{"id":777741,"date":"2024-02-23T11:05:54","date_gmt":"2024-02-23T16:05:54","guid":{"rendered":"http:\/\/spaceweekly.com\/?p=777741"},"modified":"2024-02-23T11:05:54","modified_gmt":"2024-02-23T16:05:54","slug":"the-k7ra-solar-update-18","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=777741","title":{"rendered":"The K7RA Solar Update"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div>\n\t\t\t\t\t<span class=\"date\">02\/23\/2024<\/span><\/p>\n<p>&#8220;ASWFC GEOMAGNETIC DISTURBANCE WARNING ISSUED AT 0237 UTC\/22 FEBRUARY 2024 BY THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE.<\/p>\n<p>&#8220;A solar filament has erupted from the northwest solar quadrant and<br \/>a component of the predominately westward associated CME is expected<br \/>to arrive at the Earth during the second half of 24-Feb. G1 conditions, with the chance of G2 periods are possible during the second half of 24-Feb and first half of 25-Feb. Modeling shows the bulk of the CME missing the Earth.<\/p>\n<p>&#8220;INCREASED GEOMAGNETIC ACTIVITY EXPECTED DUE TO CORONAL MASS EJECTION FROM 24-25 FEBRUARY 2024.&#8221;<\/p>\n<p>Spaceweather.com wrote on February 22:<\/p>\n<p>&#8220;TWO MAJOR SOLAR FLARES: Giant sunspot AR3590 just unleashed two<br \/>major X-class solar flares. The double blast approximately coincided<br \/>with a widely reported outage of cell phone service; however,<br \/>experts agree that the flares were probably not responsible. More<br \/>flares are in the offing. The sunspot has an unstable &#8216;delta-class&#8217;<br \/>magnetic field, and it is turning toward Earth.&#8221;<\/p>\n<p>Sunspot numbers and solar flux values dropped over the past week,<br \/>with average daily sunspot numbers down from 134.6 to 84.4 and<br \/>average daily solar flux dropping from 190 to 164.<\/p>\n<p>Geomagnetic conditions were very quiet. Planetary A index declined<br \/>from the low value of 7.4 to 4.4, and middle latitude A index from<br \/>6.1 to 3.5.<\/p>\n<p>Only four new sunspot groups appeared, three on February 15 and one<br \/>on February 18.<\/p>\n<p>Spaceweather.com says all their content is written by humans, with<br \/>no Artificial Intelligence at all.<\/p>\n<p>I decided to ask an AI bot when Solar Cycle 25 will peak:<\/p>\n<p>From Gemini AI bot:<\/p>\n<p>&#8220;There are two main perspectives on when Solar Cycle 25 will reach<br \/>its maximum:<\/p>\n<p>&#8220;Original prediction:<\/p>\n<p>&#8220;An expert panel convened by NOAA, NASA, and ISES in 2019 predicted<br \/>a peak in July 2025 with a maximum sunspot number of 115.<\/p>\n<p>&#8220;This prediction assumed a similar strength to the weak Solar Cycle<br \/>24.<\/p>\n<p>&#8220;Revised prediction:<\/p>\n<p>&#8220;In October 2023, NOAA&#8217;s Space Weather Prediction Center (SWPC)<br \/>released a revised prediction based on observed activity. This new<br \/>prediction suggests a faster rise and higher peak, likely between<br \/>January and October 2024, with a sunspot number between 137 and 173.<\/p>\n<p>&#8220;However, it&#8217;s important to note that the timing could still fall<br \/>within the broad error range of November 2024 to March 2026.<\/p>\n<p>&#8220;So, the answer depends on which prediction you consider:<\/p>\n<p>&#8220;Original prediction: July 2025<\/p>\n<p>&#8220;Revised prediction: Between January and October 2024 (more likely<br \/>than July 2025).<\/p>\n<p>&#8220;It&#8217;s important to stay updated on the latest information as<br \/>scientists continue to monitor the Sun&#8217;s activity. You can find more<br \/>details and updates on the NOAA Space Weather Prediction Center<br \/>website:<\/p>\n<p>&#8220;https:\/\/www.swpc.noaa.gov\/products\/solar-cycle-progression<\/p>\n<p>&#8220;END AI BOT CONTENT.&#8221;<\/p>\n<p>I have bookmarked that last link.<\/p>\n<p>ISES stands for the International Space Environment Service.<\/p>\n<p>Here is a revised outlook for the next month, from USAF via NOAA.<\/p>\n<p>Predicted solar flux is 175 on February 23, 180 on February 24-29,<br \/>then 160 and 165 on March 1-2, 170 on March 3-9, 165 on March 10-16,<br \/>then 162, 160, and 165 on March 17-19, 170 on March 20-21, 172 on<br \/>March 22-23, 165 on March 24-26, and 155, 160, and 165 on March<br \/>27-29, and 170 on March 30 into the first week in April.<\/p>\n<p>Predicted planetary A index is 6, 5, 20 and 10 on February 23-26,<br \/>and 5 on February 27 through March 23, 8 and 7 on March 24-25, and 5<br \/>on March 26 through the first week in April.<\/p>\n<p>Weekly Commentary on the Sun, the Magnetosphere, and the Earth&#8217;s<br \/>Ionosphere &#8211; February 23-29, 2024 from F.K. Janda, OK1HH:<\/p>\n<p>&#8220;During the last seven days, based on helioseismological<br \/>observations we first expected the rise of a larger active region at<br \/>the northeastern limb of the solar disk.<\/p>\n<p>&#8220;Meanwhile, gradually most of the sunspot groups on its western half<br \/>have faded, whereby the solar flux has dropped to 152.