{"id":799694,"date":"2025-12-12T15:23:43","date_gmt":"2025-12-12T20:23:43","guid":{"rendered":"https:\/\/spaceweekly.com\/?p=799694"},"modified":"2025-12-12T15:23:43","modified_gmt":"2025-12-12T20:23:43","slug":"the-arrl-solar-update-11","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=799694","title":{"rendered":"The ARRL Solar Update"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div>\n\t\t\t\t\t<span class=\"date\">12\/12\/2025<\/span><\/p>\n<p>Solar activity reached high levels this past week when Region 4299<br \/>produced an M1.1 (R1\/Minor) flare on December 6. Shortly after, the<br \/>region produced an M8.1\/2b (R3\/Strong) flare, also on December 6.<br \/>Associated with the M8.1 flare was a 1,100 SFU Tenflare, a 1,143<br \/>km\/s Type II sweep and a Type IV sweep. (A &#8220;sweep&#8221; is a solar radio<br \/>burst that sweeps through the RF spectrum as the energy moves<br \/>outward from the Sun.)<\/p>\n<p>Some development was observed around the leader spot of Region 4299,<br \/>while slight decay was noted among the trailer spots. Regions 4296<br \/>and 4294 remained the largest of the visible disk but have only<br \/>produced C-class activity in the past 24 hours. Only minor changes<br \/>were observed among the other numbered active regions and activity<br \/>is now moderate.<br \/>\u00a0 <br \/>Coronal mass ejection (CME) activity was observed from both M-class<br \/>flares. A slow, Earth-directed CME was observed from the M1.1 and a<br \/>faster, full-halo, Earth-directed CME was observed from the M8.1<br \/>flare. According to Spaceweather.com, it touched off a G2 (moderate)<br \/>geomagnetic storm on December 10.<br \/>\u00a0 <br \/>Solar wind parameters reflected a disturbed near-Earth environment<br \/>throughout the reporting period. Solar wind speeds showed little<br \/>reaction to the magnetic transient, averaging 375 km\/s throughout<br \/>the reporting period. The phi angle was oriented towards-the-Sun<br \/>(negative) for the majority of the reporting period, then slowly<br \/>rotated around to away-from-the-Sun (positive) 1.5 hours after the<br \/>arrival of the transient.<br \/>\u00a0 <br \/>The electron flux is expected to become elevated through December 14<br \/>as a coronal hole high speed stream (CH HSS) originating from the<br \/>negative polarity coronal hole in the northern hemisphere becomes<br \/>geoeffective. The flux is likely to surpass the 1,000 pfu threshold<br \/>during the diurnal maxima.<\/p>\n<p>As complex regions in the western hemisphere move beyond the limb,<br \/>chances for the proton flux to become elevated decrease. There is a<br \/>10% chance for an S1 (Minor) radiation storming event on December<br \/>12, with chances decreasing to 1% by December 14.<\/p>\n<p>Spaceweather.com for December 12 reports on the Geminids Meteor<br \/>Showers peaking this upcoming weekend.<\/p>\n<p>A story on the Meteor Scatter QSO Party can be found on the ARRL<br \/>website at,<br \/> .<\/p>\n<p>Weekly Commentary on the Sun, the Magnetosphere, and the Earth&#8217;s<br \/>Ionosphere, December 4, 2025, by F. K. Janda, OK1HH:<\/p>\n<p>&#8220;On December 1, an active sunspot group emerged on the southeastern<br \/>limb of the solar disk, as expected. During the last solar rotation,<br \/>it was designated AR4274. Astronomers renamed it now as AR4294,<br \/>while produced the first in a series of energetically significant<br \/>flares observed during the first third of December. In addition,<br \/>AR4296 began to grow right next to it, and together they began to<br \/>resemble the so-called Carrington region of 1859. However, the<br \/>growth of both regions slowed down, but moderately powerful<br \/>eruptions continued to occur in them, surprisingly contributed to by<br \/>the relatively small group AR4299 in the north of the solar disk.<\/p>\n<p>&#8220;Another energetically significant solar flare on December 8 came as<br \/>a surprise. Given the speed of the ejected particles, the CME was<br \/>expected to hit Earth on December 9. However, they apparently<br \/>traveled to Earth along a longer path and arrived on December 10.<br \/>Therefore, they encountered a slow and expected stream of particles<br \/>that last hit Earth on November 12. The result of the encounter<br \/>between the slow and fast particle streams was a so-called reverse<br \/>shock at around 20:00 UT on December 10, which triggered a G2-class<br \/>geomagnetic storm. However, these storms are usually short-lived<br \/>and, apart from unusual, irregular (and interesting) developments,<br \/>they did not have any significant consequences.<\/p>\n<p>&#8220;Solar activity remains high, and the state of the ionosphere<br \/>reflects this. However, the fact that the conditions for shortwave<br \/>propagation are different from previous cycles is another story.<br \/>Every eleven-year cycle is different.&#8221;<\/p>\n<p>The latest video from Dr. Tamitha Skov, WX6SWW, can be found on<br \/>YouTube at,  .<\/p>\n<p>The Predicted Planetary A Index for December 13 to 19 is 12, 12, 8,<br \/>5, 8, 10, and 8, with a mean of 9.\u00a0 Predicted Planetary K Index is<br \/>4, 4, 3, 2, 3, 3, and 3, with a mean of 3.1.\u00a0 10.7-centimeter flux<br \/>is 140, 130, 130, 135, 135, 140, and 140, with a mean of 135.8.<\/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;<em>Understanding Solar Indice<\/em>s&#8221; from September 2002 <em>QST<\/em>.<\/p>\n<p>\u00a0<\/p>\n<\/p><\/div>\n<p><br \/>\n<br \/><a href=\"http:\/\/www.arrl.org\/news\/view\/the-arrl-solar-update-12?rand=771671\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>12\/12\/2025 Solar activity reached high levels this past week when Region 4299produced an M1.1 (R1\/Minor) flare on December 6. Shortly after, theregion produced an M8.1\/2b (R3\/Strong) flare, also on December&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-799694","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\/799694","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=799694"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/799694\/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=799694"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=799694"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=799694"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}