{"id":91848,"date":"2024-02-27T16:45:51","date_gmt":"2024-02-27T15:45:51","guid":{"rendered":"https:\/\/fusion.bsc.es\/?p=91848"},"modified":"2024-02-27T16:48:16","modified_gmt":"2024-02-27T15:48:16","slug":"our-new-journal-paper-in-nuclear-fusion-on-modeling-of-frequency-sweeping-alfven-modes","status":"publish","type":"post","link":"https:\/\/fusion.bsc.es\/index.php\/2024\/02\/27\/our-new-journal-paper-in-nuclear-fusion-on-modeling-of-frequency-sweeping-alfven-modes\/","title":{"rendered":"Our new journal paper in Nuclear Fusion on modeling of frequency-sweeping Alfv\u00e9n modes"},"content":{"rendered":"<p><img loading=\"lazy\" decoding=\"async\" class=\"aligncenter wp-image-91858\" src=\"http:\/\/fusion.bsc.es\/wp-content\/uploads\/journalheader-2-400x154.jpg\" alt=\"\" width=\"700\" height=\"269\" srcset=\"https:\/\/fusion.bsc.es\/wp-content\/uploads\/journalheader-2-400x154.jpg 400w, https:\/\/fusion.bsc.es\/wp-content\/uploads\/journalheader-2.jpg 836w\" sizes=\"auto, (max-width: 700px) 100vw, 700px\" \/><\/p>\n<p style=\"text-align: justify;\"><strong>Alfv\u00e9nic instabilities driven by energetic particles pose a challenge to the efficient operation of magnetic confinement fusion devices.<\/strong> These modes can dispel fast ions leading to the introduction of significant heat loads onto plasma facing components and degradation of overall plasma confinement. One class of Alfv\u00e9nic instabilities known as reversed shear Alfv\u00e9n eigenmodes (RSAEs) are of particular risk in devices with reversed shear rotational transform profiles. Reversed shear configurations have recently been of interest because of their enhancement to confinement quality. With this in mind, further study of RSAEs is necessary.<\/p>\n<p><!--more--><\/p>\n<p style=\"text-align: justify;\"><a href=\"http:\/\/10.1088\/0029-5515\/54\/12\/123002\">RSAEs, also called Alfv\u00e9n cascades, were observed<\/a> in the <a href=\"http:\/\/fusionwiki.ciemat.es\/wiki\/TJ-II\">TJ-II flexible heliac<\/a> in hydrogen plasma discharges with varying magnetic configurations. <strong>In <a href=\"https:\/\/iopscience.iop.org\/article\/10.1088\/1741-4326\/ad1c93\">our recent journal publication in Nuclear Fusion<\/a>, we simulate the cascade events <\/strong>using the <a href=\"ttps:\/\/doi.org\/10.1063\/1.1590316\">STELLGAP<\/a> and <a href=\"https:\/\/doi.org\/10.1063\/1.3313818\">AE3D<\/a> codes <strong>and study the relationship between the frequency of the modes that form the cascade and the minimum value of the rotational transform profile<\/strong>. The simulations predict the appearance of a cascade sweeping downward in frequency formed by a set of modes with m (poloidal mode number) = 6, and n (toroidal mode number) = &#8211; 9 when the minimum value of the iota profile is varied between approximately 1.47 &lt; i<sub>min<\/sub> &lt; 1.50, which is corroborated by experiment. <strong>The results presented support the utility of MHD spectroscopy<\/strong>, a diagnostic tool whereby the temporal gradient of the frequency of an Alfven cascade can be used to determine the variation in time of the plasma\u2019s rotational transform profile<\/p>\n<figure id=\"attachment_91860\" aria-describedby=\"caption-attachment-91860\" style=\"width: 640px\" class=\"wp-caption aligncenter\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-91860\" src=\"http:\/\/fusion.bsc.es\/wp-content\/uploads\/nfad1c93f11_hr-400x222.jpg\" alt=\"\" width=\"650\" height=\"360\" srcset=\"https:\/\/fusion.bsc.es\/wp-content\/uploads\/nfad1c93f11_hr-400x222.jpg 400w, https:\/\/fusion.bsc.es\/wp-content\/uploads\/nfad1c93f11_hr.jpg 1025w\" sizes=\"auto, (max-width: 650px) 100vw, 650px\" \/><figcaption id=\"caption-attachment-91860\" class=\"wp-caption-text\">Simulation results shown in black overlaid with experimental spectrogram. Error bars assume \u00b110% error in density and \u00b10.005 error in iota. Reproduced from Fig 11 in A.G. Ghiozzi et al 2024 Nucl. Fusion 64 036005.