{"id":794795,"date":"2025-03-28T10:09:06","date_gmt":"2025-03-28T15:09:06","guid":{"rendered":"http:\/\/spaceweekly.com\/?p=794795"},"modified":"2025-03-28T10:09:06","modified_gmt":"2025-03-28T15:09:06","slug":"the-arrl-solar-report-8","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=794795","title":{"rendered":"The ARRL Solar Report"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div>\n\t\t\t\t\t<span class=\"date\">03\/28\/2025<\/span><\/p>\n<p>On Wednesday, March 26, around 2130 UTC a Major Storm occurred.\u00a0 At<br \/>one point, the Planetary A Index was 49, and the Planetary K Index<br \/>was at 6.<\/p>\n<p>Solar wind parameters are expected to remain enhanced due to<br \/>continued coronal hole high-speed stream influences with waning<br \/>effects likely by March 29.<\/p>\n<p>The Solar Radiation Storm Forecast for March 29 and 30 has a 1<br \/>percent chance of a S1 or greater storm.<\/p>\n<p>No S1 (Minor) or greater solar radiation storms are expected.\u00a0 No<br \/>significant active region activity favorable for radiation storm<br \/>production is forecast.<\/p>\n<p>The Radio Blackout forecast calls for a chance for isolated R1-R2<br \/>(Minor-Moderate) radio blackouts due to M-class flare activity will<br \/>persist through March 30 primarily due to the potential exhibited by<br \/>AR4043.<\/p>\n<p>From Space Weather Prediction Center: &#8220;Since February 25, 2025, the<br \/>Space Weather Prediction Center (SWPC) has presented new coronagraph images and data from the GOES-19 Compact Coronagraph-1 (CCOR-1). The images and data are updated every 15 minutes.<\/p>\n<p>&#8220;Imagery from the Compact Coronagraph (CCOR) instruments is used by<br \/>the SWPC Forecast Office to characterize activity in the outermost<br \/>part of the Sun&#8217;s atmosphere known as the corona. This includes<br \/>monitoring data for transient events like coronal mass ejections<br \/>(CMEs), as well as monitoring the impacts the corona has on the<br \/>steady stream of plasma, referred to as the solar wind, emanating<br \/>from the Sun. Ultimately, information derived from CCOR images will<br \/>be used as inputs to the WSA-Enlil model to forecast the impacts of<br \/>CMEs and the solar wind on Earth.<\/p>\n<p>&#8220;Note: Until such time as GOES-19 becomes operational, currently<br \/>planned for April 4th, the animations and data are to be considered<br \/>&#8216;preliminary and non-operational.&#8217; In particular, CCOR-1 data will<br \/>not update between 3\/21 and 4\/1 due to the spacecraft drifting to<br \/>its operational location.&#8221;<\/p>\n<p>Weekly Commentary on the Sun, the Magnetosphere, and the Earth&#8217;s<br \/>Ionosphere &#8211; March 27, 2025, by F. K. Janda, OK1HH:<\/p>\n<p>&#8220;Most forecasts, including those from NOAA, have been consistent<br \/>over the past week that a strong G3-class geomagnetic storm would<br \/>develop on Sunday, March 23. In fact, a CME was expected to directly<br \/>impact the Earth. Although the source of the CME was only the<br \/>M1-class solar flare from AR4028, even weaker CMEs can produce<br \/>strong geomagnetic disturbances, especially on days around the<br \/>equinoxes. In the end, however, paradoxically, 23 March was the<br \/>relatively quietest day.<\/p>\n<p>&#8220;However, a large coronal hole caught our attention this week, while<br \/>we expected that once it reached the central meridian region, the<br \/>solar wind stream would head directly towards Earth. This is what<br \/>happened and in the following days, especially on March 26, a G2<br \/>class geomagnetic storm developed. The solar wind speed increased<br \/>from 400 km\/s to 700 km\/s. On March 27, the increase continued to<br \/>over 800 km\/s (1.8 million mph).<\/p>\n<p>&#8220;Shortwave propagation conditions were particularly degraded along<br \/>paths through the higher latitudes of the Northern Hemisphere.<br \/>Outside of these, there was also a more pronounced decrease in MUF<br \/>on routes that crossed South America and the South Atlantic where<br \/>geomagnetic anomalies are located.<\/p>\n<p>&#8220;While late March and early April are periods with traditionally<br \/>better-than-average shortwave propagation conditions, this time our<br \/>expectations will only be partially met. Solar activity is lower<br \/>than would be consistent with the current phase of the solar cycle &#8211;<br \/>and disturbances are relatively common.&#8221;<\/p>\n<p>A partial Solar Eclipse occurs on March 29, 2025. Details can be<br \/>found at,<br \/>https:\/\/science.nasa.gov\/eclipses\/future-eclipses\/mar-29-2025-eclipse\/<br \/>.<\/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>The predicted 10.7 centimeter flux for March 29 to April 3 is 160,<br \/>165, 165, 170, 170, and 175, with a mean of 167.5.\u00a0 The predicted<br \/>Planetary A Index is 8, 5, 5, 5, 5, and 10, with a mean of 6.3.\u00a0 The<br \/>predicted Planetary K Index is 3, 2, 2, 2, 2, and 3, with a mean of<br \/>2.3.<br \/>\u00a0<\/p>\n<\/p><\/div>\n<p><br \/>\n<br \/><a href=\"http:\/\/www.arrl.org\/news\/view\/the-arrl-solar-report-7?rand=771671\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>03\/28\/2025 On Wednesday, March 26, around 2130 UTC a Major Storm occurred.\u00a0 Atone point, the Planetary A Index was 49, and the Planetary K Indexwas at 6. Solar wind parameters&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-794795","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\/794795","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=794795"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/794795\/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=794795"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=794795"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=794795"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}