{"id":74,"date":"2019-02-01T12:34:12","date_gmt":"2019-02-01T10:34:12","guid":{"rendered":"http:\/\/www.issibern.ch\/teams\/solflareconnectsolenerg\/?page_id=72"},"modified":"2019-02-01T12:34:12","modified_gmt":"2019-02-01T10:34:12","slug":"first-meeting","status":"publish","type":"page","link":"https:\/\/www.issibern.ch\/teams\/solflareconnectsolenerg\/first-meeting\/","title":{"rendered":"First meeting"},"content":{"rendered":"<p>First meeting schedule<\/p>\n<p>(.pdf version <a href=\"https:\/\/www.issibern.ch\/teams\/solflareconnectsolenerg\/wp-content\/uploads\/sites\/145\/2019\/02\/ISSI_team_final_schedule_M1_13_2_19.pdf\">ISSI_team_final_schedule_M1_13_2_19<\/a>).<\/p>\n<ul>\n<li>Each person has an hour for talk and discussion so we suggest that <strong>talks are ~30-40 mins so we have a short time for discussion and questions at the end of each talk.<\/strong><\/li>\n<li>We are going to try and keep to the schedule, i.e. we will stop the discussion at the end of your allocated time and any further discussion can be continued during the <strong>allocated discussion times at the end of the day, <\/strong>so everyone can talk at their scheduled time and get sufficient breaks to keep things productive each day!<\/li>\n<\/ul>\n<p><span style=\"color: #3ad42f\"><strong>Monday 25th February<\/strong><\/span><\/p>\n<table style=\"height: 110px;border-style: hidden;width: 584px\" width=\"540\">\n<tbody>\n<tr style=\"height: 10px\">\n<td style=\"height: 10px;width: 126px\"><span style=\"color: #3ad42f\"><strong>14:00-14:15<\/strong><\/span><\/td>\n<td style=\"height: 10px;width: 438px\"><strong>Maurizio Falanga &#8211; <\/strong>Welcome to ISSI<\/td>\n<\/tr>\n<tr style=\"height: 10px\">\n<td style=\"height: 10px;width: 126px\"><span style=\"color: #3ad42f\"><strong>14:15-15:00<\/strong><\/span><\/td>\n<td style=\"height: 10px;width: 438px\"><strong>Natasha Jeffrey\/Frederic Effenberger &#8211; <\/strong>Aims of the project\/first meeting<\/td>\n<\/tr>\n<tr style=\"height: 63px\">\n<td style=\"height: 10px;width: 126px\"><span style=\"color: #3ad42f\"><strong>15:00-15:30<\/strong><\/span><\/td>\n<td style=\"height: 10px;width: 438px\"><span style=\"color: #3ad42f\"><strong>Break<\/strong><\/span><\/td>\n<\/tr>\n<tr style=\"height: 87px\">\n<td style=\"height: 33px;width: 126px\"><span style=\"color: #3ad42f\"><strong>15:30-16:30<\/strong><\/span><\/td>\n<td style=\"height: 33px;width: 438px\"><strong>Natasha Jeffrey \u2013 <\/strong>Coronal plasma properties and determining the properties of solar flare-accelerated electrons<\/td>\n<\/tr>\n<tr style=\"height: 87px\">\n<td style=\"height: 23px;width: 126px\"><span style=\"color: #3ad42f\"><strong>16:30-17:30<\/strong><\/span><\/td>\n<td style=\"height: 23px;width: 438px\"><strong>Frederic Effenberger &#8211;<\/strong>Flaring region modelling with SDE methods and the relation to SEP modelling<\/td>\n<\/tr>\n<tr style=\"height: 63px\">\n<td style=\"height: 14px;width: 126px\"><span style=\"color: #3ad42f\"><strong>17:30-18:00<\/strong><\/span><\/td>\n<td style=\"height: 14px;width: 438px\"><span style=\"color: #3ad42f\"><strong>ISSI welcome drinks<\/strong><\/span><\/td>\n<\/tr>\n<tr style=\"height: 41px\">\n<td style=\"height: 10px;width: 126px\"><span style=\"color: #3ad42f\"><strong>19:00?<\/strong><\/span><\/td>\n<td style=\"height: 10px;width: 438px\"><span style=\"color: #3ad42f\"><strong>Welcome dinner?