{"id":5,"date":"2024-05-06T12:58:43","date_gmt":"2024-05-06T12:58:43","guid":{"rendered":"https:\/\/teams.issibern.ch\/shocksturbulenceelectrons\/?page_id=5"},"modified":"2025-10-24T07:53:56","modified_gmt":"2025-10-24T07:53:56","slug":"sample-page","status":"publish","type":"page","link":"https:\/\/teams.issibern.ch\/shocksturbulenceelectrons\/sample-page\/","title":{"rendered":"Team Members"},"content":{"rendered":"

Our Team consists of 12 experts in the fields of heliophysics, space science, and astronomy. We plan to add two additional Early Stage Researchers (ESR) later. Our Team includes world-class experts who have used simulation, theory, and data analysis to examine the interaction between the solar wind and the LISM, turbulence, kinetic waves in plasmas, and radio emission. The Team represents 8 different institutions spanning 4 countries (including one ESA Member), and is well balanced in both gender and seniority.<\/p>\n

 <\/p>\n

 <\/p>\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
Team Members<\/caption>\n
Name<\/th>\nInstitution\/Email<\/th>\nCountry<\/th>\nRelevant Expertise<\/th>\n<\/tr>\n<\/thead>\n
Federico Fraternale (lead)<\/td>\nUniversity of Alabama in Huntsville
\nfederico.fraternale@uah.edu<\/td>\n		US<\/td>\nTurbulence of the SW and VLISM; Global SW-LISM interaction modeling; Voyager (MAG) data analysis.<\/td>\n<\/tr>\n
Stella Ocker (co-lead, ESR<\/em>)<\/td>\nCornell University
\nsko36@cornell.edu<\/td>\n		US<\/td>\nPlasma oscillations; Voyager (PWS) data analysis; Remote observations of ISM turbulence.<\/td>\n<\/tr>\n
Olga Alexandrova<\/td>\nLESIA, Observatoire de Paris, CNRS
\nolga.alexandrova@obspm.fr<\/td>\n		FR<\/td>\nTurbulence theory & data analysis; Plasma kinetic processes; Shock-turbulence interaction<\/td>\n<\/tr>\n
Iver Cairns<\/td>\nUniversity of Sydney
\niver.cairns@sydney.edu.au<\/td>\n		AU<\/td>\nTheory, simulation, & observation of plasma waves, and radio emissions.<\/td>\n<\/tr>\n
James M. Cordes<\/td>\nCornell University
\njmc33@cornell.edu<\/td>\n		US<\/td>\nInterstellar turbulence observation and theory; Remote sensing analysis<\/td>\n<\/tr>\n
William Kurth<\/td>\nUniversity of Iowa
\nwilliam-kurth@uiowa.edu<\/td>\n		US<\/td>\nPI of Voyager\/PWS; Plasma oscillations and radio emissions (observation, theory).<\/td>\n<\/tr>\n
Nicole Meyer-Vernet<\/td>\nLESIA, Observatoire de Paris, CNRS
\nnicole.meyer@obspm.fr<\/td>\n		FR<\/td>\nPlasma waves; Electron dynamics; Quasi-Thermal Fluctuations; Instruments<\/td>\n<\/tr>\n
Parisa Mostafavi<\/td>\nJohns Hopkins APL
\nparisa.mostafavi@jhuapl.edu<\/td>\n		US<\/td>\nShocks in multicomponent plasmas; Collisional shocks theory and modeling<\/td>\n<\/tr>\n
Ameneh Mousavi<\/td>\nSpace Science Institute
\namousavi@spacescience.org<\/td>\n		US<\/td>\nPickup ion instability kinetic theory and simulation<\/td>\n<\/tr>\n
Nikolai V. Pogorelov<\/td>\nUniversity of Alabama in Huntsville
\nnp0002@uah.edu<\/td>\n		US<\/td>\nGlobal SW-LISM modeling; Shocks physics (simulation, theory); Radio emissions; Numerical methods<\/td>\n<\/tr>\n
Christian Vasconez<\/td>\nEscuela Politecnica Nacional
\nchristian.vasconez@epn.edu.ec<\/td>\n		EC<\/td>\nTurbulence simulations (MHD, PIC) theory & data analysis<\/td>\n<\/tr>\n
Ming Zhang<\/td>\nFlorida Institute of Technology (FIT)
\nmzhang@fit.edu<\/td>\n		US<\/td>\nParticle transport\/acceleration; (theory, modeling, observations); plasma shock physics<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n","protected":false},"excerpt":{"rendered":"

Our Team consists of 12 experts in the fields of heliophysics, space science, and astronomy. We plan to add two additional Early Stage Researchers (ESR) later. Our Team includes world-class experts who have used simulation, theory, and data analysis to examine the interaction between the solar wind and the LISM, turbulence, kinetic waves in plasmas, […]<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-5","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/teams.issibern.ch\/shocksturbulenceelectrons\/wp-json\/wp\/v2\/pages\/5","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/teams.issibern.ch\/shocksturbulenceelectrons\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/teams.issibern.ch\/shocksturbulenceelectrons\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/shocksturbulenceelectrons\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/shocksturbulenceelectrons\/wp-json\/wp\/v2\/comments?post=5"}],"version-history":[{"count":11,"href":"https:\/\/teams.issibern.ch\/shocksturbulenceelectrons\/wp-json\/wp\/v2\/pages\/5\/revisions"}],"predecessor-version":[{"id":56,"href":"https:\/\/teams.issibern.ch\/shocksturbulenceelectrons\/wp-json\/wp\/v2\/pages\/5\/revisions\/56"}],"wp:attachment":[{"href":"https:\/\/teams.issibern.ch\/shocksturbulenceelectrons\/wp-json\/wp\/v2\/media?parent=5"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}