{"id":778192,"date":"2024-03-01T14:54:55","date_gmt":"2024-03-01T19:54:55","guid":{"rendered":"https:\/\/spaceweekly.com\/?p=778192"},"modified":"2024-03-01T14:54:55","modified_gmt":"2024-03-01T19:54:55","slug":"the-k7ra-solar-update-19","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=778192","title":{"rendered":"The K7RA Solar Update"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div>\n\t\t\t\t\t<span class=\"date\">03\/01\/2024<\/span><\/p>\n<p>&#8220;ASWFC GEOMAGNETIC DISTURBANCE WARNING ISSUED AT 2208 UTC\/29 FEBRUARY 2024 BY THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE.<\/p>\n<p>&#8220;A filament eruption was observed at 28\/0855UT from the solar<br \/>southeast quadrant. The associated CME has been determined to<br \/>contain an Earth-directed component, with an arrival to Earth&#8217;s<br \/>magnetosphere at 02\/1100 UTC +\/- 12 hours. G1 geomagnetic conditions<br \/>are expected.<\/p>\n<p>&#8220;INCREASED GEOMAGNETIC ACTIVITY EXPECTED DUE TO CORONAL MASS EJECTION FROM 02-03 MARCH 2024.&#8221;<\/p>\n<p>Seven new sunspot groups emerged this week, four on February 23, one<br \/>on February 25, another on February 26 and one more on February 28.<\/p>\n<p>Solar activity increased this reporting week, February 22-28,<br \/>compared to the week before. Average daily sunspot number rose from<br \/>84.4 to 108.4, and solar flux from 164 to 175.<\/p>\n<p>Geomagnetic conditions were quiet, though the numbers rose.<br \/>Planetary A index went from 4.4 to 8.4, and middle latitude numbers<br \/>from 3.3 to 7.4.<\/p>\n<p>The predicted solar flux is 160, 155, and 160 on March 1-3, 165 on<br \/>March 4-5, 160 and 165 on March 6-7, 165 on March 8-9, 168 on March<br \/>10, then 165 on March 11-12, 160 on March 13-14, then 168 and 172 on<br \/>March 15-16, then 175, 175 and 178 on March 17-19, 180 on March<br \/>20-24, and 175 on March 25-26, then 180 and 175 on March 27-28, 170<br \/>on March 29-30, 172 on March 31 to April 1, 170 on April 2, and 165<br \/>on April 3-5.<br \/>\u00a0<br \/>The predicted planetary A index is 8, 12, 12 and 10 on March 1-4,<br \/>then 5 on March 5-23, then 15, 12 and 12 on March 24-26, and 5 on<br \/>March 27 to mid-April.<\/p>\n<p>Spaceweather.com reported on giant sunspot AR3590:\u00a0 &#8220;In only 23<br \/>hours spanning February 21-22, the active region unleashed three<br \/>powerful X-class solar flares (X1.8, X1.7 and X6.3). The X6.3 flare<br \/>is the strongest of Solar Cycle 25, so far, and the most powerful<br \/>flare since the great solar storms of September 2017.&#8221;<\/p>\n<p>Because there were no CMEs, there were no geomagnetic storms, but<br \/>extreme ultraviolet radiation ionized the top of Earth&#8217;s atmosphere<br \/>and caused several shortwave blackouts over Hawaii and Australia on<br \/>February 21-22.<\/p>\n<p>Sunspot group AR3590 is the largest of the current solar cycle.<\/p>\n<p>Weekly Commentary on the Sun, the Magnetosphere, and the Earth&#8217;s<br \/>Ionosphere &#8211; February 29, 2024 from OK1HH:<\/p>\n<p>&#8220;Over the past seven days, we have seen the deflection of an active<br \/>region of AR3590 on the Sun, 760 millionths of the size of the solar<br \/>disk. On February 25, it already occupied an area of 1450<br \/>millionths, making it the largest group of spots so far since the<br \/>beginning of the 25th cycle. It produced its largest and extra<br \/>proton flares on February 21-22, including three X-class flares in<br \/>23 hours. The largest of these, X6.3 on 22 February, with a maximum<br \/>at 2324 UT, was the most important flare since the beginning of<br \/>Solar Cycle 25.<\/p>\n<p>&#8220;Proton flares were no exception and caused an absorption in the<br \/>polar cap (PCA). The first of these was recorded on 9 February in<br \/>the already setting region AR3575. At the same time, there was a<br \/>region AR3576 in the southeast of the solar disk, which will rise<br \/>again in the next few days, so we do not have to worry about a<br \/>decrease in solar activity.<\/p>\n<p>&#8220;With the exception of the unsettled days of February 25-27, the<br \/>geomagnetic field was mostly calm. We expect a similar pattern in<br \/>the coming weeks. Ideally, the mostly calm development could last<br \/>until the Spring Equinox. If this happens, shortwave propagation<br \/>conditions will be mostly above average.&#8221;<\/p>\n<p>This weekend is the ARRL International DX SSB contest. For details<br \/>see:<\/p>\n<p>https:\/\/www.arrl.org\/arrl-dx<\/p>\n<p>Some articles about solar basics:<\/p>\n<p>https:\/\/www.ktvh.com\/news\/weather-wise\/weather-wise-sunspots<\/p>\n<p>https:\/\/bit.ly\/49AmNKf<\/p>\n<p>https:\/\/bit.ly\/3V0biHJ<\/p>\n<p>https:\/\/bit.ly\/3wE1Orx<\/p>\n<p>https:\/\/star-hunter.ru\/en\/sunspots-2024-02-28\/<\/p>\n<p>Popular Science article about a Solar Minima:<\/p>\n<p>https:\/\/www.popsci.com\/science\/sun-quiet\/<\/p>\n<p>I do not trust the data or the correlations in this article, but<br \/>there is some interesting content here:<\/p>\n<p>https:\/\/bit.ly\/48Ablxc<\/p>\n<p>Latest video from Dr. Tamitha Skov, WX6SWW:<\/p>\n<p><iframe loading=\"lazy\" title=\"The Biggest X-flare Yet Shooting Blanks | Space Weather News 24 February 2024\" width=\"1110\" height=\"624\" src=\"https:\/\/www.youtube.com\/embed\/V-PQSkYYEB4?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 22 through 28 2024 were 46, 116, 106,<br \/>114, 133, 103, and 127, with a mean of 106.4. 10.7 cm flux was<br \/>173.3, 172.9, 179.2, 180.8, 171.7, 168.3, and 179.1, with a mean of<br \/>175. Estimated planetary A indices were 6, 3, 7, 13, 11, 13, and 6,<br \/>with a mean of 8.4. Middle latitude A index was 6, 2, 6, 14, 10, 9,<br \/>and 5, with a mean of 7.4.<\/p>\n<p>\u00a0<\/p>\n<\/p><\/div>\n<p><br \/>\n<br \/><a href=\"http:\/\/www.arrl.org\/news\/view\/the-k7ra-solar-update-819?rand=771671\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>03\/01\/2024 &#8220;ASWFC GEOMAGNETIC DISTURBANCE WARNING ISSUED AT 2208 UTC\/29 FEBRUARY 2024 BY THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE. &#8220;A filament eruption was observed at 28\/0855UT from the solarsoutheast quadrant. The&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-778192","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\/778192","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=778192"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/778192\/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=778192"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=778192"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=778192"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}