{"id":18149,"date":"2026-08-06T12:12:26","date_gmt":"2026-08-06T00:12:26","guid":{"rendered":"https:\/\/thebuzz.apnanetwork.co.nz\/?p=18149"},"modified":"2026-08-06T12:12:26","modified_gmt":"2026-08-06T00:12:26","slug":"weve-never-seen-the-sun-in-this-much-detail-before","status":"publish","type":"post","link":"https:\/\/thebuzz.apnanetwork.co.nz\/?p=18149","title":{"rendered":"We&#8217;ve never seen the Sun in this much detail before"},"content":{"rendered":"<div class=\"\">\n<div class=\"border-stroke-default flex h-full\">\n<article class=\"relative h-full grid grid-cols-[2fr_minmax(12.4rem,1fr)] gap-x-16 md:flex md:flex-col md:gap-y-8\">\n<div class=\"image-ring\">The Sun&#8217;s surface is constantly churning with hot, glowing plasma.<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">Those swirling eddies play a huge role in the Sun&#8217;s occasional violent outbursts, but they&#8217;re difficult to see because it is so bright.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">Now astronomers have used the world&#8217;s largest solar telescope to capture the highest-resolution imagery ever taken of our star&#8217;s roiling surface.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">It shows a section of the Sun about 5000 by 3500 kilometres in size: a zone that, on Earth, could comfortably enclose mainland Australia.<\/p>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">The stunning imagery also captures a never-before-seen physical process, which the researchers have described in the journal\u00a0<em class=\"italic\">Nature<\/em>.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">Michael Wheatland, an astrophysicist at the University of Sydney who wasn&#8217;t involved with the research, said the imagery was &#8220;just incredible&#8221;.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">&#8220;We&#8217;ve never observed the Sun at that resolution,&#8221; Professor Wheatland said.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">&#8220;In this amazing detail, we see all of this really interesting fundamental physics happening.&#8221;<\/p>\n<\/div>\n<div class=\"[&amp;_h2]:text-md [&amp;_h3]:text-md [&amp;_h4]:text-md clear-left mb-12 pt-16\">\n<h3 class=\"text-fluid-md-lg leading-snug [&amp;_em]:font-sans-italic [&amp;_cite]:font-sans-italic font-sans-semibold\">Whirling patterns on the Sun&#8217;s surface<\/h3>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">The observations show the solar surface, called the photosphere, constantly swirls and flows with plasma.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">According to the researchers, these ebbs and flows show the plasma undergoes a physical process called Kelvin-Hemholtz instability.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">This effect happens when different types of fluids mix, causing small fluctuations at the borders between them.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">&#8220;You see it in clouds, you see it in the ocean, you see it whenever you have fluids,&#8221; Wheatland said.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">&#8220;But we haven&#8217;t actually seen it on the Sun in a way that&#8217;s really unambiguous. I think the evidence here is completely unambiguous.&#8221;<\/p>\n<\/div>\n<div class=\"pb-16 pt-8\">\n<div class=\"grid justify-center\">\n<figure class=\"mx-auto table\">\n<div class=\"image-ring flex w-full max-w-full -mx-16 md:mx-0 w-screen border-x-0 !max-w-[initial] md:w-[revert-layer] md:!max-w-full [&amp;_img]:w-full [&amp;_img]:md:w-[revert-layer]\"><img loading=\"lazy\" decoding=\"async\" class=\"ml:max-h-[50rem] max-w-full aspect-[16\/10] object-cover\" src=\"https:\/\/media.rnztools.nz\/rnz\/image\/upload\/s--J6PYkf-2--\/t_kt-crop-16x10\/w_614\/f_auto\/q_auto:eco\/4JKBVRF_Simulation_Figure_1_of_2_jpeg\" alt=\"A side-by-side comparison of a real observation from the Inouye Solar Telescope (top left) and a synthetic image generated by state-of-the-art, physics-based computer simulations (top right).\" width=\"614\" height=\"384\" \/><\/div><figcaption class=\"border-stroke-default w-full border-b py-12 text-sm *:inline table-caption caption-bottom mt-auto\">A side-by-side comparison of a real observation from the Inouye Solar Telescope (top left) and a synthetic image generated by state-of-the-art, physics-based computer simulations (top right).<\/p>\n<p class=\"text-foreground-secondary flex-shrink-0 ml-4\">Supplied\/NSF\/NSO\/AURA\/MPS<\/p>\n<\/figcaption><\/figure>\n<\/div>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">On Earth, this instability is often driven by fluids of different temperatures or densities, or moving at different speeds. On the Sun, the differences come from changes in magnetism.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">&#8220;When you mix the fluid, you move the magnetic field around as well,&#8221; Wheatland said.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">This mixing can lead to an increase in energy which could be the reason the Sun&#8217;s corona &#8211; the outer part of its atmosphere &#8211; is so hot.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">The Sun&#8217;s surface is roughly 5500 degrees Celsius, but the corona above it can reach 2 million degrees.<\/p>\n<\/div>\n<div class=\"[&amp;_h2]:text-md [&amp;_h3]:text-md [&amp;_h4]:text-md clear-left mb-12 pt-16\">\n<h3 class=\"text-fluid-md-lg leading-snug [&amp;_em]:font-sans-italic [&amp;_cite]:font-sans-italic font-sans-semibold\">The solar telescope in Hawaii<\/h3>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">Hannah Schunker, an astrophysicist at the University of Newcastle, said because the Sun was so close to Earth &#8211; a mere 149 million kilometres away &#8211; it was the only place astronomers could study the surface of a star in detail.