{"id":782141,"date":"2024-05-10T11:29:52","date_gmt":"2024-05-10T16:29:52","guid":{"rendered":"http:\/\/spaceweekly.com\/?p=782141"},"modified":"2024-05-10T11:29:52","modified_gmt":"2024-05-10T16:29:52","slug":"solar-radiation-storm-in-progress","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=782141","title":{"rendered":"Solar radiation storm in progress"},"content":{"rendered":"


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Proton flux started rising after 07:00 UTC on May 9, 2024, due to increased flare activity from very large and complex Active Region 3664, and reached S1 \u2013 Minor solar radiation storm threshold on May 10.<\/strong><\/p>\n

As activity in this region continued, with numerous M- and several X-class flares, proton flux levels kept rising and reached the S1 \u2013 Minor solar radiation storm threshold at 13:55 UTC on May 10. <\/p>\n

This level is the lowest on NOAA\u2019s five-level scale for solar radiation storms and is generally associated with minor impacts on high-frequency radio communication in the polar regions.<\/p>\n

Proton counts continue to rise and may reach S2 \u2013 Moderate levels within the next few hours.<\/p>\n

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\"ionosphere\"ionosphere<\/figure>\n<\/div>\n

According to NOAA, solar radiation storms occur when large-scale magnetic eruptions, often causing coronal mass ejections (CMEs), accelerate charged particles in the solar atmosphere, most importantly protons, to speeds close to the speed of light. <\/p>\n

Protons can cover the 150 million km (93 miles) from the Sun to Earth in just a few minutes. <\/p>\n

Once they reach Earth, they penetrate the magnetosphere, which normally protects us from lower-energy particles. Guided by Earth\u2019s magnetic field lines, these high-velocity protons are funneled into the atmosphere near the north and south poles.<\/p>\n

Solar radiation storms have multiple effects near Earth. When high-energy protons collide with satellites or astronauts in space, they can penetrate deeply, potentially damaging electronic circuits or altering biological DNA. In severe solar radiation storms, passengers and crew on high-altitude flights near the polar regions can also be exposed to increased radiation. <\/p>\n

Additionally, when these energetic protons interact with Earth\u2019s atmosphere, they ionize atoms and molecules, creating free electrons. This process forms a layer in the lower ionosphere that can absorb high-frequency radio waves, disrupting or completely blocking radio communication.<\/p>\n

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\"proton\"proton<\/figure>\n<\/div>\n
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\"sunspots\"sunspots
Sunspots on May 10, 2024. Credit: NASA SDO\/HMI<\/figcaption><\/figure>\n<\/div>\n
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Sunspots on May 10, 2024. Credit: NASA SDO\/HMI<\/figcaption><\/figure>\n<\/div>\n

This storm is related to very high solar activity over the past 7 days, with more than 60 M-class and 10 X-class solar flares. Most of them were produced by active region 3664 (beta-gamma-delta) and 3663 (now beyond the west limb).<\/p>\n

Even if we stay at S1 \u2013 Minor levels today, the location and strength of Region 3664 suggest an increased possibility of solar radiation storms over the next couple of days.<\/p>\n

More than 5 coronal mass ejection (CMEs) produced by this region are expected to impact Earth over the next 24+ hours.<\/p>\n

As a result, a G4 \u2013 Severe or Greater Geomagnetic Storm Watch is in effect for May 11. There is a good possibility this will extend into May 12 and further toward mid-month due to several incoming CMEs.<\/p>\n

Only three G4 \u2013 Severe geomagnetic storms have been observed during this solar cycle (SC24) which began in December 2019.<\/p>\n

The last G4 \u2013 Severe storm was on March 23, 2024, and the last G5 \u2013 Extreme was the Halloween Storm in October 2003. That G5 resulted in power outages in Sweden and damaged power transformers in South Africa.<\/p>\n

The first CME has already hit STEREO Ahead satellite and impact data suggest we are in for some serious geomagnetic storming.<\/p>\n

For more information about increased solar activity this week, visit:<\/p>\n

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Featured image credit: NOAA\/SWPC<\/em><\/p>\n

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Major X3.9 solar flare erupts from AR 3664 \u2014 the 10th X-class flare in just 7 days<\/h3>\n

Friday, May 10, 2024<\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n

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G4 \u2013 Severe or greater geomagnetic storm forecast as multiple CMEs merge and impact Earth on May 11<\/h3>\n

Thursday, May 9, 2024<\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n

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At least 5 CMEs heading toward Earth, G4 \u2013 Severe or Greater Geomagnetic Storm Watch in effect for May 11<\/h3>\n

Thursday, May 9, 2024<\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n

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Long-duration X1.0 solar flare erupts from geoeffective Region 3664, CME impact expected on May 11<\/h3>\n

Wednesday, May 8, 2024<\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n

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Major X4.5 solar flare erupts from Region 3663 \u2014 fourth X-class flare in 3 days<\/h3>\n

Monday, May 6, 2024<\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n

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Major X1.2 solar flare erupts from Region 3663 \u2014 second X-class flare of the day<\/h3>\n

Sunday, May 5, 2024<\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n

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Major X1.3 solar flare erupts from Region 3663<\/h3>\n

Sunday, May 5, 2024<\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n

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Proton flux started rising after 07:00 UTC on May 9, 2024, due to increased flare activity from very large and complex Active Region 3664, and reached S1 \u2013 Minor solar… <\/p>\n","protected":false},"author":1,"featured_media":782142,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[32],"tags":[],"class_list":["post-782141","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-space-weather-reports"],"_links":{"self":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/782141","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=782141"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/782141\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/media\/782142"}],"wp:attachment":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=782141"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=782141"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=782141"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}