{"id":63083,"date":"2025-05-22T15:10:03","date_gmt":"2025-05-22T15:10:03","guid":{"rendered":"https:\/\/nag.com\/?post_type=case-studies&#038;p=63083"},"modified":"2025-05-22T16:11:06","modified_gmt":"2025-05-22T16:11:06","slug":"ska-telescopes-hpc-next-gen-radio-astronomy","status":"publish","type":"case-studies","link":"https:\/\/nag.com\/case-studies\/ska-telescopes-hpc-next-gen-radio-astronomy\/","title":{"rendered":"Powering the SKA Telescopes: HPC for the Next Generation of Radio Astronomy"},"content":{"rendered":"\n<div class=\"gbc-title-banner ta ta-lg ta-xl\" style='background-color: #082d48ff; color: #ffffffff; border-radius: 0px; '>\n    <div class=\"container\" style='border-radius: 0px; '>\n        <div class=\"row justify-content--center\" style='color: #ffffffff;'>\n            <div class=\"col-12\"  >\n                <div class=\"wrap pv-4 \" style=\"0px\">\n                                <div class=\"col-12 col-md-12 col-lg-10 col-xl-8  banner-content\"  >\n    \n                                             <h1>Powering the SKA Telescopes: High-Performance Computing for the Next Generation of Radio Astronomy<\/h1>\n                    \n                    <div class=\"mt-1 mb-1 content\"><p>Case Study<\/p>\n<\/div>\n\n                    \n                                    <\/div>\n                <\/div>\n            <\/div>\n        <\/div>\n    <\/div>\n<\/div>\n\n\n<!-- Spacer -->\n<div class=\"pt- pt-lg- pt-xl-\" ><\/div>\n\n<!-- Spacer -->\n<div class=\"pt-3 pt-lg-3 pt-xl-3\" ><\/div>\n\n<div class=\"container content-area-default \">\n    <div class=\"row justify-content--center\">\n        <div class=\"col-12 col-md-12 col-lg-10 col-xl-8\">\n            <blockquote>\n<h4><em>We\u2019ve helped pave the way for scalable, high-performance <\/em><em>systems that will power radio telescopes for decades to come.<\/em><br \/>Sean Stansill, HPC Software Engineer, <em>n<\/em>AG<\/h4>\n<\/blockquote>\n        <\/div>\n    <\/div>\n<\/div>\n\n<!-- Spacer -->\n<div class=\"pt-1 pt-lg-1 pt-xl-1\" ><\/div>\n\n<div class=\"container content-area-default \">\n    <div class=\"row justify-content--center\">\n        <div class=\"col-12 col-md-12 col-lg-10 col-xl-8\">\n            <p><a href=\"https:\/\/www.skao.int\/en\"><img loading=\"lazy\" decoding=\"async\" class=\"aligncenter wp-image-62355 size-medium\" src=\"https:\/\/nag.com\/wp-content\/uploads\/2025\/05\/skao_logo_2021_colour_rgb_2500x1058px-300x127.jpg\" alt=\"\" width=\"300\" height=\"127\" \/><\/a><\/p>\n        <\/div>\n    <\/div>\n<\/div>\n\n\n<div class=\"content-image-split pv-4  ph-1 \" style=\"background-color: ;\" >\n    <div class=\"container\">\n        <div class=\"row ph-1\">\n            <div class=\"col-12  card-rounded\" >\n\n                <div class=\"row fdir-cr fdir-r-lg \">\n                    <div class=\"content-side df pv-3 ph-1 ph-lg-5 ph-xl-8 c-primary--white col-12 col-lg-6\" style=\"\n                    background-color: #082d48ff;\n                    color: ;\n                    align-items: center; \">\n\n                        <div>\n                                                        <h3>Overview<\/h3>\n<p>The <a href=\"https:\/\/www.skao.int\/en\">SKA Observatory<\/a> (SKAO) is an ambitious, \u20ac2 billion international endeavour to build the world\u2019s largest radio telescope arrays, capable of transforming humanity\u2019s understanding of the universe. Behind this monumental effort lies an equally groundbreaking challenge: processing petabytes of raw data every day into high-resolution astronomical images.<\/p>\n<p>\u00a0<\/p>\n<p><span class=\"nag-n-override\" style=\"margin-left: 0 !important;\"><i>n<\/i><\/span>AG\u2019s High-Performance Computing (HPC) software engineer, Sean Stansill and the <span class=\"nag-n-override\" style=\"margin-left: 0 !important;\"><i>n<\/i><\/span>AG HPC team, plays a pivotal role in making this possible. Their work ensures the seamless transformation of vast volumes of data into science-ready data products, supporting the SKAO&#8217;s mission to accelerate discovery in radio astronomy and gravitational wave science.