{"id":131,"date":"2016-08-09T13:33:37","date_gmt":"2016-08-09T13:33:37","guid":{"rendered":"http:\/\/www.issibern.ch\/teams\/iojupitermagnet\/?page_id=2"},"modified":"2016-08-09T13:33:37","modified_gmt":"2016-08-09T13:33:37","slug":"sample-page","status":"publish","type":"page","link":"https:\/\/www.issibern.ch\/teams\/iojupitermagnet\/","title":{"rendered":"Abstract"},"content":{"rendered":"<div class=\"page\" title=\"Page 1\">\n<div class=\"section\">\n<div class=\"layoutArea\">\n<div class=\"column\">\n<p style=\"text-align: left\">A large coordinated observing campaign has probed Jupiter\u2019s magnetosphere at multiple wavelengths using more than a dozen ground- and space-based facilities, including the EUV spectroscope Hisaki\/EXCEED, HST, Chandra, XMM-Newton and IRTF. These observations were focussed on the JAXA Hisaki mission which is providing quasi-continuous measurements of emissions from both Jupiter\u2019s aurora and the Io plasma torus. The concurrent observations examined Io\u2019s volcanic activity and plasma torus variability, as well as Jupiter\u2019s auroral dynamics at radio, infrared, ultraviolet and X-ray wavelengths. This team aims to bring together these observations with state of the art modelling of processes in the inner magnetosphere in order to explore the interactions between Io, Jupiter, the magnetosphere and the surrounding solar wind. Through combined analysis of these diverse measurements, facilitated by ISSI, we will develop a better understanding of how mass and energy are transferred <span style=\"font-size: 12pt\">through<\/span> the Jovian system on different timescales. This is especially timely given the arrival of the NASA Juno mission at Jupiter as our results will provide global context for interpreting Juno observations.<\/p>\n<\/div>\n<p><strong><span style=\"font-size: 14pt\">Team Members<\/span><\/strong><\/p>\n<\/div>\n<\/div>\n<\/div>\n<div>Ichiro Yoshikawa, University of Tokyo, Japan (Team Leader)<br \/>\nSarah Badman, Lancaster University, UK (Deputy Team Leader)<br \/>\nBertrand Bonfond, Universit\u00e9 de Li\u00e8ge, Belgium<\/div>\n<div>Graziella Branduardi-Raymont, University College London, UK<\/div>\n<div>Becky Gray, Lancaster University, UK<\/div>\n<div>Yasumasa Kasaba, Tohoku University, Japan<\/div>\n<div>Tomoki Kimura, RIKEN, Japan<\/div>\n<div>Hajime Kita, Tohoku University, Japan<\/div>\n<div>Go Murakami, JAXA ISAS, Japan<\/div>\n<div>Carl Schmidt, LATMOS, France<\/div>\n<div>Todd Smith, JHU\/APL, USA<\/div>\n<div>Chihiro Tao, NICT, Japan<\/div>\n<div>Fuminori Tsuchiya, Tohoku University, Japan<\/div>\n<div>Kazuo Yoshioka, University of Tokyo, Japan<\/div>\n<p><\/p>\n<div>For information about the Team, please contact the Team Leader (yoshikawa at k.u-tokyo.ac.jp) or Deputy (s.badman at lancaster.ac.uk)<\/div>\n","protected":false},"excerpt":{"rendered":"<p>A large coordinated observing campaign has probed Jupiter\u2019s magnetosphere at multiple wavelengths using more than a dozen ground- and space-based facilities, including the EUV spectroscope Hisaki\/EXCEED, HST, Chandra, XMM-Newton and IRTF. These observations were focussed on the JAXA Hisaki mission &hellip; <a href=\"https:\/\/www.issibern.ch\/teams\/iojupitermagnet\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":54,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-131","page","type-page","status-publish","has-post-thumbnail","hentry"],"_links":{"self":[{"href":"https:\/\/www.issibern.ch\/teams\/iojupitermagnet\/wp-json\/wp\/v2\/pages\/131","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.issibern.ch\/teams\/iojupitermagnet\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.issibern.ch\/teams\/iojupitermagnet\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/iojupitermagnet\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/iojupitermagnet\/wp-json\/wp\/v2\/comments?post=131"}],"version-history":[{"count":0,"href":"https:\/\/www.issibern.ch\/teams\/iojupitermagnet\/wp-json\/wp\/v2\/pages\/131\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/iojupitermagnet\/wp-json\/wp\/v2\/media\/54"}],"wp:attachment":[{"href":"https:\/\/www.issibern.ch\/teams\/iojupitermagnet\/wp-json\/wp\/v2\/media?parent=131"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}