EGU24-6867, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-6867
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Io Torus Electron Densities inward of Io's M-shell

William Kurth1, George Hospodarsky1, Jeremy Faden1, John Douglas Menietti1, Ali Sulaiman2, Sadie Elliott2, John E.P. Connerney3, Frederic Allegrini4, and Scott Bolton4
William Kurth et al.
  • 1University of Iowa, Dept. of Physics and Astronomy, Iowa City, Iowa 52242
  • 2University of Minnesota, School of Physics & Astronomy, Minneapolis, Minnesota 55455
  • 3NASA/Goddard Space Flight Center, Greenbelt, Maryland, 20771
  • 4Southwest Research Institute, San Antonio, Texas 78238

Various characteristic frequencies observed in the plasma wave spectrum inward of Io have revealed a durable electron density profile that includes a localized relative maximum near M = 4.8 with a local minimum between this and the much greater densities closer to Io.  Scale heights relative to the centrifugal equator are of order one Jovian radius, thought to be too large for a cold heavy ion population leading to the conclusion that protons are likely responsible for the large scale height.  In this paper we show evidence of the low-frequency cutoff of the z-mode at the L=0 frequency, a polarization change at the local electron plasma frequency and low-frequency cutoff of ordinary mode waves.  The determination of the electron plasma frequency and electron cyclotron frequency from the measured magnetic field strength also allow the calculation of the upper hybrid resonance frequency and R=0 cutoff of the extraordinary mode.  Often, all of these spectral features can be found in the Juno plasma wave spectra obtained in the inner Io torus.

How to cite: Kurth, W., Hospodarsky, G., Faden, J., Menietti, J. D., Sulaiman, A., Elliott, S., Connerney, J. E. P., Allegrini, F., and Bolton, S.: Io Torus Electron Densities inward of Io's M-shell, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-6867, https://doi.org/10.5194/egusphere-egu24-6867, 2024.