{"id":677,"date":"2016-10-28T14:17:14","date_gmt":"2016-10-28T05:17:14","guid":{"rendered":"http:\/\/guas-astronomy.jp\/weblog\/?p=677"},"modified":"2016-10-28T14:17:14","modified_gmt":"2016-10-28T05:17:14","slug":"interpreting-the-double-ridge-structure-in-high-frequency-time-distance-diagrams-close-loop-correction-of-residual-atmospheric-dispersion-in-high-contrast-imaging-systems","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=677","title":{"rendered":"Interpreting the double-ridge structure in high-frequency time-distance diagrams \/ Close loop correction of residual atmospheric dispersion in high-contrast imaging systems"},"content":{"rendered":"<p>[Speaker1]<br \/>\nNagaaki Kambara, M2 , Sokendai, Mitaka (supervisor : Takashi Sekii, Tetsuya Watanabe, Masahito Kubo)<\/p>\n<p>[Title]<br \/>\n Interpreting the double-ridge structure in high-frequency time-distance diagrams<\/p>\n<p>[Speaker2]<br \/>\nPrashant Pathak, D3, Sokendai, Hawaii (supervisor : Prof. Hideki Takami) <\/p>\n<p>[Title]<br \/>\nClose loop correction of residual atmospheric dispersion in high-contrast imaging systems<\/p>\n<p>[Abstract]<br \/>\nFor direct imaging of habitable exoplanets from ground-based telescopes, it is crucial to correct for all the wavefront errors. One such error comes atmospheric refraction, in this talk, I will talk about why it is important to correct for refraction to the highest degree and how it can be achieved. <\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Nagaaki Kambara, M2 , Sokendai, Mitaka (supervisor : Takashi Sekii, Tetsuya Watanabe, Masahito Kubo [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6,5],"tags":[],"class_list":["post-677","post","type-post","status-publish","format-standard","hentry","category-6","category-5"],"_links":{"self":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/677","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=677"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/677\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=677"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=677"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=677"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}