<\/figcaption><\/figure>\n<p style=\"text-align: justify;\">The full journal paper written by our ex-group member <strong>Adriana Ghiozzi <\/strong>together with our group leader Mervi Mantsinen, ex-group member Pol Pastells and collaborators can be found at the following link: <a href=\"https:\/\/iopscience.iop.org\/article\/10.1088\/1741-4326\/ad1c93\">A.G. Ghiozzi <em>et al<\/em> 2024 <em>Nucl. Fusion<\/em> <strong>64<\/strong> 036005<\/a>.<\/p>\n<p style=\"text-align: justify;\"><em><span class=\"footer-text\">The FusionCAT project with file number 001-P-001722 has been 50% co-financed with \u20ac1.960.963,66 by the European Union Regional Development Fund within the framework of the ERDF Operational Program of Catalonia 2014-2020 with support of Generalitat of Catalonia.<\/span><br \/>\n<\/em><\/p>\n<p><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-6377 aligncenter\" src=\"http:\/\/fusion.bsc.es\/wp-content\/uploads\/fusioncat_sign.png\" alt=\"\" width=\"750\" height=\"70\" srcset=\"https:\/\/fusion.bsc.es\/wp-content\/uploads\/fusioncat_sign.png 1296w, https:\/\/fusion.bsc.es\/wp-content\/uploads\/fusioncat_sign-400x37.png 400w, https:\/\/fusion.bsc.es\/wp-content\/uploads\/fusioncat_sign-1024x96.png 1024w\" sizes=\"auto, (max-width: 750px) 100vw, 750px\" \/><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Alfv\u00e9nic instabilities driven by energetic particles pose a challenge to the efficient operation of magnetic confinement fusion devices. These modes can dispel fast ions leading to the introduction of significant heat loads onto plasma facing components and degradation of overall plasma confinement. One class of Alfv\u00e9nic instabilities known as reversed shear Alfv\u00e9n eigenmodes (RSAEs) are &#8230; <a title=\"Our new journal paper in Nuclear Fusion on modeling of frequency-sweeping Alfv\u00e9n modes\" class=\"read-more\" href=\"https:\/\/fusion.bsc.es\/index.php\/2024\/02\/27\/our-new-journal-paper-in-nuclear-fusion-on-modeling-of-frequency-sweeping-alfven-modes\/\" aria-label=\"Read more about Our new journal paper in Nuclear Fusion on modeling of frequency-sweeping Alfv\u00e9n modes\">Read more<\/a><\/p>\n","protected":false},"author":3,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[9,29],"tags":[76,78,77],"class_list":["post-91848","post","type-post","status-publish","format-standard","hentry","category-group","category-publicaton","tag-alfvenic-waves","tag-fusioncat-modelling","tag-stellarator"],"_links":{"self":[{"href":"https:\/\/fusion.bsc.es\/index.php\/wp-json\/wp\/v2\/posts\/91848","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/fusion.bsc.es\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/fusion.bsc.es\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/fusion.bsc.es\/index.php\/wp-json\/wp\/v2\/users\/3"}],"replies":[{"embeddable":true,"href":"https:\/\/fusion.bsc.es\/index.php\/wp-json\/wp\/v2\/comments?post=91848"}],"version-history":[{"count":14,"href":"https:\/\/fusion.bsc.es\/index.php\/wp-json\/wp\/v2\/posts\/91848\/revisions"}],"predecessor-version":[{"id":91867,"href":"https:\/\/fusion.bsc.es\/index.php\/wp-json\/wp\/v2\/posts\/91848\/revisions\/91867"}],"wp:attachment":[{"href":"https:\/\/fusion.bsc.es\/index.php\/wp-json\/wp\/v2\/media?parent=91848"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/fusion.bsc.es\/index.php\/wp-json\/wp\/v2\/categories?post=91848"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/fusion.bsc.es\/index.php\/wp-json\/wp\/v2\/tags?post=91848"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}