{"id":38826,"date":"2025-02-23T13:45:00","date_gmt":"2025-02-23T13:45:00","guid":{"rendered":"https:\/\/www.lifeandnews.com\/articles\/?p=38826"},"modified":"2025-02-24T06:09:44","modified_gmt":"2025-02-24T06:09:44","slug":"colliding-plasma-ejections-from-the-sun-generate-huge-geomagnetic-storms-%e2%88%92-studying-them-will-help-scientists-monitor-future-space-weather","status":"publish","type":"post","link":"https:\/\/www.lifeandnews.com\/articles\/colliding-plasma-ejections-from-the-sun-generate-huge-geomagnetic-storms-%e2%88%92-studying-them-will-help-scientists-monitor-future-space-weather\/","title":{"rendered":"Colliding plasma ejections from the Sun generate huge geomagnetic storms \u2212 studying them will help scientists monitor future space&nbsp;weather"},"content":{"rendered":"\n<p><a href=\"https:\/\/theconversation.com\/profiles\/shirsh-lata-soni-2297636\">Shirsh Lata Soni<\/a>, <em><a href=\"https:\/\/theconversation.com\/institutions\/university-of-michigan-1290\">University of Michigan<\/a><\/em><\/p>\n\n\n\n<p>The Sun periodically ejects huge <a href=\"https:\/\/science.nasa.gov\/learn\/heat\/big-ideas\/big-idea-3-1\/\">bubbles of plasma<\/a> from its surface that contain an intense magnetic field. These events are called <a href=\"https:\/\/www.swpc.noaa.gov\/phenomena\/coronal-mass-ejections\">coronal mass ejections<\/a>, or CMEs. When two of these ejections collide, they can generate powerful geomagnetic storms that can lead to beautiful auroras but may disrupt satellites and GPS back on Earth.<\/p>\n\n\n\n<p>On May 10, 2024, people across the Northern Hemisphere got to witness the <a href=\"https:\/\/science.nasa.gov\/science-research\/heliophysics\/how-nasa-tracked-the-most-intense-solar-storm-in-decades\/\">impact of these solar activities<\/a> on Earth\u2019s <a href=\"https:\/\/www.ncei.noaa.gov\/news\/what-is-space-weather\">space weather<\/a>.<\/p>\n\n\n\n<figure class=\"wp-block-image\"><img src=\"https:\/\/images.theconversation.com\/files\/647476\/original\/file-20250206-19-uhuxof.png?ixlib=rb-4.1.0&amp;q=45&amp;auto=format&amp;w=237&amp;fit=clip\" alt=\"Bright colors visible across the night sky, with a tree silhouetted in the foreground.\" \/><figcaption>The northern lights, as seen here from Michigan in May 2024, are caused by geomagnetic storms in the atmosphere. Shirsh Lata Soni<\/figcaption><\/figure>\n\n\n\n<p>Two merging CMEs triggered the largest geomagnetic storm in two decades, which manifested in <a href=\"https:\/\/www.skyatnightmagazine.com\/space-science\/aurora-10-may-2024\">brightly colored auroras visible<\/a> across the sky.<\/p>\n\n\n\n<p>I\u2019m a <a href=\"https:\/\/scholar.google.com\/citations?user=4dMq4IgAAAAJ&amp;hl=en\">solar physicist<\/a>. My colleagues and I aim to track and better understand colliding CMEs with the goal of improving space weather forecasts. In the modern era, where <a href=\"https:\/\/theconversation.com\/solar-storms-can-destroy-satellites-with-ease-a-space-weather-expert-explains-the-science-177510\">technological systems are increasingly vulnerable<\/a> to space weather disruptions, understanding how CMEs interact with each other has never been more crucial.<\/p>\n\n\n\n<h2>Coronal mass ejections<\/h2>\n\n\n\n<p><a href=\"https:\/\/www.swpc.noaa.gov\/phenomena\/coronal-mass-ejections\">CMEs are long and twisted<\/a> \u2013 kind of like ropes \u2013 and how often they happen varies with an <a href=\"https:\/\/www.space.com\/solar-cycle-frequency-prediction-facts\">11-year cycle<\/a>. At the solar minimum, researchers observe about one a week, but near the solar maximum, they can observe, on average, two or three per day.<\/p>\n\n\n\n<p>When two or more CMEs interact, they generate massive clouds of charged particles and magnetic fields that may compress, merge or reconnect with each other during the collision. These interactions can amplify the impact of the CMEs on <a href=\"https:\/\/theconversation.com\/earths-magnetic-field-protects-life-on-earth-from-radiation-but-it-can-move-and-the-magnetic-poles-can-even-flip-216231\">Earth\u2019s magnetic field<\/a>, sometimes creating geomagnetic storms.