{"id":1131,"date":"2025-04-22T13:25:56","date_gmt":"2025-04-22T10:25:56","guid":{"rendered":"http:\/\/195.96.236.171\/news\/?p=1131"},"modified":"2025-04-22T13:25:56","modified_gmt":"2025-04-22T10:25:56","slug":"%d1%81%d0%b5%d0%bc%d0%b8%d0%bd%d0%b0%d1%80-%d0%bd%d0%b0-%d0%b8%d0%bd%d1%81%d1%82%d0%b8%d1%82%d1%83%d1%82%d0%b0-%d0%bf%d0%be-%d0%b0%d1%81%d1%82%d1%80%d0%be%d0%bd%d0%be%d0%bc%d0%b8%d1%8f","status":"publish","type":"post","link":"http:\/\/195.96.236.171\/news\/?p=1131","title":{"rendered":"\u0421\u0435\u043c\u0438\u043d\u0430\u0440 \u043d\u0430 \u0418\u043d\u0441\u0442\u0438\u0442\u0443\u0442\u0430 \u043f\u043e \u0410\u0441\u0442\u0440\u043e\u043d\u043e\u043c\u0438\u044f"},"content":{"rendered":"

\u0421\u0431\u0438\u0440\u043a\u0430 \u043d\u0430 \u0421\u0435\u043c\u0438\u043d\u0430\u0440\u0430 \u043d\u0430 \u0418\u043d\u0441\u0442\u0438\u0442\u0443\u0442\u0430 \u043f\u043e \u0410\u0441\u0442\u0440\u043e\u043d\u043e\u043c\u0438\u044f \u0449\u0435 \u0441\u0435 \u043f\u0440\u043e\u0432\u0435\u0434\u0435 \u043d\u0430 23 \u0410\u043f\u0440\u0438\u043b,<\/strong>
\n2025 \u0433. (\u0441\u0440\u044f\u0434\u0430), \u043e\u0442 14:00 \u0447\u0430\u0441\u0430 \u0432 \u0437\u0430\u043b\u0430 301<\/strong> \u043d\u0430 \u0441\u0433\u0440\u0430\u0434\u0430\u0442\u0430 \u043d\u0430 \u0431\u0443\u043b.
\n\u0426\u0430\u0440\u0438\u0433\u0440\u0430\u0434\u0441\u043a\u043e \u0448\u043e\u0441\u0435 \u211672.<\/p>\n

\u041c\u043e\u043c\u0447\u0438\u043b \u041c\u043e\u043b\u043d\u0430\u0440<\/strong> (Southwest Research Institute, Texas, USA), \u0449\u0435 \u043f\u0440\u0435\u0434\u0441\u0442\u0430\u0432\u0438 \u0440\u0430\u0431\u043e\u0442\u0430 \u043d\u0430 \u0442\u0435\u043c\u0430: \u201cSpectropolarimetry across the solar atmosphere – On polarization of <\/strong><\/em>light as a solar magnetometer “<\/strong><\/em><\/p>\n

\u0410\u043d\u043e\u0442\u0430\u0446\u0438\u044f: Spectropolarimetric observations of the solar atmosphere form
\nthe foundation for the regular solar magnetic field data products used
\nin both research and space weather operations. However, the pursuit to
\nmeasure the solar magnetic field is far from complete, despite the Sun`s
\nproximity and perceived brightness. Our inferences of the magnetic field
\nof the Sun are marred with instrumental, numerical, and theoretical
\nissues, relatable to the challenges of inferring magnetic fields across
\nthe Universe from remote sensing data. In this talk I will provide a
\nbrief overview of the field and highlight some of my own work that
\naddresses these outstanding challenges. In particular, I will discuss
\ntwo ongoing projects: i) using the unsaturated Hanle effect in the He I
\n1083 line to estimate the magnetic field orientation in prominence
\nmaterial in ICMEs; 2) Using Physics Informed Neural Networks for
\nimproving spectropolarimetric inversions and building the next
\ngeneration spectropolarimetric inversion codes. Both projects aim to
\nadvance our understanding and measurement of the solar magnetic field by
\nutilizing novel approaches and physical regimes of solar observations.<\/p>\n","protected":false},"excerpt":{"rendered":"

\u0421\u0431\u0438\u0440\u043a\u0430 \u043d\u0430 \u0421\u0435\u043c\u0438\u043d\u0430\u0440\u0430 \u043d\u0430 \u0418\u043d\u0441\u0442\u0438\u0442\u0443\u0442\u0430 \u043f\u043e \u0410\u0441\u0442\u0440\u043e\u043d\u043e\u043c\u0438\u044f \u0449\u0435 \u0441\u0435 \u043f\u0440\u043e\u0432\u0435\u0434\u0435 \u043d\u0430 23 \u0410\u043f\u0440\u0438\u043b, 2025 \u0433. (\u0441\u0440\u044f\u0434\u0430), \u043e\u0442 14:00 \u0447\u0430\u0441\u0430 \u0432 \u0437\u0430\u043b\u0430 301 \u043d\u0430 \u0441\u0433\u0440\u0430\u0434\u0430\u0442\u0430 \u043d\u0430 \u0431\u0443\u043b. \u0426\u0430\u0440\u0438\u0433\u0440\u0430\u0434\u0441\u043a\u043e \u0448\u043e\u0441\u0435 \u211672. \u041c\u043e\u043c\u0447\u0438\u043b \u041c\u043e\u043b\u043d\u0430\u0440 (Southwest Research Institute, Texas, USA), \u0449\u0435 \u043f\u0440\u0435\u0434\u0441\u0442\u0430\u0432\u0438 \u0440\u0430\u0431\u043e\u0442\u0430 \u043d\u0430 \u0442\u0435\u043c\u0430: \u201cSpectropolarimetry across the solar atmosphere – On polarization of light as a solar magnetometer […]<\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[2,10],"tags":[],"class_list":["post-1131","post","type-post","status-publish","format-standard","hentry","category-news","category-10","category-2-id","category-10-id","post-seq-1","post-parity-odd","meta-position-corners","fix"],"_links":{"self":[{"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=\/wp\/v2\/posts\/1131","targetHints":{"allow":["GET"]}}],"collection":[{"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=1131"}],"version-history":[{"count":1,"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=\/wp\/v2\/posts\/1131\/revisions"}],"predecessor-version":[{"id":1132,"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=\/wp\/v2\/posts\/1131\/revisions\/1132"}],"wp:attachment":[{"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1131"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1131"},{"taxonomy":"post_tag","embeddable":true,"href":"http:\/\/195.96.236.171\/news\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1131"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}