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  • NAM2019
    • Registration
    • Key Dates & Outline Schedule
    • Practical Information
    • Exhibitors
    • Grants & Bursaries
    • Contacts
  • Science
    • Science Programme
    • Parallel Sessions
    • Plenary Talks
    • Community Session
    • Special Lunches
    • Posters
    • Presenter Guidelines
  • Social
    • What's On
    • Welcome Reception
    • RAS Awards Dinner
  • Media
  • Outreach
    • Outreach and Education Day
    • Fringe Event
    • School Visit Day
  • Lancaster
    • Travel
    • Accommodation
    • Childcare
    • Campus Map
    • About Lancaster
    • Code of Conduct

Wednesday

Schedule

id
date time
PM2
16:12
Abstract
Polar Wind Outflow Model at Jupiter
Wednesday

Abstract details

id
Polar Wind Outflow Model at Jupiter
Date Submitted
2019-03-11 11:07:37
Carley
Martin
Lancaster University
Planetary Magnetospheres
Invited
C.J.Martin (Lancaster University), L.C.Ray (Lancaster University)
Polar wind is an important source of plasma in the magnetosphere at Earth, and it has been shown to be a contributor to the magnetospheric population at Saturn and Jupiter. We are developing a semi-kinetic, non-classical polar wind model for rapidly rotating systems to characterise the material escaping the upper atmosphere and the physical processes that dominate the escape, including evaluating with the auroral current systems. We present early results from the model and compare to in situ data at Jupiter and Saturn.

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