{"id":236,"date":"2023-10-27T15:26:37","date_gmt":"2023-10-27T15:26:37","guid":{"rendered":"https:\/\/dev-cu-sites.pantheonsite.io\/chorus-mhd\/?page_id=236"},"modified":"2026-02-07T18:21:24","modified_gmt":"2026-02-07T18:21:24","slug":"research-outcomes","status":"publish","type":"page","link":"https:\/\/sites.clarkson.edu\/chorus-mhd\/research-outcomes\/","title":{"rendered":"Research Outcomes"},"content":{"rendered":"\n<blockquote class=\"wp-block-quote is-layout-flow wp-block-quote-is-layout-flow\">\n<p>CHORUS is a novel and powerful Compressible High-ORder Unstructured Spectral-difference (CHORUS) code for simulating thermal convection and related fluid dynamics in the interiors of stars and planets.<\/p>\n<cite><a href=\"http:\/\/dx.doi.org\/10.1016\/j.jcp.2015.02.047\">http:\/\/dx.doi.org\/10.1016\/j.jcp.2015.02.047<\/a><\/cite><\/blockquote>\n\n\n\n<blockquote class=\"wp-block-quote is-layout-flow wp-block-quote-is-layout-flow\">\n<p>CHORUS+ employs higher degree reference elements (p5\/p6) and transfinite mapping. CHORUS+ is approximately 10 times faster than CHORUS! <\/p>\n<cite><a rel=\"noreferrer noopener\" href=\"https:\/\/doi.org\/10.1063\/5.0158146\" target=\"_blank\">https:\/\/doi.org\/10.1063\/5.0158146<\/a><\/cite><\/blockquote>\n\n\n\n<p><\/p>\n\n\n\n<blockquote class=\"wp-block-quote is-layout-flow wp-block-quote-is-layout-flow\">\n<p>CHORUS-MHD is an extension of CHORUS++ to magnetohydrodynamics and GPU-accelerated.<\/p>\n<cite><a href=\"https:\/\/arc.aiaa.org\/doi\/10.2514\/6.2025-97583\">https:\/\/arc.aiaa.org\/doi\/10.2514\/6.2025-97583<\/a><\/cite><\/blockquote>\n\n\n\n<p><\/p>\n","protected":false},"excerpt":{"rendered":"<p>CHORUS is a novel and powerful Compressible High-ORder Unstructured Spectral-difference (CHORUS) code for simulating thermal convection and related fluid dynamics in the interiors of stars and planets. http:\/\/dx.doi.org\/10.1016\/j.jcp.2015.02.047 CHORUS+ employs higher degree reference elements (p5\/p6) and transfinite mapping. CHORUS+ is approximately 10 times faster than CHORUS! https:\/\/doi.org\/10.1063\/5.0158146 CHORUS-MHD is an extension of CHORUS++ to magnetohydrodynamics [&hellip;]<\/p>\n","protected":false},"author":174,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"advgb_blocks_editor_width":"","advgb_blocks_columns_visual_guide":"","footnotes":""},"class_list":["post-236","page","type-page","status-publish","hentry"],"coauthors":[],"author_meta":{"author_link":"https:\/\/sites.clarkson.edu\/chorus-mhd\/author\/cliang\/","display_name":"cliang"},"relative_dates":{"created":"Posted 2 years ago","modified":"Updated 2 months ago"},"absolute_dates":{"created":"Posted on October 27, 2023","modified":"Updated on February 7, 2026"},"absolute_dates_time":{"created":"Posted on October 27, 2023 3:26 pm","modified":"Updated on February 7, 2026 6:21 pm"},"featured_img_caption":"","featured_img":false,"series_order":"","_links":{"self":[{"href":"https:\/\/sites.clarkson.edu\/chorus-mhd\/wp-json\/wp\/v2\/pages\/236","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/sites.clarkson.edu\/chorus-mhd\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/sites.clarkson.edu\/chorus-mhd\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/sites.clarkson.edu\/chorus-mhd\/wp-json\/wp\/v2\/users\/174"}],"replies":[{"embeddable":true,"href":"https:\/\/sites.clarkson.edu\/chorus-mhd\/wp-json\/wp\/v2\/comments?post=236"}],"version-history":[{"count":2,"href":"https:\/\/sites.clarkson.edu\/chorus-mhd\/wp-json\/wp\/v2\/pages\/236\/revisions"}],"predecessor-version":[{"id":439,"href":"https:\/\/sites.clarkson.edu\/chorus-mhd\/wp-json\/wp\/v2\/pages\/236\/revisions\/439"}],"wp:attachment":[{"href":"https:\/\/sites.clarkson.edu\/chorus-mhd\/wp-json\/wp\/v2\/media?parent=236"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}