HDPWS

Juno - Jovian Magnetic Field Models - JRM33 + Con2020 M-Shell

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/Juno/Models/jun-jrm33-mshell

Description
Juno M-Shell calculated with JRM33+CON2020 between PJ1 (2016-08-27) and PJ56 (2023-11-22) with 1s-resolution. Spatial resolution is 1/250 Rj ~ 300 km. Outer boundary is set to R=30 Rj.

View XML | Edit

Details

Version:2.4.1

NumericalData

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/Juno/Models/jun-jrm33-mshell
ResourceHeader
ResourceName
Juno - Jovian Magnetic Field Models - JRM33 + Con2020 M-Shell
AlternateName
JRM33 + Con2020 M-Shell
ReleaseDate
2024-02-15 01:01:36Z
Description
Juno M-Shell calculated with JRM33+CON2020 between PJ1 (2016-08-27) and PJ56 (2023-11-22) with 1s-resolution. Spatial resolution is 1/250 Rj ~ 300 km. Outer boundary is set to R=30 Rj.
Contacts
Role Person StartDate StopDate Note
1. DataProducer spase://CNES/Person/CDPP-AMDA/Jonas.Rabia
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA HAPI Server
URL
Style
HAPI
ProductKey
jun-jrm33-mshell
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
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA Web application
URL
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
IRAP
InstrumentIDs
MeasurementType
MagneticField
TemporalDescription
TimeSpan
StartDate
2016-08-27 00:00:00Z
StopDate
2023-11-22 00:00:00Z
Cadence
PT1S
ObservedRegion
Jupiter
Caveats
Due to the limitation in the spatial resolution used for the computation, small stalls in M-Shell colatitude, longitude and curvilinear distance may occasionally occur close to the magnetic equator
Parameter #1
Name
M-Shell
ParameterKey
mshell_juno_m
Description
M-Shell - Radial distance of the intersection between the magnetic field line and themagnetic equator
Support
SupportQuantity
Other
Parameter #2
Name
M-Shell colatitude
ParameterKey
mshell_juno_t
Description
Colatitude (S3RH) of the intersection between the magnetic field line and themagnetic equator
Units
deg
Support
SupportQuantity
Positional
Parameter #3
Name
M-Shell longitude
ParameterKey
mshell_juno_p
Description
Longitude (S3RH) of the intersection between the magnetic field line and themagnetic equator
Units
deg
Support
SupportQuantity
Positional
Parameter #4
Name
curvilinear distance s
ParameterKey
mshell_juno_s
Description
Curvilinear distance along the magnetic field line between the magnetic equator and the spacecraft
Units
Rj
Support
SupportQuantity
Positional