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|    Message 333 of 3,036    |
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|    ARLP025    |
|    24 Jun 11 19:35:14    |
      SB PROP @ ARL $ARLP025       ARLP025 Propagation de K7RA              ZCZC AP25       QST de W1AW        Propagation Forecast Bulletin 25 ARLP025       From Tad Cook, K7RA       Seattle, WA June 24, 2011       To all radio amateurs               SB PROP ARL ARLP025       ARLP025 Propagation de K7RA              Over the past week (June 16-22) the average daily sunspot number       rose nearly 20 points to 55, and average daily solar flux readings       increased by nearly 9 points to 98.6. All geomagnetic indices       declined slightly. These increases or decreases are relative to the       previous seven days, before June 16.              For the past month we've been looking nervously toward ARRL Field       Day, because a forecast from NOAA and USAF showed possibly unsettled       geomagnetic conditions on Friday, June 24, and continuing through       Field Day weekend.              The forecast has evolved from troubling to frightening, and back       again. Early in June the predicted planetary A index for June 24-26       was 18, 18 and 15. Then on June 7 it changed to 15, 15, and 10, a       little better. Then a week later things looked even more promising       on June 14 at 15, 10 and 5. But on June 17 it was revised upward, to       30, 15 and 5. A planetary A index of 30 indicates a geomagnetic       storm.              The next day on June 18 the forecast shifted to 25, 18 and 8, and on       June 19 it changed again to 25, 18 and 10. June 20 saw a slight       change to 25, 18 and 8 again, then June 21 it shifted to 15, 40 and       25. An A index of 40 on the first day of Field Day sounds ominous.       Then June 22 it changed again to 30, 10 and 10, and now the June 23       prediction for June 24-26 shows a planetary A index of 30, 18 and       12.              Basically we would love to see the A index as low as possible, five       or less would be wonderful. The latest news is that the solar wind       from a Coronal Mass Ejection which occurred on the solstice is       moving slower than originally thought, which means a weaker effect       here on Earth. A planetary K index of 5 is expected when the storm       arrives, now predicted at 0700z on June 24, which is 35 hours before       the start of Field Day, 1800z on June 25.              At 0640z on June 23, the Australian IPS Radio and Space Services       released a bulletin stating that increased geomagnetic activity is       expected on Jun4 23-24 due to the coronal mass ejection, but that       the effect on June 23 is expected to be mild, with a small chance of       isolated storm periods.              Geophysical Institute Prague predicts active conditions June 24,       unsettled to active on June 25, quiet to unsettled June 26-27, and       quiet on June 28-30.              The last forecast before Field Day should be on Friday, June 24,       released after 2100z. Check       http://www.swpc.noaa.gov/ftpmenu/forecasts/45DF.html and also       http://www.swpc.noaa.gov/ftpdir/indices/DGD.txt for the latest K       indices. The similar       http://www.swpc.noaa.gov/ftpdir/indices/DSD.txt shows you solar       flux, sunspot number, and other data such as sunspot area.              The most recent forecast from USAF and NOAA has solar flux at 95 on       June 24-25, 90 on June 26-30, 85 on July 1, and 95, 93 and 90 on       July 2-4 Predicted planetary A index for June 24-26 is 30, 18, and       12, 8 on June 27-28, and 5 on Jun 29 through July 1.              Ron Zond, K3MIY of Clarion, Pennsylvania found an interesting       article in an old QST from a half century ago. John Chambers, W6NLZ       published "After Sunspots - What?" on pages 66-67 in the March 1960       QST. I was about to dig out that old issue when I remembered that       ARRL members can access an archive of QST magazines running from       December 1915 to December 2007 at       http://www.arrl.org/arrl-periodicals-archive-search. I just       searched on Name: Chambers Call: W6NLZ Year: 1960 and went right to       it.              This article was written just after the peak of Cycle 19 (which was       huge!) and in it the author speculates on what a future with little       or no sunspots might hold.              I thought W6NLZ seemed like a familiar call from my childhood, and       he was known back then for his VHF records establishing contact with       KH6UK. Check out       http://wy6k.com/Shack%20Photos/1961/Great%20Shack%20Photos%20196       %20Page%202.htm       for photos of both of them.              Thanks to Howard Lester, N7SO of Schuylerville, New York, K3CWF and       a number of others who sent in this article from Sky & Telescope       about disappearing sunspots:       http://www.skyandtelescope.com/community/skyblog/newsblog/123844859.html.       Howard notes that there is no mention of the dissenting view.              Jeff Hartley, N8II of Shepherdstown, West Virginia sent in his       observations on recent conditions: "Conditions have seemed down from       2-3 weeks ago, but there has been a decent amount of sporadic-E as       we near the peak of the season which seems to me to be right around       July 1 on average. Late into the evening openings to EU on 15 meters       and higher have been much rarer, but there was some good propagation       reported in the All Asia CW contest by others.              "Around 0100Z Sunday on 15 phone, I worked Jim, E51JD in Rarotonga,       South Cook with a S9 signal. He was only running 100W to a small low       tribander.              "Saturday June 18, I was active in the WV QSO party and the       sporadic-E continued to abound again this year as it did in 2010.       Not much was happening right at the 1600Z start, but by 1700Z skip       on 20 phone was short enough to work the other side of WV, southern       VA, and many in NC. I even worked a guy in Weaverville, NC in the       Smokies where I had stopped for breakfast a day ago - small world!       There were plenty of OH and KY stations for a while, then the band       opened to the northeast and even as close as DE about 140 miles from       here! I managed to work all states except AK and VT (propagation       and QSO total to neighboring NH was good) in a few hours. 10M was       not quite good enough to spend much time there while I was able to       operate, but at 0100Z there was double hop Es to CA, NV, and AZ.              "On Friday June 17 around 2200Z, 6 meters was open to FM5AA, FM5AN,       V44KAI, and FG5FR.              "There were about the normal amount of Es on 6 meters during the       June VHF contest with C6, VP9, a few double hop stations in the       Rockies and lots of 4s, 5s and southern 0s logged."              Lawrence, GJ3RAX of the Isle of Jersey observes: "I have had some       comments from Nick VE3OWV. I have known him for a long time as we       were at university together in England in the early 60s. He has also       noticed that, although the sunspots have been increasing recently,       the propagation has not improved in the way it did at a similar       stage of previous cycles. We have not been able to get back to our       skeds on 17 that we used to keep so email has had to do instead. He       did say that he has been having QSOs to Europe on 17 at about 11 to       12 pm my time. Normally I only look on the bands during the       afternoons so I will start checking them again at that time. I used       to enjoy late night QSOs when I was younger but my stamina is now       rather less than it used to be!"              Check out K9LA, Carl Luetzelschwab's Propagation column on pages       16-19 in the July 2011 issue of Worldradio, which you can download       for free at http://worldradiomagazine.com/. He talks about signal       comparisons on the air in the 1980s, and how to use some new tools       such as internet connected remote receivers and a reverse beacon       network for similar comparisons today.              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 June 16 through 22 were 62, 65, 67, 47, 43, 57,       and 44, with a mean of 55. 10.7 cm flux was 103.3, 104.3, 99.2,       99.1, 96.4, 95.1, and 92.9, with a mean of 98.6. Estimated planetary       A indices were 4, 11, 4, 4, 7, 10, and 12, with a mean of 7.4.       Estimated mid-latitude A indices were 3, 8, 4, 3, 7, 8, and 7, 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.              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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