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BEGIN:VEVENT
DTSTART;TZID=Atlantic/Canary:20231025T121500
DTEND;TZID=Atlantic/Canary:20231025T131500
UID:iactalks-1726
X-WR-CALNAME: IAC Talks: Open Astronomy Seminars
X-ORIGINAL-URL: /iactalks/Talks/view/1726
CREATED:2023-10-25T12:15:00+01:00
X-WR-CALDESC: IAC Talks upcomming talks
SUMMARY:High resolution observations of solar jets from the photosphere to 
 the corona.
DESCRIPTION:High resolution observations of solar jets from the photosphere
  to the corona.\nDrs. Reetika Joshi\n\nAbstract: Solar jets are ubiqu
 itous, sharp-edged collimated plasma ejections that are detected in all la
 yers of the Sun from the photosphere to the corona. Observed as impulsive 
 events, jets can originate in all kinds of solar environments, from active
  regions to the quiet Sun. Occasionally, these jets interact with large sc
 ale solar filaments and can set them into oscillation, sometimes followed 
 by instability and eruption. I will present high spatial, temporal, and sp
 ectral resolution observational studies of jets to probe the fundamental p
 hysical process behind them and integrate these observations with theoreti
 cal models. We use the coordinated observations from space-borne (SDO, IRI
 S) and ground-based (SST) telescopes. Space-borne telescopes provide the E
 UV/UV data for the outer atmosphere of the sun (chromosphere, transition r
 egion and corona), while ground-based telescopes give access to high resol
 ution data for the inner solar atmosphere (lower chromosphere, photosphere
 ) through H-alpha, Ca II, and Fe I lines. In this way, coordinated observa
 tions cover the solar atmosphere in multi-wavelength range from the photos
 phere to the corona through the chromosphere and transition region.\nZoom 
 link: https://rediris.zoom.us/j/82374881929?pwd=ZEVPNzg5SklqamN2WDRoVGNraW
 Nndz09Meeting ID: 823 7488 1929\nPasscode: 994281
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