Ions and electrons from the solar wind plasma, a local pick-up
ion
plasma
or a plasma trapped in a planetary magnetosphere can
impinge
on an atmosphere. This can cause heating of the thermo-
sphere
and loss of atmosphere. To describe this quantitatively elastic
and
inelastic
collision cross sections are needed. Since in many cases
these
are not measured we carry out semi-classical or classical
molecular
dynamics calculations to the required cross sections.
CHARGE
EXCHANGE CROSS SECTION DATA
Relevent
Calculations:
Johnson, R. E., and Strobel, D. F., "Charge Exchange in the Io Torus and
Exosphere," J. Geophys. Res., 87 (1982), p. 385.
McGrath,
M. A., and Johnson, R. E., "Charge Exchange Cross Sections for
the Io's Plasma Torus," J. Geophys. Res. 94 (1989) p. 2677-2683.
Johnson,
R.E. "Formation of Na-containing Molecular Ions at Io"
Icarus 111 (1994) p.65-72.
Luna,
H., M. Michael, M.B. Shah, R.E. Johnson, C.J. Latimer, and
J.W. McConkey, "Dissociation of N2 in capture and ionization collisions
with fast H+ and N+ ions and modeling of positive ion formation in the
Titan atmosphere" JGR 108, NO E4, 5033,
doi:10.1029/2002JE001950
(2003). (PDF)
Johnson,
R.E. and M. Liu, Sputtering of the atmosphere of Mars,
1. Collisional dissociation of CO2,
Geophys. Res. 103 (1998) 3639-3647.
Johnson,
R.E., M. Liu and C. Tully, Collisional Dissociation Cross
Section for O + O2, CO and N2 and N + N2.
Planet
& Space Sci. 50(1) 123-128 (2002). (pdf)
Tully,
C. and R.E.Johnson, "Low Energy Collisions Between Ground
State Oxygen Atoms",
Planet & Space Sci. 49(6) (2001) 533-537.
Tully, C. and
R.E.Johnson,
"Semiclassical calculation of collisional
dissociation cross section for N+N2"
J. Chem. Phys. 117 (2002) 6556-6561.
(pdf)
Tully, C., R.E. Johnson, "Erratum :
'Semiclassical
calculation of collisional
dissociation cross section for N+N2' [ J. Chem. Phys. 117, 6556
(2002)]",
J. Chem. Phys. 119, 10452-10453 (2003) . (PDF)