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Outer planet moon - magnetosphere interaction workshop

5–6 Nov 2020
Europe/Amsterdam timezone

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Session

Oral presentations

5 Nov 2020, 14:00

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  1. 58. Invited presentation: The variable energetic charged particle environment of outer planet moons
    Elias Roussos (Max Planck Institute for Solar System Research)
    05/11/2020, 14:00
    Oral
  2. 59. Effects of Titan's magnetospheric environment on its atmosphere
    Leonardo Regoli (Johns Hopkins University Applied Physics Laboratory)
    05/11/2020, 14:20
    Oral
  3. 60. Ambient magnetic and plasma conditions at moon orbits
    Nicholas Achilleos (UCL)
    05/11/2020, 14:40
    Oral
  4. 61. Modelling of Energy-Transfer Processes at Ganymede’s Upstream Magnetopause
    Nawapat Kaweeyanun (Imperial College London)
    05/11/2020, 15:00
    Oral
  5. 62. Io plasma torus and Jovian aurora activities seen by Hisaki: Recent result, current status, and future plan
    Fuminori Tsuchiya (Graduate school of Science, Tohoku University)
    05/11/2020, 15:20
    Poster
  6. 67. Invited presentation: Variability of the Galilean moon plasma environment and implications for moon-magnetosphere interactions
    Fran Bagenal (University of Colorado, Boulder, CO USA)
    05/11/2020, 17:20
    Oral
  7. 68. The Io and Europa plasma tori as potential ultra-low-frequency resonators
    Harry Manners (Imperial College London)
    05/11/2020, 17:40
    Oral
  8. 69. The Io-torus interaction as seen through a telescope
    Carl Schmidt (Boston University)
    05/11/2020, 18:00
    Oral
  9. 70. Determining the Io volcanic source with Hisaki neutral oxygen observations and 3D modeling
    Howard Smith (JHU APL)
    05/11/2020, 18:20
    Oral
  10. 71. Plasma flow around a satellite with an ionosphere: Theoretical models of the moon-magnetosphere interaction
    Frank Crary (University of Colorado, LASP)
    05/11/2020, 18:40
    Oral
  11. 76. Pickup ions in the outer solar system
    Andrew Coates (UCL Mullard Space Science Laboratory)
    05/11/2020, 19:00
    Oral
  12. 91. Low-energy electrons in Saturn’s inner magnetosphere from the Cassini Langmuir Probe
    George Xystouris (Lancaster University)
    06/11/2020, 14:00
    Oral
  13. 92. The Langmuir probe observations of the dust and plasma at Enceladus plume and the E-ring
    Michiko Morooka (Swedish Institute of Space Physics)
    06/11/2020, 14:20
    Oral
  14. 93. Fast and Slow Water Ion Populations in the Enceladus Plume
    Richard Haythornthwaite (University College London)
    06/11/2020, 14:40
    Oral
  15. 95. Remote Detection of Surface Charging at Saturn’s Icy Moons
    Geraint Jones (UCL Mullard Space Science Laboratory)
    06/11/2020, 15:00
    Oral
  16. 85. Invited presentation: Moon-magnetosphere interactions of Io and Enceladus: A high-resolution, in-situ parametric study
    Ali Sulaiman (University of Iowa)
    06/11/2020, 15:30
    Oral
  17. 86. Moon-induced auroral radio emission in the outer solar system
    Corentin Louis (IRAP - Toulouse)
    06/11/2020, 15:50
    Oral
  18. 87. Triton Plasma Interactions
    Mats Holmstrom (Swedish Institute of Space Physics)
    06/11/2020, 16:10
    Oral
  19. 89. Investigating the energy inputs to Triton’s enigmatic ionosphere
    Tom Nordheim (NASA JPL)
    06/11/2020, 16:30
  20. 100. Invited presentation: Connecting the Galileo particle, plasma, and field data with ionospheric, exospheric, and MHD models
    Marina Galand (Imperial College London)
    06/11/2020, 18:00
    Oral
  21. 101. Detectability of subsurface oceans and their flows by JUICE
    Ingo Mueller-Wodarg (Imperial College London)
    06/11/2020, 18:20
    Oral
  22. 102. Investigating the origin of sulfur-bearing species on the Galilean moon Callisto
    Richard Cartwright (Carl Sagan Center at the SETI Institute)
    06/11/2020, 18:40
    Oral
  23. 103. Interaction of plasma with the surface of icy moons: insights from laboratory experiments
    André Galli (University of Bern)
    06/11/2020, 19:00
    Oral
  24. 46. Determining the Io volcanic source with Hisaki neutral oxygen observations and 3D modeling
    Howard Smith (JHU APL)
    Oral

    The Jovian system is very intriguing with extremely different particle sources ranging from the volcanic Io to the frozen world of Europa with both existing within Jupiter’s relatively high radiation magnetospheric environment. While Voyager, Galileo and Cassini provided historic observations of this unique environment, they also raised numerous questions. As the dominant source of particles...

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  25. 49. Pickup ions in the outer solar system
    Prof. Andrew Coates (UCL Mullard Space Science Laboratory)
    Oral

    Ion pickup provides the key mechanism by which comets interact with the solar wind. Following ionization of neutral particles, the new-born ions are accelerated in the convection electric field and gyrate around the magnetic field – forming a cycloid in real space and an unstable ring in velocity space. Pickup is present at most other planetary objects, and in the outer solar system there are...

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  26. 39. Plasma flow around a satellite with an ionosphere: Theoretical models of the moon-magnetosphere interaction
    Frank Crary (University of Colorado, LASP)
    Oral

    Key aspect of moon-magnetosphere interactions are dependent on the diversion of the flow around the conducting body of the moon and the acceleration of the flow along the flanks of the moon. Analytic solutions for the magnetic field perturbations [Neubauer, 1980; Saur et al., 2004 and references therein] have been derived assuming the moon’s conductance is constant within a specified radius...

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  27. 13. The Io and Europa Plasma Tori as Potential Ultra-Low-Frequency Resonators
    Harry Manners (Imperial College London)
    Oral

    The plasma torus at Io’s orbit has been shown to be a locus of intense Alfvén and ion cyclotron waves, which are trapped in the region by the waveguide properties of the torus. Research featuring these waves has progressed towards a detailed understanding of temporal variability in the region, which is vital to the upcoming JUICE mission’s aim to characterise the Galilean moons. Here we show...

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  28. 24. The Io-Torus Interaction as Seen Through a Telescope
    Dr Carl Schmidt (Boston University)
    Oral

    The Io plasma torus offers our only opportunity to take a picture of a planetary magnetosphere. Torus ion emissions are excited through electron impact and so line ratios of like ions species can effectively map the plasma density and electron temperature. This provides us with some empirical constraints on the upstream plasma conditions that sweep past the moon. A rich spectrum of emission...

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