(Planetary Solar Ecliptic, Planet centered X=Sun, V2=Orbital normal) X - Along the Planet->Sun line (S), positive towards the Sun. Y - V2 x X Z - Parallel to the Planetary orbital plane upward normal. (Planetary Solar Equatorial, Planet centered Z=Omega, V2=Planet-Sun vector) X - In the Planet->Sun plane, positive towards the Sun. Y - Z x X Z - Northward spin axis of the Planet. KSM - This coordinate system will be similar to the GSM (Geocentric Solar Magnetospheric) coordinate system used at Earth. Because Saturn's rotation axis and magnetic dipole axis are < 1 degree different, we will not differentiate them when defining this coordinate system. X = S (where S is the unit vector from Saturn to the Sun) Y = K x X (where K is the unit vector of the rotation axis) Z = X x Y The geographic coordinate system is defined so that its x-axis is in the planet's equatorial plane, but is fixed with the rotation of the planet, so that it passes through the prime meridian. Its z-axis is parallel to the rotation axis of the planet, and its y-axis completes a right-handed orthogonal set. The centrifugal latitude ("CentLat") is computed using the method described in https://doi.org/10.1029/2020JA028713. PhiO (Satellite centered inertial Phi-Omega coordinates) [Co-rotational coordinate system] The X-direction is defined to be in the direction of corotation, at the center of the satellite (System III Phi direction [DESSLER1983]). The Z-axis is defined to be orthogonal to the X direction such that the X-Z plane contains the Jupiter spin axis (Omega), positive in the direction of angular momentum. The Y-axis is defined to complete the right-handed set. Since the major jovian satellites all lie very close to the jovian equatorial plane, it is often convenient to visualize this coordinate system as follows: X lies in the direction of plasma flow, Y points towards Jupiter, and Z points 'up'.