{"id":798721,"date":"2025-10-10T18:27:31","date_gmt":"2025-10-10T23:27:31","guid":{"rendered":"https:\/\/spaceweekly.com\/?p=798721"},"modified":"2025-10-10T18:27:31","modified_gmt":"2025-10-10T23:27:31","slug":"the-arrl-solar-update-3","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=798721","title":{"rendered":"The ARRL Solar Update"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div>\n\t\t\t\t\t<span class=\"date\">10\/10\/2025<\/span><\/p>\n<p>Solar activity has been at moderate levels for the past 24 hours. Solar<br \/>activity is expected to be low with a chance for M class flares. Solar wind<br \/>speed reached a peak of 1124 km\/s.<\/p>\n<p>Solar activity reached moderate levels following an M2.0 flare (R1-Minor) at<br \/>from a region just around the Northwestern limb. Only low-level C-class<br \/>activity was observed from the remaining spotted regions on the visible disk.<br \/>New Regions 4248 and 4249 were numbered as they emerged late in the period, but<br \/>were otherwise unremarkable.<\/p>\n<p>A chance for R1-R2 (Minor-Moderate) radio blackouts exists over October 10 to 12 due<br \/>to flare potential from several active regions returning from the Suns far<br \/>side.<\/p>\n<p>Spaceweather.com reports on October 10, a hole has opened in the sun&#8217;s<br \/>atmosphere, and it is venting a stream of solar wind directly toward Earth<\/p>\n<p>Weekly Commentary on the Sun, the Magnetosphere, and the Earth&#8217;s Ionosphere \u2013<br \/>October 10,2025<\/p>\n<p>Solar activity has been declining since the beginning of October, as expected.<br \/>The last slightly larger sunspot group, designated as active region AR 4236,<br \/>disappeared behind the northwestern limb of the solar disk in the middle of the<br \/>present week. Almost immediately after it became invisible to us, a moderately<br \/>strong eruption occurred. This happened on Thursday, October 9, peaking at<br \/>12:31 UTC. However, the decline in solar activity will continue, followed by an<br \/>increase that should last for almost the entire second half of October. <\/p>\n<p>This will include a positive effect on the state of the F2 ionospheric layer.<br \/>Although this did not bring such good conditions for shortwave propagation,<br \/>precisely because of the decline in solar radiation, there were interesting<br \/>improvements here and there \u2013 especially at the beginning of geomagnetic<br \/>disturbances, most recently on the afternoon of October 7. However, another<br \/>phenomenon played a major role in the surprising improvement in shortwave<br \/>propagation conditions between Europe and the Antipodes on October 8 \u2013 the rare<br \/>and rather unusual occurrence of a sporadic E layer at this time of year&#8230;<\/p>\n<p>Official forecasts of increased solar activity for the second half of October<br \/>are rather skeptical for the time being. This is probably because the activity<br \/>on the far side of the Sun, as measured by helioseismological methods, is not<br \/>high. However, this may change. A surprise in the form of faster growth cannot<br \/>be ruled out.<\/p>\n<p>The latest report from Dr. Tamitha Skov, WX6SWW, can be found on Youtube.<\/p>\n<p>The predicted Planetary A Index for October 11 to 17 is 15, 12, 10, 8, 5, 5,<br \/>and 5 with a mean of 8.5. The Predicted Planetary K Index is 5, 4, 3, 3, 2, 2<br \/>and 2 with a mean of 3. Predicted 10.7 centimeter flux is 140, 135, 135, 140,<br \/>135, 140 and 145 with a mean of 137.1.<\/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 \/> . Information and<br \/>tutorials on propagation can be found at,  .<\/p>\n<p>Also, check this:<\/p>\n<p>https:\/\/bit.ly\/3Rc8Njt<\/p>\n<p>&#8220;Understanding Solar Indices&#8221; from September 2002 QST.<br \/>\u00a0<\/p>\n<\/p><\/div>\n<p><br \/>\n<br \/><a href=\"http:\/\/www.arrl.org\/news\/view\/the-arrl-solar-update-4?rand=771671\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>10\/10\/2025 Solar activity has been at moderate levels for the past 24 hours. Solaractivity is expected to be low with a chance for M class flares. Solar windspeed reached a&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-798721","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\/798721","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=798721"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/798721\/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=798721"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=798721"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=798721"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}