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
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