{"id":60,"date":"2021-09-21T11:07:00","date_gmt":"2021-09-21T10:07:00","guid":{"rendered":"https:\/\/www.master-planeto.universite-paris-saclay.fr\/?page_id=60"},"modified":"2025-11-14T09:52:10","modified_gmt":"2025-11-14T08:52:10","slug":"ue-1-physique-du-rayonnement-et-methodes-dobservation-associees","status":"publish","type":"page","link":"https:\/\/www.master-planeto.universite-paris-saclay.fr\/?page_id=60","title":{"rendered":"UE 1 &#8211; Transfert radiatif dans les atmosph\u00e8res et surfaces plan\u00e9taires"},"content":{"rendered":"\n<p class=\"wp-block-paragraph\">Le transfert radiatif d\u00e9crit l\u2019interaction du rayonnement \u00e9lectromagn\u00e9tique et de la mati\u00e8re. Il est \u00e0 la base des m\u00e9thodes de t\u00e9l\u00e9d\u00e9tection, actives et passives. Le cours portera, entre autres, sur le sondage spectroscopique des atmosph\u00e8res plan\u00e9taires et l&rsquo;observation radiom\u00e9trique et radar des surfaces du syst\u00e8me solaire.<\/p>\n\n\n\n<figure class=\"wp-block-image size-large is-resized\"><a href=\"https:\/\/www.master-planeto.universite-paris-saclay.fr\/wp-content\/uploads\/2022\/01\/Capture-de\u0301cran-2022-01-31-a\u0300-10.01.42-2.png\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"720\" src=\"https:\/\/www.master-planeto.universite-paris-saclay.fr\/wp-content\/uploads\/2022\/01\/Capture-de\u0301cran-2022-01-31-a\u0300-10.01.42-2-1024x720.png\" alt=\"\" class=\"wp-image-532\" style=\"width:519px;height:364px\" srcset=\"https:\/\/www.master-planeto.universite-paris-saclay.fr\/wp-content\/uploads\/2022\/01\/Capture-de\u0301cran-2022-01-31-a\u0300-10.01.42-2-1024x720.png 1024w, https:\/\/www.master-planeto.universite-paris-saclay.fr\/wp-content\/uploads\/2022\/01\/Capture-de\u0301cran-2022-01-31-a\u0300-10.01.42-2-300x211.png 300w, https:\/\/www.master-planeto.universite-paris-saclay.fr\/wp-content\/uploads\/2022\/01\/Capture-de\u0301cran-2022-01-31-a\u0300-10.01.42-2-768x540.png 768w, https:\/\/www.master-planeto.universite-paris-saclay.fr\/wp-content\/uploads\/2022\/01\/Capture-de\u0301cran-2022-01-31-a\u0300-10.01.42-2-1536x1080.png 1536w, https:\/\/www.master-planeto.universite-paris-saclay.fr\/wp-content\/uploads\/2022\/01\/Capture-de\u0301cran-2022-01-31-a\u0300-10.01.42-2-2048x1440.png 2048w, https:\/\/www.master-planeto.universite-paris-saclay.fr\/wp-content\/uploads\/2022\/01\/Capture-de\u0301cran-2022-01-31-a\u0300-10.01.42-2-2000x1406.png 2000w\" sizes=\"auto, (max-width: 1024px) 100vw, 1024px\" \/><\/a><\/figure>\n\n\n\n<p class=\"wp-block-paragraph\"><strong>Programme<\/strong><\/p>\n\n\n\n<p class=\"wp-block-paragraph\">1 &#8211; <strong>\u00c9lectromagn\u00e9tisme, interactions rayonnement-mati\u00e8re<\/strong><br>&#8211; Processus physiques : absorption, diffusion, \u00e9mission thermique ;<br><img loading=\"lazy\" decoding=\"async\" width=\"8\" height=\"11\" src=\"http:\/\/planeto.geol.u-psud.fr\/local\/cache-vignettes\/L8xH11\/puce-32883.gif\" alt=\"-\">&nbsp;Bases de spectroscopie et de radiom\u00e9trie.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><strong>2 &#8211; Transfert de rayonnement<\/strong><br>&#8211; Solutions exactes et approch\u00e9es ;<br>&#8211;&nbsp;Au sein des atmosph\u00e8res (gaz, a\u00e9rosols, nuages) ;<br>&#8211;&nbsp;Au sein des milieux compacts (r\u00e9golites, surfaces).<\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><strong>3 &#8211; Applications \u00e0 la t\u00e9l\u00e9d\u00e9tection des atmosph\u00e8res et des surfaces plan\u00e9taires<\/strong><br><img loading=\"lazy\" decoding=\"async\" width=\"8\" height=\"11\" src=\"http:\/\/planeto.geol.u-psud.fr\/local\/cache-vignettes\/L8xH11\/puce-32883.gif\" alt=\"-\">\u00a0Sondages en rayonnement thermique ou r\u00e9fl\u00e9chi, sondages par occultation, radiom\u00e9trie micro-onde, radars imageurs et sondeurs, lidars ;<br><img loading=\"lazy\" decoding=\"async\" width=\"8\" height=\"11\" src=\"http:\/\/planeto.geol.u-psud.fr\/local\/cache-vignettes\/L8xH11\/puce-32883.gif\" alt=\"-\">\u00a0Tour d\u2019horizon des applications dans le syst\u00e8me solaire.