<\/p>\n<p>Image Copyright: SKAO<\/p>\n                                                    <\/div>\n\n                    <\/div>\n                    <div class=\"img-side small-image-holder col-12 col-lg-6 ph-0 df\" style=\"align-items: center; background-color: #082d48ff;  color: ; \">\n                        <img loading=\"lazy\" decoding=\"async\" width=\"1000\" height=\"566\" src=\"https:\/\/nag.com\/wp-content\/uploads\/2025\/05\/SKAO-at-night-3sites-web.png\" class=\"bg-media \" alt=\"\" style=\"object-position: % %;\" \/>\n                        <div class=\"wrap \">\n                                                    <\/div>\n\n                    <\/div>\n                <\/div>\n\n\n            <\/div>\n\n        <\/div>\n    <\/div>\n<\/div>\n\n<!-- Spacer -->\n<div class=\"pt-1 pt-lg-1 pt-xl-1\" ><\/div>\n\n<div class=\"container content-area-default \">\n    <div class=\"row justify-content--center\">\n        <div class=\"col-12 col-md-12 col-lg-10 col-xl-8\">\n            <h3>Challenge: Turning an Ambitious Concept into an Operational Reality<\/h3>\n<p>While the SKA telescopes have been envisioned since late 1980s, the computing infrastructure required to realise them only recently became feasible. Described as \u201csoftware telescopes,\u201d the SKA project does not rely on a single giant dish. Instead, it combines data from hundreds of smaller dishes and thousands of antennas using complex software pipelines. The computing demand is unprecedented \u2014 the two systems must sustain read\/write speeds around 8 terabytes per second, non-stop.<\/p>\n        <\/div>\n    <\/div>\n<\/div>\n\n<!-- Spacer -->\n<div class=\"pt-1 pt-lg-1 pt-xl-1\" ><\/div>\n\n<div class=\"container content-area-default \">\n    <div class=\"row justify-content--center\">\n        <div class=\"col-12 col-md-12 col-lg-10 col-xl-8\">\n            <p>The real bottleneck? I\/O performance. Unlike embarrassingly parallel tasks, radio astronomy workflows require tightly synchronised data movement across many nodes. This choreography is dictated by the physics of how radio waves are processed. Efficiently managing this scale and complexity is a frontier problem in modern HPC.<\/p>\n        <\/div>\n    <\/div>\n<\/div>\n\n<!-- Spacer -->\n<div class=\"pt-4 pt-lg-4 pt-xl-4\" ><\/div>\n\n<div class=\"container content-area-default \">\n    <div class=\"row justify-content--center\">\n        <div class=\"col-12 col-md-12 col-lg-10 col-xl-8\">\n            <h3>Solution: Engineering Scalable, Future-Proof HPC Software Pipelines\u00a0<\/h3>\n<p><span class=\"nag-n-override\" style=\"margin-left: 0 !important;\"><i>n<\/i><\/span>AG <a href=\"https:\/\/nag.com\/hpc-services\/\">HPC Services<\/a> are playing a significant role in the Science Data Processing (SDP) phase where raw telescope data becomes scientifically useful. Sean Stansill, <span class=\"nag-n-override\" style=\"margin-left: 0 !important;\"><i>n<\/i><\/span>AG HPC Engineer working on the SKAO project has contributed to:<\/p>\n        <\/div>\n    <\/div>\n<\/div>\n\n<div class=\"container content-area-default \">\n    <div class=\"row justify-content--center\">\n        <div class=\"col-12 col-md-12 col-lg-10 col-xl-8\">\n            <ul>\n<li>Development and integration of MSv4, a next-generation data format poised to become the global standard for radio telescopes.<\/li>\n<li>Enhancement of DP3, a calibration tool critical to ensuring scientific accuracy, now with distributed processing support for greater scalability.<\/li>\n<li>Leading input on I\/O architecture and performance optimisation during an international review consisting of 24 institutions.