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SUMMARY:Konstantin Kim (IRF Uppsala): Dynamic processes in Titan's plasma 
 environment (pre-defence seminar)
DTSTART:20260604T120000Z
DTEND:20260604T130000Z
DTSTAMP:20260719T223700Z
UID:indico-event-2058@indico.uu.se
DESCRIPTION:Title: Dynamic processes in Titan's plasma environmentSpeaker
 : Konstantin KimAffiliation: IRF UppsalaRoom: Å2001 Time: 14:00-15:0
 0Abstract:Titan is the only moon with a dense atmosphere and has a dynamic
  plasma environment\, standing out among all moons of the Solar System. Th
 e interaction between Saturn's magnetosphere and Titan's dense atmosphere 
 leads to the formation of the interface between the two environments\, the
  induced magnetospheric boundary (IMB). In this seminar\, the overall and 
 local structure and processes shaping this region are presented. The measu
 rements of the magnetic field and plasma parameters from a total of 126 Ti
 tan flybys by Cassini-Huygens (orbiting Saturn from 2004 to 2017) are used
  to determine the overall electromagnetic and plasma structure of the IMB 
 and the outflow region. We found that the IMB consists of localized curren
 t sheets and that the magnetotail forms an Alfvén wing structure as a res
 ult of the interaction. In addition\, it is shown that low-frequency waves
  may contribute to the energy dispersion of ionospheric electrons when Tit
 an is near Saturn's magnetopause. The results also reveal that the IMB of 
 Titan exhibits an asymmetry driven by the gyromotion of pickup ions follow
 ing the convective electric field.  \n\nhttps://indico.uu.se/event/2058/
LOCATION:Å2001
URL:https://indico.uu.se/event/2058/
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