<\/strong><\/span><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p>&nbsp;<\/p>\n<p><span style=\"color: #ff0000\"><strong>Tuesday 26th February<\/strong><\/span><\/p>\n<table style=\"height: 350px;width: 581px\" width=\"586\">\n<tbody>\n<tr style=\"height: 63px\">\n<td style=\"height: 10px;width: 122.40625px\"><span style=\"color: #ff0000\"><strong>09:00-09:30<\/strong><\/span><\/td>\n<td style=\"height: 10px;width: 438.625px\"><span style=\"color: #ff0000\"><strong>Coffee<\/strong><\/span><\/td>\n<\/tr>\n<tr style=\"height: 87px\">\n<td style=\"height: 10px;width: 122.40625px\"><span style=\"color: #ff0000\"><strong>09:30-10:30<\/strong><\/span><\/td>\n<td style=\"height: 10px;width: 438.625px\"><strong>Alexander Warmuth &#8211; \u00a0<\/strong>Constraining electron acceleration: X-rays, radio, and additional spectral regimes.<\/td>\n<\/tr>\n<tr style=\"height: 87px\">\n<td style=\"height: 14px;width: 122.40625px\"><span style=\"color: #ff0000\"><strong>10:30-11:30<\/strong><\/span><\/td>\n<td style=\"height: 14px;width: 438.625px\"><strong>Eduard Kontar &#8211; <\/strong>Solar energetic electrons in the inner heliosphere: particles, plasma waves and radio emission<\/td>\n<\/tr>\n<tr style=\"height: 63px\">\n<td style=\"height: 10px;width: 122.40625px\"><span style=\"color: #ff0000\"><strong>11:30-12:00<\/strong><\/span><\/td>\n<td style=\"height: 10px;width: 438.625px\"><span style=\"color: #ff0000\"><strong>Break<\/strong><\/span><\/td>\n<\/tr>\n<tr style=\"height: 111px\">\n<td style=\"height: 51px;width: 122.40625px\"><span style=\"color: #ff0000\"><strong>12:00-13:00<\/strong><\/span><\/td>\n<td style=\"height: 51px;width: 438.625px\"><strong>Nicolas Bian &#8211; <\/strong>Ups and downs: modelling the first arrival times of energetic electrons at 1AU &amp; the effect of magnetic convergence on the diffusion of flare accelerated electrons in coronal loops<\/td>\n<\/tr>\n<tr style=\"height: 10px\">\n<td style=\"height: 10px;width: 122.40625px\"><span style=\"color: #ff0000\"><strong>13:00-14:30<\/strong><\/span><\/td>\n<td style=\"height: 10px;width: 438.625px\"><span style=\"color: #ff0000\"><strong>Lunch<\/strong><\/span><\/td>\n<\/tr>\n<tr style=\"height: 56px\">\n<td style=\"height: 25px;width: 122.40625px\"><span style=\"color: #ff0000\"><strong>14:30-15:30<\/strong><\/span><\/td>\n<td style=\"height: 25px;width: 438.625px\"><strong>Discussion: <\/strong><em>Monday + Tuesday talk topics (mainly acceleration and transport issues at the Sun\/high corona)<\/em><\/td>\n<\/tr>\n<tr style=\"height: 63px\">\n<td style=\"height: 12px;width: 122.40625px\"><span style=\"color: #ff0000\"><strong>15:30-16:00<\/strong><\/span><\/td>\n<td style=\"height: 12px;width: 438.625px\"><span style=\"color: #ff0000\"><strong>Break<\/strong><\/span><\/td>\n<\/tr>\n<tr style=\"height: 247px\">\n<td style=\"height: 208px;width: 122.40625px\"><span style=\"color: #ff0000\"><strong>16:00-17:30<\/strong><\/span><\/td>\n<td style=\"height: 208px;width: 438.625px\"><strong>Discussion:\u00a0<\/strong><em>Monday + Tuesday talk topics (mainly acceleration and transport issues at the Sun\/high corona)<\/em><\/p>\n<ul style=\"list-style-type: circle\">\n<li><em>Different plasma environments and different transport processes at the Sun, upper corona, and in the heliosphere?\u00a0 <\/em><\/li>\n<li><em>How do we best determine the properties of the acceleration region(s)? <\/em><\/li>\n<li><em>Role of transport versus acceleration?<\/em><\/li>\n<li><em>State-of the art modelling? <\/em><\/li>\n<li><em>Current observational evidence?<\/em><\/li>\n<li><em>Results from remote observations.<\/em><\/li>\n<li><em>Continued discussion from talks.