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A self‐consistent model of the Jovian auroral thermal structure
- D. Grodent, J. Waite, J. Gérard
- Physics
- 1 July 2001
A one-dimensional (1-D) model coupling a two-stream electron transport model of energy deposition with a 1-D thermal conduction model has been developed. It is applied to investigate the links…
Cassini Ion and Neutral Mass Spectrometer: Enceladus Plume Composition and Structure
TLDR
Abundant molecular oxygen in the coma of comet 67P/Churyumov–Gerasimenko
- A. Bieler, K. Altwegg, P. Wurz
- Geology, PhysicsNature
- 29 October 2015
TLDR
Magnetospheric energization by interaction between planetary spin and the solar wind
- J. Isbell, A. Dessler, J. Waite
- Physics, Geology
- 1 December 1984
If the solar wind is capable of driving magnetospheric convection, then solar-wind flow past any spinning, magnetized planet with a conducting ionosphere must cause the magnetic field lines in the…
Cassini finds molecular hydrogen in the Enceladus plume: Evidence for hydrothermal processes
TLDR
The ionosphere as a fully adequate source of plasma for the Earth's magnetosphere
- C. Chappell, T. Moore, J. Waite
- Physics
- 1 June 1987
A series of recent measurements of the outflow of ionization from the ionosphere have further heightened our awareness of the strength of the ionospheric source of magnetospheric plasmas. In this…
Molecular nitrogen in comet 67P/Churyumov-Gerasimenko indicates a low formation temperature
- M. Rubin, K. Altwegg, P. Wurz
- Physics, GeologyScience
- 10 April 2015
TLDR
Ion Neutral Mass Spectrometer Results from the First Flyby of Titan
- J. Waite, H. Niemann, K. Arnett
- Physics, Environmental ScienceScience
- 13 May 2005
The Cassini Ion Neutral Mass Spectrometer (INMS) has obtained the first in situ composition measurements of the neutral densities of molecular nitrogen, methane, molecular hydrogen, argon, and a host…
Jupiter's main auroral oval observed with HST-STIS
- D. Grodent, J. Clarke, Jihyun Kim, J. Waite, S. Cowley
- Physics
- 1 November 2003
[1] An extended series of FUV images obtained on 7 days during winter 2000–2001, with fixed pointing, yielded highly accurate tracking of emisson features as Jupiter rotated. They provided newly…
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