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">&#8220;The Sun is like an astrophysical laboratory,&#8221; Dr Schunker, who also wasn&#8217;t involved with the new research, said.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">The observations were made with the Daniel K. Inouye Solar Telescope, in Hawaii, which is run by the US National Science Foundation.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">Solar telescopes use the same basic technology as other large optical telescopes &#8211; large mirrors and lenses which magnify light &#8211; but since they&#8217;re designed to focus on the Sun, they need to be purpose-built.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">&#8220;The Sun is just so bright and produces so much more heat and light than a distant star,&#8221; Schunker said.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">&#8220;So it requires specialised filters, cooling systems and instruments that can be safely pointed at the Sun without damaging the telescope.&#8221;<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">Friedrich Woeger, senior scientist at the US National Solar Observatory and co-lead author on the paper, said that while preparing for and analysing the observations required months of work, the imagery they captured spans only a few minutes.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">&#8220;The acquisition of the data used in the study itself actually did not take much longer than five minutes,&#8221; Dr Woeger said.<\/p>\n<\/div>\n<div class=\"[&amp;_h2]:text-md [&amp;_h3]:text-md [&amp;_h4]:text-md clear-left mb-12 pt-16\">\n<h3 class=\"text-fluid-md-lg leading-snug [&amp;_em]:font-sans-italic [&amp;_cite]:font-sans-italic font-sans-semibold\">Predicting space weather<\/h3>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">Schunker said it was important to understand the Sun&#8217;s magnetic field because it drives all space weather.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">While these images only capture a small part of the Sun&#8217;s surface for a small period of time, she said data and modelling like this could eventually be used to predict things like solar flares.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">&#8220;These very small-scale changes that are happening on the surface of the Sun, they are responsible for all the larger scale things happening in the atmosphere, and we&#8217;ve never been able to see them before,&#8221; Schunker said.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">Flares and other solar phenomena can cause bright auroras on Earth, and in serious cases prompt power outages and damage to satellites and other technology.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">&#8220;We can take the small-scale physics and put it into the larger-scale models, and this will open the door to, hopefully, better weather predictions, better predictions of flares, [and] better predictions of how heat is transported up to the corona,&#8221; Schunker said.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">Woeger said it would be valuable to have observations of a larger section of the Sun&#8217;s surface to get more data on the patterns they observed.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">&#8220;We are planning for future Inouye Solar Telescope measurements with instruments that provide more information about velocities and magnetic field of the plasma on the Sun,&#8221; Woeger said.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">Wheatland said the imagery signified an exciting time for solar astronomy.<\/p>\n<\/div>\n<div class=\"font-serif-text mb-12 leading-normal\">\n<p class=\"[&amp;_em]:font-serif-text-italic [&amp;_cite]:font-serif-text-italic\">&#8220;Progress will be made in some of the big, outstanding questions in solar physics.&#8221;<\/p>\n<p>Source: ABC &amp; RNZ<\/p>\n<\/div>\n<\/div>\n<\/article>\n<\/div>\n<\/div>\n","protected":false},"excerpt":{"rendered":"<p>The Sun&#8217;s surface is constantly churning with hot, glowing plasma. Those swirling eddies play a huge role in the Sun&#8217;s occasional violent outbursts, but they&#8217;re difficult to see because it is so bright. Now astronomers have used the world&#8217;s largest solar telescope to capture the highest-resolution imagery ever taken of our star&#8217;s roiling surface. It [&hellip;]<\/p>\n","protected":false},"author":6,"featured_media":18150,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[177],"tags":[],"class_list":["post-18149","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-world"],"amp_enabled":true,"_links":{"self":[{"href":"https:\/\/thebuzz.apnanetwork.co.nz\/index.php?rest_route=\/wp\/v2\/posts\/18149","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/thebuzz.apnanetwork.co.nz\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/thebuzz.apnanetwork.co.nz\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/thebuzz.apnanetwork.co.nz\/index.php?rest_route=\/wp\/v2\/users\/6"}],"replies":[{"embeddable":true,"href":"https:\/\/thebuzz.apnanetwork.co.nz\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=18149"}],"version-history":[{"count":1,"href":"https:\/\/thebuzz.apnanetwork.co.nz\/index.php?rest_route=\/wp\/v2\/posts\/18149\/revisions"}],"predecessor-version":[{"id":18151,"href":"https:\/\/thebuzz.apnanetwork.co.nz\/index.php?rest_route=\/wp\/v2\/posts\/18149\/revisions\/18151"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/thebuzz.apnanetwork.co.nz\/index.php?rest_route=\/wp\/v2\/media\/18150"}],"wp:attachment":[{"href":"https:\/\/thebuzz.apnanetwork.co.nz\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=18149"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/thebuzz.apnanetwork.co.nz\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=18149"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/thebuzz.apnanetwork.co.nz\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=18149"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}