{"id":2,"date":"2023-06-20T11:49:33","date_gmt":"2023-06-20T11:49:33","guid":{"rendered":"https:\/\/teams.issibern.ch\/middlecorona\/?page_id=2"},"modified":"2024-05-16T15:28:50","modified_gmt":"2024-05-16T15:28:50","slug":"home","status":"publish","type":"page","link":"https:\/\/teams.issibern.ch\/middlecorona\/","title":{"rendered":"Home"},"content":{"rendered":"<p><\/p>\r\n<p class=\"p1\">The region between the mainly magnetically closed inner corona and the mostly radial outer corona\u2013the middle corona\u2013 is largely unexplored in long-term data-sets, despite the fact that important, but unknown, physical processes and transitions, which accelerate the solar wind and affect the inner corona are acting there. Studies have relied on sporadic off-point campaigns from space-based instrumentation and ground-based eclipse observations.<\/p>\r\n<p class=\"p1\">Several space-based missions aim to soon fill this observational gap. However, obtaining information on the plasma state (such as densities, temperatures, velocities, magnetic field, and chemical abundances) is a non-trivial task.<\/p>\r\n<p class=\"p2\">We have gathered a range of leading experts to assess\/compare forward modelling techniques and benchmark them against observations to obtain such information. Emphasis is on 1) 3-D codes for the calculation of spectral line intensities taking into account resonant photo-excitation and Doppler dimming effects; 2) 3-D codes for the calculation of the Stokes profiles including the magnetic field, estimated from global MHD simulations.\u00a0<\/p>\r\n<p>We will also coordinate multi-wavelength campaigns and recommend future observations and\u00a0 missions.<\/p>\r\n<p>&nbsp;<\/p>\r\n<p>We acknowledge the use of Zulip for communicating among the team members. Zulip is an open-source modern team chat app designed to keep both live and asynchronous conversations organized, see https:\/\/zulip.com\/ <img loading=\"lazy\" decoding=\"async\" class=\"alignnone  wp-image-75\" src=\"https:\/\/teams.issibern.ch\/middlecorona\/wp-content\/uploads\/sites\/85\/2024\/05\/zulip-icon-128x128-1.png\" alt=\"\" width=\"51\" height=\"51\" \/><\/p>\r\n","protected":false},"excerpt":{"rendered":"<p>The region between the mainly magnetically closed inner corona and the mostly radial outer corona\u2013the middle corona\u2013 is largely unexplored in long-term data-sets, despite the fact that important, but unknown, physical processes and transitions, which accelerate the solar wind and affect the inner corona are acting there. Studies have relied on sporadic off-point campaigns from [&hellip;]<\/p>\n","protected":false},"author":95,"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\/middlecorona\/wp-json\/wp\/v2\/pages\/2","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/teams.issibern.ch\/middlecorona\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/teams.issibern.ch\/middlecorona\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/middlecorona\/wp-json\/wp\/v2\/users\/95"}],"replies":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/middlecorona\/wp-json\/wp\/v2\/comments?post=2"}],"version-history":[{"count":5,"href":"https:\/\/teams.issibern.ch\/middlecorona\/wp-json\/wp\/v2\/pages\/2\/revisions"}],"predecessor-version":[{"id":76,"href":"https:\/\/teams.issibern.ch\/middlecorona\/wp-json\/wp\/v2\/pages\/2\/revisions\/76"}],"wp:attachment":[{"href":"https:\/\/teams.issibern.ch\/middlecorona\/wp-json\/wp\/v2\/media?parent=2"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}