{"id":227569,"date":"2025-10-27T04:42:18","date_gmt":"2025-10-27T04:42:18","guid":{"rendered":"https:\/\/www.newsbeep.com\/uk\/227569\/"},"modified":"2025-10-27T04:42:18","modified_gmt":"2025-10-27T04:42:18","slug":"theres-something-about-our-sun-that-doesnt-make-sense-scientists-may-just-have-cracked-it","status":"publish","type":"post","link":"https:\/\/www.newsbeep.com\/uk\/227569\/","title":{"rendered":"There&#8217;s something about our Sun that doesn&#8217;t make sense. Scientists may just have cracked it"},"content":{"rendered":"<p>How can the outermost atmosphere of the Sun be hotter than its surface?<\/p>\n<p>It might seem contradictory, but it&#8217;s a well-known phenomenon known as the &#8216;<a href=\"https:\/\/www.skyatnightmagazine.com\/space-science\/coronal-heating-problem\" rel=\"nofollow noopener\" target=\"_blank\">coronal-heating problem<\/a>&#8216; that&#8217;s plagued solar scientists for decades.<\/p>\n<p>A team of scientists might have just cracked it.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" width=\"1200\" height=\"1200\" src=\"https:\/\/www.newsbeep.com\/uk\/wp-content\/uploads\/2025\/10\/proba-3-first-images-coronal-green.jpg\" alt=\"The Sun\u2019s inner corona, coloured artificially to appear dark green, in an image taken on 23 May 2025 by the ASPIICS coronagraph aboard ESA's Proba-3 spacecraft. The image shows observations in the coronal green line, which enables scientists to see the hottest contents of the corona. Credit: ESA\/Proba-3\/ASPIICS. Licence: CC BY-SA 3.0 IGO or ESA Standard Licence\" class=\"wp-image-171782\"\/>The Sun\u2019s inner corona, coloured artificially to appear dark green, in an image taken on 23 May 2025 by the ASPIICS coronagraph aboard ESA&#8217;s Proba-3 spacecraft. The image shows observations in the coronal green line, which enables scientists to see the hottest contents of the corona. Credit: ESA\/Proba-3\/ASPIICS. Licence: CC BY-SA 3.0 IGO or ESA Standard Licence<br \/>\nSolution from solar science sleuths<\/p>\n<p>Researchers say they&#8217;ve achieved a major breakthrough in our understanding of the Sun by solving one of its biggest mysteries.<\/p>\n<p>They&#8217;ve directly observed a mysterious type of magnetic wave rippling through the Sun\u2019s atmosphere.<\/p>\n<p>If true, this could help explain one of the biggest puzzles in solar physics: why the Sun\u2019s outer atmosphere, its corona, is millions of degrees hotter than its surface.<\/p>\n<p>The discovery, published in Nature Astronomy, confirms the existence of small-scale waves known as Alfv\u00e9n waves.<\/p>\n<p>These twisting motions in the Sun\u2019s magnetic field were first predicted back in 1942.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" width=\"1200\" height=\"675\" src=\"https:\/\/www.newsbeep.com\/uk\/wp-content\/uploads\/2025\/10\/NASA-SDO-active-region-6395f38.jpg\" alt=\"An active region on the Sun, as seen by NASA's Solar Dynamics Observatory between 5-17 July 2017. This image shows a sunspot in visible and extreme ultraviolet light, with particles seen spiralling along magnetic field lines. Credit: NASA\u2019s Goddard Space Flight Center\/SDO\" class=\"wp-image-60896\"\/>An active region on the Sun, as seen by NASA&#8217;s Solar Dynamics Observatory between 5-17 July 2017. This image shows a sunspot in visible and extreme ultraviolet light, with particles seen spiralling along magnetic field lines. Credit: NASA\u2019s Goddard Space Flight Center\/SDO<br \/>\nMystery dating almost 100 years<\/p>\n<p>Alfv\u00e9n waves are named after Nobel Prize-winning physicist Hannes Alfv\u00e9n, who predicted them in 1942.<\/p>\n<p>They&#8217;re magnetic disturbances that carry energy through plasma, the hot, charged gas that makes up most of the Sun.<\/p>\n<p>Scientists have detected larger versions of these waves before, usually linked to explosions on the surface of the Sun called <a href=\"https:\/\/www.skyatnightmagazine.com\/space-science\/solar-flares\" rel=\"nofollow noopener\" target=\"_blank\">solar flares<\/a>.<\/p>\n<p>But this new study marks the first direct evidence of the small, constantly occurring twisting kind that may continuously power the Sun\u2019s outer atmosphere.<\/p>\n<p>&#8220;This discovery ends a protracted search for these waves that has its origins in the 1940s,&#8221; says Professor Richard Morton, a UKRI Future Leader Fellow at Northumbria University in the UK, who led the research.<\/p>\n<p>&#8220;We\u2019ve finally been able to directly observe these torsional motions twisting the magnetic field lines back and forth in the corona.&#8221;<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" width=\"1200\" height=\"675\" src=\"https:\/\/www.newsbeep.com\/uk\/wp-content\/uploads\/2025\/10\/Torsional-Lines-sun.jpg\" alt=\"Artist\u2019s representation of twisting magnetic waves revealed for the first time by the NSF Inouye Solar Telescope. They could be key to understanding why the Sun\u2019s atmosphere is so hot. For more information see Morton et al. (2025). Credit: NSF\/NSO\/AURA\/J. Williams\" class=\"wp-image-177787\"\/>Artist\u2019s representation of twisting magnetic waves revealed for the first time by the NSF Inouye Solar Telescope. They could be key to understanding why the Sun\u2019s atmosphere is so hot. For more information see Morton et al. (2025). Credit: NSF\/NSO\/AURA\/J. Williams<br \/>\nPeering into the Sun with the world\u2019s most powerful solar telescope<\/p>\n<p>The breakthrough was made possible by the U.S. National Science Foundation\u2019s Daniel K. Inouye Solar Telescope in Hawaii.