{"id":1109,"date":"2019-07-03T11:00:27","date_gmt":"2019-07-03T02:00:27","guid":{"rendered":"https:\/\/guas-astronomy.jp\/weblog\/?p=1109"},"modified":"2019-07-09T10:15:50","modified_gmt":"2019-07-09T01:15:50","slug":"plasma-dynamics-in-the-solar-photosphere-studied-by-spectral-line-widths","status":"publish","type":"post","link":"https:\/\/guas-astronomy.jp\/weblog\/?p=1109","title":{"rendered":"Plasma dynamics in the solar photosphere studied by spectral line widths \/ Detecting planets around very low mass stars with the radial velocity method"},"content":{"rendered":"\n<p class=\"wp-block-paragraph\">[Speaker1]<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">Ryohtaroh Ishikawa,<br>\n SOKENDAI 3rd year (D1)<br>\n(Supervisor: Suematsu, Yoshinori, Katsukawa, Yukio, Kubo, Masahito) <\/p>\n\n\n\n<p class=\"wp-block-paragraph\">[Title1]<\/p>\n\n\n\n<p class=\"wp-block-paragraph\"> Plasma dynamics in the solar hotosphere studied by spectral line widths<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">[Speaker2]<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">Yui Kasagi,<br>\n SOKENDAI 1st year (M1) <br>\n(Supervisor: Takayuki Kotani, Saeko Hayashi, Wako Aoki) <\/p>\n\n\n\n<p class=\"wp-block-paragraph\">[Title2]<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">Detecting planets around very low mass stars with the radial velocity method<\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><\/p>\n","protected":false},"excerpt":{"rendered":"<p>[Speaker1] Ryohtaroh Ishikawa, SOKENDAI 3rd year (D1) (Supervisor: Suematsu, Yoshinori, Katsukawa, Yukio, 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-1109","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\/1109","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=1109"}],"version-history":[{"count":0,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=\/wp\/v2\/posts\/1109\/revisions"}],"wp:attachment":[{"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1109"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1109"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/guas-astronomy.jp\/weblog\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1109"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}