{"id":2,"date":"2024-09-03T13:32:26","date_gmt":"2024-09-03T13:32:26","guid":{"rendered":"https:\/\/teams.issibern.ch\/electronsearthsmagnetosphere\/?page_id=2"},"modified":"2024-09-05T18:10:11","modified_gmt":"2024-09-05T18:10:11","slug":"home","status":"publish","type":"page","link":"https:\/\/teams.issibern.ch\/electronsearthsmagnetosphere\/","title":{"rendered":"Team focus"},"content":{"rendered":"<p>The focus of the team is on compiling what is known and what is still unknown regarding the<br \/>\nphysics of plasma sheet and inner magnetospheric 1-100 keV electrons and their precipitation into<br \/>\nthe ionosphere. While several studies, including recent machine-learning models, have quantified the<br \/>\nhours-and-longer flux variations of these electrons, their most intense fluctuations occur on a time<br \/>\nscale of minutes with strong local time (MLT)-dependence. Models cannot account for these large<br \/>\nchanges on smaller spatial and temporal scales. Furthermore, while we know the fundamental<br \/>\nconnections between plasma waves and keV-electron scattering, predicting when and how much<br \/>\nprecipitation will occur for any particular space weather event is difficult. That is, it has been very<br \/>\nhard to find definite dependencies for the drivers of precipitation. This ISSI team would conduct a<br \/>\nthorough review of the state of knowledge about keV electrons to codify what is known, then use this<br \/>\nto create a list of goals for achieving significant advancement on this topic.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>The focus of the team is on compiling what is known and what is still unknown regarding the physics of plasma sheet and inner magnetospheric 1-100 keV electrons and their precipitation into the ionosphere. While several studies, including recent machine-learning models, have quantified the hours-and-longer flux variations of these electrons, their most intense fluctuations occur [&hellip;]<\/p>\n","protected":false},"author":135,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-2","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/teams.issibern.ch\/electronsearthsmagnetosphere\/wp-json\/wp\/v2\/pages\/2","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/teams.issibern.ch\/electronsearthsmagnetosphere\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/teams.issibern.ch\/electronsearthsmagnetosphere\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/electronsearthsmagnetosphere\/wp-json\/wp\/v2\/users\/135"}],"replies":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/electronsearthsmagnetosphere\/wp-json\/wp\/v2\/comments?post=2"}],"version-history":[{"count":3,"href":"https:\/\/teams.issibern.ch\/electronsearthsmagnetosphere\/wp-json\/wp\/v2\/pages\/2\/revisions"}],"predecessor-version":[{"id":32,"href":"https:\/\/teams.issibern.ch\/electronsearthsmagnetosphere\/wp-json\/wp\/v2\/pages\/2\/revisions\/32"}],"wp:attachment":[{"href":"https:\/\/teams.issibern.ch\/electronsearthsmagnetosphere\/wp-json\/wp\/v2\/media?parent=2"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}