<\/p>\n<p>It&#8217;s the world\u2019s most powerful solar telescope, featuring a four-meter-wide mirror and instruments capable of detecting incredibly fine detail on the Sun.<\/p>\n<p>Its Cryogenic Near Infrared Spectropolarimeter (Cryo-NIRSP) instrument allowed scientists to measure tiny shifts in the motion of plasma heated to 1.6 million\u00b0C (2.9 million \u00b0F).<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" width=\"1200\" height=\"800\" src=\"https:\/\/www.newsbeep.com\/uk\/wp-content\/uploads\/2025\/10\/sunspots-Daniel-K-Inouye-Solar-Telescope-social.jpg\" alt=\"Narrowband image of sunspots on the Sun captured by the Daniel K. Inouye Solar Telescope during its Visible Tunable Filter instrument's first light, released 24 April 2025. Credit: VTF\/KIS\/NSF\/NSO\/AURA\" class=\"wp-image-169632\"\/>Narrowband image of sunspots on the Sun captured by the Daniel K. Inouye Solar Telescope during its Visible Tunable Filter instrument&#8217;s first light, released 24 April 2025. Credit: VTF\/KIS\/NSF\/NSO\/AURA<br \/>\nSpotting a twist hidden in the Sun&#8217;s waves<\/p>\n<p>To identify the elusive torsional waves, Professor Morton developed new techniques to separate different kinds of motion seen in data collected by the telescope.<\/p>\n<p>&#8220;The movement of plasma in the Sun\u2019s corona is dominated by swaying motions,&#8221; he says.<\/p>\n<p>&#8220;These mask the torsional motions, so I had to develop a way of removing the swaying to find the twisting.&#8221;<\/p>\n<p>While the more familiar &#8216;kink&#8217; waves make entire magnetic structures sway back and forth \u2013 visible in solar imagery \u2013 the newly detected torsional Alfv\u00e9n waves create subtle twisting motions.<\/p>\n<p>These can only be revealed by measuring how plasma moves toward and away from Earth, which produces red and blue Doppler shifts on opposite sides of magnetic structures.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" width=\"1640\" height=\"1640\" src=\"https:\/\/www.newsbeep.com\/uk\/wp-content\/uploads\/2025\/10\/Inouye-First-Light-Zoom-Image-high-res-fa63324.jpg\" alt=\"A view of the Sun's surface captured by the Daniel K. Inouye Solar Telescope. Credit: NSO\/AURA\/NSF\" class=\"wp-image-44699\"\/>A view of the Sun&#8217;s surface captured by the Daniel K. Inouye Solar Telescope. Credit: NSO\/AURA\/NSF<br \/>\nUnlocking the secrets of the superheated corona<\/p>\n<p>The finding could finally help scientists explain why the Sun\u2019s corona burns at over a million degrees Celsius, while the surface below remains at a comparatively cool 5,500\u00b0C.<\/p>\n<p>Twisting waves may transport and release magnetic energy throughout the corona.<\/p>\n<p>That could be heating plasma and helping drive the solar wind, which is a stream of charged particles that fills our Solar System and generates <a href=\"https:\/\/www.skyatnightmagazine.com\/space-science\/space-weather\" rel=\"nofollow noopener\" target=\"_blank\">space weather<\/a>.<\/p>\n<p>Understanding how these waves work could also improve forecasts of solar activity that can interfere with GPS systems, satellites and power grids.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" width=\"1200\" height=\"616\" src=\"https:\/\/www.newsbeep.com\/uk\/wp-content\/uploads\/2025\/10\/coronal-mass-ejection-earth.jpg\" alt=\"Illustration of a coronal mass ejection impacting the Earth's atmosphere. Credit: Mark Garlick \/ Science Photo Library \/ Getty Images\" class=\"wp-image-173878\"\/>Credit: Mark Garlick \/ Science Photo Library \/ Getty Images<br \/>\nGlobal effort with cosmic implications<\/p>\n<p>The research was an international collaboration involving scientists from Northumbria University, Peking University, KU Leuven, Queen Mary University of London, the Chinese Academy of Sciences, and the NSF National Solar Observatory.<\/p>\n<p>&#8220;This research provides essential validation for the range of theoretical models that describe how Alfv\u00e9n wave turbulence powers the solar atmosphere,&#8221; says Professor Morton.<\/p>\n<p>&#8220;Having direct observations finally allows us to test these models against reality.&#8221;<\/p>\n<p>Read the full paper via <a href=\"https:\/\/www.nature.com\/articles\/s41550-025-02690-9\" target=\"_blank\" rel=\"noreferrer noopener nofollow\">Nature Astronomy<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"How can the outermost atmosphere of the Sun be hotter than its surface? It might seem contradictory, but&hellip;\n","protected":false},"author":2,"featured_media":227570,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[23],"tags":[90,416,56,54,55],"class_list":{"0":"post-227569","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-space","8":"tag-science","9":"tag-space","10":"tag-uk","11":"tag-united-kingdom","12":"tag-unitedkingdom"},"_links":{"self":[{"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/posts\/227569","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/comments?post=227569"}],"version-history":[{"count":0,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/posts\/227569\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/media\/227570"}],"wp:attachment":[{"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/media?parent=227569"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/categories?post=227569"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/tags?post=227569"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}