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><strong>Intervenants<\/strong><\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><strong>Emmanuel Marcq<\/strong> (responsable), Laboratoire Atmosph\u00e8res, Observations Spatiales (LATMOS), Observatoire de Versailles Saint-Quentin-en-Yvelines, F-78280 Guyancourt. Tel&nbsp;: 01 80 28 52 83 &#8211; E-mail&nbsp;: emmanuel.marcq[@robas]latmos.ipsl.fr<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">Alice Le Gall, Laboratoire Atmosph\u00e8res, Observations Spatiales (LATMOS), Observatoire de Versailles Saint-Quentin-en-Yvelines, F-78280 Guyancourt &#8211; Tel&nbsp;: 01 80 28 52 35 (Guyancourt) &#8211; 01 44 27 52 82 (Jussieu) &#8211; E-mail&nbsp;: alice.legall[@robas]latmos.ipsl.fr<\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><strong>D\u00e9tails pratiques<\/strong><br><img loading=\"lazy\" decoding=\"async\" width=\"8\" height=\"11\" src=\"http:\/\/planeto.geol.u-psud.fr\/local\/cache-vignettes\/L8xH11\/puce-32883.gif\" alt=\"-\">&nbsp;<em>Lieux&nbsp;:<\/em> B\u00e2timent LATMOS-OVSQ (11 Boulevard d\u2019Alembert \u00e0 Guyancourt) ou Jussieu.<br><img loading=\"lazy\" decoding=\"async\" width=\"8\" height=\"11\" src=\"http:\/\/planeto.geol.u-psud.fr\/local\/cache-vignettes\/L8xH11\/puce-32883.gif\" alt=\"-\">&nbsp;<em>Volume horaire&nbsp;:<\/em> 12 h de cours magistraux (6 s\u00e9ances), 9h de travaux dirig\u00e9s (4 s\u00e9ances), 9h de travaux pratiques sur ordinateur (3 s\u00e9ances)<\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Le transfert radiatif d\u00e9crit l\u2019interaction du rayonnement \u00e9lectromagn\u00e9tique et de la mati\u00e8re. Il est \u00e0 la base des m\u00e9thodes de t\u00e9l\u00e9d\u00e9tection, actives et passives. Le cours portera, entre autres, sur le sondage spectroscopique des atmosph\u00e8res plan\u00e9taires et l&rsquo;observation radiom\u00e9trique et radar des surfaces du syst\u00e8me solaire. Programme 1 &#8211; \u00c9lectromagn\u00e9tisme, interactions rayonnement-mati\u00e8re&#8211; Processus physiques : &hellip; <\/p>\n<p class=\"link-more\"><a href=\"https:\/\/www.master-planeto.universite-paris-saclay.fr\/?page_id=60\" class=\"more-link\">Lire la suite de<span class=\"screen-reader-text\">\u00ab\u00a0UE 1 &#8211; Transfert radiatif dans les atmosph\u00e8res et surfaces plan\u00e9taires\u00a0\u00bb<\/span><\/a><\/p>\n","protected":false},"author":14,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"inspiro_hide_title":false,"inspiro_hide_featured_image":false,"footnotes":""},"class_list":["post-60","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.master-planeto.universite-paris-saclay.fr\/index.php?rest_route=\/wp\/v2\/pages\/60","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.master-planeto.universite-paris-saclay.fr\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.master-planeto.universite-paris-saclay.fr\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.master-planeto.universite-paris-saclay.fr\/index.php?rest_route=\/wp\/v2\/users\/14"}],"replies":[{"embeddable":true,"href":"https:\/\/www.master-planeto.universite-paris-saclay.fr\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=60"}],"version-history":[{"count":8,"href":"https:\/\/www.master-planeto.universite-paris-saclay.fr\/index.php?rest_route=\/wp\/v2\/pages\/60\/revisions"}],"predecessor-version":[{"id":955,"href":"https:\/\/www.master-planeto.universite-paris-saclay.fr\/index.php?rest_route=\/wp\/v2\/pages\/60\/revisions\/955"}],"wp:attachment":[{"href":"https:\/\/www.master-planeto.universite-paris-saclay.fr\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=60"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}