<\/p>\n\n\n\n<h2>Why study interacting CMEs?<\/h2>\n\n\n\n<p>Nearly <a href=\"https:\/\/doi.org\/10.1007\/s11207-017-1091-6\">one-third of CMEs interact<\/a> with other CMEs or <a href=\"https:\/\/science.nasa.gov\/sun\/what-is-the-solar-wind\/\">the solar wind<\/a>, which is a stream of charged particles released from the outer layer of the Sun.<\/p>\n\n\n\n<p><a href=\"https:\/\/doi.org\/10.1051\/0004-6361\/202347552\">In my research team\u2019s study<\/a>, published in May 2024, we found that CMEs that do interact or collide with each other are much more likely to cause a geomagnetic storm \u2013 two times more likely than an individual CME. The mix of strong magnetic fields and high pressure in these CME collisions is likely what causes them to generate storms.<\/p>\n\n\n\n<p>During <a href=\"https:\/\/www.space.com\/solar-cycle-frequency-prediction-facts\">solar maxima<\/a>, when there can be more than 10 CMEs per day, the likelihood of CMEs interacting with each other increases. But researchers aren\u2019t sure whether they become more likely to generate a geomagnetic storm during these periods.<\/p>\n\n\n\n<p>Scientists can study interacting CMEs as they move through space and watch them contribute to geomagnetic storms using observations from space- and ground-based observatories.<\/p>\n\n\n\n<p>In this study, we looked at three CMEs that interacted with each other as they traveled through space using the space-based observatory <a href=\"https:\/\/stereo.gsfc.nasa.gov\/instruments\/instruments.shtml\">STEREO<\/a>. We validated these observations <a href=\"https:\/\/ccmc.gsfc.nasa.gov\/models\/EUHFORIA%20Heliosphere%7E1.1\/\">with three-dimensional simulations<\/a>.<\/p>\n\n\n\n<p>The CME interactions we studied generated a complex magnetic field and a compressed plasma sheath, which is a layer of charged particles in the upper atmosphere that interacts with Earth\u2019s magnetic field.<\/p>\n\n\n\n<p>When this complex structure <a href=\"https:\/\/www.swpc.noaa.gov\/phenomena\/earths-magnetosphere\">encountered Earth\u2019s magnetosphere<\/a>, it compressed the magnetosphere and triggered an intense geomagnetic storm.<\/p>\n\n\n\n<figure class=\"wp-block-image\"><img src=\"https:\/\/images.theconversation.com\/files\/647482\/original\/file-20250206-19-zsm4o9.png?ixlib=rb-4.1.0&amp;q=45&amp;auto=format&amp;w=754&amp;fit=clip\" alt=\"Four images showing a CME\u2013CME interaction based on white-light observations from the STEREO telescope.\" \/><figcaption>Four images show three interacting CMEs, based on observations from the STEREO telescope. In images C and D, you can see the northeast flank of CME-1 and CME-2 that interact with the southwest part of CME-3. Shirsh Lata Soni<\/figcaption><\/figure>\n\n\n\n<p>This same process generated the geomagnetic storm from May 2024.<\/p>\n\n\n\n<p>Between May 8-9, multiple Earth-directed CMEs erupted from the Sun. When these CMEs merged, they formed a massive, combined structure that arrived at Earth late on May 10, 2024. This structure triggered the extraordinary geomagnetic storm many people observed. People even in parts of the southern U.S. were able to see the northern lights in the sky that night.<\/p>\n\n\n\n<h2>More technology and higher stakes<\/h2>\n\n\n\n<p>Scientists have an expansive network of space- and ground-based observatories, such as the <a href=\"https:\/\/science.nasa.gov\/mission\/parker-solar-probe\/\">Parker Solar Probe<\/a>, <a href=\"https:\/\/www.esa.int\/Science_Exploration\/Space_Science\/Solar_Orbiter\">Solar Orbiter<\/a>, the <a href=\"https:\/\/sdo.gsfc.nasa.gov\/\">Solar Dynamics Observatory<\/a> and others, available to <a href=\"https:\/\/theconversation.com\/scientists-call-the-region-of-space-influenced-by-the-sun-the-heliosphere-but-without-an-interstellar-probe-they-dont-know-much-about-its-shape-227131\">monitor the heliosphere<\/a> \u2013 the region surrounding the Sun \u2013 from a variety of vantage points.