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VERSION:2.0
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BEGIN:VEVENT
DTSTAMP:20260523T133557Z
UID:https://www.mps.mpg.de/events/44097/7840847
DTSTART:20251127T100000Z
DTEND:20251127T110000Z
CLASS:PUBLIC
CREATED:20251206T145322Z
DESCRIPTION:During a solar flare\, fluxes in various lines and continua of 
 the solar spectrum increase\, causing enhanced ionisation in the illuminat
 ed part of the Earth’s ionosphere and an increase in the total electron 
 content (TEC). The dynamics of TEC driven by the impulsive phase of solar 
 flares have been studied extensively through both modelling and experiment
 al measurements. However\, the ionospheric effects of the late phase of so
 lar flares\, which occur in nearly half of X-class flares\, were discovere
 d only in 2024. This talk presents the results of the first multi-event st
 udy of the ionospheric response to the late phase of X-class solar flares.
  It also investigates how the flare’s location on the solar disk affects
  the ratio of ionospheric responses between the impulsive and late phases.
 \nSpeaker: Susanna Bekker
LAST-MODIFIED:20251206T145630Z
LOCATION:https://uio.zoom.us/j/63138938090
ORGANIZER;CN=Valeriia Liakh:mailto:
SUMMARY:ESPOS: ESPOS: Earth’s Ionospheric Response to the Impulsive and L
 ate Phases of Solar Flares (Susanna Bekker)
URL;VALUE=URI:https://www.mps.mpg.de/events/44097/7840847
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