{"id":17,"date":"2025-01-22T17:07:09","date_gmt":"2025-01-22T17:07:09","guid":{"rendered":"https:\/\/teams.issibern.ch\/quantifyingspaceweatherimpacts\/?page_id=17"},"modified":"2025-01-22T17:08:27","modified_gmt":"2025-01-22T17:08:27","slug":"team-members","status":"publish","type":"page","link":"https:\/\/teams.issibern.ch\/quantifyingspaceweatherimpacts\/team-members\/","title":{"rendered":"Team Members"},"content":{"rendered":"<table style=\"width: 100%;height: 623px\">\n<tbody>\n<tr style=\"height: 24px\">\n<td style=\"width: 147.1px;height: 24px\"><strong>Name<\/strong><\/td>\n<td style=\"width: 260.867px;height: 24px\"><strong>Institute\/Location<\/strong><\/td>\n<td style=\"width: 676.033px;height: 24px\"><strong>Expertise<\/strong><\/td>\n<\/tr>\n<tr style=\"height: 71px\">\n<td style=\"width: 147.1px;height: 71px\">Simon Thomas (Lead)<\/td>\n<td style=\"width: 260.867px;height: 71px\">IRAP, France<\/td>\n<td style=\"width: 676.033px;height: 71px\">Analysis of observations in the solar wind &amp; ionosphere. Quantify risks from worst-case scenarios.<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 147.1px;height: 48px\">Stephanie Yardley (Co-lead)<\/td>\n<td style=\"width: 260.867px;height: 48px\">Northumbria University, UK<\/td>\n<td style=\"width: 676.033px;height: 48px\">Observational analysis &amp; data-driven magnetic field modelling, and magnetic connectivity of SEP source regions.<\/td>\n<\/tr>\n<tr style=\"height: 96px\">\n<td style=\"width: 147.1px;height: 96px\">David Brooks<\/td>\n<td style=\"width: 260.867px;height: 96px\">GMU, US\/JAXA, Japan<\/td>\n<td style=\"width: 676.033px;height: 96px\">Tracing SEP events back to their source regions by applying and adapting his composition diagnostic technique to Hinode\/EIS and SolO datasets.<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 147.1px;height: 48px\">Du Toit Strauss<\/td>\n<td style=\"width: 260.867px;height: 48px\">North-West University, South Africa<\/td>\n<td style=\"width: 676.033px;height: 48px\">Modelling of energetic particles in the heliosphere, with a focus on the interactions with solar wind transients. Contribute to selection of SEP and GLE events.<\/td>\n<\/tr>\n<tr style=\"height: 24px\">\n<td style=\"width: 147.1px;height: 24px\">Nicolas Wijsen<\/td>\n<td style=\"width: 260.867px;height: 24px\">KU Leuven, Belgium<\/td>\n<td style=\"width: 676.033px;height: 24px\">To run PARADISE SEP test-particle model this for each of the events analysed in the study.<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 147.1px;height: 48px\">Laura Rodriguez-Garcia<\/td>\n<td style=\"width: 260.867px;height: 48px\">ESAC\/ESA, Spain<\/td>\n<td style=\"width: 676.033px;height: 48px\">To analyse spacecraft observations within the inner heliosphere for each of the SEP events.<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 147.1px;height: 48px\">Mathew Owens<\/td>\n<td style=\"width: 260.867px;height: 48px\">University of Reading, UK<\/td>\n<td style=\"width: 676.033px;height: 48px\">Giving historical context to SEP and GLE events from results of recent studies. Model heliospheric magnetic field using HUXt data assimilation scheme.<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 147.1px;height: 48px\">Ilya Usoskin<\/td>\n<td style=\"width: 260.867px;height: 48px\">University of Oulu, Finland<\/td>\n<td style=\"width: 676.033px;height: 48px\">Provide expertise in defining extreme events &amp; help to direct the methodology to apply this to SEP hazards.<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 147.1px;height: 48px\">Monika Szelag<\/td>\n<td style=\"width: 260.867px;height: 48px\">Finnish Meteorological Institute, Finland<\/td>\n<td style=\"width: 676.033px;height: 48px\">Evaluate the influence each SEP event has on the chemistry of Earth\u2019s upper atmosphere using methodology from recent study.<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 147.1px;height: 48px\">Fran\u00e7ois Trompier<\/td>\n<td style=\"width: 260.867px;height: 48px\">IRSN, France<\/td>\n<td style=\"width: 676.033px;height: 48px\">Investigate the radiation doses from SEP events in the atmosphere to evaluate the impacts to aviation using observations and the Sievert PN tool.<\/td>\n<\/tr>\n<tr style=\"height: 24px\">\n<td style=\"width: 147.1px;height: 24px\">Karen Aplin<\/td>\n<td style=\"width: 260.867px;height: 24px\">University of Bristol, UK<\/td>\n<td style=\"width: 676.033px;height: 24px\">Investigating the impact of SEP events on atmospheric electricity on Earth and other planets.<\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 147.1px;height: 48px\">Jingnan Guo<\/td>\n<td style=\"width: 260.867px;height: 48px\">University of Science and Technology of China, China<\/td>\n<td style=\"width: 676.033px;height: 48px\">Provide expertise on SEP transport and impacts at the planets, providing her methodology utilised in recent studies focussed on Mars<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n","protected":false},"excerpt":{"rendered":"<p>Name Institute\/Location Expertise Simon Thomas (Lead) IRAP, France Analysis of observations in the solar wind &amp; ionosphere. Quantify risks from worst-case scenarios. Stephanie Yardley (Co-lead) Northumbria University, UK Observational analysis &amp; data-driven magnetic field modelling, and magnetic connectivity of SEP source regions. David Brooks GMU, US\/JAXA, Japan Tracing SEP events back to their source regions [&hellip;]<\/p>\n","protected":false},"author":131,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-17","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/teams.issibern.ch\/quantifyingspaceweatherimpacts\/wp-json\/wp\/v2\/pages\/17","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/teams.issibern.ch\/quantifyingspaceweatherimpacts\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/teams.issibern.ch\/quantifyingspaceweatherimpacts\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/quantifyingspaceweatherimpacts\/wp-json\/wp\/v2\/users\/131"}],"replies":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/quantifyingspaceweatherimpacts\/wp-json\/wp\/v2\/comments?post=17"}],"version-history":[{"count":4,"href":"https:\/\/teams.issibern.ch\/quantifyingspaceweatherimpacts\/wp-json\/wp\/v2\/pages\/17\/revisions"}],"predecessor-version":[{"id":22,"href":"https:\/\/teams.issibern.ch\/quantifyingspaceweatherimpacts\/wp-json\/wp\/v2\/pages\/17\/revisions\/22"}],"wp:attachment":[{"href":"https:\/\/teams.issibern.ch\/quantifyingspaceweatherimpacts\/wp-json\/wp\/v2\/media?parent=17"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}