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|    Daryl Stout to All    |
|    ARRL Propagation Bulletin    |
|    04 Nov 22 10:30:14    |
      TZUTC: -0500       MSGID: 275.fidonet-ls_arrl@1:2320/33 27ca6719       PID: Synchronet 3.19c-Win32 master/fb4e4ce96 Oct 25 2022 MSC 1929       TID: SBBSecho 3.15-Win32 master/fb4e4ce96 Oct 25 2022 MSC 1929       BBSID: TBOLT       CHRS: ASCII 1              SB PROP @ ARL $ARLP044       ARLP044 Propagation de K7RA              ZCZC AP44       QST de W1AW        Propagation Forecast Bulletin 44 ARLP044       From Tad Cook, K7RA       Seattle, WA November 4, 2022       To all radio amateurs              SB PROP ARL ARLP044       ARLP044 Propagation de K7RA              Solar activity perked up this week. Average daily sunspot number       rose from 58.4 to 70.3, and solar flux averages increased from 113.3       to 129.9.              There are still problems with the Fredericksburg magnetometer, so I       used numbers from the Boulder, Colorado magnetometer for the middle       latitude A index.              At 2318 UTC on November 3, 2022 the Australian Space Weather       Forecasting Centre issued a geomagnetic disturbance warning:              "Increased geomagnetic activity expected due to coronal hole high       speed wind stream from November 4-5."              Planetary A index averages went from 19.4 to 13.7, and middle       latitude numbers changed from 9.1 to 14.3.              The solar flux prediction shows the highest values over the next       week, starting with 130 on November 4, then 135 on November 5-6,       then 130, 135, 130, and 125 on November 7-10, 115 on November 11-12,       112 on November 13-14, 110 on November 15, 108 on November 16-18,       104 on November 19, 100 on November 20-23, 98 on November 24-25,       then 100, 105, 105 and 110 on November 26-29, then 112 on November       30 through December 2, then 118 on December 3-6, 115 on December       7-9, and 112 on December 10-11.              Predicted planetary A index is 22. 30, 15, and 8 on November 4-7, 5       on November 8-10, then 18 and 15 on November 11-12, 5 on November       13-17, then 25, 15 and 8 on November 18-20, 5 on November 21-22,       then 8, 15 and 25 on November 23-25, 15 on November 26-27, then 18,       12, 10, 12, 20 and 15 on November 28 through December 3, then 5 on       December 4-6, 18 on December 7-8, 15 on December 9, and 5 on       December 10-14, and 25 on December 15.              F.K. Janda, OK1HH wrote:              "The evolution of solar activity, the Earth's magnetic field and the       state of the ionosphere in recent days has been varied, but not easy       to describe in a concise way (which is my aim).              "The reason for this is the variability of the evolution and the       absence of energetically significant phenomena.              "A week ago, there were five quiet sunspot groups on the Sun. None       of them posed a threat of strong flares. All had stable magnetic       fields that did not look like they would result in an eruption.              "Then, on the far side of the Sun, a sunspot appeared so large that       it changed the way the Sun vibrated.              "Helioseismic maps revealed its acoustic echo several days beyond       the Sun's northeastern edge. What mattered to us was that it was       about to appear at the northeastern limb of the Sun's disk.              "On October 26, we were delighted to see the Solar Dynamics       Observatory (SOD) satellite, which is in geostationary orbit,       studying the Sun's influence on planet Earth and the surrounding       universe.              "Most important for the forecast is the SDO/AIA image of coronal       holes, which may alert us to the possibility of an ionospheric       disturbance. We were cheered up by the fact that the Sun looks like       a jolly smiley face or a Halloween pumpkin, seen on       https://bit.ly/3fB1VvQ, just days before Halloween!              "A cheerful image, created by coronal holes in the Sun's atmosphere,       but mainly spewing a triple stream of solar wind toward Earth.              "Solar wind data from NOAA's DSCOVR spacecraft indicated that a       small, unexpected CME may have impacted Earth's magnetic field on       October 28 around 1400 UTC. A G1-class geomagnetic storm followed       after midnight UTC on October 29 after Earth entered the solar wind       stream flowing from the merry hole in the solar atmosphere.              "(The DSCOVR spacecraft is the Deep Space Climate Observatory. See       https://bit.ly/3E2yWKV )              "Further, there were only four sunspots on the Sun, all of which had       stable magnetic fields that were unlikely to explode.              "Another flare took place on November 1 on the far side of the Sun.       The eruption hurled a CME into space. The blast site will flip to       the Earth side of the Sun in about a week.              "Watch for a larger coronal hole that has since moved to the Sun's       western hemisphere. Minor G1-class geomagnetic storms may result on       November 5, when a solar wind stream is expected to hit Earth's       magnetic field. Which will definitely affect shortwave propagation       conditions. Ideally, and with appropriate timing (daytime, ideally       afternoon), a significant improvement in the positive phase of the       disturbance could follow."              Oleh, KD7WPJ of San Diego, California reported: "On November 1st I       worked 3 Japanese stations on 10 m CW at 2238-2248 UTC from       Dictionary Hill (SOTA W6/SC-366) in San Diego, CA. I used 40 watts       and a homemade vertical with 4 radials."              Solar blasts in the news:              https://bit.ly/3NxbY1v              A Jack-o-Lantern Sun:              https://www.popsci.com/science/nasa-smile-sun/              News about radio blackouts!              https://bit.ly/3fzEi6W              A smiley Sun:              https://bit.ly/3UmMRRd              New videos from Dr. Tamitha Skov, WX6SWW.              https://youtu.be/gO0wP6eiS8I              Part 3 of her mini-course:              https://youtu.be/-X-zE44x5Fk              This weekend is the ARRL CW Sweepstakes Contest, in which you work       domestic stations, and unlike ARRL Field Day, you do get multipliers       for sections worked. See https://www.arrl.org/sweepstakes for       details.              Send your tips, reports, observations, questions, and comments to       k7ra@arrl.net.              For more information concerning shortwave radio propagation, see       http://www.arrl.org/propagation and the ARRL Technical Information       Service at http://arrl.org/propagation-of-rf-signals . For an       explanation of 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 . More good       information and tutorials on propagation are at http://k9la.us/ .              Instructions for starting or ending email distribution of ARRL       bulletins are at http://arrl.org/bulletins .              Sunspot numbers for October 27 through November 2, 2022 were 72, 87,       97, 68, 56, 63, and 49, with a mean of 70.3. 10.7 cm flux was 129.7,       129.3, 133.9, 130.5, 127.9, 128.1, and 129.7, with a mean of 129.9.       Estimated planetary A indices were 9, 16, 26, 12, 11, 8, and 14,       with a mean of 13.7. Middle latitude A index was 6, 15, 24, 14, 12,       6, and 11, with a mean of 12.6.       NNNN       /EX       --- SBBSecho 3.15-Win32        * Origin: The Thunderbolt BBS - Little Rock, Arkansas (1:2320/33)       SEEN-BY: 1/120 123 15/0 18/0 50/109 90/1 105/81 106/201 116/17 18       SEEN-BY: 116/116 120/340 123/0 10 25 131 180 200 525 755 3001 135/300       SEEN-BY: 153/7715 154/10 30 40 50 700 218/700 840 220/70 90 221/1       SEEN-BY: 221/6 222/2 226/17 18 30 227/114 229/110 111 112 113 206       SEEN-BY: 229/317 424 426 428 470 664 700 240/1120 1200 250/1 266/512       SEEN-BY: 267/800 275/1000 282/1038 299/6 301/1 113 317/3 320/219 322/757       SEEN-BY: 335/364 341/66 342/200 396/45 460/58 467/888 633/267 280       SEEN-BY: 633/281 412 416 418 712/620 848 1321 770/1 100 340 772/210       SEEN-BY: 772/220 230 2320/0 33 105 304 3634/0 12 15 27 50 56 57 119       SEEN-BY: 4500/1 5001/100 5005/49 5020/715 1042 4441 5030/49 5054/8       SEEN-BY: 5058/104 5064/56 5075/128 5083/1 444 5090/958       PATH: 2320/33 105 154/10 3634/12 5020/1042 301/1 221/6 218/840       PATH: 770/1 712/848 633/280 229/426           |
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