{"id":75,"date":"2022-01-28T14:29:51","date_gmt":"2022-01-28T13:29:51","guid":{"rendered":"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/?page_id=75"},"modified":"2022-04-25T15:02:03","modified_gmt":"2022-04-25T13:02:03","slug":"steering-committee","status":"publish","type":"page","link":"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/steering-committee\/","title":{"rendered":"Steering Committee"},"content":{"rendered":"\n<p>Contact us: <a href=\"mailto:bureau.aips@sympa.obspm.fr\">bureau.aips@sympa.obspm.fr<\/a><\/p>\n\n\n\n<div class=\"wp-block-image\"><figure class=\"alignleft is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/files\/2022\/02\/Kevin.jpeg\" alt=\"\" class=\"wp-image-110\" width=\"117\" height=\"133\" \/><\/figure><\/div>\n\n\n\n<p><strong>K\u00e9vin Belkacem<\/strong> (co-chair) is working at LESIA. His main scientific interests are stellar seismology, physics of waves and their interactions with turbulence, transport of angular momentum in stellar interiors. He is involved in the preparation of the ESA space-borne mission PLATO.&nbsp;&nbsp;<\/p>\n\n\n\n<p><br><\/p>\n\n\n\n<p>  <\/p>\n\n\n\n<p><\/p>\n\n\n\n<div class=\"wp-block-image\"><figure class=\"alignright is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/files\/2022\/04\/2022-02-15-172910.jpg\" alt=\"\" class=\"wp-image-261\" width=\"239\" height=\"135\" srcset=\"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/files\/2022\/04\/2022-02-15-172910.jpg 640w, https:\/\/sites.lesia.obspm.fr\/stellarphysics\/files\/2022\/04\/2022-02-15-172910-300x169.jpg 300w, https:\/\/sites.lesia.obspm.fr\/stellarphysics\/files\/2022\/04\/2022-02-15-172910-500x281.jpg 500w\" sizes=\"auto, (max-width: 239px) 100vw, 239px\" \/><\/figure><\/div>\n\n\n\n<p><strong>Franck Delahaye<\/strong> is working at LERMA. His main interests are atomic physics and stellar physics making the bridge between the two domains via the opacities.   Member of The Opacity Project, he is approaching the opacities with theoretical calculation, leading laboratory experiments and through their use in stellar modeling<\/p>\n\n\n\n<p>     <\/p>\n\n\n\n<p>  <\/p>\n\n\n\n<p><\/p>\n\n\n\n<div class=\"wp-block-image\"><figure class=\"alignleft is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/files\/2022\/02\/Misha.png\" alt=\"\" class=\"wp-image-112\" width=\"109\" height=\"129\" \/><\/figure><\/div>\n\n\n\n<p><strong>Misha Haywood<\/strong> is working at GEPI. His main scientific interests are galactic archeology, Galactic structure and evolution, Milky Way stellar populations. He is involved in the Gaia mission and spectroscopic surveys WEAVE and MOONS.<\/p>\n\n\n\n<p>     <\/p>\n\n\n\n<p>  <\/p>\n\n\n\n<p><\/p>\n\n\n\n<p>  <br><\/p>\n\n\n\n<div class=\"wp-block-image\"><figure class=\"alignright is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/files\/2022\/02\/OUAZZANI_RHITA-MARIA_MYSELF-1002x1024.jpg\" alt=\"\" class=\"wp-image-115\" width=\"146\" height=\"155\" \/><\/figure><\/div>\n\n\n\n<p><strong>Rhita-Maria Ouazzani<\/strong> is a member of the pole \u00c9toile at LESIA. Her main scientific interest is stellar rotation and its interaction with pulsations in stars, with the aim of using stellar pulsations to constrain dynamical transport processes in stellar interiors. She is also involved in the scientific preparation of the ESA PLATO mission.<\/p>\n\n\n\n<p>     <\/p>\n\n\n\n<p><br><\/p>\n\n\n\n<div class=\"wp-block-image\"><figure class=\"alignleft is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/files\/2022\/02\/Ludovic.jpeg\" alt=\"\" class=\"wp-image-116\" width=\"148\" height=\"151\" \/><\/figure><\/div>\n\n\n\n<p><strong>Ludovic Petitdemange<\/strong> (co-chair) is interested in understanding dynamo action occurring in astrophysical objects (stars and planets). He uses massively parallel spherical multidimensional simulations to model deep turbulent flows responsible for planetary and stellar magnetism. He currently works at LERMA, of which he is deputy director. <\/p>\n\n\n\n<p><br><\/p>\n\n\n\n<p>     <\/p>\n\n\n\n<div class=\"wp-block-image\"><figure class=\"alignright is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/files\/2022\/04\/unnamed.jpg\" alt=\"\" class=\"wp-image-205\" width=\"142\" height=\"159\" \/><\/figure><\/div>\n\n\n\n<p><strong>Fr\u00e9d\u00e9ric Royer<\/strong> is working in GEPI. He specialised in spectroscopic data reduction and analysis. He is involved in different instrumental projects and surveys (Gaia, MOONS, WEAVE) and his main scientific interest is the axial rotation of early-type stars.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Contact us: bureau.aips@sympa.obspm.fr K\u00e9vin Belkacem (co-chair) is working at LESIA. His main scientific interests are stellar seismology, physics of waves and their interactions with turbulence, transport of angular momentum in stellar interiors. He is involved in the preparation of the &hellip; <a href=\"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/steering-committee\/\">Continuer la lecture <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":73,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-75","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/wp-json\/wp\/v2\/pages\/75","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/wp-json\/wp\/v2\/users\/73"}],"replies":[{"embeddable":true,"href":"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/wp-json\/wp\/v2\/comments?post=75"}],"version-history":[{"count":24,"href":"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/wp-json\/wp\/v2\/pages\/75\/revisions"}],"predecessor-version":[{"id":274,"href":"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/wp-json\/wp\/v2\/pages\/75\/revisions\/274"}],"wp:attachment":[{"href":"https:\/\/sites.lesia.obspm.fr\/stellarphysics\/wp-json\/wp\/v2\/media?parent=75"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}