Commit e9840441390d9b6b21beb4c0ffc28bca502420c7

Authored by Elena.Budnik
1 parent 88541f54

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NumericalData/AMDA/Cassini/MAG/cass-mag-jup.xml
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8 8 <AlternateName>high resolution MAG data during Jupiter flyby</AlternateName>
9 9 <ReleaseDate>2017-10-12T15:43:00</ReleaseDate>
10 10 <Description>High-resolution magnetic field data from the Cassini magnetometer during the Jupiter flyby obtained from NASA/PDS plasma node
11   - * J3 - J3 (IAU_JUPITER) is a Jovicentric cartesian coordinate system consistent with the IAU 1997 definition of the System 3 prime meridian.
12   - 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).
13   - * 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
14   - right handed set), and Z (the Jupiter dipole).
15   - * RTN - RTN coordinates consist of R (radial component, Sun to the spacecraft), T (tangential component, parallel to the Solar Equatorial plane and perpendicular
16   - to R), and N (normal component, completes right handed set).
  11 + * 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).
  12 + * 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).
  13 + * 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).
17 14 </Description>
18 15 <Contact>
19 16 <PersonID>spase://CDPP/Person/Michele.Dougherty</PersonID>
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