BEGIN:VCALENDAR
VERSION:2.0
PRODID:icalendar-ruby
CALSCALE:GREGORIAN
METHOD:PUBLISH
BEGIN:VEVENT
DTSTAMP:20260524T024542Z
UID:https://www.mps.mpg.de/events/42213/7840847
DTSTART:20250619T090000Z
DTEND:20250619T100000Z
CLASS:PUBLIC
CREATED:20250613T062958Z
DESCRIPTION: With the increase of space EUV observations (SoHO\, SDO\, Sola
 r Orbiter and soon the Vigil mission)\, this diagnostic has become an esse
 ntial tool to bridge the gap between models and our current understanding 
 of coronal phenomena. We will present a review of the recent studies using
  the Wind Predict model and its different versions\, which is a 3-dimensio
 n magnetohydrodynamic code to model the solar chromosphere\, corona and th
 e expansion of the solar wind. We will in particular discuss the influence
  of observations on the simulation results (with the question of spatial r
 esolution\, as well as the inclusion of far-side active regions observed b
 y Solar Orbiter)\, and vice-versa how the generation of synthetic data can
  help us improve our simulations (with the implementation of a feedback lo
 op based on automated coronal hole detection). Finally\, we will present t
 he next developments foreseen for the Wind Predict code.\nSpeaker: Barbara
  Perri
LAST-MODIFIED:20250613T063119Z
LOCATION:https://zoom.us/j/165498165
ORGANIZER;CN=Shahin Jafarzadeh:mailto:
SUMMARY:ESPOS: ESPOS: Wind Predict: Modeling the solar corona and its EUV e
 mission (Barbara Perri)
URL;VALUE=URI:https://www.mps.mpg.de/events/42213/7840847
END:VEVENT
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