{"id":800072,"date":"2026-01-09T15:08:30","date_gmt":"2026-01-09T20:08:30","guid":{"rendered":"https:\/\/spaceweekly.com\/?p=800072"},"modified":"2026-01-09T15:08:30","modified_gmt":"2026-01-09T20:08:30","slug":"the-arrl-solar-update-14","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=800072","title":{"rendered":"The ARRL Solar Update"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div>\n\t\t\t\t\t<span class=\"date\">01\/09\/2026<\/span><\/p>\n<p>Geomagnetic field activity is likely to reach G1 (Minor) geomagnetic<br \/>storm levels on January 13 and 14, and then from January 17 to 20.<\/p>\n<p>Unsettled levels are likely on January 12, and then from January 21<br \/>and 22.\u00a0 All enhancements in geomagnetic activity are due to the<br \/>anticipated influence of multiple, recurrent, coronal holes. The<br \/>remainder of the outlook period is expected to be mostly quiet.<\/p>\n<p>A tracking model from NOAA\/SWPC shows a Coronal Mass Ejection (CME)<br \/>could pass close to Earth by January 11.\u00a0 Multiple faint coronal<br \/>mass ejections were observed off the SE limb originating from Region<br \/>4334. However, modeling appeared to show no Earth-directed<br \/>component.<br \/>\u00a0 <br \/>Solar activity is expected to be low with a chance (45 percent) for<br \/>M-class flares (R1-R2, minor-moderate), and a slight chance (10<br \/>percent) for isolated X-class flares (R3-strong) until January 10.<br \/>\u00a0 <br \/>Solar wind parameters became mildly enhanced after January 7.<br \/>However, Coronal Hole High Speed Stream (CH HSS) influence is<br \/>expected to persist through January 10.<\/p>\n<p>Unsettled to active conditions are expected to continue on January<br \/>10 and 11 as the coronal hole moves further into a geo-effective<br \/>position, along with the possible arrival of CMEs that left the Sun<br \/>on January 8, with a chance for isolated G1 (Minor) storm conditions<br \/>late on January 10.<br \/>\u00a0 <br \/>Weekly Commentary on the Sun, the Magnetosphere, and the Earth&#8217;s<br \/>Ionosphere, January 8, 2026, by F. K. Janda, OK1HH:<\/p>\n<p>&#8220;According to the original forecast, solar activity was expected to<br \/>gradually decline until mid-January. However, an active region,<br \/>AR4336, emerged in the southeast of the solar disk, in a location<br \/>where nothing unusual had occurred during the previous solar<br \/>rotation. As a result, overall solar activity is already beginning<br \/>to increase.<\/p>\n<p>&#8220;Other formations important for the forecast are coronal holes No.<br \/>12 and 13, whose proximity to active regions will cause an<br \/>intensification of the solar wind. Its effects will be felt in the<br \/>Earth&#8217;s magnetosphere and ionosphere since January 9, when the<br \/>shorter disturbance is expected. This will be followed by a brief<br \/>lull and a renewed increase in geomagnetic activity before<br \/>mid-January.<\/p>\n<p>&#8220;The forecast for the coming days is very uncertain. If the<br \/>situation from the last solar rotation repeats itself, solar<br \/>activity could continue to increase since mid-January, while the<br \/>days of January 15-18 could be geomagnetically active or even<br \/>disturbed. However, it seems that a reliable forecast cannot be made<br \/>at this time.&#8221;<\/p>\n<p>The Predicted Planetary A Index for January 10 to 16 is 8, 5, 10,<br \/>15, 15, 5, and 5, with a mean of 9.\u00a0 Predicted Planetary K Index is<br \/>3, 2, 3, 5, 5, 2, and 2, with a mean of 3.1.\u00a0 10.7-centimeter flux<br \/>is 135, 130, 135, 135, 140, 145, and 145, with a mean of 137.9.<\/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 Indices<\/em>&#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-15?rand=771671\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>01\/09\/2026 Geomagnetic field activity is likely to reach G1 (Minor) geomagneticstorm levels on January 13 and 14, and then from January 17 to 20. Unsettled levels are likely on January&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-800072","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\/800072","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=800072"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/800072\/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=800072"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=800072"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=800072"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}