<\/li>\n<\/ul>\n        <\/div>\n    <\/div>\n<\/div>\n\n<div class=\"container content-area-default \">\n    <div class=\"row justify-content--center\">\n        <div class=\"col-12 col-md-12 col-lg-10 col-xl-8\">\n            <p>He has also championed object storage \u2014 a mainstay in cloud computing \u2014 as a novel approach within HPC. Although unconventional in this domain, it offers the flexibility and scalability needed for SKAO\u2019s evolving data landscape, reflecting a broader convergence of HPC and big data technologies.<\/p>\n        <\/div>\n    <\/div>\n<\/div>\n\n<!-- Spacer -->\n<div class=\"pt-2 pt-lg-2 pt-xl-2\" ><\/div>\n\n\n<div class=\"content-image-split pv-4  ph-1 \" style=\"background-color: ;\" >\n    <div class=\"container\">\n        <div class=\"row ph-1\">\n            <div class=\"col-12  card-rounded\" >\n\n                <div class=\"row fdir-cr fdir-r-lg \">\n                    <div class=\"content-side df pv-3 ph-1 ph-lg-5 ph-xl-8 c-primary--white col-12 col-lg-6\" style=\"\n                    background-color: #082d48ff;\n                    color: ;\n                    align-items: center; \">\n\n                        <div>\n                                                        <h3>Impact: <strong>Accelerating Science and Scaling the Future of Astronomy<\/strong><\/h3>\n<p>Sean&#8217;s work ensures that SKA software runs not just effectively, but efficiently \u2014 squeezing maximum performance from existing infrastructure within a cost-conscious budget. One optimisation experiment revealed 4\u00d7 speed improvements simply by doubling the node memory, a change with outsized performance benefits at minimal investment.<\/p>\n<p>These advancements are not confined to code alone \u2014 they enable the SKAO to integrate data processing as a core part of the telescopes, freeing astronomers from manual workflows and fast-tracking discovery. From imaging black hole jets to verifying gravitational waves detected by LIGO, SKAO&#8217;s science goals will be made possible by the robust, scalable systems <span class=\"nag-n-override\" style=\"margin-left: 0 !important;\"><i>n<\/i><\/span>AG engineers are building.<\/p>\n<p>Image Copyright: SKAO Image Author: SKAO<\/p>\n                                                    <\/div>\n\n                    <\/div>\n                    <div class=\"img-side small-image-holder col-12 col-lg-6 ph-0 df\" style=\"align-items: center; background-color: #082d48ff;  color: ; \">\n                        <img loading=\"lazy\" decoding=\"async\" width=\"700\" height=\"700\" src=\"https:\/\/nag.com\/wp-content\/uploads\/2025\/05\/SKA-Mid-close-up-artist-impression-web.jpg\" class=\"bg-media \" alt=\"\" style=\"object-position: % %;\" \/>\n                        <div class=\"wrap \">\n                                                    <\/div>\n\n                    <\/div>\n                <\/div>\n\n\n            <\/div>\n\n        <\/div>\n    <\/div>\n<\/div>\n\n<!-- Spacer -->\n<div class=\"pt-1 pt-lg-1 pt-xl-1\" ><\/div>\n\n<div class=\"container content-area-default \">\n    <div class=\"row justify-content--center\">\n        <div class=\"col-12 col-md-12 col-lg-10 col-xl-8\">\n            <h3>Collaboration and Global Reach<\/h3>\n<p>This effort is deeply collaborative. Sean works not only within the SKAO team but also alongside counterparts at the US National Radio Astronomy Observatory (NRAO) and the South African Radio Astronomy Observatory (SARAO). Weekly working groups ensure technical alignment and smooth software integration across continents.<\/p>\n        <\/div>\n    <\/div>\n<\/div>\n\n<!-- Spacer -->\n<div class=\"pt-3 pt-lg-3 pt-xl-3\" ><\/div>\n\n<div class=\"container content-area-default \">\n    <div class=\"row justify-content--center\">\n        <div class=\"col-12 col-md-12 col-lg-10 col-xl-8\">\n            <h3>Looking Ahead<\/h3>\n<p>As the SKAO prepares for full operations towards the end of the decade, the innovations taking place today are setting the standard for scientific computing tomorrow. <span class=\"nag-n-override\" style=\"margin-left: 0 !important;\"><i>n<\/i><\/span>AG\u2019s work is paving the way for resilient, high-performance data systems that will serve the radio astronomy community for decades.