One year on, NASA scientists are still making huge discoveries about the largest geomagnetic storm to hit Earth in two decades, the Gannon storm. The findings are helping us better understand and prepare for the ways in which the Sun\u2019s activity can affect us.<\/p>\n<\/p>\n
On May 10, 2024, the first G5 or \u201csevere\u201d geomagnetic storm in over two decades hit Earth. The event did not cause any catastrophic damages, but it did produce surprising effects on Earth. The storm, which has been called the best-documented geomagnetic storm in history, spread auroras to unusually low latitudes and produced effects spanning from the ground to near-Earth space. Data captured during this historic event will be analyzed for years to come, revealing new lessons about the nature of geomagnetic storms and how best to weather them. Credit: NASA\/Joy Ng<\/p>\n
One year ago today, representatives from NASA and about 30 other U.S. government agencies gathered for a special meeting to simulate and address a threat looming in space. The threat was not an asteroid or aliens, but our very own life-giving Sun.<\/p>\n
The inaugural Space Weather Tabletop Exercise<\/a> was supposed to be a training event, where experts could work through the real-time ramifications of a geomagnetic storm, a global disruption to Earth\u2019s magnetic field. Driven by solar eruptions, geomagnetic storms can decimate satellites, overload electrical grids, and expose astronauts to dangerous radiation. Minimizing the impacts of such storms requires close coordination, and this meeting was their chance to practice.<\/p>\n Then, their simulation turned into reality.<\/p>\n \u201cThe plan was to run through a hypothetical scenario, finding where our existing processes worked and where they needed improvement,\u201d said Jamie Favors, director of NASA\u2019s Space Weather Program at NASA Headquarters in Washington. \u201cBut then our hypothetical scenario was interrupted by a very real one.\u201d<\/p>\n On May 10, 2024, the first G5 or \u201csevere\u201d geomagnetic storm in over two decades hit Earth. The event, named the Gannon storm in memory of leading space weather physicist Jennifer Gannon, did not cause any catastrophic damages. But a year on, key insights from the Gannon storm are helping us understand and prepare for future geomagnetic storms.<\/p>\n The Gannon storm had effects on and off our planet.<\/p>\n On the ground, some high-voltage lines tripped, transformers overheated, and GPS-guided tractors veered off-course in the Midwestern U.S., further disrupting planting that had already been delayed by heavy rains that spring.<\/p>\n \u201cNot all farms were affected, but those that were lost on average about $17,000 per farm,\u201d said Terry Griffin, a professor of Agricultural Economics at Kansas State University. \u201cIt\u2019s not catastrophic, but they’ll miss it.\u201d<\/p>\n In the air, the threat of higher radiation exposure, as well as communication and navigation losses, forced trans-Atlantic flights to change course.<\/p>\n During the storm, Earth\u2019s upper atmospheric layer called the thermosphere heated to unusually high temperatures. At 100 miles altitude, the temperature typically peaks at 1,200 degrees Fahrenheit, but during the storm it surpassed 2,100 degrees Fahrenheit<\/a>. NASA\u2019s GOLD (Global-scale Observations of the Limb and Disk<\/a>) mission observed<\/a> the atmosphere expanding from the heat to create a strong wind that lofted heavy nitrogen particles higher.<\/p>\n In orbit, the expanded atmosphere increased drag on thousands of satellites. NASA\u2019s ICESat-2<\/a> lost altitude and entered safe mode<\/a> while NASA\u2019s Colorado Inner Radiation Belt Experiment<\/a> (CIRBE) CubeSat deorbited prematurely five months after the storm. Others, such as the European Space Agency\u2019s Sentinel<\/a> mission, required more power to maintain their orbits and perform maneuvers to avoid collisions with space debris.<\/p>\n The storm also dramatically changed the structure of an atmospheric layer called the ionosphere. A dense zone of the ionosphere that normally covers the equator at night dipped toward the South Pole in a check mark shape<\/a>, causing a temporary gap near the equator.<\/p>\n The Gannon storm also rocked Earth\u2019s magnetosphere, the magnetic bubble surrounding the planet. Data from NASA missions MMS<\/a> (Magnetospheric Multiscale) and THEMIS-ARTEMIS<\/a> \u2014 short for Time History of Events and Macroscale Interactions-Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon\u2019s Interaction with the Sun \u2014 saw giant, curling waves of particles and rolled-up magnetic fields along the edge of the CMEs. These waves were perfectly sized to periodically dump extra magnetic energy and mass into the magnetosphere upon impact, creating the largest electrical current<\/a> seen in the magnetosphere in 20 years.