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VERSION:2.0
PRODID:icalendar-ruby
CALSCALE:GREGORIAN
METHOD:PUBLISH
BEGIN:VEVENT
DTSTAMP:20260411T172625Z
UID:https://www.mps.mpg.de/events/28447/7840830
DTSTART:20210603T090000Z
DTEND:20210603T100000Z
CLASS:PUBLIC
CREATED:20210602T133815Z
DESCRIPTION:The Mg I b2 line at 5173 Å forms over a large range of heights
  but itscore\, which forms under conditions of non-local thermodynamicequi
 librium\, is most sensitive to heights near the temperature minimum\,a reg
 ion of the solar atmosphere that has not been sufficientlyexplored. The ne
 xt-generation solar observatories will have access tothis spectral line an
 d will allow for multi-line observations to studythe different layers of t
 he solar atmosphere simultaneously and withunprecedented polarimetric sens
 itivity. We will present a morphologicalclassification of the intensity an
 d circular polarization profiles ofthis spectral line at high-spatial-reso
 lution\, using observations fromthe Swedish 1-m Solar Telescope. We will a
 lso discuss the results of theweak field approximation applied to the Mg I
  b2 line\, and theircomparison with inversion results of the Fe I 6173 Å 
 line to understandhow the magnetic field changes with height in the solar 
 atmosphere.\nVortragende(r): Azaymi Litzi Siu Tapia 
LAST-MODIFIED:20260219T095205Z
LOCATION:Max-Planck-Institut für Sonnensystemforschung\, Raum: Zoom
ORGANIZER;CN=Pradeep Chitta:mailto:
SUMMARY:ESPOS: ESPOS Online Seminar: The solar atmosphere as observed throu
 gh the Mg I b2 line at highspatial resolution (Azaymi Litzi Siu Tapia)
URL;VALUE=URI:https://www.mps.mpg.de/events/28447/7840830
END:VEVENT
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