SB PROP @ ARL $ARLP010 ARLP010 Propagation de K7RA ZCZC AP10 QST de W1AW Propagation Forecast Bulletin 10 ARLP010 From Tad Cook, K7RA Seattle, WA March 5, 2021 To all radio amateurs SB PROP ARL ARLP010 ARLP010 Propagation de K7RA We saw one day (Monday) with no sunspots during this week, so average daily sunspot numbers declined slightly from 19.6 to 18.9. Two new sunspot groups (2806 and 2807) appeared on the following day. Average daily solar flux remained about the same, increasing slightly during the reporting week (February 25 through March 3) from 75.7 to 76.7. Average daily planetary A index softened slightly from 16 to 14.7, and the middle latitude average went from 12.4 to 10.4. Geomagnetic indicators remained somewhat active due to persistent solar wind. The most active day was Monday, when Alaska's High Latitude College A index reached 34. Spaceweather.com reported a G2 class geomagnetic storm on Monday, aided by a significant crack in Earth's magnetic field. Although activity was otherwise moderate this week, the March 1 event was the largest storm since a G3 event 94 weeks earlier, on May 14, 2019. Predicted solar flux for the next 30 days is 80 on March 5, 78 on March 6, 78 on March 7-9, 72 on March 10-11, then 71, 72, 70, 71, 72 and 71 on March 12-17, then 73, 76, 75, 76, 78 and 81 on March 18-23, then 80 on March 24 and 25, then 79, 78 and 73 on March 26-28, 74 on March 29-30, 73 on March 31 through April 1, and 74 on April 2-3. Predicted planetary A index is 10, 20 and 15 on March 5-7, 10 on March 8-9, then 8, 5, 15, 10 and 5 on March 10-14, then 15, 8, 5 and 18 on March 15-18, 20 on March 19-20, then 18, 12, and 8 on March 21-23, 5 on March 24-27, then 20, 15 and 10 on March 28-30, 5 on March 31 and April 1, then 12 on April 2, and 5 on April 3-7. Geomagnetic activity forecast for the period March 5-30, 2021 from OK1HH. "Geomagnetic field will be, quiet on: March 9-10, 14, (26-27) quiet to unsettled on: March 5, 16-17, 25 quiet to active on: March 7-8, 11, 13, 15, 20-24 unsettled to active: March 12, 29 active to disturbed: March 6, 18-19, 28, 30 "Solar wind will intensify on: March (5-9, 12-14, 16-22, 27,) 28-29. "Remarks: - Parenthesis means lower probability of activity enhancement. - Predictability of changes remains low." W6MVT reports a surprising 10 meter opening to South America on the same Tuesday when sunspots re-appeared. "It never hurts to turn on 10 meters or check the spots on DXMaps or your favorite spotter. I saw some action and was pleased I was at the radio. On March 2 around 2130 UTC 10 meter SSB was alive with South American stations and a good path to those of us in Southern California. With 100w and a rotatable dipole only up 20 feet I was able to log LU4DJB, PU2LUC, PY2EX, PY5QW, PU2SDX and PY4NY in rapid succession, all with good reports both ways. Things faded out around 2200 UTC, but I was glad I caught it. W6MVT." Larry, K8MU sent this article concerning a space plasma hurricane: https://phys.org/news/2021-03-space-hurricane.html Don't miss Larry's page on QRZ.com, showing lines and arrows with humorous text about his modest station, complete with steerable ground plane and incoming QSL receptacle. This is from an email exchange with Frank Donovan, W3LPL regarding "Total Sunspot Area" which is shown daily along with SFI and SSN (Sunspot Number) in this table: ftp://ftp.swpc.noaa.gov/pub/indices/DSD.txt (SFI is 10.7 cm solar flux, uHem (micro-Hem) is solar micro-hemispheres, and EUV is extreme ultra-violet radiation.) "Here are some additional insights regarding total sunspot area. "SFI and total sunspot area are well correlated with each other and with EUV flux at the wavelengths that ionize the F2 region. "Daily sunspot number is not well correlated because tiny sunspots greatly affect it but they have no effect on HF propagation. I usually ignore daily sunspot numbers unless total micro-Hem exceeds 200. "Today is a classic case with daily SISLO sunspot number of 30 but total sunspot area is under 100 micro-Hem and SFI is stuck at 75. "Roughly 100 micro-Hem elevates the SFI into the mid 70s, but has only a minor effect on HF propagation. "200 micro-Hem roughly corresponds to SFI of 80 and usually improves 17 and 15 meter propagation. But the normal daily variability of F2 MUFs is not well correlated to SFIs of about 80 and often swamps out the expected improvements from SFI of 80. "HF MUFs increase more consistently when the SFI approaches 90. You may recall active region 12786 area was as high as 1000 micro-Hem last November and the SFI was above 100 for nine days. It greatly improved 15 meter propagation during the CQWW CW DX Contest and there was significant 10 meter DX propagation too. Daily sunspot number varied wildly from 40 to 94 during this period mostly because there were also three smaller active regions at during the period when 12786 was by far the most significant contributor to SFI greater than 100. "The rough equivalencies are: "uHem SFI 100 75 200 80 400 90 600 100 800 110 1000 120 1200 130 1400 140 1500 150 1600 160 1800 170 2000 180" This weekend is the ARRL International SSB DX Contest. See http://www.arrl.org/arrl-dx for details. NASA video of solar flare from Science Times: https://bit.ly/3re3WP7 A recent video forecast from Dr. Tamitha Skov, WX6SWW: https://youtu.be/j1rSS9iVsK4 If you would like to make a comment or have a tip for our readers, please email the author at, k7ra@arrl.net . For more information concerning radio propagation, see http://www.arrl.org/propagation and the ARRL Technical Information Service web page 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 February 25 through March 3, 2021 were 31, 16, 14, 13, 0, 28, and 30, with a mean of 18.9. 10.7 cm flux was 80.1, 80.1, 79.2, 77.7, 71, 74.7, and 74.2, with a mean of 76.7. Estimated planetary A indices were 13, 11, 4, 6, 26, 20, and 23, with a mean of 14.7. Middle latitude A index was 13, 8, 3, 4, 16, 14, and 15, with a mean of 10.4. NNNN /EX