<\/p>\n Incoming energy and particles from the Sun also created two new temporary belts<\/a> of energetic particles within the magnetosphere. Discovered by CIRBE, these belts formed between the Van Allen radiation belts that permanently surround Earth. The belt\u2019s discovery is important to spacecraft and astronauts that can be imperiled by high-energy electrons and protons in the belts.<\/p>\n The storm also ignited auroras<\/a> around the globe, including places where these celestial light shows are rare. NASA\u2019s Aurorasaurus<\/a> project was flooded with more than 6,000 observer reports from over 55 countries and all seven continents.<\/p>\n Photographers helped scientists understand why auroras observed throughout Japan were magenta rather than the typical red. Researchers studied hundreds of photos and found the auroras were surprisingly high \u2014 around 600 miles above the ground (200 miles higher than red auroras typically appear).<\/p>\n In a paper<\/a> published in the journal Scientific Reports, the research team says the peculiar color likely resulted from a mix of red and blue auroras, produced by oxygen and nitrogen molecules lofted higher than usual as the Gannon storm heated and expanded the upper atmosphere.<\/p>\n \u201cIt typically needs some special circumstances, like we saw last May,\u201d co-author Josh Pettit of NASA\u2019s Goddard Space Flight Center said of Japan\u2019s magenta auroras. \u201cA very unique event indeed.\u201d<\/p>\n Impacts of the Sun\u2019s amped-up solar activity didn\u2019t end at Earth. The solar active region that sparked the Gannon storm eventually rotated away from our planet and redirected its outbursts toward Mars.<\/p>\n As energetic particles from the Sun struck the Martian atmosphere, NASA\u2019s MAVEN<\/a> (Mars Atmosphere and Volatile Evolution) orbiter watched auroras engulf the Red Planet from May 14 to 20.<\/p>\n Solar particles overwhelmed the star camera on NASA\u2019s 2001 Mars Odyssey<\/a> orbiter (which uses stars to orient the spacecraft), causing the camera to cut out for almost an hour.<\/p>\n On the Martian surface, images from the navigation cameras on NASA\u2019s Curiosity<\/a> rover were freckled with \u201csnow\u201d \u2014 streaks and specks caused by charged particles. Meanwhile, Curiosity\u2019s Radiation Assessment Detector<\/a> recorded the biggest surge of radiation since the rover landed in 2012. If astronauts had been there, they would have received a radiation dose of 8,100 micrograys \u2014 equivalent to 30 chest X-rays.<\/p>\n The Gannon storm spread auroras to unusually low latitudes and has been called the best-documented geomagnetic storm in history. A year on, we have just begun unraveling its story. Data captured during this historic event will be analyzed for years to come, revealing new lessons about the nature of geomagnetic storms and how best to weather them.<\/p>\n By Mara Johnson-Groh<\/a>, Miles Hatfield<\/a>, and Vanessa Thomas<\/a><\/strong>
NASA\u2019s Goddard Space Flight Center, Greenbelt, Md.<\/strong><\/p>\n","protected":false},"excerpt":{"rendered":"One year on, NASA scientists are still making huge discoveries about the largest geomagnetic storm to hit Earth…\n","protected":false},"author":2,"featured_media":89005,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[3844],"tags":[42316,13453,42317,3888,42318,42319,42320,42321,42322,42323,42324,42325,42326,42329,70,5635,22970,42327,413,3891,14268,42328,42330,16,15],"class_list":{"0":"post-89004","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-space","8":"tag-auroras","9":"tag-curiosity-rover","10":"tag-earths-magnetic-field","11":"tag-goddard-space-flight-center","12":"tag-gold-global-scale-observations-of-the-limb-and-disk","13":"tag-heliophysics","14":"tag-heliophysics-division","15":"tag-magnetosphere","16":"tag-magnetospheric-multiscale-mms","17":"tag-mars-odyssey","18":"tag-maven-mars-atmosphere-and-volatile-evolution","19":"tag-nasa-centers-facilities","20":"tag-nasa-directorates","21":"tag-reconnection","22":"tag-science","23":"tag-science-research","24":"tag-science-mission-directorate","25":"tag-solar-dynamics-observatory-sdo","26":"tag-space","27":"tag-the-solar-system","28":"tag-the-sun","29":"tag-themis-artemis-time-history-of-events-and-macroscale-interactions-during-substorms-acceleration","30":"tag-turbulence-and-electrodynamics-of-moons-interaction-with-the-sun","31":"tag-uk","32":"tag-united-kingdom"},"share_on_mastodon":{"url":"","error":"Validation failed: Text character limit of 500 exceeded"},"_links":{"self":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/posts\/89004","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/comments?post=89004"}],"version-history":[{"count":0,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/posts\/89004\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/media\/89005"}],"wp:attachment":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/media?parent=89004"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/categories?post=89004"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/tags?post=89004"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}