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Cluster-Tango Spatio-Temporal Analysis of Field Fluctuations (STAFF) Data at the ESA Cluster Science Archive

ResourceID
spase://ESA/NumericalData/Cluster-Tango/STAFF/CSA/PT0.125S

Description

Magnetic field and electric field data products from the Cluster Spatio-Temporal Analysis of Field Fluctuations (STAFF) available from the Cluster Active Archive include: Level 2 calibrated data -- STAFF Waveform Analyzer (STAFF-SC) Complex Spectra of the magnetic field in GSE coordinates (normal mode, up to 12.5 Hz and burst mode up to 225 Hz) with a time resolution of 10 second and a frequency resolution of 0.1 Hz; STAFF-SC Calibrated Magnetic Field WaveForm in ISR2 coordinates (normal mode, 25 Hz sampling and burst mode, 450 Hz sampling); STAFF Spectrum Analyzer (STAFF-SA) Spectral Matrix (8 Hz to 4 KHz) which is the cross-product of the magnetic and electric fileds values computed on-board the spacecraft with time resolutions of 4 seconds and 1 second; and Power Spectral Density (8 Hz to 4 KHz) with time resolutions of 1, 0.125 and 0.25 second. Level 3 value-added products include STAFF-SA Polarization and Propagation Parameters (8 Hz to 4 KHz). In the base mode in normal bit rate the auto-spectra are averaged over 1 s, and the complete 25-component matrix is averaged over 4 s for five components. In high bit rate, only the two highest frequency bands are analyzed. In the fast modes, time resolution is 1 s for the cross-spectra, and either 0.125 s or 0.25 s for the auto-spectra. The physical units for magnetic field spectral power are nT^2 Hz^-1, and electric field spectral power, V^2 m^-2 Hz^-1. Ancillary data included preliminary spectra, uncalibrated waveform, caveats, and calibration information. For more details, see "The Cluster Active Archive: Studying the Earth's Space Plasma Environment", edited by Dr. Harri Laakso, Matthew G. T. T. Taylor, C. Philippe Escoubet, from which this information was obtained.

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Details

Version:2.3.0

NumericalData

ResourceID
spase://ESA/NumericalData/Cluster-Tango/STAFF/CSA/PT0.125S
ResourceHeader
ResourceName
Cluster-Tango Spatio-Temporal Analysis of Field Fluctuations (STAFF) Data at the ESA Cluster Science Archive
AlternateName
Cluster 2 Tango Spatio-Temporal Analysis of Field Fluctuations (STAFF) Data at the ESA Cluster Active Archive
ReleaseDate
2019-05-05 12:34:56Z
Description

Magnetic field and electric field data products from the Cluster Spatio-Temporal Analysis of Field Fluctuations (STAFF) available from the Cluster Active Archive include: Level 2 calibrated data -- STAFF Waveform Analyzer (STAFF-SC) Complex Spectra of the magnetic field in GSE coordinates (normal mode, up to 12.5 Hz and burst mode up to 225 Hz) with a time resolution of 10 second and a frequency resolution of 0.1 Hz; STAFF-SC Calibrated Magnetic Field WaveForm in ISR2 coordinates (normal mode, 25 Hz sampling and burst mode, 450 Hz sampling); STAFF Spectrum Analyzer (STAFF-SA) Spectral Matrix (8 Hz to 4 KHz) which is the cross-product of the magnetic and electric fileds values computed on-board the spacecraft with time resolutions of 4 seconds and 1 second; and Power Spectral Density (8 Hz to 4 KHz) with time resolutions of 1, 0.125 and 0.25 second. Level 3 value-added products include STAFF-SA Polarization and Propagation Parameters (8 Hz to 4 KHz). In the base mode in normal bit rate the auto-spectra are averaged over 1 s, and the complete 25-component matrix is averaged over 4 s for five components. In high bit rate, only the two highest frequency bands are analyzed. In the fast modes, time resolution is 1 s for the cross-spectra, and either 0.125 s or 0.25 s for the auto-spectra. The physical units for magnetic field spectral power are nT^2 Hz^-1, and electric field spectral power, V^2 m^-2 Hz^-1. Ancillary data included preliminary spectra, uncalibrated waveform, caveats, and calibration information. For more details, see "The Cluster Active Archive: Studying the Earth's Space Plasma Environment", edited by Dr. Harri Laakso, Matthew G. T. T. Taylor, C. Philippe Escoubet, from which this information was obtained.

Acknowledgement
Dr. Nicole.Cornilleau-Wehrlin, the STAFF team and the ESA Cluster Active Archive
Contacts
RolePersonStartDateStopDateNote
1.PrincipalInvestigatorspase://SMWG/Person/Nicole.Cornilleau-Wehrlin
2.ProjectScientistspase://SMWG/Person/Melvyn.L.Goldstein
InformationURL
Name
NSSDC Master Catalog listing for Cluster II Tango Spatio-Temporal Analysis of Field Fluctuations(STAFF)
URL
Description

This site provides information concerning the Cluster II Tango Spatio-Temporal Analysis of Field Fluctuations (STAFF) Instrument.

InformationURL
Name
Cluster Science Archive (CSA) Documentation
URL
Description

CAA Instrument User Guides, Calibration Reports and ICDS.

Association
AssociationID
AssociationType
ObservedBy
PriorIDs
spase://VSPO/NumericalData/Cluster-Tango/STAFF/CSA/PT0.125S
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
Access to files at the Cluster Science Archive (CSA)
URL
Description

Cluster II Tango Spatio-Temporal Analysis of Field Fluctuations (STAFF) data. It's open access but registration is required.

Format
CEF
ProcessingLevel
Calibrated
InstrumentIDs
MeasurementType
MagneticField
MeasurementType
ElectricField
TemporalDescription
TimeSpan
StartDate
2001-01-01 00:00:00.000
RelativeStopDate
-P8M
Cadence
PT0.125S
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