{"id":1914,"date":"2015-01-04T10:07:40","date_gmt":"2015-01-04T10:07:40","guid":{"rendered":"http:\/\/revoscience.com\/en\/?p=1914"},"modified":"2023-09-06T12:56:08","modified_gmt":"2023-09-06T07:11:08","slug":"the-sun-exploring-as-fire-from-an-ice-cube","status":"publish","type":"post","link":"https:\/\/www.revoscience.com\/en\/the-sun-exploring-as-fire-from-an-ice-cube\/","title":{"rendered":"The sun exploring as fire from an ice cube"},"content":{"rendered":"\n<p><span style=\"color: #000000;\"><b>This is one of the amazing image of the sun exploring the colored and sparkling stuff that one has ever watched.<\/b><\/span><\/p>\n\n\n\n<p><span style=\"color: #000000;\">The reddish stuff may look familiar. That\u2019s&nbsp;material in the Sun\u2019s atmosphere, or corona, as imaged by NASA\u2019s orbiting&nbsp;<a style=\"color: #ff0000;\" href=\"http:\/\/sdo.gsfc.nasa.gov\/mission\/\" target=\"_blank\" rel=\"noopener\"><span style=\"color: #000000;\">Solar Dynamics Observatory<\/span><\/a>, which has been sending back data for nearly four years. But that ethereal blue and green glow? \u2014 that\u2019s something else entirely.<\/span><\/p>\n\n\n\n<p><span style=\"color: #000000;\">The glow&nbsp;was captured separately&nbsp;by the orbiting&nbsp;<a style=\"color: #ff0000;\" href=\"http:\/\/www.nustar.caltech.edu\/page\/about\" target=\"_blank\" rel=\"noopener\"><span style=\"color: #000000;\">Nuclear Spectroscopic Telescope Array<\/span><\/a>&nbsp;spacecraft, or NuSTAR, and laid over the SDO image to create a composite.&nbsp; As&nbsp;the most sensitive view of&nbsp;high-energy X-ray radiation streaming off the sun, NuSTAR\u2019s contribution may help scientists solve a long-standing mystery: Why is the corona blisteringly hot while the solar surface is considerably cooler?<\/span><\/p>\n\n\n\n<p><span style=\"color: #000000;\">An hypothesized&nbsp;phenomenon called \u201cnanoflares\u201d may provide the answer.<\/span><\/p>\n\n\n\n<p><span style=\"color: #000000;\">\u201cAt first I thought the whole idea was crazy,\u201d&nbsp;<a style=\"color: #ff0000;\" href=\"http:\/\/www.jpl.nasa.gov\/news\/news.php?feature=4422\" target=\"_blank\" rel=\"noopener\"><span style=\"color: #000000;\">says Fiona Harrison<\/span><\/a>, NuSTAR\u2019s principal investigator and a scientist&nbsp;at&nbsp;the California Institute of Technology in Pasadena. But she warmed to the idea when she realized that&nbsp;NuSTAR\u2019s sensor could pick up the&nbsp;faint&nbsp;flashes of X-ray radiation&nbsp;that would be emitted by hypothesized nanoflares.Scientists did not originally intend to use NuSTAR to&nbsp;examine the Sun.&nbsp;The orbiting telescope&nbsp;was actually&nbsp;designed to peer deep into the universe \u2014 to&nbsp;look for collapsed stars and black holes, map supernova remnants, and examine galaxies hosting supermassive black holes.<\/span><\/p>\n\n\n\n<p><span style=\"color: #000000;\">Regular solar flares&nbsp;are not hypothetical at all. I\u2019ve written about them many times (<span style=\"color: #000000;\">here<\/span>&nbsp;and&nbsp;<a style=\"color: #ff0000;\" href=\"http:\/\/blogs.discovermagazine.com\/imageo\/2014\/10\/21\/flares-erupt-active-region-sun\/#.VJm4AtAA\" target=\"_blank\" rel=\"noopener\"><span style=\"color: #000000;\">here<\/span><\/a>, for example).&nbsp;They occur when magnetic energy builds up in the Sun\u2019s atmosphere and is then released suddenly with an accompanying burst of radiation across the electromagnetic spectrum.<\/span><\/p>\n\n\n\n<p><span style=\"color: #000000;\">As their name implies, nanoflares would be much smaller. Should they exist, they may explain why the temperature of the solar corona&nbsp;is 1.8 million degrees Fahrenheit&nbsp;on average while the surface of the sun below it is just 10,800 F.<\/span><\/p>\n\n\n\n<p><span style=\"color: #000000;\">\u201cIt is like a flame coming out of an ice cube,\u201d as NASA explained it in a&nbsp;<a style=\"color: #ff0000;\" href=\"http:\/\/www.jpl.nasa.gov\/news\/news.php?feature=4422\" target=\"_blank\" rel=\"noopener\"><span style=\"color: #000000;\">press release<\/span><\/a>.<\/span><\/p>\n\n\n\n<p><span style=\"color: #000000;\">Among scientists, the mystery is known as the \u201ccoronal heating problem.\u201d In short, where is all that heat coming from? The energy released by regular flares alone&nbsp;is not enough to account for it. But if nanoflares really do exist, that might solve the mystery.<\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>This is one of the amazing image of the sun exploring the colored and sparkling stuff that one has ever watched. The reddish stuff may look familiar. That\u2019s&nbsp;material in the Sun\u2019s atmosphere, or corona, as imaged by NASA\u2019s orbiting&nbsp;Solar Dynamics Observatory, which has been sending back data for nearly four years. But that ethereal blue [&hellip;]<\/p>\n","protected":false},"author":6,"featured_media":1915,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[3],"tags":[],"class_list":["post-1914","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-news"],"featured_image_urls":{"full":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520.jpg",1024,520,false],"thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520-150x150.jpg",150,150,true],"medium":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520-300x152.jpg",300,152,true],"medium_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520.jpg",750,381,false],"large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520.jpg",750,381,false],"1536x1536":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520.jpg",1024,520,false],"2048x2048":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520.jpg",1024,520,false],"ultp_layout_landscape_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520.jpg",1024,520,false],"ultp_layout_landscape":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520.jpg",870,442,false],"ultp_layout_portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520.jpg",600,305,false],"ultp_layout_square":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520.jpg",600,305,false],"newspaper-x-single-post":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520.jpg",760,386,false],"newspaper-x-recent-post-big":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520.jpg",550,279,false],"newspaper-x-recent-post-list-image":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520.jpg",95,48,false],"web-stories-poster-portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520.jpg",640,325,false],"web-stories-publisher-logo":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520.jpg",96,49,false],"web-stories-thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/01\/PIA18906_hires-1024x520.jpg",150,76,false]},"author_info":{"info":["Amrita Tuladhar"]},"category_info":"<a href=\"https:\/\/www.revoscience.com\/en\/category\/news\/\" rel=\"category tag\">News<\/a>","tag_info":"News","comment_count":"0","_links":{"self":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/1914","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/users\/6"}],"replies":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/comments?post=1914"}],"version-history":[{"count":0,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/1914\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media\/1915"}],"wp:attachment":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media?parent=1914"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/categories?post=1914"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/tags?post=1914"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}