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|    Daryl Stout to All    |
|    ARRL Propagation Bulletin    |
|    02 Jun 23 16:03:48    |
      TZUTC: -0500       MSGID: 486.fidonet-ls_arrl@1:2320/33 28df911a       PID: Synchronet 3.20a-Win32 master/1c63f4d2c May 24 2023 MSC 1929       TID: SBBSecho 3.20-Win32 master/1c63f4d2c May 24 2023 MSC 1929       BBSID: TBOLT       CHRS: ASCII 1              SB PROP @ ARL $ARLP022       ARLP022 Propagation de K7RA              ZCZC AP22       QST de W1AW        Propagation Forecast Bulletin 22 ARLP022       From Tad Cook, K7RA       Seattle, WA June 2, 2023       To all radio amateurs              SB PROP ARL ARLP022       ARLP022 Propagation de K7RA              Average daily solar flux values dropped over the past week, but       sunspot numbers were nearly the same, comparing May 25 to 31 to the       previous week.              Average daily solar flux declined from 161.2 to 155.3. Geomagnetic       indicators were quieter, with average daily planetary A index       declining from 17.1 to 7.3, and middle latitude numbers from 14.4 to       7.9.              Predicted solar flux is 160 on June 2, 155 on June 3-4, 150 on June       5-8, 130 on June 9-11, then 135, 140, 143, 145, and 150 on June       12-16, 155 on June 17-20, 150 on June 21-25, then 145, 140 and 135       on June 26-28 and 130 on June 29 to July 8.              Predicted planetary A index is 15, 12, 10 and 8 on June 2-5, 5 on       June 6-17, then 22, 15, 12 and 10 on June 18-21, 5 on June 22-24, 12       and 10 on June 25-26, then 5 on June 27-28, then 15, 12, 15, 10 and       8 on June 29 through July 3, then 5 on July 4 through the middle of       the month.              Weekly Commentary on the Sun, the Magnetosphere, and the Earth's       Ionosphere - June 1, 2023 from OK1HH.              "The Sun still surprises us, it has been in the habit for billions       of years, but we only observe it for a few hundred years. So, we       have a right to be surprised by what it is doing and what we can       observe with instruments on satellites and powerful solar telescopes       on Earth, including the largest four-metre one on the island of Maui       in Hawaii, which can see the very fine structures of sunspot nuclei.              "What's more, we're seeing spots on the far side of the Sun that are       so big, they affect the vibration of the whole Sun. But we can only       see their structure and predict possible flares after they appear on       the eastern limb of the solar disk, which was not at all the case       with the current most active AR3315, which did not appear there. It       emerged later, thereafter began to grow rapidly.              "Conversely, the source of the next big flare was hidden behind the       southeastern limb, and we only saw the prominence above it.              "Meanwhile, the larger groups of sunspots have mostly moved to the       western half of the solar disk. A large coronal hole in the southern       hemisphere now crosses the central meridian. This increases the       likelihood of geomagnetic disturbances starting on June 2."              Mike, AK7ML wrote:              "I recall in a movie about Pearl Harbor that they could not reach       Hawaii from stateside on HF and then they sent the message by cable       telegraph in routine status, so Pearl was not informed of the attack       in time.              "For years I have been able to work Australia in the morning and now       it is Indonesia that is workable instead!"              A story about a big sunspot:              https://www.fox9.com/news/giant-sunspot-ar3310-visible-earth              I've added information from this resource to the text appearing at       the bottom of every propagation forecast bulletin (this resource       comes from September 2002 QST):              https://www.arrl.org/files/file/Technology/tis/info/pdf/0209038.pdf              I was sad to learn that old friend Chip Margelli, K7JA became a       Silent Key on May 25. Chip was from the Seattle area, and first came       to my attention when he became proficient in the Japanese language       during high school, then specialized in running JA stations at the       old Rush Drake, W7RM contest station on Foulweather Bluff in Puget       Sound. At one time he may have been the most famous American ham in       Japan, or so I heard at the time.              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 .              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 May 25 through 31, 2023 were 121, 127, 125, 119,       153, 144, and 147, with a mean of 133.7. 10.7 cm flux was 152.1,       149, 156.9, 151.3, 154.4, 162, and 161.4, with a mean of 155.3.       Estimated planetary A indices were 11, 6, 4, 11, 4, 5, and 10, with       a mean of 7.3. Middle latitude A index was 11, 6, 5, 11, 5, 6, and       11, with a mean of 7.9.       NNNN       /EX       --- SBBSecho 3.20-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: 116/116 123/0 10 25 131 170 180 200 525 755 3001 135/115       SEEN-BY: 135/300 153/7715 154/10 30 40 50 700 218/700 840 220/70 90       SEEN-BY: 221/1 6 222/2 226/17 18 30 227/114 229/110 112 113 206 307       SEEN-BY: 229/317 426 428 470 664 700 240/1120 1200 250/1 266/512 267/800       SEEN-BY: 275/1000 282/1038 291/111 299/6 301/1 113 317/3 320/219 322/757       SEEN-BY: 335/364 341/66 342/200 396/45 460/58 467/888 633/267 280       SEEN-BY: 633/281 412 418 712/620 848 1321 770/1 100 340 772/210 220       SEEN-BY: 772/230 2320/0 33 105 304 401 3634/0 12 27 56 57 119 5001/100       SEEN-BY: 5005/49 5020/715 1042 4441 5030/49 5058/104 5061/133 5064/56       SEEN-BY: 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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