{"id":170,"date":"2025-12-14T08:18:15","date_gmt":"2025-12-14T07:18:15","guid":{"rendered":"https:\/\/www.harmoni-elt.eu\/harmoni\/?page_id=170"},"modified":"2025-12-14T08:35:35","modified_gmt":"2025-12-14T07:35:35","slug":"scao","status":"publish","type":"page","link":"https:\/\/www.harmoni-elt.eu\/harmoni\/harmoni\/instrument\/scao\/","title":{"rendered":"scao"},"content":{"rendered":"\n<div class=\"wp-block-group alignfull is-layout-flow wp-container-core-group-is-layout-f9cb6abc wp-block-group-is-layout-flow\" style=\"margin-top:0;margin-bottom:0\">\n<div class=\"wp-block-columns alignfull is-not-stacked-on-mobile is-layout-flex wp-container-core-columns-is-layout-3018e991 wp-block-columns-is-layout-flex\" style=\"margin-top:0;margin-bottom:0;padding-top:0;padding-right:var(--wp--preset--spacing--20);padding-bottom:0;padding-left:var(--wp--preset--spacing--30)\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\" style=\"flex-basis:100%\">\n<div class=\"wp-block-group is-vertical is-content-justification-stretch is-layout-flex wp-container-core-group-is-layout-7e003bba wp-block-group-is-layout-flex\">\n<div class=\"wp-block-group has-global-padding is-layout-constrained wp-container-core-group-is-layout-0b40682b wp-block-group-is-layout-constrained\">\n<h2 class=\"wp-block-heading has-xx-large-font-size\">Single Conjugate AO<\/h2>\n\n\n\n<p class=\"has-x-large-font-size\">The Single Conjugate Adaptive Optics (SCAO) mode of HARMONI is designed to deliver diffraction-limited performance by correcting atmospheric turbulence using a single bright natural guide star located on-axis or within a small patrol field around the science target. The correction is optimised for the direction of that guide star and therefore provides the highest possible image quality over a limited field of view.<\/p>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns alignfull is-style-section-2 is-layout-flex wp-container-core-columns-is-layout-d9884270 wp-block-columns-is-layout-flex is-style-section-2--1\" style=\"padding-top:0;padding-bottom:0\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\" style=\"flex-basis:50%\">\n<div class=\"wp-block-group is-vertical is-content-justification-stretch is-layout-flex wp-container-core-group-is-layout-098fff0a wp-block-group-is-layout-flex\" style=\"min-height:33vh;padding-top:var(--wp--preset--spacing--50);padding-right:var(--wp--preset--spacing--50);padding-bottom:var(--wp--preset--spacing--50);padding-left:var(--wp--preset--spacing--50)\">\n<p>In SCAO mode, visible light from the guide star is separated from the science beam by a dichroic and sent to a dedicated adaptive optics wavefront sensor. HARMONI uses a pyramid wavefront sensor, which offers high sensitivity to small wavefront aberrations when operated with appropriate modulation. The wavefront sensor measures distortions introduced by atmospheric turbulence and telescope aberrations at high temporal frequency. These measurements are processed in real time by the adaptive optics control system, which computes the corrective commands applied to the ELT deformable mirror. The correction is applied continuously, closing the adaptive optics loop and stabilising the wavefront delivered to the science instrument.<\/p>\n\n\n\n<p>In addition to the main high-order correction loop, SCAO includes a low-order loop that compensates for slowly varying aberrations such as non-common path errors between the wavefront sensing and science channels. This ensures that the wavefront quality measured by the sensor is accurately transferred to the science focal plane, maintaining long-term stability of the point spread function.