<\/p>\n\n\n\n<p>These resources, coupled with advanced modeling capabilities, provide timely and effective ways to investigate how CMEs cause geomagnetic storms. The <a href=\"https:\/\/science.nasa.gov\/science-research\/heliophysics\/nasa-noaa-sun-reaches-maximum-phase-in-11-year-solar-cycle\/\">Sun will reach its solar maximum<\/a> in the years 2024 and 2025. So, with more complex CMEs coming from the Sun in the next few years and an increasing reliance on space-based infrastructure for communication, navigation and scientific exploration, monitoring these events is more important than ever.<\/p>\n\n\n\n<p>Integrating the observational data from space-based missions such as <a href=\"https:\/\/science.nasa.gov\/mission\/wind\/\">Wind<\/a> and <a href=\"https:\/\/science.nasa.gov\/mission\/ace\/\">ACE<\/a> and data from ground-based facilities such as <a href=\"https:\/\/www.e-callisto.org\/\">the e-Callisto network<\/a> and radio observatories with state-of-the-art simulation tools allows researchers to analyze the data in real time. That way, they can quickly make predictions about what the CMEs are doing.<\/p>\n\n\n\n<p>These advancements are important for keeping infrastructure safe and preparing for the next solar maximum. Addressing these challenges today ensures <a href=\"https:\/\/theconversation.com\/space-weather-forecasting-needs-an-upgrade-to-protect-future-artemis-astronauts-224921\">resilience against future space weather<\/a>.<\/p>\n\n\n\n<p><a href=\"https:\/\/theconversation.com\/profiles\/shirsh-lata-soni-2297636\">Shirsh Lata Soni<\/a>, Postdoctoral Research Fellow, <em><a href=\"https:\/\/theconversation.com\/institutions\/university-of-michigan-1290\">University of Michigan<\/a><\/em><\/p>\n\n\n\n<p>This article is republished from <a href=\"https:\/\/theconversation.com\">The Conversation<\/a> under a Creative Commons license. Read the <a href=\"https:\/\/theconversation.com\/colliding-plasma-ejections-from-the-sun-generate-huge-geomagnetic-storms-studying-them-will-help-scientists-monitor-future-space-weather-248384\">original article<\/a>.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Shirsh Lata Soni, University of Michigan The Sun periodically ejects huge bubbles of plasma from its surface that contain an intense magnetic field. These events are called coronal mass ejections, or CMEs. When two of these ejections collide, they can generate powerful geomagnetic storms that can lead to beautiful auroras but may disrupt satellites and [&hellip;]<\/p>\n","protected":false},"author":56,"featured_media":38827,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":[],"categories":[292,1862,10,3410],"tags":[16063,11532,11531,16064,885,891,886,860,6016,1188,16066,11528,5614,187,16065,2913],"_links":{"self":[{"href":"https:\/\/www.lifeandnews.com\/articles\/wp-json\/wp\/v2\/posts\/38826"}],"collection":[{"href":"https:\/\/www.lifeandnews.com\/articles\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.lifeandnews.com\/articles\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.lifeandnews.com\/articles\/wp-json\/wp\/v2\/users\/56"}],"replies":[{"embeddable":true,"href":"https:\/\/www.lifeandnews.com\/articles\/wp-json\/wp\/v2\/comments?post=38826"}],"version-history":[{"count":1,"href":"https:\/\/www.lifeandnews.com\/articles\/wp-json\/wp\/v2\/posts\/38826\/revisions"}],"predecessor-version":[{"id":38828,"href":"https:\/\/www.lifeandnews.com\/articles\/wp-json\/wp\/v2\/posts\/38826\/revisions\/38828"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.lifeandnews.com\/articles\/wp-json\/wp\/v2\/media\/38827"}],"wp:attachment":[{"href":"https:\/\/www.lifeandnews.com\/articles\/wp-json\/wp\/v2\/media?parent=38826"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.lifeandnews.com\/articles\/wp-json\/wp\/v2\/categories?post=38826"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.lifeandnews.com\/articles\/wp-json\/wp\/v2\/tags?post=38826"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}