<\/p>\n        <\/div>\n    <\/div>\n<\/div>\n\n<!-- Spacer -->\n<div class=\"pt-2 pt-lg-2 pt-xl-2\" ><\/div>\n\n<div class=\"container content-area-default \">\n    <div class=\"row justify-content--center\">\n        <div class=\"col-12 col-md-12 col-lg-10 col-xl-8\">\n            <blockquote>\n<h4><em>We\u2019ve helped pave the way for scalable, high-performance <\/em><em>systems that will power radio telescopes for decades to come.<\/em><br \/>Sean Stansill, HPC Software Engineer, <em>n<\/em>AG<\/h4>\n<\/blockquote>\n        <\/div>\n    <\/div>\n<\/div>\n\n<!-- Spacer -->\n<div class=\"pt-3 pt-lg-3 pt-xl-3\" ><\/div>\n\n<div class=\"container content-area-default \">\n    <div class=\"row justify-content--center\">\n        <div class=\"col-12 col-md-12 col-lg-10 col-xl-8\">\n            <h3>Key Takeaways<\/h3>\n        <\/div>\n    <\/div>\n<\/div>\n\n<div class=\"container content-area-default \">\n    <div class=\"row justify-content--center\">\n        <div class=\"col-12 col-md-12 col-lg-10 col-xl-8\">\n            <ul>\n<li><strong>8 TB\/s I\/O<\/strong> is needed \u2013 the SKAO\u2019s HPC systems must continuously sustain these rates.<\/li>\n<li><strong>Global standards<\/strong>: MSv4 is becoming the benchmark format for radio astronomy worldwide.<\/li>\n<li><strong>Innovative architecture<\/strong>: Adoption of object storage marks a shift in HPC design for data-intensive workloads.<\/li>\n<li><strong>Scientific impact<\/strong>: From studying the cosmic down to understanding galaxy evolution, the SKAO&#8217;s discoveries depend on the Science Data Processor software that <span class=\"nag-n-override\" style=\"margin-left: 0 !important;\"><i>n<\/i><\/span>AG\u2019s experts are helping to develop.<\/li>\n<li><strong>Cost-effective performance<\/strong>: Hardware tuning yielded up to <strong>4\u00d7 efficiency gains<\/strong> with minimal investment.<\/li>\n<\/ul>\n        <\/div>\n    <\/div>\n<\/div>\n\n\n<div class=\"gbc-title-banner tac tac-lg tac-xl\" style='border-radius: 0px; '>\n    <div class=\"container\" style='border-radius: 0px; '>\n        <div class=\"row justify-content--center\" >\n            <div class=\"col-12\"  >\n                <div class=\"wrap pv-1 \" style=\"0pxbackground-color: \">\n                                <div class=\"col-12 col-md-12 col-lg-10 col-xl-8  banner-content\"  >\n    \n                    \n                    <div class=\"mt-1 mb-1 content\"><\/div>\n\n                    \n                    <a href='https:\/\/nag.com\/hpc-services\/' style='background-color: #ff7d21ff; border-radius: 30px; font-weight: 600; ' class='btn mr-1  ' ><span class=\"nag-n-override\" style=\"margin-left: 0 !important;\"><i>n<\/i><\/span>AG HPC Services <i class='fas fa-angle-right'><\/i><\/a><a href='https:\/\/nag.com\/case-studies\/' style='border: 2px solid #082d48ff; border-radius: 30px; font-weight: 600; ' class='btn mr-1 outline ' >More Case Studies <i class='fas fa-angle-right'><\/i><\/a><a href='https:\/\/nag.com\/contact-us\/' style='font-weight: 600; padding: 0px!important; ' class='btn mr-1  ' >Talk to Us <i class='fas fa-angle-right'><\/i><\/a>                <\/div>\n                <\/div>\n            <\/div>\n        <\/div>\n    <\/div>\n<\/div>\n","protected":false},"excerpt":{"rendered":"<p>Discover how HPC powers the SKA telescopes. <span class=\"nag-n-override\" style=\"margin-left: 0 !important;\"><i>n<\/i><\/span>AG engineer Sean Stansill shares insights on data processing, MSv4, and scaling science with software.<\/p>\n","protected":false},"author":8,"featured_media":62347,"parent":0,"menu_order":0,"template":"","meta":{"content-type":"","footnotes":""},"post-tag":[59,106,43],"class_list":["post-63083","case-studies","type-case-studies","status-publish","has-post-thumbnail","hentry"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v25.8 - 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