{"id":36,"date":"2025-08-22T11:06:42","date_gmt":"2025-08-22T11:06:42","guid":{"rendered":"https:\/\/teams.issibern.ch\/globalinertialmodes\/?page_id=36"},"modified":"2025-08-22T11:15:27","modified_gmt":"2025-08-22T11:15:27","slug":"team-members","status":"publish","type":"page","link":"https:\/\/teams.issibern.ch\/globalinertialmodes\/team-members\/","title":{"rendered":"Team members"},"content":{"rendered":"<h3>Team leaders<\/h3>\n<ul>\n<li><span style=\"color: #333399\">Laurent Gizon<\/span> (lead)<br \/>\nprofessor, MPI for Solar System Research, Germany<br \/>\nExpertise: Helioseismology. Contributed to the first papers reporting the discovery and identification of solar inertial modes.<\/li>\n<li><span style=\"color: #008000\">Rhita-Maria Ouazzani<\/span> (co-lead)<br \/>\nAssociate astronomer, LIRA Observatoire de Paris-PSL, France<br \/>\nExpertise: modeling of stellar pulsations including effect of rotation and magnetic field in 2D. Contributed to the first paper reporting the detection of pure inertial modes in stars.<\/li>\n<\/ul>\n<h3>Team experts<\/h3>\n<ul>\n<li><span style=\"color: #008000\">Victoria Antoci,<\/span> senior researcher, DTU Technical University of Denmark<br \/>\nAsteroseismic and spectrocopic data analysis of rotational and pulsational variables. Specialist of intermediate-mass stars (Leader of Kepler WG4: A- and F-type stars).<\/li>\n<li><span style=\"color: #333399\">Yuto Bekki<\/span>, postdoc, MPI for Solar System Research, Germany<br \/>\nRealistic linear models of solar inertial modes; Nonlinear evolution of baroclinicaly unstable high-latitude modes.<\/li>\n<li><span style=\"color: #008000\">Lisa Bugnet<\/span>, assistant professor, Institute of Science and Technology Austria<br \/>\nModeling of stellar pulsations using perturbative approaches. Seismic inferences of magnetic fields in sellar interiors.<\/li>\n<li><span style=\"color: #333399\">Nick Featherstone<\/span>, lead scientist, SWRI Boulder, USA<br \/>\nState-of-the-art numerical simulations of solar rotating magnetoconvection.<\/li>\n<li><span style=\"color: #333399\">Hideyuki Hotta<\/span>, professor, ISEE Nagoya, Japan<br \/>\nState-of-the-art numerical simulations of solar rotating magnetoconvection.<\/li>\n<li><span style=\"color: #333399\">Rekha Jain<\/span>, reader, University of Sheffield, UK<br \/>\nAnalytical models of travelling modes of solar rotating convection.<\/li>\n<li><span style=\"color: #333399\">Shravan Hanasoge<\/span>, professor, TIFR Mumbai, India<br \/>\nMode-coupling helioseismology applied to the study of solar inertial modes.<\/li>\n<li><span style=\"color: #008000\">Francois Ligni\u00e8res<\/span>, directeur de recherche, IRAP, Observatoire Midi-Pyr\u00e9n\u00e9es, Toulouse, France<br \/>\nDynamics of stellar interiors; convection, rotation, magnetic field, and pulsations.<\/li>\n<li><span style=\"color: #008000\">Hideyuki Saio<\/span>, emeritus professor, Tohoku University, Sendai, Japan<br \/>\nModels of stellar inertial and gravito-inertial modes, including stability. Interpretation of Kepler photometry of intermediate-mass stars.<\/li>\n<li><span style=\"color: #008000\">Masao Takata<\/span>, assistant professor, University of Tokyo, Japan<br \/>\nModels of stellar inertial and gravito-inertial modes. Seismic diagnostics based on gravito-inertial modes (including Rossby and pure inertial modes) in intermediate-mass stars.<\/li>\n<\/ul>\n<p><span style=\"color: #008000\">Stellar members<\/span> \/ <span style=\"color: #000080\">Solar members<\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Team leaders Laurent Gizon (lead) professor, MPI for Solar System Research, Germany Expertise: Helioseismology. Contributed to the first papers reporting the discovery and identification of solar inertial modes. Rhita-Maria Ouazzani (co-lead) Associate astronomer, LIRA Observatoire de Paris-PSL, France Expertise: modeling of stellar pulsations including effect of rotation and magnetic field in 2D. Contributed to the [&hellip;]<\/p>\n","protected":false},"author":169,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-36","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/teams.issibern.ch\/globalinertialmodes\/wp-json\/wp\/v2\/pages\/36","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/teams.issibern.ch\/globalinertialmodes\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/teams.issibern.ch\/globalinertialmodes\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/globalinertialmodes\/wp-json\/wp\/v2\/users\/169"}],"replies":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/globalinertialmodes\/wp-json\/wp\/v2\/comments?post=36"}],"version-history":[{"count":3,"href":"https:\/\/teams.issibern.ch\/globalinertialmodes\/wp-json\/wp\/v2\/pages\/36\/revisions"}],"predecessor-version":[{"id":40,"href":"https:\/\/teams.issibern.ch\/globalinertialmodes\/wp-json\/wp\/v2\/pages\/36\/revisions\/40"}],"wp:attachment":[{"href":"https:\/\/teams.issibern.ch\/globalinertialmodes\/wp-json\/wp\/v2\/media?parent=36"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}