<\/em><\/li>\n<li><strong>Possible telecon (Scattering and turbulence) at 17:00-17:30<\/strong><\/li>\n<\/ul>\n<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p>&nbsp;<\/p>\n<p><span style=\"color: #3366ff\"><strong>Wednesday 27th February\u00a0<\/strong><\/span><\/p>\n<table style=\"height: 285px\" width=\"583\">\n<tbody>\n<tr style=\"height: 75px\">\n<td style=\"width: 129.25px;height: 10px\"><span style=\"color: #3366ff\"><strong>09:00-09:30<\/strong><\/span><\/td>\n<td style=\"width: 434.78125px;height: 10px\"><span style=\"color: #3366ff\"><strong>Coffee (+ a quick discussion summary if required)<\/strong><\/span><\/td>\n<\/tr>\n<tr style=\"height: 23px\">\n<td style=\"width: 129.25px;height: 10px\"><span style=\"color: #3366ff\"><strong>09:30-10:30<\/strong><\/span><\/td>\n<td style=\"width: 434.78125px;height: 10px\"><strong>Nina Dresing &#8211; <\/strong>Energy spectra of solar energetic electron events observed by STEREO\/Widespread SEP events and multi-spacecraft observations.<\/td>\n<\/tr>\n<tr style=\"height: 103px\">\n<td style=\"width: 129.25px;height: 10px\"><span style=\"color: #3366ff\"><strong>10:30-11:30<\/strong><\/span><\/td>\n<td style=\"width: 434.78125px;height: 10px\"><strong>Du Toit Strauss &#8211; <\/strong>Modelling electron transport in the inner heliosphere.<\/td>\n<\/tr>\n<tr style=\"height: 75px\">\n<td style=\"width: 129.25px;height: 10px\"><span style=\"color: #3366ff\"><strong>11:30-12:00<\/strong><\/span><\/td>\n<td style=\"width: 434.78125px;height: 10px\"><span style=\"color: #3366ff\"><strong>Break<\/strong><\/span><\/td>\n<\/tr>\n<tr style=\"height: 131px\">\n<td style=\"width: 129.25px;height: 24px\"><span style=\"color: #3366ff\"><strong>12:00-13:00<\/strong><\/span><\/td>\n<td style=\"width: 434.78125px;height: 24px\"><strong>Gang Li &#8211;<\/strong> Fieldline meandering and Supergranule on the Sun &#8212; what observations can constrain the perpendicular diffusion of energetic particles<\/td>\n<\/tr>\n<tr style=\"height: 75px\">\n<td style=\"width: 129.25px;height: 10px\"><span style=\"color: #3366ff\"><strong>13:00-14:30<\/strong><\/span><\/td>\n<td style=\"width: 434.78125px;height: 10px\"><span style=\"color: #3366ff\"><strong>Lunch<\/strong><\/span><\/td>\n<\/tr>\n<tr style=\"height: 131px\">\n<td style=\"width: 129.25px;height: 27px\"><span style=\"color: #3366ff\"><strong>14:30-15:30<\/strong><\/span><\/td>\n<td style=\"width: 434.78125px;height: 27px\"><strong>Timo Laitinen &#8211; <\/strong>Particle propagation along meandering field lines: how to determine the length of the meandering path?<\/td>\n<\/tr>\n<tr style=\"height: 75px\">\n<td style=\"width: 129.25px;height: 10px\"><span style=\"color: #3366ff\"><strong>15:30-16:00<\/strong><\/span><\/td>\n<td style=\"width: 434.78125px;height: 10px\"><span style=\"color: #3366ff\"><strong>Break<\/strong><\/span><\/td>\n<\/tr>\n<tr style=\"height: 388px\">\n<td style=\"width: 129.25px;height: 174px\"><span style=\"color: #3366ff\"><strong>16:00-17:30<\/strong><\/span><\/td>\n<td style=\"width: 434.78125px;height: 174px\"><strong>Discussion:\u00a0<\/strong><em>Wednesday talk topics (transport issues in the heliosphere)<\/em><\/p>\n<ul style=\"list-style-type: circle\">\n<li><em>Best ways of modelling electron transport in the heliosphere?<\/em><\/li>\n<li><em>What do we know from current in situ observations?<\/em><\/li>\n<li><em>How are we going to use new in situ observations?<\/em><\/li>\n<li><em>Visitor presentation?<\/em><\/li>\n<li><em>Continued discussion from talks?