{"id":7971,"date":"2022-05-03T09:39:00","date_gmt":"2022-05-03T09:39:00","guid":{"rendered":"https:\/\/www.istp.cnr.it\/?post_type=product&#038;p=7971"},"modified":"2022-06-21T09:46:57","modified_gmt":"2022-06-21T09:46:57","slug":"a-power-balance-model-for-the-l-mode-radiative-density-limit-in-fusion-plasmas","status":"publish","type":"product","link":"https:\/\/www.istp.cnr.it\/it\/research-product\/a-power-balance-model-for-the-l-mode-radiative-density-limit-in-fusion-plasmas\/","title":{"rendered":"A power-balance model for the L-mode radiative density limit in fusion plasmas"},"content":{"rendered":"<p>A 1D cylindrical power-balance model of the radiation density limit (DL) gives a unified description of this phenomenon for stellarators, reversed field pinches and L-mode tokamaks (Zanca et al 2019 Nucl. Fusion 59 126011). The DL scaling laws for the three different configurations are all derived from a combination of just two equations: (a) a single-fluid heat-transport equation; (b) on-axis Ohm&#8217;s law with Spitzer resistivity, taken in a suitable limit for the stellarator. Here, we present a refined version of the model, alongside further experimental evidence supporting its successful application.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Zanca P.; Sattin F.; Escande D.F.; Auriemma F.<\/p>\n","protected":false},"featured_media":1294,"comment_status":"closed","ping_status":"open","template":"","meta":[],"product_cat":[574],"product_tag":[3523,748,894,3459,3521,3522],"class_list":["post-7971","product","type-product","status-publish","has-post-thumbnail","hentry","product_cat-journal-articles","product_tag-limit","product_tag-plasmas","product_tag-fusion","product_tag-l-mode","product_tag-spower-balance-model","product_tag-density","prodpage-style2"],"acf":[],"_links":{"self":[{"href":"https:\/\/www.istp.cnr.it\/it\/wp-json\/wp\/v2\/product\/7971","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.istp.cnr.it\/it\/wp-json\/wp\/v2\/product"}],"about":[{"href":"https:\/\/www.istp.cnr.it\/it\/wp-json\/wp\/v2\/types\/product"}],"replies":[{"embeddable":true,"href":"https:\/\/www.istp.cnr.it\/it\/wp-json\/wp\/v2\/comments?post=7971"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.istp.cnr.it\/it\/wp-json\/wp\/v2\/media\/1294"}],"wp:attachment":[{"href":"https:\/\/www.istp.cnr.it\/it\/wp-json\/wp\/v2\/media?parent=7971"}],"wp:term":[{"taxonomy":"product_cat","embeddable":true,"href":"https:\/\/www.istp.cnr.it\/it\/wp-json\/wp\/v2\/product_cat?post=7971"},{"taxonomy":"product_tag","embeddable":true,"href":"https:\/\/www.istp.cnr.it\/it\/wp-json\/wp\/v2\/product_tag?post=7971"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}