{"id":9115,"date":"2024-01-31T14:58:29","date_gmt":"2024-01-31T19:58:29","guid":{"rendered":"https:\/\/spaceandplanetarynewswire.com\/?p=9115"},"modified":"2024-01-31T14:58:29","modified_gmt":"2024-01-31T19:58:29","slug":"the-hottest-catalog-of-the-year-the-most-comprehensive-list-of-slow-building-solar-flares-yet","status":"publish","type":"post","link":"https:\/\/spaceandplanetarynewswire.com\/?p=9115","title":{"rendered":"The Hottest Catalog of the Year: The Most Comprehensive List of Slow-Building Solar Flares Yet"},"content":{"rendered":"
This image, taken on Aug. 5, 2023, shows a blend of extreme ultraviolet light that highlights the intensely hot material in flares and which is colorized in red and orange.<\/figcaption><\/figure>\n

Solar flares occur when magnetic energy builds up in the Sun\u2019s atmosphere and is released as electromagnetic radiation. Lasting anywhere from a few minutes to a few hours, flares usually reach temperatures around 10 million degrees Kelvin. Because of their intense electromagnetic energy, solar flares can cause disruptions in radio communications, Earth-orbiting satellites and even result in blackouts.<\/p>\n

Although flares have been classified based on the amount of energy they emit at their peak, there has not been significant study into differentiating flares based on the speed of energy build-up since slow-building flares were first discovered in the 1980s. In a new paper in Solar Physics<\/a><\/em>, a team, led by UC San Diego astrophysics graduate student Aravind Bharathi Valluvan, has shown that there is a significant amount of slower-type flares worthy of further investigation.<\/p>\n

The width-to-decay ratio of a flare is the time it takes to reach maximum intensity to the time it takes to dissipate its energy. Most commonly, flares spend more time dissipating than rising. In a 5-minute flare, it may take 1 minute to rise and 4 minutes to dissipate for a ratio of 1:4. In slow-building flares, that ratio may be 1:1, with 2.5 minutes to rise and 2.5 minutes to dissipate.<\/p>\n

Valluvan was a student at the Indian Institute of Technology Bombay (IITB) when this work was conducted. Exploiting the increased capabilities of the Chandrayaan-2 solar orbiter, IITB researchers used the first three years of observed data to catalog nearly 1400 slow-rising flares \u2014 a dramatic increase over the roughly 100 that had been previously observed over the past four decades. <\/p>\n

It was thought that solar flares were like the snap of a whip \u2014 quickly injecting energy before slowly dissipating. Now seeing slow-building flares in such high quantities may change that thinking.<\/p>\n

\u201cThere is thrilling work to be done here,\u201d stated Valluvan who now works in UC San Diego Professor of Astronomy and Astrophysics Steven Boggs\u2019 group. \u201cWe\u2019ve identified two different types of flares, but there may be more. And where do the processes differ? What makes them rise and fall at different rates? This is something we need to understand.\u201d<\/p>\n","protected":false},"excerpt":{"rendered":"

Solar flares occur when magnetic energy builds up in the Sun\u2019s atmosphere and is released as electromagnetic radiation. Lasting anywhere from a few minutes to a few hours, flares usually reach temperatures around 10 million degrees Kelvin. Because of their intense electromagnetic energy, solar flares can cause disruptions in radio communications, Earth-orbiting satellites and even…<\/p>\n","protected":false},"author":71,"featured_media":9116,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"ngg_post_thumbnail":0,"fifu_image_url":"https:\/\/earimediaprodweb.azurewebsites.net\/Api\/v1\/Multimedia\/307c01b9-6283-4ef6-ada7-a136a9686f6e\/Rendition\/low-res\/Content\/Public","fifu_image_alt":"The Hottest Catalog of the Year: the Most Comprehensive List of Slow-Building Solar Flares Yet","footnotes":""},"categories":[213],"tags":[],"class_list":["post-9115","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-impact"],"_links":{"self":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/9115","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/users\/71"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=9115"}],"version-history":[{"count":1,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/9115\/revisions"}],"predecessor-version":[{"id":9117,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/9115\/revisions\/9117"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/media\/9116"}],"wp:attachment":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=9115"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=9115"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=9115"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}