2.3.0 spase://ESA/NumericalData/Cluster-Samba/STAFF/CSA/PT0.125S Cluster-Samba Spatio-Temporal Analysis of Field Fluctuations (STAFF) Data at the ESA Cluster Science Archive Cluster 2 Samba Spatio-Temporal Analysis of Field Fluctuations (STAFF) Data at the ESA Cluster Active Archive 2019-05-05T12:34:56Z 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. Dr. Nicole.Cornilleau-Wehrlin, the STAFF team and the ESA Cluster Active Archive spase://SMWG/Person/Nicole.Cornilleau-Wehrlin PrincipalInvestigator spase://SMWG/Person/Melvyn.L.Goldstein ProjectScientist NSSDC Master Catalog listing for Cluster II Samba Spatio-Temporal Analysis of Field Fluctuations(STAFF) https://nssdc.gsfc.nasa.gov/nmc/experiment/display.action?id=2000-041A-09 This site provides information concerning the Cluster II Samba Spatio-Temporal Analysis of Field Fluctuations (STAFF) Instrument. Cluster Science Archive (CSA) Documentation https://www.cosmos.esa.int/?project=CLUSTER&page=caa_documentation CAA Instrument User Guides, Calibration Reports and ICDS. spase://SMWG/Observatory/Cluster-Samba ObservedBy spase://VSPO/NumericalData/Cluster-Samba/STAFF/CSA/PT0.125S spase://SMWG/Repository/CSA Online Open Access to files at the Cluster Science Archive (CSA) https://www.cosmos.esa.int/ Cluster II Samba Spatio-Temporal Analysis of Field Fluctuations (STAFF) data. It's open access but registration is required. CEF Calibrated spase://SMWG/Instrument/Cluster-Samba/STAFF MagneticField ElectricField 2001-01-01T00:00:00.000 -P8M PT0.125S Earth.Magnetosheath Earth.Magnetosphere Earth.Magnetosphere.Magnetotail Earth.Magnetosphere.Main Earth.Magnetosphere.Polar Earth.Magnetosphere.RadiationBelt Earth.NearSurface.AuroralRegion Earth.NearSurface.Ionosphere Earth.NearSurface.Plasmasphere Earth.NearSurface.PolarCap Heliosphere.NearEarth