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Cassini - MAG - flyby jupiter

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/Cassini/MAG/cass-mag-jup

Description
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).

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Details

Version:2.4.1

NumericalData

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/Cassini/MAG/cass-mag-jup
ResourceHeader
ResourceName
Cassini - MAG - flyby jupiter
AlternateName
high resolution MAG data during Jupiter flyby
ReleaseDate
2019-08-23 12:50:36Z
Description
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).
Contacts
Role Person StartDate StopDate Note
1. PrincipalInvestigator spase://CNES/Person/CDPP-AMDA/Michele.Dougherty
2. DataProducer spase://CNES/Person/CDPP-AMDA/Steve.Kellock

AccessInformation
RepositoryID
spase://SMWG/Repository/CDPP/AMDA
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA HAPI Server
URL
https://amda.irap.omp.eu/service/hapi
Style
HAPI
ProductKey
cass-mag-jup
Description
Web Service to this product using the HAPI interface.
Format
CSV
Acknowledgement
Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.
AccessInformation
RepositoryID
spase://SMWG/Repository/CDPP/AMDA
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA Web application
URL
https://amda.cdpp.eu
Description
Access to Data via CDPP/AMDA Web application.
Format
CSV
Format
VOTable
Format
CDF
Format
PNG
Acknowledgement
Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.
ProviderName
PDS
ProviderResourceName
CO-E_SW_J_S-MAG-3-RDR-FULL-RES-V2.0
InstrumentIDs
spase://CNES/Instrument/CDPP-AMDA/Cassini/MAG
MeasurementType
MagneticField
TemporalDescription
TimeSpan
StartDate
2001-01-01 02:26:04Z
StopDate
2001-03-02 06:32:37Z
CadenceMin
PT0.031S
CadenceMax
PT8S
ObservedRegion
Jupiter
Caveats
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.
Parameter #1
Name
b_j3
ParameterKey
cass_bj3_jup
Description
Magnetic field vector components in Jup_IAU coordinates
UCD
phys.magField
Units
nT
RenderingHints
DisplayType
TimeSeries
Structure
Size
3
Element
Name
bx
Index
1
ParameterKey
cass_bj3_jup(0)
Element
Name
by
Index
2
ParameterKey
cass_bj3_jup(1)
Element
Name
bz
Index
3
ParameterKey
cass_bj3_jup(2)
Field
Qualifier
Vector
FieldQuantity
Magnetic
Parameter #2
Name
b_jm
ParameterKey
cass_bjm_jup
Description
Magnetic field vector components in JMAG coordinates
UCD
phys.magField
Units
nT
RenderingHints
DisplayType
TimeSeries
Structure
Size
3
Element
Name
bx
Index
1
ParameterKey
cass_bjm_jup(0)
Element
Name
by
Index
2
ParameterKey
cass_bjm_jup(1)
Element
Name
bz
Index
3
ParameterKey
cass_bjm_jup(2)
Field
Qualifier
Vector
FieldQuantity
Magnetic
Parameter #3
Name
b_rtn
ParameterKey
cass_b_jup
Description
Magnetic field vector components in RTN coordinates
UCD
phys.magField
Units
nT
RenderingHints
DisplayType
TimeSeries
Structure
Size
3
Element
Name
br
Index
1
ParameterKey
cass_b_jup(0)
Element
Name
bt
Index
2
ParameterKey
cass_b_jup(1)
Element
Name
bn
Index
3
ParameterKey
cass_b_jup(2)
Field
Qualifier
Vector
FieldQuantity
Magnetic
Parameter #4
Name
|b|
ParameterKey
cass_bmag_jup
Description
Magnetic field vector magnitude
UCD
phys.magField
Units
nT
RenderingHints
DisplayType
TimeSeries
Field
Qualifier
Magnitude
FieldQuantity
Magnetic
Parameter #5
Name
phi
ParameterKey
cass_b_jup_phi
Description
Magnetic field phi angle
UCD
phys.magField
Units
degrees
UnitsConversion
1e-9>T
RenderingHints
DisplayType
TimeSeries
Structure
Size
1
Field
FieldQuantity
Magnetic
Parameter #6
Name
theta
ParameterKey
cass_b_jup_theta
Description
Magnetic field theta angle
UCD
phys.magField
Units
degrees
UnitsConversion
1e-9>T
RenderingHints
DisplayType
TimeSeries
Structure
Size
1
Field
FieldQuantity
Magnetic