\nSecond team meeting: January 21st to 25th, 2019<\/strong>
\nThird team meeting:\u00a0October 29th to 31st, 2019<\/strong><\/p>\n
An extra 1-day meeting was held in St Andrews on June 10th, 2019<\/strong> before the 9th Coronal Loops Workshop<\/a><\/p>\n Presentations from the third meeting (October 2019):<\/strong><\/p>\n Agenda_3<\/a><\/p>\n <\/li>\n<\/ul>\n ————————————————————————————————————-<\/p>\n Presentations from the St Andrews meeting (June 2019):<\/strong><\/p>\n programme_issi_10June2019<\/a><\/p>\n Presentations from the second meeting (January 2019):<\/strong><\/p>\n Agenda_2<\/a><\/p>\n Day 1 –\u00a0Main variables affecting TNE cycles in the parameter space<\/strong><\/p>\n Day 2: Simulations and influence of the setup and modelling of the transition region\u00a0<\/strong>– Character of the thermal instability in TNE cycles (complete vs incomplete, detection of flows)<\/strong><\/p>\n Day 3: Coronal rain, magnetic field and heating mechanisms<\/strong><\/p>\n Day 4: Loop modelling, coronal rain and solar flares<\/strong><\/p>\n<\/div>\n<\/div>\n<\/div>\n ————————————————————————————————————–<\/p>\n Presentations from the first meeting (January 2018):<\/strong><\/p>\n Agenda<\/a><\/p>\n <\/p>\n I – Observations of evaporation-condensations in the solar atmosphere<\/strong><\/p>\n Main topics for the presentation and discussions : II – Numerical models<\/strong><\/p>\n Main topics for the presentation and discussions : <\/p>\n <\/p>\n","protected":false},"excerpt":{"rendered":" The team met three times at the International Space Science Institute in Bern, Switzerland. First team meeting:\u00a0January 22nd to 26th, 2018 Second team meeting: January 21st to 25th, 2019 Third team meeting:\u00a0October 29th to 31st, 2019 An extra 1-day meeting … Continue reading
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\n– Thermal non-equilibrium events (cycles) and coronal rain
\n– Study of flows associated with pulsations in loops
\n– Prominence connection
\n– Detection of EUV pulsations and coronal rain, what fraction of the coronal volume experiences these events?<\/p>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n\n
\n– 1D and multi-dimensional modeling
\n– Formation and dynamics of coronal rain
\n– Large scale simulations (active regions) of thermal non-equilibrium events<\/p>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n\n