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VERSION:2.0
PRODID:icalendar-ruby
CALSCALE:GREGORIAN
METHOD:PUBLISH
BEGIN:VEVENT
DTSTAMP:20260522T005001Z
UID:https://www.mps.mpg.de/events/45012/7840847
DTSTART:20260312T100000Z
DTEND:20260312T110000Z
CLASS:PUBLIC
CREATED:20260308T133849Z
DESCRIPTION:This work takes advantage of new observational data collected b
 y the High-resolution Coronal Imager (Hi-C) at the highest spatial and tem
 poral resolutions available. This most recent Hi-C dataset is the first to
  make use of the hot 129 Å channel and the first to consist of targeted o
 bservations of a solar flare\, rather than the quiescent corona. Images fr
 om Hi-C are analysed and compared with complementary EUV observations from
  SDO/AIA. The widths of the loop strands are measured\, and the resulting 
 populations analysed. Preliminary results suggest the majority of loop str
 ands have a width in the range 500-2\,000 km\, but there is some variation
  in the loop strand widths observed in plasma at different temperatures. T
 here is some evidence that there are smaller structures present which are 
 partially resolved by Hi-C\, with the very smallest smallest loop strands 
 of a similar order of magnitude to the spatial resolution of the Hi-C imag
 es. Further results will be presented\, as well as a discussion of future 
 work\, investigating individual events within the Hi-C observations\, maki
 ng use of the high cadence available to track the dynamic behaviour of the
  corona.\nSpeaker: Anna Rankin
LAST-MODIFIED:20260308T134021Z
LOCATION:https://uio.zoom.us/j/63138938090
ORGANIZER;CN=Valeriia Liakh:mailto:
SUMMARY:ESPOS: ESPOS: Exploring small-scale coronal loop structures using u
 ltra high resolution observations from the latest Hi-C sounding rocket cam
 paign (Anna Rankin)
URL;VALUE=URI:https://www.mps.mpg.de/events/45012/7840847
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