       map to display all the stations that it could hear over a specified       period of time. You can also click in the balloon on "Show all seen       by" link. With the ability to check links on different bands and       over different time periods, this is an interesting and useful tool       for observing HF propagation.              There are some interesting videos showing use of this tool at       http://www.youtube.com/watch?v=gMPUmRG7GqkNR=1,       http://www.youtube.com/watch?v=w7trCDxJMZs, and       http://www.youtube.com/watch?v=zkvOZJIqLTQ.              Last week's Propagation Forecast Bulletin ARLP016 mentioned Bud       Trench, AA3B of Boyertown, Pennsylvania. At       http://www.qrz.com/db/aa3b you can see some detail on his radios and       antenna system.              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 April 21 through 27 were 100, 103, 80, 78, 67,       57, and 39, with a mean of 74.9. 10.7 cm flux was 113, 114.8, 119.1,       117.2, 112.1, 109.4, and 107.9, with a mean of 113.4. Estimated       planetary A indices were 5, 6, 6, 6, 6, 3, and 3, with a mean of 5.       Estimated mid-latitude A indices were 4, 3, 4, 6, 2, 1, and 0, with       a mean of 2.9.       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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