University of Kansas

Cassini Studies

A THREE-DIMENSIONAL MHD MODEL OF PLASMA FLOW AROUND TITAN:
A TOOL FOR CASSINI MISSION PLANNING

S. A. Ledvina, T. E. Cravens
Aaron Hoppe, and James Holliday

Dept. of Physics and Astronomy
University of Kansas, Lawrence, KS 66045 USA
phone 001-785-864-4739
e-mail cravens@ku.edu

Figures for Passes 1 - 5

Pass 1

Geometry A Geometry B
Magnetic Field Plasma Velocity
Density/Pressure/Temperature

Pass 2

Geometry A Geometry B
Magnetic Field Plasma Velocity
Density/Pressure/Temperature

Pass 3

Geometry A Geometry B
Magnetic Field Plasma Velocity
Density/Pressure/Temperature

Pass 4

Geometry A Geometry B
Magnetic Field Plasma Velocity
Density/Pressure/Temperature

Pass 5

Geometry A Geometry B
Magnetic Field Plasma Velocity
Density/Pressure/Temperature

Figures for passes 6-10

Return to A Tool for Cassini Mission Planning Main Page.
Return to Titan Studies Main Page.
Return to Space Physics Home Page.

Last modified February 9, 2004
Tizby Hunt-Ward
tizby@ku.edu