BEGIN:VCALENDAR
VERSION:2.0
PRODID:icalendar-ruby
CALSCALE:GREGORIAN
METHOD:PUBLISH
BEGIN:VEVENT
DTSTAMP:20260524T111821Z
UID:https://www.mps.mpg.de/events/43619/7840847
DTSTART:20251030T100000Z
DTEND:20251030T110000Z
CLASS:PUBLIC
CREATED:20251023T192614Z
DESCRIPTION: In July 2024\, Sunrise III flew from Sweden to Canada at strat
 ospheric heights capturing high resolution diffraction-limited images of t
 he Sun for 6.5 days. The telescope carried three scientific instruments ea
 ch complementing the other by observing in different parts of the solar sp
 ectrum from the near-ultraviolet by SUSI (309 nm - 417 nm)\, the visible b
 y TuMag (517 nm - 525 nm) to the near infrared by SCIP (765 nm - 855 nm). 
 During its flight\, Sunrise III observed a wide variety of features on the
  Sun including the quiet region\, sunspots\, plages\, filaments\, spicules
 \, flux emergence\, and also flares. By combining the data from the three 
 instruments\, it is possible to infer and understand various properties of
  the solar atmosphere from the photosphere to the upper chromosphere. In t
 his talk\, I will walk you through the Sunrise III journey\, the science p
 lanning\, present observational highlights and provide a glimpse into some
  of the exciting ongoing scientific analysis from the Sunrise III data.\nS
 peaker: Smitha Narayanamurthy
LAST-MODIFIED:20251023T192847Z
LOCATION:https://uio.zoom.us/j/63138938090
ORGANIZER;CN=Valeriia Liakh:mailto:
SUMMARY:ESPOS: ESPOS: Sunrise III Flight and Early Science Highlights (Smit
 ha Narayanamurthy)
URL;VALUE=URI:https://www.mps.mpg.de/events/43619/7840847
END:VEVENT
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