diff --git a/NumericalData/AMDA/Cassini/MAG/cass-mag-jup.xml b/NumericalData/AMDA/Cassini/MAG/cass-mag-jup.xml index df5fe59..ddc4e3e 100644 --- a/NumericalData/AMDA/Cassini/MAG/cass-mag-jup.xml +++ b/NumericalData/AMDA/Cassini/MAG/cass-mag-jup.xml @@ -8,12 +8,9 @@ high resolution MAG data during Jupiter flyby 2017-10-12T15:43:00 High-resolution magnetic field data from the Cassini magnetometer during the Jupiter flyby obtained from NASA/PDS plasma node - * J3 - J3 (IAU_JUPITER) is a Jovicentric cartesian coordinate system consistent with the IAU 1997 definition of the System 3 prime meridian. - It consists of X (in Jovian equatorial plane, along S3 1997 prime meridian), Y (completes right handed set), and Z (parallel to the Jovian spin axis). - * JMXYZ - JMAG XYZ is a Jovicentric cartesian coordinate system which consists of X (in the plane containing Z and the S3 1997 Prime Meridian), Y (completes - right handed set), and Z (the Jupiter dipole). - * RTN - RTN coordinates consist of R (radial component, Sun to the spacecraft), T (tangential component, parallel to the Solar Equatorial plane and perpendicular - to R), and N (normal component, completes right handed set). + * J3 - J3 (IAU_JUPITER) is a Jovicentric cartesian coordinate system consistent with the IAU 1997 definition of the System 3 prime meridian. It consists of X (in Jovian equatorial plane, along S3 1997 prime meridian), Y (completes right handed set), and Z (parallel to the Jovian spin axis). + * JMXYZ - JMAG XYZ is a Jovicentric cartesian coordinate system which consists of X (in the plane containing Z and the S3 1997 Prime Meridian), Y (completes right handed set), and Z (the Jupiter dipole). + * RTN - RTN coordinates consist of R (radial component, Sun to the spacecraft), T (tangential component, parallel to the Solar Equatorial plane and perpendicular to R), and N (normal component, completes right handed set). spase://CDPP/Person/Michele.Dougherty -- libgit2 0.21.2