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|    Message 567 of 3,036    |
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|    ARLP004    |
|    27 Jan 12 22:25:10    |
      SB PROP @ ARL $ARLP004       ARLP004 Propagation de K7RA              ZCZC AP04       QST de W1AW        Propagation Forecast Bulletin 4 ARLP004       From Tad Cook, K7RA       Seattle, WA January 27, 2012       To all radio amateurs               SB PROP ARL ARLP004       ARLP004 Propagation de K7RA              This was another week in which average daily sunspot numbers       declined, but average daily solar flux increased.              Predicted solar flux is 120 on January 27-30, 125 on January 31       through February 2, 120 on February 3, 140 on February 4-8, 145 and       150 on February 9-10, 155 on February 11-13, 150 on February 14-19,       and 145 on February 20-23. That's right, the long anticipated short       term solar flux peak of 165 from February 17-21 is gone. The last       forecast which still held this number was on January 23 (see       http://www.swpc.noaa.gov/ftpdir/forecasts/45DF/012345DF.txt) and on       January 24       (http://www.swpc.noaa.gov/ftpdir/forecasts/45DF/012445DF.txt) it       changed.              Predicted planetary A index is 8 on January 27-28, 5 on January 29       to February 7, 8 on February 8-9, and 5 again on February 10-23.              At 0617 UTC on January 22 an impact from a coronal mass ejection       caused the high-latitude college A index to reach 38, and sparked       aurora. The index hit 38 again on January 25. On January 23 around       0400 UTC a powerful M9 solar flare erupted, and this was right on       the threshold of becoming an X-class flare. The CME hit Earth around       1500 UTC on January 24, causing bright aurora.              Watch a lovely video of the event:       http://www.youtube.com/watch?v=-ilr8p13A2o. Also check this British       report:       http://www.wired.co.uk/news/archive/2012-01/24/sunspot-explosion and       this one from Montreal:       http://montreal.ctv.ca/servlet/an/local/CTVNews/20120124/norther       -lights-solar-s       torm-120124/20120124/?hub=MontrealHome.              As this bulletin is being written early Friday morning, sunspot       group 1408 is facing Earth directly, but it is weak. Group 1402 is       passing below the western horizon, and 1410 is coming around from       the east.              At http://stereo.gsfc.nasa.gov/ it looks like a very active region       is all the way on the other side of the Sun, at the 180 degree       meridian.              Fritz Huttelmayer, WB2QWH of Cheektowaga (Buffalo) New York wrote:       "I just wanted to give you my observations of six meters during the       contest this past weekend. I have been on six a couple of times over       the past two years, running an Icom IC-703 Plus into a 40 meter       attic dipole. I am not a serious VHF operator, as I operate mostly       HF QRP CW.              "I listened in on some of the activity during the January VHF       contest. I heard a W4 in Florida exchange grid squares with a W7 in       the state of Washington. Also heard were stations from Indiana,       Nevada, Texas, etc. The band sounded more like 20 meters on a good       day. No wonder they call it 'The Magic Band.'"              Mike Schaffer, KA3JAW of Tampa, Florida sent an article about solar       flares. Read it at       http://www.nasa.gov/mission_pages/sunearth/news/classify-flares.html.              Mike also commented about a recent television signal he received       from XHTV (running 64 KW) in Mexico City: "On Tuesday, January 24 a       Mexican broadcaster on television channel 4 suddenly flashed upon       the screen for about five minutes (0002-0007 UTC) due to a       Sporadic-E flash event that produced a moderately strong signal       coming in with a color carrier and audio.              "The event occurred nine hours after the Coronal Mass Ejection had       hit the Earth's magnetic field at approximately 1500 UTC.              "Mexico City is 1,205 air mile distance at 245 degrees from my       location. The best part of an Es storm is that you do not have to       park your antenna at the precise azimuth toward the transmitter       tower site.              "In my case the antenna was aimed due south at 180 degrees, which       would be 65 degrees off the main beam."              Thanks, Mike!              Ron McCollum, W7GTF of Winthrop, Washington wrote to ask if I ever       heard any theories about the stock market correlating with the       sunspot cycle.              I have heard of the stock market theory, and various other       correlations with solar activity. Every time I hear of it, I think       back to my eighth grad math class, when the text had a chapter on       correlation, causation and post hoc fallacies. To illustrate, the       book displayed a graph comparing smoothed sunspot numbers with       cardboard box production in the United States. They seemed to track       quite closely.              K7SJB years ago swore that periods of social unrest tracked with       sunspot numbers. "Tad. Remember how much fun we had in 1968-1970?,"       Stan would insist. "And the mania in securities trading till the       1929 crash?"              I get a lot of mail asking about this sort of thing. I like to       recall a presentation by Dr. James Alcock - professor of psychology       at York University, Canada - at Skeptic's Toolbox in Eugene Oregon       about the mind as a belief engine. One of the concepts presented was       that the human brain is hard wired for correlation and belief, and       how this figures into the evolution of the brain.              This weekend is the CW portion of the CQ World Wide 160-Meter       Contest. Expect good conditions, with quiet stable geomagnetic       indicators and a temporarily declining sunspot number. You can find       details at http://www.cq160.com/.              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 January 19 through 25 were 117, 88, 102, 103,       108, 105, and 68, with a mean of 98.7. 10.7 cm flux was 157, 141.2,       141.6, 141, 144.3, 135.7, and 126.4, with a mean of 141. Estimated       planetary A indices were 3, 4, 6, 21, 9, 17, and 14, with a mean of       10.6. Estimated mid-latitude A indices were 1, 3, 6, 22, 7, 13, and       17, with a mean of 9.9.       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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