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|    Message 2,775 of 3,036    |
|    Daryl Stout to All    |
|    ARRL Propagation Bulletin    |
|    23 Dec 22 10:41:59    |
      TZUTC: -0600       MSGID: 308.fidonet-ls_arrl@1:2320/33 280b118b       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: UTF-8 4              SB PROP @ ARL $ARLP051       ARLP051 Propagation de K7RA              ZCZC AP51       QST de W1AW        Propagation Forecast Bulletin 51 ARLP051       From Tad Cook, K7RA       Seattle, WA December 23, 2022       To all radio amateurs              SB PROP ARL ARLP051       ARLP051 Propagation de K7RA              I am writing this first draft of my penultimate bulletin of 2022,       about seven hours after the start of Winter Solstice in the Northern       Hemisphere, which was on Wednesday, December 21, 2022 at 2147 UTC.       It is very cold in Seattle, about 17 degrees F on the longest night       of the year.              Solar activity was down a bit from the previous week, although it       was one of those odd occasions when average daily sunspot numbers       and solar flux changed in opposite directions.              Average daily sunspot number declined from 136.9 to 124.1, while       solar flux rose from 150 to 153.8.              Two new sunspot groups emerged on December 17, one more on December       19, another on December 21, and two more on December 22.              Geomagnetic indicators were a bit lower, with average planetary A       index changing from 7.7 to 6.7, and middle latitude numbers from 6       to 5.1.              Due to missing data, I had to fudge one of the numbers, the December       16 middle latitude A index which I pegged at 7 by eyeballing trends.              Predicted solar flux appears to reach a short term peak of 160 on       January 4-7, 2023, which may repeat on the last day of January and       the first few days in February.              The forecast shows 130 on December 23-25, 135 on December 26–30,       138 on December 31, then 140, 150 and 155 on January 1-3, 2023, 160       on January 4-7, then 158, 156, 154, 154 and 152 on January 8-12, 150       on January 13-15, then 145, 130 and 120 on January 16-18, 118 on       January 19-20, then 120, 125 and 127 on January 21-23, 130 on       January 24-25, then 135, 138, 140, 150 and 155 on January 26, and       160 on January 31 through the first few days of February.              Predicted planetary A index is 8, 5 and 8 on December 23-25, 5 on       December 26-29, 10 and 12 on December 30-31, then 8, 5 and 18 on       January 1-3, 2023, 10 on January 4-5, then 8, 10 and 6 on January       6-8, 5 on January 9-14, then 12, 10 and 20 on January 15-17, then       12, 8, 5 and 18 on January 18-21, and 20 on January 22-24, then 12,       10, 12, 8 and 5 on January 25-29.              OK1HH writes:              "Over the past seven days, we observed up to seven sunspot groups on       the solar disk, three in succession had sizes and configurations       suggesting the possibility of an M-class flare.              "AR3165 fell behind the western limb on December 17, while we       observed AR3169 the same day. The largest AR3163 went over the limb       on December 22. Solar activity, both total and flare activity,       slowly decreased.              "A shock wave (probably the CME released by sunspot AR3165 last       week) hit Earth's magnetic field late on December 18, but a       geomagnetic storm did not develop, only a slight increase in       geomagnetic activity. This was repeated on December 21 and       especially the next day, when it was a recurrent disturbance,       repeated after about 27 days.              "Solar activity is likely to remain low until Christmas. The       situation may change next week, when one or more active sunspot       groups will appear on the eastern limb of the solar disk.              "Shortwave propagation was mostly above average with slightly       elevated MUF values. Diurnal variations were erratic. This pattern       will continue."              Jon, N0JK wrote:              "A strong sporadic-E opening on 50 MHz from Kansas to the Gulf Coast       Sunday December 18.              "I logged K3FM EM50, WA3GWK EM60, W5THT EM50, and N4UPX EM50 on       50.313 MHz FT8 around 1600 UTC with strong signals. My station was       100 watts and an attic dipole."              More big solar flare news:              https://bit.ly/3YHi5Wf              https://bit.ly/3PKXts4              https://bit.ly/3HXk1DW              https://bit.ly/3FPgipw              Found this interesting resource in the ARRL Letter:              https://haarp.gi.alaska.edu/diagnostic-suite              From Dr. Tony Phillips on cycles:              https://spaceweatherarchive.com/2022/12/              On Thursday using remotehamradio.com I made a 10 meter contact with       Ralph, VE3LOE. He sent me an email, which I have edited:              "About 2 years ago I was in touch with Scott McIntosh at the       National Center for Atmospheric Research in Boulder, CO, who made a       minority-opinion propagation forecast for Solar Cycle 25 which       suggests much higher solar activity than what his colleagues       predict. See 'Overlapping Magnetic Activity Cycles and the Sunspot       Number: Forecasting Sunspot Cycle 25 Amplitude' (text dated October       2020).              "The latest installment, entitled 'Deciphering Solar Magnetic       Activity: The (Solar) Hale Cycle Terminator of 2021,' which is at:              "https://arxiv.org/a/mcintosh_s_1.html              "I scanned this latter paper just now. Although I am a retired       engineer from the telecom sector with a PhD in statistical traffic       analysis of pre-Internet data networks, and understand the       statistical math used in these papers, I am not a propagation       expert. However, in the last publication, Figure 10 predicts a mean       SSN just under 200, higher than other expert predictions. This       present cycle has been interesting in its statistical variability.              "I am primarily a 10m enthusiast and use this band on a daily basis,       generally in the 1300-1700 UTC timeframe when the EU openings take       place. For some of my other ham interests and operating conditions       you can visit my QRZ.com page."              K7RA notes - download this pdf:              https://arxiv.org/pdf/2209.10577.pdf              A new report from Dr. Tamitha Skov, WX6SWW:              https://youtu.be/pU6i_2FVR2g              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 December 15 through 21, 2022 were 140, 108, 139,       128, 132, 119, and 103, with a mean of 124.1. 10.7 cm flux was       165.9, 163.1, 154.6, 155,6, 152.4, 146.4, and 138.7, with a mean of       153.8. Estimated planetary A indices were 5, 9, 3, 4, 11, 6, and 9,       with a mean of 6.7. Middle latitude A index was 4, 7, 2, 2, 9, 5,       and 7, with a mean of 5.1.       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: 317/3 320/219 322/757 342/200 396/45 460/58 633/267 280 712/620       SEEN-BY: 712/848 770/1 100 340 772/210 220 230 2320/0 33 105 304 3634/12       PATH: 2320/33 105 154/10 221/6 218/840 770/1 712/848 229/426           |
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