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CLU1 STAFF-SA Caveats - Polarization and Propagation Parameters

ResourceID
spase://CNES/NumericalData/CDPP-Archive/Cluster-1/STAFF/CLU_C1_STA_PPP_CAV

Description
This dataset contains caveats for the PPP (L3) datasets from the STAFF-SA instrument on Cluster 1.

Here are given times where there are either low coverage FGM data or too low attitudes magnetic field to transform SM data in MFA coordinate system.

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Details

Version:2.4.0

NumericalData

ResourceID
spase://CNES/NumericalData/CDPP-Archive/Cluster-1/STAFF/CLU_C1_STA_PPP_CAV
ResourceHeader
ResourceName
CLU1 STAFF-SA Caveats - Polarization and Propagation Parameters
DOI
https://doi.org/10.24400/802406/9anm-kwct
ReleaseDate
2022-02-22 17:30:22Z
Description
This dataset contains caveats for the PPP (L3) datasets from the STAFF-SA instrument on Cluster 1.

Here are given times where there are either low coverage FGM data or too low attitudes magnetic field to transform SM data in MFA coordinate system.
Contacts
RolePerson
1.PrincipalInvestigatorspase://CNES/Person/CDPP-Archive/Patrick.Canu
AccessInformation
RepositoryID
spase://CNES/Repository/CDPP-Archive/REGARDS-CDPP
Availability
Online
AccessURL
Name
REGARDS
URL
https://regards.cnes.fr/user/cdpp/modules/1777?sp=DatasetName;q=DatasetName:CLU_C1_STA_PPP_CAV
Description
Access via CNES Data Archive for CDPP
Format
CEF
InstrumentIDs
spase://CNES/Instrument/CDPP-Archive/Cluster-1/STAFF
MeasurementType
InstrumentStatus
TemporalDescription
TimeSpan
StartDate
2000-12-02 00:00:00Z
StopDate
2018-08-31 00:00:00Z
ObservedRegion
Earth.Magnetosheath
ObservedRegion
Earth.Magnetosphere
ObservedRegion
Earth.Magnetosphere.Magnetotail
ObservedRegion
Earth.Magnetosphere.Main
ObservedRegion
Earth.Magnetosphere.Polar
ObservedRegion
Earth.Magnetosphere.RadiationBelt
ObservedRegion
Earth.NearSurface.AuroralRegion
ObservedRegion
Earth.NearSurface.Ionosphere
ObservedRegion
Earth.NearSurface.Plasmasphere
ObservedRegion
Earth.NearSurface.PolarCap
ObservedRegion
Heliosphere.NearEarth
Parameter #1
Name
Cluster 1 STAFF Caveats - Polarization and Propagation Parameters
Description
Cluster 1 STAFF times where there are either low coverage FGM data or too low attitudes magnetic field to transform SM data in MFA coordinate system.
Support
SupportQuantity
Other