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VERSION:2.0
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BEGIN:VEVENT
DTSTAMP:20260524T093424Z
UID:https://www.mps.mpg.de/events/43903/7840847
DTSTART:20251211T100000Z
DTEND:20251211T110000Z
CLASS:PUBLIC
CREATED:20251120T191040Z
DESCRIPTION: On 26 September 2022\, we observed a quiescent solar prominenc
 e with Hα imaging spectroscopy using the Solar Dynamics Doppler Imager (S
 DDI) on the SMART telescope. Unlike earlier works that detected 4- and 15-
 min oscillations through long-slit\, 1D wavelet methods\, we adapt the wav
 elet analysis to 3D data to explore the full prominence structure. Complem
 entary data from SDO/AIA (304 Å\, 171 Å) STEREO-A/EUVI (304 Å)\, and So
 lar Orbiter EUI/FSI (304 Å\, 174 Å) enable a multi-view\, multi-thermal 
 investigation of wave periodicity across the prominence. Our aim is to cha
 racterize how oscillatory periods are distributed in plasma at different t
 emperatures and viewing angles\, thereby assessing wave propagation and va
 riability throughout the prominence body.\nSpeaker: Aneta Wiśniewska
LAST-MODIFIED:20251206T150246Z
LOCATION:https://uio.zoom.us/j/63138938090
ORGANIZER;CN=Valeriia Liakh:mailto:
SUMMARY:ESPOS: ESPOS: Wave Period Variability in a Quiescent Solar Prominen
 ce (Aneta Wiśniewska) 
URL;VALUE=URI:https://www.mps.mpg.de/events/43903/7840847
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