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|    ARRL Propagation Bulletin    |
|    28 Jul 23 17:07:23    |
      TZUTC: -0500       MSGID: 617.fidonet-ls_arrl@1:2320/33 29297484       PID: Synchronet 3.20a-Win32 master/777fb6d8b Jun 13 2023 MSC 1929       TID: SBBSecho 3.20-Win32 master/777fb6d8b Jun 13 2023 MSC 1929       BBSID: TBOLT       CHRS: ASCII 1              SB PROP @ ARL $ARLP030       ARLP030 Propagation de K7RA              ZCZC AP30       QST de W1AW        Propagation Forecast Bulletin 30 ARLP030       From Tad Cook, K7RA       Seattle, WA July 28, 2023       To all radio amateurs               SB PROP ARL ARLP030       ARLP030 Propagation de K7RA              Average daily sunspot numbers declined slightly over the past week       (July 20-26) to 128.1, compared to 130.6 over the previous seven       days.              Average daily solar flux declined significantly from 190.5 to 172.2.              The solar flux forecast sees values at 165 and 162 on July 28-29,       158 on July 30-31, then 155 on August 1-3, then 165, 170 and 175 on       August 4-6, 180 on August 7-10, 175 on August 11-13, 180 on August       14-15, 175 on August 16-18, 170 on August 19, then 165, 165 and 160       on August 20-22, and 155 on August 23-26, 160 on August 27, 165 on       August 28-30, 170 and 175 on August 31 through September 1, and 180       on September 2-6.              Predicted planetary A index is 5 on July 28-29, 15 and 10 on July       30-31, 5 on August 1-3, 8 on August 4, 5 on August 5-9, 10 on August       10, 8 on August 11-13, 5 on August 14-19, then 10, 8 and 5 on August       20-22, 12 on August 23-24, 10 on August 25-26, 5 on August 27-29, 10       and 8 on August 30-31, and 5 on September 1-5.              Weekly Commentary on the Sun, the Magnetosphere, and the Earth's       Ionosphere -- July 27, 2023 from OK1HH.              "The likelihood of more massive solar flares has slowly decreased in       recent days as large groups of spots have fallen behind the western       limb of the solar disk and the magnetic configuration of the        remaining regions has become increasingly simple over the past few       days.              On July 20 and 21, two CMEs struck Earth's magnetic field in       accordance with the prediction. However, both impacts were weak and       did not produce even a minor geomagnetic storm.              Another weak halo CME was expected to leave the Sun on 23 July at       about 1530 UTC in a C5 class flare in spot group AR3376, coinciding       with the outburst of a relatively nearby magnetic filament. The       Earth's magnetic field detected its arrival at 0200 UTC on 26 July.       The result was an increase in geomagnetic activity and a       deterioration of shortwave propagation conditions. The disturbance       actually started on 25 July at 2235 UTC, but it was not clear       whether it was an early arrival of the same CME or another one that       we did not detect.              Note: since I will be abroad next week, I will not post the next       comment on August 3, but on August 10."              Sunspots, flares and aurora. https://bit.ly/44JxcRp              Mars Rover sees the far side of the sun. https://bit.ly/3KbRV8b              Rocket punches hole in ionosphere. https://bit.ly/3KceBFB              Nearly five decades ago I witnessed the same thing, viewed from       Marin County, California. It was a huge dramatic display, My friend       had seen it before, and said it was created by a rocket launch from       Vandenberg AFB in Southern California.              Another CME. https://bit.ly/44LhRjx              On July 27, Spaceweather.com sent this alert:              "A STRONG FARSIDE CME JUST HIT SOLAR ORBITER: Europe's Solar Orbiter       just got hit by the kind of CME that may have once caused a major       power blackout on Earth. This time, Earth was not in the line of       fire. It was a farside eruption that flew away from our planet.       Maybe next time?"              Massive flare? https://bit.ly/3Ya7OSC              Latest from Dr. Tamitha Skov. https://youtu.be/cD5VbWvBXsE              Send your tips, reports, observations, questions and comments to       k7ra@arrl.net. When reporting observations, don't forget to tell       us which mode you were operating.              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 .              Also, check this article from September, 2002 QST:              https://www.arrl.org/files/file/Technology/tis/info/pdf/0209038.pdf              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 July 20 through 26, 2023 were 131, 121, 103,       117, 141, 137, and 147, with a mean of 128.1 10.7 cm flux was       184.3, 172.8, 174.4, 172.5, 165.1, 169, and 167.4, with a mean of       172.2. Estimated planetary A indices were 10, 13, 9, 6, 7, 11, and       21, with a mean of 11. Middle latitude A index was 10, 11, 9, 5, 8,       12, and 23, with a mean of 11.1.       NNNN       /EX       --- SBBSecho 3.20-Win32        * Origin: The Thunderbolt BBS - Little Rock, Arkansas (1:2320/33)       SEEN-BY: 1/123 15/0 90/1 105/81 106/201 123/131 153/7715 154/10 203/0       SEEN-BY: 218/700 840 220/70 221/1 6 360 226/17 30 227/114 229/110       SEEN-BY: 229/112 113 206 307 317 426 428 470 664 700 240/1120 1634       SEEN-BY: 240/5832 8001 8002 8005 266/512 267/800 280/5003 5006 282/1038       SEEN-BY: 291/111 301/1 313/41 317/3 320/219 322/757 335/364 341/66       SEEN-BY: 342/200 371/0 396/45 423/81 460/58 633/267 280 281 412 418       SEEN-BY: 712/620 848 770/1 100 340 772/210 220 230 3634/12 5020/400       SEEN-BY: 5075/35       PATH: 2320/33 105 154/10 3634/12 240/1120 280/5003 221/1 6 218/840       PATH: 770/1 712/848 633/280 229/426           |
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