<\/p>\n<p>&#8220;The larger active region came out, was designated AR3590, and is<br \/>large enough to observe with the naked eye (in relation to the area<br \/>over 700 millionths of the solar disk), for example, using a solar<br \/>eclipse filter. However, its beta-gamma magnetic configuration was<br \/>not conducive to larger flares. All the more surprising were two<br \/>successive X-class flares: X1.8 on 21 February with a maximum at<br \/>2307 UT and X.1.7 on 22 February with a maximum at 0632 UT. However,<br \/>they were short-lived and not accompanied by CMEs. During the first<br \/>of these, shortwave propagation subsided, particularly in the<br \/>western USA and the Pacific (the Dellinger effect).<\/p>\n<p>&#8220;Expect an increase in solar X-ray and ultraviolet radiation in the<br \/>coming days and mostly geomagnetically quiet conditions. As Spring<br \/>approaches, shortwave propagation will be mostly above average or<br \/>even better.&#8221;<\/p>\n<p>K7BTW posted this to the Western Washington DX Club email list on<br \/>February 20:<\/p>\n<p>&#8220;Fantastic band conditions.<\/p>\n<p>&#8220;If you&#8217;re not taking advantage of these band conditions, you are<br \/>missing a lot. On 20 meters FT8 in the last few minutes around 8pm<br \/>(0400 UTC) I worked Middle East stations in Lebanon, Jordan, Saudi<br \/>Arabia, and Qatar, plus several UN and many Russians. Over the pole<br \/>conditions are incredible.<\/p>\n<p>&#8220;Take advantage of the sunspot cycle.\u00a0 We know what it will be like<br \/>in 5 years!&#8221;<\/p>\n<p>Jeff, N8II wrote on February 16:<\/p>\n<p>&#8220;If we are at the peak, I would think this is a poor cycle.<\/p>\n<p>&#8220;Not long ago the flux dropped below 130 briefly.<\/p>\n<p>&#8220;10 meter conditions are excellent now with much better conditions<br \/>to East Asia in the evening than the first 3 weeks of January.<\/p>\n<p>&#8220;Today at 2400 UTC 10 meters was open well to Taiwan working BX5AA<br \/>and also a BD4 around 0030 UTC. Japanese signals were excellent<br \/>until just before 0100 UTC. I heard 8R7X in Guyana running many<br \/>Japanese until 0100 UTC on 10 CW.&#8221;<\/p>\n<p>Here in Seattle where I (K7RA) live we have always had a pipeline to<br \/>Japan, which at times can seem overwhelming.<\/p>\n<p>Reader David Moore sent this article from the European Space Agency:<\/p>\n<p>https:\/\/tinyurl.com\/bdz3uxnp<\/p>\n<p>Articles about powerful Solar Flares:<\/p>\n<p>https:\/\/tinyurl.com\/5ysj6xyt<\/p>\n<p>https:\/\/tinyurl.com\/vkyfpyr4<\/p>\n<p>https:\/\/tinyurl.com\/mrxa7uhb<\/p>\n<p>GeoNews article about the Solar max:<\/p>\n<p>https:\/\/tinyurl.com\/53zena9c<\/p>\n<p>Big sunspot AR3590 visible to the eye:<\/p>\n<p>https:\/\/tinyurl.com\/mrbw3fms<\/p>\n<p>The latest report from Dr. Tamitha Skov, WX6SWW:<\/p>\n<p><iframe loading=\"lazy\" title=\"Space Weather Outlook 21 February 2024\" width=\"1110\" height=\"624\" src=\"https:\/\/www.youtube.com\/embed\/T292oXH12Hk?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" allowfullscreen><\/iframe><\/p>\n<p>Send your tips, reports, observations, questions and comments to<br \/>k7ra@arrl.net. When reporting observations, don&#8217;t forget to tell us<br \/>which mode you were operating.<\/p>\n<p>For more information concerning shortwave radio propagation, see<br \/> and the ARRL Technical Information<br \/>Service web page at,  . For<br \/>an explanation of numbers used in this bulletin, see<br \/> .<\/p>\n<p>An archive of past propagation bulletins is at<br \/> . More good<br \/>information and tutorials on propagation are at  .<\/p>\n<p>Also, check this QST article about Solar Indices:<\/p>\n<p>https:\/\/bit.ly\/3Rc8Njt<\/p>\n<p>Instructions for starting or ending email distribution of ARRL<br \/>bulletins are at  .<\/p>\n<p>Sunspot numbers for February 15 through 21 2024 were 151, 97, 100,<br \/>84, 64, 50, and 45, with a mean of 84.4. 10.7 cm flux was 178.3,<br \/>168.8, 169.9, 156.5, 152.1, 152.6, and 169.9, with a mean of 164.<br \/>Estimated planetary A indices were 4, 4, 4, 6, 3, 6, and 4, with a<br \/>mean of 4.4. Middle latitude A index was 3, 3, 4, 4, 1, 5, and 3,<br \/>with a mean of 3.3.<br \/>\u00a0<\/p>\n<\/p><\/div>\n<p><br \/>\n<br \/><a href=\"http:\/\/www.arrl.org\/news\/view\/the-k7ra-solar-update-818?rand=771671\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>02\/23\/2024 &#8220;ASWFC GEOMAGNETIC DISTURBANCE WARNING ISSUED AT 0237 UTC\/22 FEBRUARY 2024 BY THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE. &#8220;A solar filament has erupted from the northwest solar quadrant anda component&hellip; <\/p>\n","protected":false},"author":1,"featured_media":771673,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[7],"tags":[],"class_list":["post-777741","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-ARRL"],"_links":{"self":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/777741","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=777741"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/777741\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/media\/771673"}],"wp:attachment":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=777741"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=777741"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=777741"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}