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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

Poster

id
Electrodynamic heating of Jupiter’s GRS Thermosphere
Magnetospheres
Licia
Ray
Date Submitted
2019-03-15 17:09:02
Lancaster University
L.C. Ray (Lancaster University), C.T.S. Lorch (Lancaster University), J. O'Donoghue (NASA/GSFC), J.N. Yates (ESA/ESAC), S.V. Badman (Lancaster University), T.S. Stallard (Leicester University), C.G.A. Smith (Brooksbank School)
Recent observations of Jupiter's Great Red Spot indicate that the thermosphere above the storm is hotter than its surroundings by more than 700 K. Possible suggested sources for this heating have thus far included atmospheric gravity waves and lightning-driven acoustic waves. Joule heating, driven by Great Red Spot vorticity penetrating up into the lower stratosphere and coupling to the thermosphere, may contribute to the large observed temperatures. The strength of Joule heating will depend on the local inclination angle of the magnetic field and thus the observed emissions and inferred temperatures should vary with planetary longitude as the Great Red Spot tracks across the planet. We derive estimates for the Joule heating rate as a function of GRS longitude and discuss in the context of H3+ observations.

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