A Sensitivity Study of the Enceladus Torus
B. L. Fleshman, P. A. Delamere, F. Bagenal

TL;DR
This study models the Enceladus torus's physical chemistry, revealing key constraints on water input, electron energies, and transport timescales, with implications for ion composition and electron populations.
Contribution
It introduces a homogeneous model incorporating detailed electron and chemical processes, providing new constraints on the torus's physical parameters and dynamics.
Findings
Radial transport exceeds 12 days.
Water input rate is 100-180 kg/s.
Hot electrons have energies of 100-250 eV.
Abstract
We have developed a homogeneous model of physical chemistry to investigate the neutral-dominated, water-based Enceladus torus. Electrons are treated as the summation of two isotropic Maxwellian distributionsa thermal component and a hot component. The effects of electron impact, electron recombination, charge exchange, and photochemistry are included. The mass source is neutral HO, and a rigidly-corotating magnetosphere introduces energy via pickup of freshly-ionized neutrals. A small fraction of energy is also input by Coulomb collisions with a small population ( 1%) of supra-thermal electrons. Mass and energy are lost due to radial diffusion, escaping fast neutrals produced by charge exchange and recombination, and a small amount of radiative cooling. We explore a constrained parameter space spanned by water source rate, ion radial diffusion, hot-electron temperature, and…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
