{"id":795873,"date":"2025-05-02T13:31:04","date_gmt":"2025-05-02T18:31:04","guid":{"rendered":"http:\/\/spaceweekly.com\/?p=795873"},"modified":"2025-05-02T13:31:04","modified_gmt":"2025-05-02T18:31:04","slug":"the-arrl-solar-report-12","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=795873","title":{"rendered":"The ARRL Solar Report"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div>\n\t\t\t\t\t<span class=\"date\">05\/02\/2025<\/span><\/p>\n<p>On May 2, Spaceweather.com reported: &#8220;Astronomers are monitoring a<br \/>very large sunspot now turning toward Earth. Sunspot AR4079<br \/>stretches more than 140,000 km from end to end and has two dark<br \/>cores each large enough to swallow Earth. Moreover, it is surrounded<br \/>by a ring of Ellerman Bombs.<\/p>\n<p>&#8220;Ellerman bombs are a sign of magnetic complexity in a sunspot.<br \/>Opposite polarities bump together, reconnect, and&#8211;boom! A<br \/>full-fledged flare may not be far behind.&#8221;<\/p>\n<p>Solar activity increased to moderate levels this past week. The<br \/>largest flare was on April 30 from an area where there was a major<br \/>M-class flare producer on its previous rotation last week.<\/p>\n<p>No Earth-directed Coronal Mass Ejections (CMEs) were observed. Solar<br \/>activity is expected to be low with a chance for M-class flares<br \/>(R1-R2, minor-moderate), and a slight chance for X-class flares<br \/>(R3-strong) through May 2.<br \/>\u00a0<br \/>Radio blackouts reaching the R1 levels were observed over the past<br \/>24 hours. The largest was on April 30.<\/p>\n<p>Weekly Commentary on the Sun, the Magnetosphere, and the Earth&#8217;s<br \/>Ionosphere &#8211; May 1, 2025, by F. K. Janda, OK1HH:<\/p>\n<p>&#8220;In the past few weeks I have allowed myself to take a break because<br \/>I have been under the care of excellent doctors and caring nurses in<br \/>a top Prague hospital. Fortunately, I had a receiver available and<br \/>could and did use it occasionally, but the computer was at home, QRB<br \/>53 km away. Now I&#8217;m back and continuing my usual activities:<br \/>observing the events between the Sun and the Earth, analyzing the<br \/>context and trying to predict the future developments (yes, I know<br \/>that more accurate predictions are not possible, while I can well<br \/>justify why &#8211; but why not take science a bit as a sport too,<br \/>right&#8230;?).<\/p>\n<p>&#8220;In the last few days of April, AR4079 rose on the northeastern limb<br \/>of the solar disk, while soon increased in area to over 1000<br \/>millionths. Already during the early months of this year, the Sun<br \/>had subtly hinted that the centre of gravity of activity might shift<br \/>from its southern to its northern hemisphere, but only now can we<br \/>see this trend more clearly. So, it&#8217;s possible that we&#8217;re in for<br \/>another upward swing within the current 11-year cycle, with active<br \/>regions mostly north of the equator. This could hold the promise of<br \/>improved ionospheric shortwave propagation conditions this Autumn.<\/p>\n<p>&#8220;During this April, we experienced a really large number of<br \/>geomagnetically disturbed days and mostly low MUF values. The calm<br \/>and improvement occurred only in the last decade of April, when we<br \/>witnessed all six geomagnetically quiet days of the whole April.<\/p>\n<p>&#8220;Going forward, although we do not expect a major increase in solar<br \/>activity for the time being, it will not be important during the<br \/>Northern Hemisphere ionospheric Summer. Solar activity will more or<br \/>less remain at the current level, the geomagnetic field will be<br \/>calmer compared to the past weeks &#8211; and the situation in the<br \/>ionosphere will be more favourable.&#8221;<br \/>\u00a0 <br \/>Solar wind parameters remained slightly enhanced due to waning<br \/>positive polarity of the Coronal Hole High-Speed Stream (CH HSS)<br \/>influences. A return to a mostly ambient-like state is expected for<br \/>May 1, but by May 2, an enhancement in solar wind parameters is<br \/>likely with the arrival of a recurrent, negative polarity CH HSS.<\/p>\n<p>Unsettled to active levels will likely persist into May 4 as an<br \/>additional negative polarity CH HSS moves into place.<\/p>\n<p>Geomagnetic field activity is likely to reach G1 (Minor) storm<br \/>levels on May 5 and 6 due to negative polarity CH HSS influences,<br \/>and again on May 18 due to positive polarity CH HSS influences.<\/p>\n<p>Periods of active conditions are likely on May 07 to 10, and on May<br \/>16 and 17 in response to CH HSS influences. Quiet and quiet to<br \/>unsettled levels are expected to prevail throughout the remainder of<br \/>the period.<\/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 Planetary A Index for May 3 to 9 is 10, 8, 18, 18, 15,<br \/>15, and 15, with a mean of 14.1.\u00a0 Predicted Planetary K Index is 3,<br \/>3, 5, 5, 4, 4, and 4, with a mean of 4.\u00a0 Predicted 10.7 centimeter<br \/>flux is 140, 140, 150, 160, 160, 165, and 165, with a mean of 154.3.<\/p>\n<p>\u00a0<\/p>\n<\/p><\/div>\n<p><br \/>\n<br \/><a href=\"http:\/\/www.arrl.org\/news\/view\/the-arrl-solar-report-12?rand=771671\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>05\/02\/2025 On May 2, Spaceweather.com reported: &#8220;Astronomers are monitoring avery large sunspot now turning toward Earth. Sunspot AR4079stretches more than 140,000 km from end to end and has two darkcores&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-795873","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\/795873","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=795873"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/795873\/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=795873"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=795873"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=795873"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}