{"id":1452,"date":"2021-08-03T22:02:48","date_gmt":"2021-08-03T20:02:48","guid":{"rendered":"http:\/\/vega78astronomie.fr\/?p=1452"},"modified":"2022-08-22T15:47:44","modified_gmt":"2022-08-22T13:47:44","slug":"doplergramme-solex","status":"publish","type":"post","link":"https:\/\/vega78astronomie.fr\/index.php\/2021\/08\/03\/doplergramme-solex\/","title":{"rendered":"Dopplergramme Sol&rsquo;Ex"},"content":{"rendered":"\n<figure class=\"wp-block-image size-large\"><a href=\"http:\/\/vega78astronomie.fr\/wp-content\/uploads\/2021\/08\/2021-08-02-dopplergramme.jpg\"><img loading=\"lazy\" decoding=\"async\" width=\"1024\" height=\"544\" src=\"http:\/\/vega78astronomie.fr\/wp-content\/uploads\/2021\/08\/2021-08-02-dopplergramme-1024x544.jpg\" alt=\"\" class=\"wp-image-1453\" srcset=\"https:\/\/vega78astronomie.fr\/wp-content\/uploads\/2021\/08\/2021-08-02-dopplergramme-1024x544.jpg 1024w, https:\/\/vega78astronomie.fr\/wp-content\/uploads\/2021\/08\/2021-08-02-dopplergramme-300x159.jpg 300w, https:\/\/vega78astronomie.fr\/wp-content\/uploads\/2021\/08\/2021-08-02-dopplergramme-768x408.jpg 768w, https:\/\/vega78astronomie.fr\/wp-content\/uploads\/2021\/08\/2021-08-02-dopplergramme-1536x817.jpg 1536w, https:\/\/vega78astronomie.fr\/wp-content\/uploads\/2021\/08\/2021-08-02-dopplergramme-200x106.jpg 200w, https:\/\/vega78astronomie.fr\/wp-content\/uploads\/2021\/08\/2021-08-02-dopplergramme.jpg 1565w\" sizes=\"auto, (max-width: 1024px) 100vw, 1024px\" \/><\/a><\/figure>\n\n\n\n<p>Mise en \u00e9vidence de la rotation du soleil par Dopplergramme.<\/p>\n\n\n\n<p>Les couches d&rsquo;image rouge et bleu sont faites par d\u00e9calage spectrale autour de la raie Ha ( 656nm) <\/p>\n\n\n\n<p>Image B de la trichromie avec la longueur d\u2019onde situ\u00e9e \u00e0 gauche de H-alpha (courte longueur d\u2019onde),<br>Image R avec l\u2019image \u00e0 droite de H-alpha<br>Image V = (R + B)\/2.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Mise en \u00e9vidence de la rotation du soleil par Dopplergramme. Les couches d&rsquo;image rouge et bleu sont faites par d\u00e9calage spectrale autour de la raie Ha ( 656nm) Image B de la trichromie avec la longueur d\u2019onde situ\u00e9e \u00e0 gauche de H-alpha (courte longueur d\u2019onde),Image R avec l\u2019image \u00e0 droite de H-alphaImage V = (R [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[20,17],"tags":[],"class_list":["post-1452","post","type-post","status-publish","format-standard","hentry","category-soleil","category-spectroscopie"],"_links":{"self":[{"href":"https:\/\/vega78astronomie.fr\/index.php\/wp-json\/wp\/v2\/posts\/1452","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/vega78astronomie.fr\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/vega78astronomie.fr\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/vega78astronomie.fr\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/vega78astronomie.fr\/index.php\/wp-json\/wp\/v2\/comments?post=1452"}],"version-history":[{"count":5,"href":"https:\/\/vega78astronomie.fr\/index.php\/wp-json\/wp\/v2\/posts\/1452\/revisions"}],"predecessor-version":[{"id":1458,"href":"https:\/\/vega78astronomie.fr\/index.php\/wp-json\/wp\/v2\/posts\/1452\/revisions\/1458"}],"wp:attachment":[{"href":"https:\/\/vega78astronomie.fr\/index.php\/wp-json\/wp\/v2\/media?parent=1452"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/vega78astronomie.fr\/index.php\/wp-json\/wp\/v2\/categories?post=1452"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/vega78astronomie.fr\/index.php\/wp-json\/wp\/v2\/tags?post=1452"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}