Animations

The 4 movies below are made from a model based on Voyager 1 PLS data. They were presented by Parker Hinton on the NASA Hyperwall exhibit at AGU 2017. See references

	Voyager 1 trajectory through the magnetic field of Jupiter by Parker Hinton These animated field lines were generated with a simple tilted dipole magnetic field model. The view is in a cylindrical coordinate system. (View Movie)
	Voyager 1 trajectory projected along magnetic field lines by Parker Hinton These animated field lines were generated with the VIP4 + Connerney current sheet model. The Voyager 1 trajectory is shown in pink and is traced along the magnetic field to the magnetic equator (white) and the centrifugal equator (blue). (View Movie)
	Contours of electron density in the Io Plasma Torus at 4 System III longitudes by Parker Hinton The contours of electron density are based on the Voyager PLS data extrapolated along magnetic field lines and assuming azimuthal symmetry. The 4 longitudes correspond to locations where the equators cross and where there is maximum tilt. (View Movie)
	Full 3-D torus animation by Parker Hinton Assuming azimuthal symmetry, the contours of electron density in the Io Plasma Torus are wrapped around Jupiter. Io and Europa trajectories are shown with appropriate distances and period – but random timing. (View Movie)

The 3 movies below are made in the (non-rotating) coordinate frame that is centered on Jupiter with X towards the Sun, Z is Jupiter’s spin axis.

Field Lines – Equatorial Slice
by Adam Shinn

These animated field lines were generated with Krishan Khurana’s magnetic field model in fortran. The dashed lines represent the field lines that hit the magnetopause boundary. The movie runs through two rotations of Jupiter.

(View movie)