Just a sample of the Echomail archive
Cooperative anarchy at its finest, still active today. Darkrealms is the Zone 1 Hub.
|    LS_ARRL    |    Bulletins from the ARRL    |    3,036 messages    |
[   << oldest   |   < older   |   list   |   newer >   |   newest >>   ]
|    Message 349 of 3,036    |
|    Bulletin autopost to All    |
|    ARLP027    |
|    08 Jul 11 22:13:18    |
      SB PROP @ ARL $ARLP027       ARLP027 Propagation de K7RA              ZCZC AP27       QST de W1AW        Propagation Forecast Bulletin 27 ARLP027       From Tad Cook, K7RA       Seattle, WA July 8, 2011       To all radio amateurs               SB PROP ARL ARLP027       ARLP027 Propagation de K7RA              Average daily sunspot numbers for the past week dropped less than a       point (from 42 to 41.6) compared to the previous week, and average       daily solar flux was down over 5 points to 86.2.               Predicted solar flux for the near term is lower than of late, with       values at 88 for July 8, 90 on July 9-11, 92 on July 12-13, 94 on       July 14 then 90 on July 15-17, then 88 on July 18-21 and 86 on July       22-29.               Predicted planetary A index for July 8-13 is 7, 10, 5, 5, 7, and 7,       followed by 5 on July 14-18. This is followed by a rise in       geomagnetic activity on July 19-24 with planetary A index at 7, 8,       12, 15, 10 and 7.               The latest smoothed sunspot number prediction on page 13 at       http://www.swpc.noaa.gov/weekly/pdf/prf1870.pdf shows the numbers       for December 2010 through December 2011 slightly lower. Last month's       prediction showed smoothed sunspot numbers for that period at 30,       34, 38, 41, 45, 49, 54, 59, 63, 66, 68, 71 and 74. The latest has       the values for those same months changed to 29, 32, 36, 39, 43, 47,       52, 57, 61, 64, 66, 69 and 72. The reason that in July we see last       December's number change is because the smoothed sunspot number       represents an average of data over one year. The data for       approximately six months after December 2010 wasn't completely known       until the end of June, and each successive month after that contains       one more month of predicted data, instead of data that is actually       measured.               Geophysical Institute Prague predicts unsettled activity on July 8,       quiet July 9, unsettled July 10-11, quiet to unsettled July 12, and       quiet July 13-14.               NASA has a new (monthly) solar cycle prediction. Because these are       not archived and the URL never changes, tracking the updates can be       a bit daunting, but here are the changes from a month ago.               In paragraph 9, this sentence: "We find a starting time of May 2008       with minimum occurring in December 2008 and maximum of about 59 in       June/July of 2013" in last month's prediction changed to "We find a       starting time of October 2008 with minimum occurring in December       2008 and maximum of about 69 in June/July of 2013" in this month's.       So they now believe the cycle started five months later than       previously reported, and that the smoothed sunspot peak will be 10       points or seventeen percent higher. These are international sunspot       numbers, not the Boulder numbers used in this bulletin, which are       higher.               Also changed at the end of that same paragraph, from last month's       prediction: "At this phase of cycle 24 we now give 40 percent weight       to the curve-fitting technique of Hathaway, Wilson, and Reichmann       Solar Physics 151, 177 (1994). That technique currently gives       highly uncertain (but smaller) values to Ohl's method" to "At this       phase of cycle 24 we now give 50 percent weight to the curve-fitting       technique of Hathaway, Wilson, and Reichmann Solar Physics 151, 177       (1994). That technique currently gives somewhat uncertain (but       similar) values to Ohl's method" in the latest prediction. So 40       percent was changed to 50 percent, and "smaller" was changed to       "similar".               Joe Molon, KA1PPV of Stamford, Connecticut likes to play around with       lower power on digital modes, and was running 1.5 watts with PSK-31       at 0101z on July 1 when he worked Ukrainian station UX7MX on 20       meters. I think he must use a simple wire antenna, because when I       look at an image of his QTH using the hi-resolution images on Bing       Maps, I don't see a tower and Yagi. Or perhaps he uses a vertical.       Later that same evening he logged stations in Belarus and France.       You can see some nice photos of UX7MX if you log into QRZ.com and go       to http://www.qrz.com/db/ux7mx.               In the current July 2011 issue of CQ Magazine, Tomas Hood, NW7US for       his monthly Propagation column has this headline: "Don't Believe       the Pessimistic Forecasts!" complete with exclamation point. He       points out that predictions have been all over the place and are       revised frequently. He also notes that some might be tempted to       just turn off the radio because of forecasts, but this is       self-defeating, because if stations aren't listening and       transmitting, then there is nothing to work. I would also note that       while marvelous new tools for solar observation exist now that even       a decade ago we didn't have, there just hasn't been enough data       (only 23 sunspot cycles so far) to make predictions with complete       reliability. Maybe after another millennia!               On his website (http://prop.hfradio.org/) NW7US has similar info to       material in his column about the importance of x-rays in enhancing       ionospheric propagation. Just page down a little way to "More about       Background X-rays".               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 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 30 through July 6 were 34, 51, 54, 42, 44,       30, and 36, with a mean of 41.6. 10.7 cm flux was 89.2, 87.6, 85.6,       86.2, 85, 84.8, and 84.6, with a mean of 86.1. Estimated planetary A       indices were 6, 13, 6, 8, 11, 14, and 8, with a mean of 9.4.       Estimated mid-latitude A indices were 3, 7, 3, 6, 7, 8, and 7, with       a mean of 5.9.       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)    |
[   << oldest   |   < older   |   list   |   newer >   |   newest >>   ]
(c) 1994, bbs@darkrealms.ca