{"id":3581,"date":"2024-05-24T11:48:10","date_gmt":"2024-05-24T11:48:10","guid":{"rendered":"https:\/\/digitaltradecenter.com\/index.php\/2024\/05\/24\/scientists-say-theyve-found-where-the-suns-magnetic-field-originates\/"},"modified":"2024-05-24T11:48:10","modified_gmt":"2024-05-24T11:48:10","slug":"scientists-say-theyve-found-where-the-suns-magnetic-field-originates","status":"publish","type":"post","link":"https:\/\/digitaltradecenter.com\/index.php\/2024\/05\/24\/scientists-say-theyve-found-where-the-suns-magnetic-field-originates\/","title":{"rendered":"Scientists say they\u2019ve found where the sun\u2019s magnetic field originates"},"content":{"rendered":"<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi1180k000m1oqj33od2o4g@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            The sun has a powerful magnetic field that creates sunspots on the star\u2019s surface and unleashes solar storms such as the one that bathed much of the planet in beautiful auroras this month.    <\/p>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4xav8000j356jc5qa46ep@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            But exactly how that magnetic field is generated inside the sun is a puzzle that has vexed astronomers for centuries, going back to the time of Italian astronomer Galileo,<strong> <\/strong>who made the first observations of sunspots in the early 1600s, and noticed how they varied over time.    <\/p>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4xav8000k356jwfud1qnc@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            Researchers behind an interdisciplinary study have put forth a new theory in a report published Wednesday in the journal Nature. In contrast to previous research that assumed the sun\u2019s magnetic field originates from deep within the celestial body, they suspect the the source is much closer to the surface.    <\/p>\n<div data-uri=\"cms.cnn.com\/_components\/related-content\/instances\/clwi620u100003b6hbuispxt5@published\" class=\"related-content_full-width related-content_full-width--article\" data-article-gutter=\"true\">\n<div class=\"related-content_full-width__image image__related-content\">            <\/div>\n<p class=\"related-content_full-width__headline\">            <span class=\"related-content_full-width__title-text\" data-editable=\"content.title\">Related article<\/span>      <span class=\"related-content_full-width__headline-text\" data-editable=\"content.headline\">Study proves black holes have a \u2018plunging region,\u2019 just as Einstein predicted<\/span>    <\/p>\n<\/p>\n<\/div>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4xav8000l356j1ey4n1me@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            The model developed by the team could help scientists better understand the 11-year solar cycle and improve the forecasting of space weather, which can disrupt GPS and communication satellites as well as dazzle night sky watchers with auroras.    <\/p>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4xav8000m356jjbm1zwf0@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            \u201cThis work proposes a new hypothesis for how the sun\u2019s magnetic field is generated that better matches solar observations, and, we hope, could be used to make better predictions of solar activity,\u201d said Daniel Lecoanet, an assistant professor of engineering sciences and applied mathematics at Northwestern University\u2019s McCormick School of Engineering and a member of the Center for Interdisciplinary Exploration and Research in Astrophysics.    <\/p>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4xav9000n356jrea3reaf@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            \u201cWe want to forecast if the next solar cycle will be particularly strong, or maybe weaker than normal. The previous models (assuming the solar magnetic field is generated deep within the Sun) have not been able to make accurate forecasts or (determine) if&nbsp;the next solar cycle will be strong or weak,\u201d he added.    <\/p>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4xav9000o356jzgejto9q@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            Sunspots help scientists track the sun\u2019s activity. They are the origin point for the explosive flares and ejection events that release light, solar material and energy into space. The recent solar storm is evidence of the sun approaching \u201csolar maximum\u201d \u2014 the point in its 11-year cycle when there is the highest number of sunspots.    <\/p>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4xav9000p356jbzyoipnz@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            \u201cBecause we think the number of sunspots tracks with the strength of the magnetic field within the Sun, we think the 11-year sunspot cycle is reflecting a cycle in the strength of the Sun\u2019s interior magnetic field,\u201d Lecoanet said.    <\/p>\n<h3 class=\"subheader\" data-editable=\"text\" data-uri=\"cms.cnn.com\/_components\/subheader\/instances\/clwi4xav9000q356jpcvc0jtt@published\" data-component-name=\"subheader\" id=\"modeling-the-suns-magnetic-field\" data-article-gutter=\"true\">    Modeling the sun\u2019s magnetic field<\/h3>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4zg210017356jserujo8o@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            It\u2019s difficult to see the sun\u2019s magnetic field lines, which loop through the solar atmosphere to form a complicated web of magnetic structures far more complex than Earth\u2019s magnetic field. To better grasp how the sun\u2019s magnetic field works, scientists turn to mathematical models.    <\/p>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4zidi0019356jmm8bg8ys@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            In a scientific first, the model that Lecoanet and his colleagues developed accounted for a phenomenon called torsional oscillation \u2014 magnetically driven flows of gas and plasma within and around the sun that contribute to sunspot formation.    <\/p>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4zidi001a356j722eed8h@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            In some areas, the rotation of this solar feature speeds up or slows down, while in others it remains steady. Like the 11-year solar magnetic cycle, torsional oscillations also experience an 11-year cycle.    <\/p>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4zidi001b356jib4iyp1i@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            \u201cSolar observations have given us a good idea for how material moves around inside of the Sun. For our supercomputing calculations, we solved equations to determine how the magnetic field changes within the Sun due to the observed motions,\u201d Lecoanet said.    <\/p>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4zidi001c356jwd0cag0j@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            \u201cNo one had done this calculation before because no one knew how to efficiently perform the calculation,\u201d he added.    <\/p>\n<div data-uri=\"cms.cnn.com\/_components\/related-content\/instances\/clwi50h22001z356jb0cb9w78@published\" class=\"related-content_full-width related-content_full-width--gallery\" data-article-gutter=\"true\">\n<div class=\"related-content_full-width__image image__related-content\">\n<div class=\"image__label image__label--type-gallery image__label--small image__label--visible\">            <span class=\"image__label-icon\"><\/span>gallery          <\/div>\n<\/div>\n<p class=\"related-content_full-width__headline\">            <span class=\"related-content_full-width__title-text\" data-editable=\"content.title\">Related gallery<\/span>      <span class=\"related-content_full-width__headline-text\" data-editable=\"content.headline\">In pictures: Auroras light the sky during rare solar storm<\/span>    <\/p>\n<\/p>\n<\/div>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4zidi001d356je1fclgdf@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            The group\u2019s calculations showed that magnetic fields can be generated about 20,000 miles (32,100 kilometers) below the sun\u2019s surface \u2014 far closer to the surface than had previously been assumed. Other models had suggested it was much deeper \u2014 around 130,000 miles (209,200 kilometers).    <\/p>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4zidi001e356jvwr5y965@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            \u201cOur new hypothesis provides a natural explanation for the torsional oscillations that is missing from previous models,\u201d Lecoanet said.    <\/p>\n<h3 class=\"subheader\" data-editable=\"text\" data-uri=\"cms.cnn.com\/_components\/subheader\/instances\/clwi4zidi001f356jp0lyoyeo@published\" data-component-name=\"subheader\" id=\"astrophysical-enigma\" data-article-gutter=\"true\">    \u2018Astrophysical enigma\u2019<\/h3>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4zidi001g356jm6fyy6x5@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            An important breakthrough was developing new numerical algorithms for running the calculations, Lecoanet said. The paper\u2019s lead author Geoff Vasil, a professor at the University of Edinburgh in the United Kingdom, came up with the idea about 20 years ago, Lecoanet said, but it took over 10 years to develop the algorithms and required a powerful NASA supercomputer to conduct the simulations.    <\/p>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4zidi001h356jjkrjfqst@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            \u201cWe have used around 15 million CPU-hours for this investigation,\u201d he said. \u201cThat means that if I had tried to run the calculations on my laptop, it would have taken me about 450 years.\u201d    <\/p>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4zidi001i356jwr0b6l4k@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            In a commentary published alongside the study, Ellen Zweibel, a professor of astronomy and physics at the University of Wisconsin-Madison, said the initial results were intriguing and would help inform future models and research. She was not involved in the study.    <\/p>\n<p class=\"paragraph inline-placeholder vossi-paragraph-primary-core-light\" data-uri=\"cms.cnn.com\/_components\/paragraph\/instances\/clwi4zidi001j356jr4lvg3fo@published\" data-editable=\"text\" data-component-name=\"paragraph\" data-article-gutter=\"true\">            Zweibel said the team had added \u201ca provocative ingredient to the theoretical mix that could prove key to unravelling this astrophysical enigma.\u201d    <\/p>\n<\/p>\n<div>This post appeared first on cnn.com<\/div>\n<p><\/p>\n","protected":false},"excerpt":{"rendered":"<p>The sun has a powerful magnetic field that creates sunspots on the star\u2019s surface and unleashes solar storms such as the one that bathed much of the planet in beautiful auroras this month. But exactly how that magnetic field is generated inside the sun is a puzzle that has vexed astronomers for centuries, going back <\/p>\n","protected":false},"author":1,"featured_media":3582,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[23],"tags":[],"class_list":{"0":"post-3581","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-world-news"},"_links":{"self":[{"href":"https:\/\/digitaltradecenter.com\/index.php\/wp-json\/wp\/v2\/posts\/3581","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/digitaltradecenter.com\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/digitaltradecenter.com\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/digitaltradecenter.com\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/digitaltradecenter.com\/index.php\/wp-json\/wp\/v2\/comments?post=3581"}],"version-history":[{"count":0,"href":"https:\/\/digitaltradecenter.com\/index.php\/wp-json\/wp\/v2\/posts\/3581\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/digitaltradecenter.com\/index.php\/wp-json\/wp\/v2\/media\/3582"}],"wp:attachment":[{"href":"https:\/\/digitaltradecenter.com\/index.php\/wp-json\/wp\/v2\/media?parent=3581"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/digitaltradecenter.com\/index.php\/wp-json\/wp\/v2\/categories?post=3581"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/digitaltradecenter.com\/index.php\/wp-json\/wp\/v2\/tags?post=3581"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}