{"id":2055,"date":"2024-10-18T15:16:50","date_gmt":"2024-10-18T13:16:50","guid":{"rendered":"https:\/\/wordpress-test.app.u-pariscite.fr\/diip\/?p=2055"},"modified":"2024-10-21T16:50:11","modified_gmt":"2024-10-21T14:50:11","slug":"learning-the-magneto-ionic-side-of-the-turbulence-in-the-interstellar-medium-in-radio-astronomy","status":"publish","type":"post","link":"https:\/\/wordpress-test.app.u-pariscite.fr\/diip\/learning-the-magneto-ionic-side-of-the-turbulence-in-the-interstellar-medium-in-radio-astronomy\/","title":{"rendered":"Learning the magneto-ionic side of the turbulence in the interstellar medium in radio-astronomy"},"content":{"rendered":"<p>[et_pb_section fb_built=&#8221;1&#8243; _builder_version=&#8221;3.22&#8243;][et_pb_row _builder_version=&#8221;3.22&#8243; background_size=&#8221;initial&#8221; background_position=&#8221;top_left&#8221; background_repeat=&#8221;repeat&#8221;][et_pb_column type=&#8221;1_4&#8243; _builder_version=&#8221;3.0.47&#8243;][et_pb_text _builder_version=&#8221;3.22.1&#8243; background_color=&#8221;#072c72&#8243; border_color_all=&#8221;#3255c9&#8243; text_orientation=&#8221;right&#8221; background_layout=&#8221;dark&#8221; custom_padding=&#8221;20px|15px|15px|&#8221; z_index_tablet=&#8221;500&#8243;]<\/p>\n<p><em>2022<\/em><\/p>\n<p><em>PhD\/DIAI Projects<\/em><\/p>\n<p><span data-sheets-root=\"1\">@Astrophysique<\/span><\/p>\n<p>[\/et_pb_text][et_pb_text _builder_version=&#8221;3.22.1&#8243; text_orientation=&#8221;right&#8221; z_index_tablet=&#8221;500&#8243;]<\/p>\n<p><strong>Jack Berat<br \/><\/strong>(LPENS, UPC)<\/p>\n<p>[\/et_pb_text][\/et_pb_column][et_pb_column type=&#8221;3_4&#8243; _builder_version=&#8221;3.0.47&#8243;][et_pb_text _builder_version=&#8221;3.22.1&#8243; z_index_tablet=&#8221;500&#8243;]<\/p>\n<h3><strong>Project Summary<\/strong><\/h3>\n<p>The phase transition from warm neutral medium to cold neutral medium in the interstellar medium (ISM) is affected by the magnetic field. The polarization of the synchrotron emission is one of the tracer of the magnetic field in the ISM. We investigate how correlated the phases are with the polarized emission, the use of machine vision algorithm and machine learning are a useful tool to compare numerical simulations and observations of these processes.<\/p>\n<p>[\/et_pb_text][\/et_pb_column][\/et_pb_row][et_pb_row custom_margin=&#8221;120px||&#8221; _builder_version=&#8221;3.22.1&#8243; locked=&#8221;off&#8221;][et_pb_column type=&#8221;4_4&#8243; _builder_version=&#8221;3.22.1&#8243;][et_pb_divider _builder_version=&#8221;3.22.1&#8243;][\/et_pb_divider][et_pb_text admin_label=&#8221;\u00c0 lire aussi&#8221; _builder_version=&#8221;3.22.1&#8243; z_index_tablet=&#8221;500&#8243; locked=&#8221;off&#8221;]<\/p>\n<h2><span class=\"st\">Other projects<br \/><\/span><\/h2>\n<p>[\/et_pb_text][et_pb_blog posts_number=&#8221;4&#8243; include_categories=&#8221;63&#8243; show_author=&#8221;off&#8221; show_date=&#8221;off&#8221; show_pagination=&#8221;off&#8221; module_id=&#8221;page_type_blog&#8221; _builder_version=&#8221;3.22.1&#8243; header_level=&#8221;h4&#8243; border_width_bottom_fullwidth=&#8221;1px&#8221; border_color_bottom_fullwidth=&#8221;rgba(51,51,51,0.18)&#8221; custom_padding=&#8221;||50px|&#8221; z_index_tablet=&#8221;500&#8243; locked=&#8221;off&#8221;][\/et_pb_blog][\/et_pb_column][\/et_pb_row][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"<p>2022 PhD\/DIAI Projects @AstrophysiqueJack Berat(LPENS, UPC)Project Summary The phase transition from warm neutral medium to cold neutral medium in the interstellar medium (ISM) is affected by the magnetic field. The polarization of the synchrotron emission is one of the tracer of the magnetic field in the ISM. We investigate how correlated the phases are with&hellip; <a class=\"continue\" href=\"https:\/\/wordpress-test.app.u-pariscite.fr\/diip\/learning-the-magneto-ionic-side-of-the-turbulence-in-the-interstellar-medium-in-radio-astronomy\/\">Lire la suite<span> Learning the magneto-ionic side of the turbulence in the interstellar medium in radio-astronomy<\/span><\/a><\/p>\n","protected":false},"author":560,"featured_media":2263,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_et_pb_use_builder":"on","_et_pb_old_content":"","_et_gb_content_width":"","footnotes":""},"categories":[55,63,1,37],"tags":[],"class_list":["post-2055","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-55","category-diai","category-diip","category-physics-astronomy"],"_links":{"self":[{"href":"https:\/\/wordpress-test.app.u-pariscite.fr\/diip\/wp-json\/wp\/v2\/posts\/2055","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/wordpress-test.app.u-pariscite.fr\/diip\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/wordpress-test.app.u-pariscite.fr\/diip\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/wordpress-test.app.u-pariscite.fr\/diip\/wp-json\/wp\/v2\/users\/560"}],"replies":[{"embeddable":true,"href":"https:\/\/wordpress-test.app.u-pariscite.fr\/diip\/wp-json\/wp\/v2\/comments?post=2055"}],"version-history":[{"count":6,"href":"https:\/\/wordpress-test.app.u-pariscite.fr\/diip\/wp-json\/wp\/v2\/posts\/2055\/revisions"}],"predecessor-version":[{"id":2281,"href":"https:\/\/wordpress-test.app.u-pariscite.fr\/diip\/wp-json\/wp\/v2\/posts\/2055\/revisions\/2281"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/wordpress-test.app.u-pariscite.fr\/diip\/wp-json\/wp\/v2\/media\/2263"}],"wp:attachment":[{"href":"https:\/\/wordpress-test.app.u-pariscite.fr\/diip\/wp-json\/wp\/v2\/media?parent=2055"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/wordpress-test.app.u-pariscite.fr\/diip\/wp-json\/wp\/v2\/categories?post=2055"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/wordpress-test.app.u-pariscite.fr\/diip\/wp-json\/wp\/v2\/tags?post=2055"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}