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BEGIN:VEVENT
DTSTAMP:20260428T040158Z
DTSTART;VALUE=DATE-TIME:20220307T150000
DTEND;VALUE=DATE-TIME:20220307T160000
SUMMARY:Ali Sulaiman (University of Iowa): The Gas Giants as Unique Labor
 atories for Space Plasma Processes
TZID:Europe/London
UID:20220307-8a17841b7e442832017e489ffac1523d@warwick.ac.uk
CREATED:20220228T114014Z
DESCRIPTION:Abstract: Jupiter and Saturn’s internal magnetic fields carve
  out a cavity in the solar wind (and its embedded interplanetary magneti
 c field) to form two of the largest magnetospheres in our solar system. 
 Their locations in the heliosphere are characterized by vastly different
  solar wind conditions than are available at Earth\, thus affording\, fo
 r example\, the exploration of some of the highest Mach number shocks ev
 er recorded in situ. In addition to their external interactions with the
  solar wind\, they have geologically active moons continuously loading p
 lasmas into their magnetospheres: Io’s volcanoes at Jupiter and Enceladu
 s’ geysers at Saturn. These internally sourced plasmas interact with the
  surrounding planetary magnetic fields\, giving rise to mechanisms that 
 ultimately control the magnetospheres’ states and drive their dynamics. 
 Furthermore\, our evolving understanding of Saturn’s rings is revealing 
 their influence in this context as well. In 2016\, NASA’s Juno spacecraf
 t undertook the first polar orbit of Jupiter\, and in 2017\, NASA/ESA’s 
 Cassini spacecraft performed its final orbit\, which were highly incline
 d and adjusted to pass through the gap between Saturn’s atmosphere and i
 nnermost ring\; both providing unprecedented coverage and proximity to t
 heir planets. These highly inclined\, proximal orbits enable the spacecr
 aft to directly sample the ionospheres and traverse magnetic field lines
  threading the auroral regions\, as well as those connecting the planets
  to their active moons and ring systems (for Saturn\, at least). Such me
 asurements are essential to understanding coupling processes and establi
 shing the big picture of these planetary systems operate on a global sca
 le. Altogether\, these place Jupiter and Saturn each in unique points in
  the parameter landscape of both solar wind and satellite interactions w
 ith planetary magnetospheres. I will highlight recent observations that 
 provide a new view of the gas giants and underline them\, to our current
  understanding\, as the most dynamic and diverse environments in our sol
 ar system.
LOCATION:
CATEGORIES:CFSA Seminar
LAST-MODIFIED:20220228T114014Z
ORGANIZER;CN=Anne-Marie Broomhall:
END:VEVENT
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