{"id":22,"date":"2016-09-28T16:10:45","date_gmt":"2016-09-28T14:10:45","guid":{"rendered":"http:\/\/www.issibern.ch\/teams\/iojupitermagnet\/?page_id=22"},"modified":"2016-09-28T16:10:45","modified_gmt":"2016-09-28T14:10:45","slug":"meeting-1","status":"publish","type":"page","link":"https:\/\/www.issibern.ch\/teams\/iojupitermagnet\/meeting-1\/","title":{"rendered":"Meetings"},"content":{"rendered":"

The first team meeting was held at ISSI on 26-30 September 2016<\/p>\n

Presentations<\/p>\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
Tsuchiya<\/td>\nLocal electron heating around Io<\/td>\n<\/tr>\n
Kimura<\/td>\nEnergetic events seen as auroras and their responses to the plasma mass loading from Io<\/td>\n<\/tr>\n
Schmidt<\/td>\nCharacteristics of the S II Ribbon in Io’s Plasma Torus<\/td>\n<\/tr>\n
Murakami<\/td>\nSolar wind influence on Jupiter’s inner magnetosphere observed by Hisaki<\/td>\n<\/tr>\n
Yoshikawa<\/td>\nResponse of Io-plasma-torus to transient internally-driven aurora at Jupiter<\/td>\n<\/tr>\n
Gray<\/td>\nAuroral imaging of planetward transport and its consequences in the inner magnetosphere<\/td>\n<\/tr>\n
Yoshioka<\/td>\nResponse of Jupiter’s Inner Magnetosphere to Io’s Volcanic Activity Seen by Hisaki<\/td>\n<\/tr>\n
Tao<\/td>\nJupiter auroral spectra taken by Hisaki\/EXCEED<\/td>\n<\/tr>\n
Kita<\/td>\nStatistical study of solar wind control on Jovian UV auroral activity obtained from long-term Hisaki EXCEED observations<\/td>\n<\/tr>\n
Kasaba<\/td>\nGround-based observations during Hisaki campaigns<\/td>\n<\/tr>\n
Nichols<\/td>\nHST observations of Jupiter’s FUV aurorae during Juno’s approach<\/td>\n<\/tr>\n
Bonfond<\/td>\nAnalysis of the jovian\u00a0aurora<\/td>\n<\/tr>\n
Badman<\/td>\nWeakening of Jupiter’s aurora in January 2014<\/td>\n<\/tr>\nBranduardi-Raymont<\/td>\nX-ray views of the Jupiter system: past, present and future<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

\"team_beer1\"<\/p>\n

\"team_beer2\"<\/p>\n

The second team meeting was held at ISSI on 11-15 September 2017<\/p>\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
Tsuchiya<\/td>\n(1)Plasma density at Io: model to explain the Io phase effect observed by HISAKI
\n(2)Change in Alfven transit time from Io to Jupiter’s ionosphere due to increased plasma density in Io plasma torus
\n(3)Evolution of radial distribution of Io plasma torus during Io’s volcanic event in 2015<\/td>\n<\/tr>\n
Yoshikawa<\/td>\nVolcanic activity on Io and its influence to the IPT<\/td>\n<\/tr>\n
Suzuki<\/td>\nDetailed features of IPT brightenings deduced from statistical modeling of light curve<\/td>\n<\/tr>\n
Koga<\/td>\nSpatial distribution of Io’s oxygen neutral cloud during volcanically quiet and active periods in 2014-2015 observed by Hisaki\/EXCEED<\/td>\n<\/tr>\n
Yoshioka<\/td>\nRadial variation of S and O ions deduced from EUV spectra.
\nIo’s control on the Jovian magnetospheric dynamics<\/td>\n<\/tr>\n
Murakami<\/td>\nResponse of Jupiter’s inner magnetosphere to solar wind derived from Hisaki observations<\/td>\n<\/tr>\n
Smith<\/td>\nNeutral cloud distributions and response to Io source activity<\/td>\n<\/tr>\n
Schmidt<\/td>\n<\/td>\n<\/tr>\n
Kimura<\/td>\nGlobal plasma transport in Jupiter’s magnetosphere during transient auroral brightening<\/td>\n<\/tr>\n
Bonfond<\/td>\nJuno-UVS and Hubble Space Telescope observations during Juno’s first year in orbit” during the meeting<\/td>\n<\/tr>\n
Will<\/td>\nJupiter’s auroral response to a Co-rotating Interaction Region<\/td>\n<\/tr>\n
Grey<\/td>\nCharacterisation of Jupiter’s Second Auroral Oval<\/td>\n<\/tr>\n
Kita<\/td>\nSolar wind control of Jovian aurora & recent activities of ground based observations<\/td>\n<\/tr>\n
Tao<\/td>\nVariation of Jupiter auroral spectra during Io volcanic events taken by Hisaki\/EXCEED: additional analysis<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n","protected":false},"excerpt":{"rendered":"

The first team meeting was held at ISSI on 26-30 September 2016 Presentations Tsuchiya Local electron heating around Io Kimura Energetic events seen as auroras and their responses to the plasma mass loading from Io Schmidt Characteristics of the S … Continue reading →<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":56,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-22","page","type-page","status-publish","has-post-thumbnail","hentry"],"_links":{"self":[{"href":"https:\/\/www.issibern.ch\/teams\/iojupitermagnet\/wp-json\/wp\/v2\/pages\/22","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=22"}],"version-history":[{"count":0,"href":"https:\/\/www.issibern.ch\/teams\/iojupitermagnet\/wp-json\/wp\/v2\/pages\/22\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/iojupitermagnet\/wp-json\/wp\/v2\/media\/56"}],"wp:attachment":[{"href":"https:\/\/www.issibern.ch\/teams\/iojupitermagnet\/wp-json\/wp\/v2\/media?parent=22"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}