<\/em><\/li>\n<\/ul>\n<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p><strong>\u00a0<\/strong><\/p>\n<p><span style=\"color: #800080\"><strong>Thursday 28th February\u00a0<\/strong><\/span><\/p>\n<table style=\"width: 584px;height: 513px\">\n<tbody>\n<tr style=\"height: 28px\">\n<td style=\"width: 129.25px;height: 10px\"><span style=\"color: #800080\"><strong>09:00-09:30<\/strong><\/span><\/td>\n<td style=\"width: 434.765625px;height: 10px\"><span style=\"color: #800080\"><strong>Coffee (+ a quick discussion summary if required)<\/strong><\/span><\/td>\n<\/tr>\n<tr style=\"height: 28px\">\n<td style=\"width: 129.25px;height: 10px\"><span style=\"color: #800080\"><strong>09:30-10:30<\/strong><\/span><\/td>\n<td style=\"width: 434.765625px;height: 10px\"><strong>Junxiang Hu &#8211; ?<\/strong><\/td>\n<\/tr>\n<tr style=\"height: 112px\">\n<td style=\"width: 129.25px;height: 48px\"><span style=\"color: #800080\"><strong>10:30-11:30<\/strong><\/span><\/td>\n<td style=\"width: 434.765625px;height: 48px\"><strong>Vah\u00e9 Petrosian &#8211; <\/strong>Connections between flare Radiation Producing Particle (RPPs) and Solar Energetic Particles (SEPs):The role of RPPs in production of SEPs and the role of SEPs in producing radiation.<\/td>\n<\/tr>\n<tr style=\"height: 28px\">\n<td style=\"width: 129.25px;height: 54px\"><span style=\"color: #800080\"><strong>11:30-12:00<\/strong><\/span><\/td>\n<td style=\"width: 434.765625px;height: 54px\"><span style=\"color: #800080\"><strong>Break<\/strong><\/span><\/td>\n<\/tr>\n<tr style=\"height: 56px\">\n<td style=\"width: 129.25px;height: 10px\"><span style=\"color: #800080\"><strong>12:00-13:00<\/strong><\/span><\/td>\n<td style=\"width: 434.765625px;height: 10px\"><strong>Sophie Musset &#8211; <\/strong>Energetic electrons in flare-related jets<\/td>\n<\/tr>\n<tr style=\"height: 28px\">\n<td style=\"width: 129.25px;height: 58px\"><span style=\"color: #800080\"><strong>13:00-14:30<\/strong><\/span><\/td>\n<td style=\"width: 434.765625px;height: 58px\"><span style=\"color: #800080\"><strong>Lunch<\/strong><\/span><\/td>\n<\/tr>\n<tr style=\"height: 28px\">\n<td style=\"width: 129.25px;height: 10px\"><span style=\"color: #800080\"><strong>14:30-15:30<\/strong><\/span><\/td>\n<td style=\"width: 434.765625px;height: 10px\"><strong>Karl-Ludwig Klein &#8211;\u00a0<\/strong>Radio bursts and SEP events as tracers of energetic particle acceleration<\/td>\n<\/tr>\n<tr style=\"height: 28px\">\n<td style=\"width: 129.25px;height: 76px\"><span style=\"color: #800080\"><strong>15:30-16:00<\/strong><\/span><\/td>\n<td style=\"width: 434.765625px;height: 76px\"><span style=\"color: #800080\"><strong>Break<\/strong><\/span><\/td>\n<\/tr>\n<tr>\n<td style=\"width: 129.25px\"><span style=\"color: #800080\"><strong>16:00-17:00<\/strong><\/span><\/td>\n<td style=\"width: 434.765625px\"><strong>Lindsay\u00a0Glesener\u00a0<em>(remote from Minnesota)<\/em>&#8211;\u00a0<\/strong><em>Hard X-ray observations of accelerated electrons in small microflares.<\/em><\/td>\n<\/tr>\n<tr style=\"height: 310px\">\n<td style=\"width: 129.25px;height: 227px\"><span style=\"color: #800080\"><strong>17:00-18:00<\/strong><\/span><\/td>\n<td style=\"width: 434.765625px;height: 227px\"><strong>Discussion:\u00a0<\/strong><em>Thursday talk topics (related events \u2013 flare- jets\/CMEs)<\/em><\/p>\n<ul style=\"list-style-type: circle\">\n<li><em>Insights from ions\/gamma-ray observations?<\/em><\/li>\n<li><em>Acceleration and transport in flare-jets\/CMEs?<\/em><\/li>\n<li><em>Differences and similarities in the properties of different particle populations in flares only, and flare-jet\/CME events?<\/em><\/li>\n<li><em>What do we know from current observations and theory?<\/em><\/li>\n<li><em>Visitor presentation?