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  • NAM2017
    • Timetable
    • Delegates
    • Registration
  • Science
    • Parallel sessions
    • Plenary talks
    • Posters
    • Publishing workshop
    • Media workshop
    • Community forum
    • Special lunches
    • Hack day
  • Social
    • Welcome reception
    • Conference dinner
    • Football + BBQ evening
  • Outreach
    • Public talk
    • Outreach day
    • Media
  • Hull
    • Travel
    • Accommodation
    • Going out
    • Childcare
  • Contacts

Schedule by Session

Abstract

id
Generation and evolution of Solar and Stellar Magnetic Fields, and Implications for the Solar-Stellar Connection
Magnetism in hot Jupiter Atmospheres
Date Submitted
2017-04-21 04:07:22
Tamara Rogers
Jim McElwaine
Newcastle University
In this presentation I will discuss how a dynamo can be driven in the thin stably-stratified atmosphere of a hot Jupiter. This dynamo is driven by horizontal conductivity variations arising from the constant day-night temperature differential. While the hot Jupiter case is extreme, due to its strong asymmetry, its possible a variable conductivity could lead to interesting, unexplored dynamics in other MHD systems.

Schedule

id
Monday
date time
16:30 - 18:00
16:56
Abstract
Magnetism in hot Jupiter Atmospheres
Wilberforce LT-1

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