<\/p>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\" style=\"flex-basis:50%\">\n<div class=\"wp-block-cover is-light\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"614\" class=\"wp-block-cover__image-background wp-image-182 size-large\" alt=\"\" src=\"https:\/\/www.harmoni-elt.eu\/wp-content\/uploads\/2025\/12\/SCAO-1024x614.png\" style=\"object-position:21% 24%\" data-object-fit=\"cover\" data-object-position=\"21% 24%\" srcset=\"https:\/\/www.harmoni-elt.eu\/wp-content\/uploads\/2025\/12\/SCAO-1024x614.png 1024w, https:\/\/www.harmoni-elt.eu\/wp-content\/uploads\/2025\/12\/SCAO-300x180.png 300w, https:\/\/www.harmoni-elt.eu\/wp-content\/uploads\/2025\/12\/SCAO-768x460.png 768w, https:\/\/www.harmoni-elt.eu\/wp-content\/uploads\/2025\/12\/SCAO-1536x920.png 1536w, https:\/\/www.harmoni-elt.eu\/wp-content\/uploads\/2025\/12\/SCAO.png 1552w\" sizes=\"auto, (max-width: 1024px) 100vw, 1024px\" \/><span aria-hidden=\"true\" class=\"wp-block-cover__background has-background-dim-0 has-background-dim\" style=\"background-color:#dddfdf\"><\/span><div class=\"wp-block-cover__inner-container is-layout-flow wp-block-cover-is-layout-flow\">\n<div style=\"height:var(--wp--preset--spacing--20)\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n<\/div><\/div>\n\n\n\n<p>The expected performance of SCAO is driven by a top-level requirement of achieving high Strehl ratio in the near-infrared. Under median atmospheric conditions and with a sufficiently bright guide star, simulations show that the system can achieve Strehl ratios of around 70% in K band, and in many cases close to or exceeding 80%. Performance degrades gracefully with worsening seeing or fainter guide stars, but remains compliant with requirements up to approximately magnitude 12 under typical conditions. The delivered image quality is dominated by a diffraction-limited core with a stable halo, enabling high spatial resolution spectroscopy at the smallest HARMONI spaxel scales.<\/p>\n<\/div>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-buttons is-layout-flex wp-block-buttons-is-layout-flex\">\n<div class=\"wp-block-button has-custom-width wp-block-button__width-100 is-style-outline is-style-outline--2\"><a class=\"wp-block-button__link has-contrast-color has-accent-5-background-color has-text-color has-background has-link-color wp-element-button\" href=\"https:\/\/www.harmoni-elt.eu\/harmoni\/harmoni\/instrument\/\" style=\"font-style:normal;font-weight:600\">Back to Overall Instrument<\/a><\/div>\n<\/div>\n","protected":false},"excerpt":{"rendered":"<p>Single Conjugate AO The Single Conjugate Adaptive Optics (SCAO) mode of HARMONI is designed to deliver diffraction-limited performance by correcting atmospheric turbulence using a single bright natural guide star located on-axis or within a small patrol field around the science target. The correction is optimised for the direction of that guide star and therefore provides [&hellip;]<\/p>\n","protected":false},"author":3,"featured_media":0,"parent":129,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-170","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.harmoni-elt.eu\/harmoni\/wp-json\/wp\/v2\/pages\/170","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.harmoni-elt.eu\/harmoni\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.harmoni-elt.eu\/harmoni\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.harmoni-elt.eu\/harmoni\/wp-json\/wp\/v2\/users\/3"}],"replies":[{"embeddable":true,"href":"https:\/\/www.harmoni-elt.eu\/harmoni\/wp-json\/wp\/v2\/comments?post=170"}],"version-history":[{"count":5,"href":"https:\/\/www.harmoni-elt.eu\/harmoni\/wp-json\/wp\/v2\/pages\/170\/revisions"}],"predecessor-version":[{"id":198,"href":"https:\/\/www.harmoni-elt.eu\/harmoni\/wp-json\/wp\/v2\/pages\/170\/revisions\/198"}],"up":[{"embeddable":true,"href":"https:\/\/www.harmoni-elt.eu\/harmoni\/wp-json\/wp\/v2\/pages\/129"}],"wp:attachment":[{"href":"https:\/\/www.harmoni-elt.eu\/harmoni\/wp-json\/wp\/v2\/media?parent=170"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}