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 6 - 10

Pass 6

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

Pass 7

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

Pass 8

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

Pass 9

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

Pass 10

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

Figures for passes 11-15

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