Europlanet Science Congress 2020
Virtual meeting
21 September – 9 October 2020
Europlanet Science Congress 2020
Virtual meeting
21 September – 9 October 2020
EPSC Abstracts
Vol.14, EPSC2020-496, 2020
https://doi.org/10.5194/epsc2020-496
Europlanet Science Congress 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

The plasma/atmosphere interaction at Io: revisiting the ion/neutral charge-exchange cross-sections and their ion-velocity dependency

Vincent Dols1, Robert Johnson2, and Fran Bagenal1
Vincent Dols et al.
  • 1LASP Colorado University Boulder, Colorado, USA (vincent.dols@lasp.colorado.edu)
  • 2Department of Materials Science and Engineering, University of Virginia, Charlottesville, Virginia, USA (rej@virginia.edu)

The Io Torus plasma is mostly composed of singly and multi-charged S and O ions. These ions interact with the neutrals of Io’s atmosphere (S, O, SO2 and SO) through symmetrical (i.e. O+ + O => O + O+) and asymmetrical (i.e. S++ + O => S + O++) charge-exchanges. Charge-exchange cross-sections were estimated in Johnson & Strobel, 1982 and McGrath & Johnson, 1989 at 60 km/s (the plasma corotation velocity in Io’s frame), and are used in numerical simulations of the torus/neutral cloud interaction (i.e. Delamere and Bagenal, 2003).

Dols et al., 2008 proposed numerical simulations of the multi-species chemistry interaction at Io using these cross-sections at 60 km/s. The plasma/atmosphere interaction at Io is strong and the flow velocity and ion temperature are drastically reduced close to Io (v < 10 km/s). Thus, velocity-dependent charge-exchange cross-sections are critical for such numerical simulations and their effect on the local plasma and neutral supply at Io should be explored.

We propose to revisit the calculation of ion/neutral charge-exchange cross-sections following Johnson & Strobel, 1982’s approach for plasma velocities relevant to the local interaction at Io (V=10-120 km/s). More sophisticated calculations were proposed in McGrath & Johnson, 1989 but both publications offered very few details about their procedure.

We will illustrate the effect of using velocity-depend charge-exchange cross-sections in numerical simulations of the multi-species plasma/atmosphere interaction at Io.

More generally, this presentation aimed at providing an incentive for the community to expand the work of McGrath & Johnson, 1989.

 

Johnson & Strobel, Charge-exchange in the Io torus and exosphere, JGR, 87,1982

McGrath & Johnson, Charge exchange cross sections for the Io plasma torus, JGR, 94, 1989

Delamere & Bagenal, Modeling variability of plasma conditions in the Io torus, JGR, 108, 2003

Dols, Delamere, Bagenal, Kurth, Paterson, A multi-species chemistry model of Io’s local interaction with the plasma torus, JGR, 113, 2008

How to cite: Dols, V., Johnson, R., and Bagenal, F.: The plasma/atmosphere interaction at Io: revisiting the ion/neutral charge-exchange cross-sections and their ion-velocity dependency, Europlanet Science Congress 2020, online, 21 September–9 Oct 2020, EPSC2020-496, https://doi.org/10.5194/epsc2020-496, 2020