From 88541f54d2b9813d109aa6fd8f307f1aa76de77b Mon Sep 17 00:00:00 2001 From: Elena.Budnik Date: Fri, 23 Aug 2019 11:42:50 +0200 Subject: [PATCH] cass mag jup --- NumericalData/AMDA/Cassini/MAG/cass-mag-jup.xml | 80 +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++------- 1 file changed, 73 insertions(+), 7 deletions(-) diff --git a/NumericalData/AMDA/Cassini/MAG/cass-mag-jup.xml b/NumericalData/AMDA/Cassini/MAG/cass-mag-jup.xml index acf5587..df5fe59 100644 --- a/NumericalData/AMDA/Cassini/MAG/cass-mag-jup.xml +++ b/NumericalData/AMDA/Cassini/MAG/cass-mag-jup.xml @@ -7,7 +7,14 @@ flyby jupiter 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 in RTN coordinates obtained from NASA/PDS plasma node + 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). + spase://CDPP/Person/Michele.Dougherty PrincipalInvestigator @@ -28,7 +35,7 @@ NetCDF PDS - CO-E_SW_J_S-MAG-3-RDR-FULL-RES-V1.0 + CO-E_SW_J_S-MAG-3-RDR-FULL-RES-V2.0 spase://CDPP/Instrument/AMDA/Cassini/MAG MagneticField @@ -40,16 +47,75 @@ PT8S Jupiter - Interstellar - Jupiter.Ganymede - Jupiter.Io - Jupiter.Callisto - Jupiter.Europa These data contain persistent noise signals at 0.2, 8, 16 Hz, and associated harmonics. This noise was not observed during ground testing of the instruments and is anticipated to be interference arising from the spacecraft. Removal of these signals is at the user's discretion. + b_j3 + cass_bj3_jup + Magnetic field vector components in Jup_IAU coordinates + phys.magField + nT + + TimeSeries + + + 3 + + bx + 1 + cass_bj3_jup(0) + + + by + 2 + cass_bj3_jup(1) + + + bz + 3 + cass_bj3_jup(2) + + + + Vector + Magnetic + + + + b_jm + cass_bjm_jup + Magnetic field vector components in JMAG coordinates + phys.magField + nT + + TimeSeries + + + 3 + + bx + 1 + cass_bjm_jup(0) + + + by + 2 + cass_bjm_jup(1) + + + bz + 3 + cass_bjm_jup(2) + + + + Vector + Magnetic + + + b_rtn cass_b_jup Magnetic field vector components in RTN coordinates -- libgit2 0.21.2