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|    ARRL Propagation Bulletin    |
|    03 Feb 23 08:23:38    |
      TZUTC: -0600       MSGID: 335.fidonet-ls_arrl@1:2320/33 28425039       PID: Synchronet 3.19c-Win32 master/d1dfc9c1b Dec 7 2022 MSC 1929       TID: SBBSecho 3.15-Win32 master/d1dfc9c1b Dec 7 2022 MSC 1929       BBSID: TBOLT       CHRS: ASCII 1              SB PROP @ ARL $ARLP005       ARLP005 Propagation de K7RA              ZCZC AP05       QST de W1AW        Propagation Forecast Bulletin 5 ARLP005       From Tad Cook, K7RA       Seattle, WA February 3, 2023       To all radio amateurs              SB PROP ARL ARLP005       ARLP005 Propagation de K7RA              Solar activity softened again this week, with average daily sunspot       numbers changing from 162 to 80.7, and solar flux from 198.9 to       139.5.              This is quite a dramatic shift from the excitement of a couple of       weeks ago. To review, average weekly sunspot numbers from the first       Propagation Forecast bulletin of 2023 went from 97 to 135.9, 173.4       and 162. Average weekly solar flux from 157.8 to 181.2, 221.8 and       198.9.              This variability is expected. Soon, perhaps in the next solar       rotation, activity will rise again. The graphs we see of smoothed       sunspot numbers are smooth because the numbers are averaged over a       whole year.              Geomagnetic numbers barely changed at all, with planetary A index       shifting only from 8.1 to 7.9 and the middle latitude numbers did       not change at all, 5.9 last week and 5.9 this week.              Predicted solar flux is 135 on February 3, 140 on February 4-5, 145       on February 6, 150 on February 7-9, 155 on February 10-13, 150 on       February 14-16, 145 on February 17, 140 on February 18-19, 135 on       February 20, 130 on February 21-23, 125 on February 24-25, 140 on       February 26-27, 135 on February 28 through March 4, then 140 and 145       on March 5-6, 150 on March 7-8. and 155 on March 9-12.              Predicted planetary A index is 8, 5 and 5 on February 3-5, 10 on       February 6-7, 8 on February 8-9, then 12, 5, 8 and 8 on February       10-13, 5 on February 14-17, then 8, 7, 5 and 5 on February 18-21, 10       on February 22-24, 5 on February 25-27, then 15, 10 and 8 on       February 28 to March 2, and 5 on March 3-5, then 15 on March 6-8,       then 12, 8 and 7 on March 9-11 and 5 on March 12-16.              Weekly Commentary on the Sun, the Magnetosphere, and the Earth's       Ionosphere February 3-9, 2023 from F.K. Janda, OK1HH:              "January this year was another surprise in the development of Solar       Cycle 25, although we are still about two years away from its peak.       Sunspots have grown larger, while the configuration of the magnetic       fields that make them up has become increasingly complex, leading to       an increase in the number and intensity of eruptions, so far only       moderately powerful.              "Solar flux between 12 and 21 January was above 200, while the solar       wind increased.              "In the last week, after the large sunspot groups AR3190 and AR3192       fell behind the western limb of the solar disk, solar activity       decreased. Between January 27-29 and February 1, solar wind       intensified, apparently still blowing from the active regions that       had already set.              "Further, we expect an irregular evolution without major       fluctuations. Helioseismological observations show that the activity       of AR3190 and AR3192 continue on the Sun's far side. We'll have to       wait another week for their reappearance on the eastern limb."              Mike Schaffer, KA3JAW in Easton, Pennsylvania reports again on his       10 meter FM activity. He notes the daily solar flux dropped about       100 points from mid-January, but good 10 meter propagation       continues.              Daily from 1300-1600 UTC he has good propagation to Europe, and is       recently hearing Israel on 10 meter FM, about 5,700 miles away via       F2 propagation.              Mike notes, "Remember, 29.6 MHz is the national FM calling       frequency, after making the initial contact you should QSY to a       lower frequency, such as 29.5 or 29.49 MHz, to continue the QSO."              Jim Hadlock, posting to the email list for the Western Washington DX       Club noted that sunspot numbers recently hit a 9-year high.              Jim posted this from Spaceweather.com:              https://bit.ly/40DEzsj              Scott Avery, WA6LIE wrote:              "Today was a fluke on 10 meters FT8. I worked LA7HJA on FT8 on       Thursday February 2nd at 0041 UTC. He gave me a +04 and I gave him       a -13 dB report. Great reports and tried calling one other LA, but       no luck. I confirmed the QSO with his ClubLog.              "For the past month or so, European openings are from about       1500-1730 UTC here in California.              "Have no clue to the method of propagation on this late afternoon's       QSO. LP?              "I was just using a wire Delta Loop at 30' feedpoint, part of my       inverted Vees all common feedpoint.              "You know in this hobby you just got to be in the right place at the       right time!"              Toivo Mykkanen, W8TJM in Liberty Lake, Washington wrote:              "Just had the best Aurora Path into Scandinavia since we last spoke       last year. Today, 1 Feb, I was able to work 4 stations on SSB in       Finland from Eastern Washington and all of them were 10-15 dB over       S9 with a slight bit of flutter. It was 10 PM in Finland, well after       15 meters usually shuts down there. Was great to connect with my       heritage as my parents are from Finland. The Finnish stations were       working stations all across the USA and Canada."              Bil Paul, KD8JUI, recalling television reception at the peak of       Solar Cycle 19, wrote:              "We were in Wisconsin, around '58 or '59, and we could usually only       pick up with good reception two TV stations. One Sunday morning I       got up and switched on the TV. I started getting good reception from       the SE U.S., Georgia and Florida.              "As time went on, the skip gradually changed to receiving Alabama       and Mississippi, and finally ended with Texas. I'm not sure what       frequencies were being used for those channels (2 through 13) back       then."              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 January 26 through February 1, 2023 were 104, 84,       76, 80, 67, 65, and 89, with a mean of 80.7. 10.7 cm flux was 150.6,       144.9, 137.6, 137, 135.9, 137, and 133.5, with a mean of 139.5.       Estimated planetary A indices were 11, 9, 10, 5, 5, 9, and 6, with a       mean of 7.9. Middle latitude A index was 9, 6, 8, 5, 4, 6, and 3,       with a mean of 5.9.       NNNN       /EX       --- SBBSecho 3.15-Win32        * Origin: The Thunderbolt BBS - Little Rock, Arkansas (1:2320/33)       SEEN-BY: 1/123 15/0 90/1 105/81 106/201 116/17 18 120/340 123/10 131       SEEN-BY: 153/7715 154/10 30 40 50 700 218/700 840 220/70 90 221/6       SEEN-BY: 226/17 18 30 227/114 229/110 111 112 113 114 206 307 317       SEEN-BY: 229/424 426 428 470 664 700 266/512 267/800 282/1038 301/1       SEEN-BY: 317/3 320/219 322/757 342/200 396/45 460/58 633/267 280 281       SEEN-BY: 633/412 416 418 712/620 848 770/1 100 340 772/210 220 230       SEEN-BY: 2320/0 33 105 304 3634/12       PATH: 2320/33 105 154/10 221/6 218/840 770/1 712/848 633/280 229/426           |
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