<\/em><\/li>\n<li><em>Continued discussion from talks?<\/em><\/li>\n<\/ul>\n<\/td>\n<\/tr>\n<tr style=\"height: 36px\">\n<td style=\"width: 129.25px;height: 10px\"><span style=\"color: #800080\"><strong>19.30-<\/strong><\/span><\/td>\n<td style=\"width: 434.765625px;height: 10px\"><span style=\"color: #800080\"><strong>End of meeting dinner?<\/strong><\/span><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p>&nbsp;<\/p>\n<p><span style=\"color: #ff6600\"><strong>Friday 1st March<\/strong><\/span><\/p>\n<table class=\" alignleft\" style=\"width: 596px;border-style: none;height: 329px\">\n<tbody>\n<tr style=\"height: 10px\">\n<td style=\"width: 125px;height: 10px\"><span style=\"color: #ff6600\"><strong>09:00-09:30<\/strong><\/span><\/td>\n<td style=\"width: 438px;height: 10px\"><span style=\"color: #ff6600\"><strong>Coffee (+ a quick discussion summary if required)<\/strong><\/span><\/td>\n<\/tr>\n<tr style=\"height: 10px\">\n<td style=\"width: 125px;height: 10px\"><span style=\"color: #ff6600\"><strong>09:30-10:30<\/strong><\/span><\/td>\n<td style=\"width: 438px;height: 10px\"><strong>N. Jeffrey\/F. Effenberger \u2013 <\/strong>Summary of the week<\/td>\n<\/tr>\n<tr style=\"height: 24px\">\n<td style=\"width: 125px;height: 24px\"><span style=\"color: #ff6600\"><strong>10:30-11:30<\/strong><\/span><\/td>\n<td style=\"width: 438px;height: 24px\"><strong>Future\/on-going work\/plans for meeting two<\/strong><\/td>\n<\/tr>\n<tr style=\"height: 24px\">\n<td style=\"width: 125px;height: 24px\"><span style=\"color: #ff6600\"><strong>11:30-12:00<\/strong><\/span><\/td>\n<td style=\"width: 438px;height: 24px\"><span style=\"color: #ff6600\"><strong>Break<\/strong><\/span><\/td>\n<\/tr>\n<tr style=\"height: 48px\">\n<td style=\"width: 125px;height: 48px\"><span style=\"color: #ff6600\"><strong>12:00-13:00<\/strong><\/span><\/td>\n<td style=\"width: 438px;height: 48px\"><strong>Future\/on-going work\/plans for meeting two (if more time is required)<\/strong><\/td>\n<\/tr>\n<tr style=\"height: 24px\">\n<td style=\"width: 125px;height: 24px\"><span style=\"color: #ff6600\"><strong>13:00-14:30<\/strong><\/span><\/td>\n<td style=\"width: 438px;height: 24px\"><span style=\"color: #ff6600\"><strong>Lunch\/End of meeting<\/strong><\/span><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n","protected":false},"excerpt":{"rendered":"<p>First meeting schedule (.pdf version ISSI_team_final_schedule_M1_13_2_19). Each person has an hour for talk and discussion so we suggest that talks are ~30-40 mins so we have a short time for discussion and questions at the end of each talk. We &hellip; <a href=\"https:\/\/www.issibern.ch\/teams\/solflareconnectsolenerg\/first-meeting\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-74","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.issibern.ch\/teams\/solflareconnectsolenerg\/wp-json\/wp\/v2\/pages\/74","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.issibern.ch\/teams\/solflareconnectsolenerg\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.issibern.ch\/teams\/solflareconnectsolenerg\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/solflareconnectsolenerg\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/solflareconnectsolenerg\/wp-json\/wp\/v2\/comments?post=74"}],"version-history":[{"count":0,"href":"https:\/\/www.issibern.ch\/teams\/solflareconnectsolenerg\/wp-json\/wp\/v2\/pages\/74\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.issibern.ch\/teams\/solflareconnectsolenerg\/wp-json\/wp\/v2\/media?parent=74"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}