{"id":627,"date":"2016-07-06T14:59:37","date_gmt":"2016-07-06T05:59:37","guid":{"rendered":"http:\/\/guas-astronomy.jp\/weblog\/?p=627"},"modified":"2016-07-06T14:59:37","modified_gmt":"2016-07-06T05:59:37","slug":"radiation-mhd-simulation-of-clumpy-outflow-from-supercritical-accretion-flow-test-of-3d-calculation-a-high-precision-technique-to-correct-for-residual-atmospheric-dispersion-in-high-contrast-imagi","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=627","title":{"rendered":"Radiation-MHD Simulation of Clumpy Outflow from Supercritical Accretion Flow: Test of 3D Calculation. \/ A High Precision Technique To Correct For Residual Atmospheric Dispersion In High-contrast Imaging Systems"},"content":{"rendered":"<p>[Speaker 1]<br \/>\nHiroshi Kobayashi, D3, SOKENDAI (Supervisor: Ken Ohsuga)<br \/>\n[Title]<br \/>\nRadiation-MHD Simulation of Clumpy Outflow from Supercritical Accretion Flow: Test of 3D Calculation.<\/p>\n<p>[Speaker 2]<br \/>\nPrashant Pathak, D2, SOKENDAI (Supervisor: Hideki Takami)<br \/>\n[Title]<br \/>\nA High Precision Technique To Correct For Residual Atmospheric Dispersion In High-contrast Imaging Systems<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker 1] Hiroshi Kobayashi, D3, SOKENDAI (Supervisor: Ken Ohsuga) [Title] Radiation-MHD Simulation of Clump [&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-627","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\/627","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=627"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/627\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=627"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=627"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=627"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}