2.4.0 spase://CNES/NumericalData/CDPP-Archive/Cluster-3/STAFF/CLU_PP_C3_STA Cluster 3 STAFF Prime Parameters https://doi.org/10.24400/802406/h15b-a67h 2022-02-28T09:20:15Z This data set contains the Cluster 3 STAFF Prime Parameters (spin time resolution) : the parallel and perpendicular (to the FGM measured magnetic field) power of the magnetic field and the power of the spin-plane components of the electric field for several frequency ranges. Caveats The STAFF prime parameters do not have the standard CSDS timing which is synchronous with the spacecraft spin clock. The operation of the STAFF digital spectrum analyser is synchronised with the DWP clock. The summary parameters are the average of all those instrument measurements made during STAFF 4 s periods whose middle times lie within the minute boundaries. The difference from the standard CSDS definition is negligible for all practical purposes. The summary parameter and prime parameter E_pow_f2 is supplied by STAFF only when the satellites are in normal mode. In burst mode both STAFF and EFW measure the waveform to 180 Hz, and the onboard spectrum analyser is not used to determine the spectrum in the band 10--180 Hz. The parameters B_pow_f2, E_pow_f2, B_par_f2, and B_perp_f2 are determined from the waveform measurements which, in the case of the electric field, come from EFW. Thus in normal mode the parameter E_pow_f2 is supplied by STAFF, while in burst mode it is replaced by the parameter of the same name from the EFW experiment. spase://CNES/Person/CDPP-Archive/Patrick.Canu PrincipalInvestigator spase://CNES/Repository/CDPP-Archive/REGARDS-CDPP Online REGARDS https://regards.cnes.fr/user/cdpp/modules/1777?sp=DatasetName;q=DatasetName:CLU_PP_C3_STA Access via CNES Data Archive for CDPP CDF Calibrated spase://CNES/Instrument/CDPP-Archive/Cluster-3/STAFF ElectricField MagneticField Waves.Passive 2001-01-09T00:00:00Z 2012-12-31T00:00:00Z 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 Cluster 3 STAFF Magnetic Field Spectral Power Parallel to Bo (0.3-10 Hz) Cluster 3 Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) magnetic field spectral power parallel to the mean magnetic field as measured by the onboard Cluster Fluxgate Magnetometer (FGM) in the 0.3-10 Hz (f1) frequency range at spin time resolution nT^2 Hz^-1 1.0e-18>T^2 Hz^-1 Parallel Magnetic 0.3 10 Hz Cluster 3 STAFF Magnetic Field Spectral Power Parallel to Bo (10-180 Hz) Cluster 3 Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) magnetic field spectral power parallel to the mean magnetic field as measured by the onboard Cluster Fluxgate Magnetometer (FGM) in the 10-180 Hz (f2) frequency range at spin time resolution nT^2 Hz^-1 1.0e-18>T^2 Hz^-1 Parallel Magnetic 10 180 Hz Cluster 3 STAFF Magnetic Field Spectral Power Parallel to Bo (180-4000 Hz) Cluster 3 Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) magnetic field spectral power parallel to the mean magnetic field as measured by the onboard Cluster Fluxgate Magnetometer (FGM) in the 180-4000 Hz (f3) frequency range at spin time resolution nT^2 Hz^-1 1.0e-18>T^2 Hz^-1 Parallel Magnetic 180 4000 Hz Cluster 3 STAFF Magnetic Field Spectral Power Perpendicular to Bo (0.3-10 Hz) Cluster 3 Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) magnetic field spectral power perpendicular to the mean magnetic field as measured by the onboard Cluster Fluxgate Magnetometer (FGM) in the 0.3-10 Hz (f1) frequency range at spin time resolution nT^2 Hz^-1 1.0e-18>T^2 Hz^-1 Perpendicular Magnetic 0.3 10 Hz Cluster 3 STAFF Magnetic Field Spectral Power Perpendicular to Bo (10-180 Hz) Cluster 3 Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) magnetic field spectral power perpendicular to the mean magnetic field as measured by the onboard Cluster Fluxgate Magnetometer (FGM) in the 10-180 Hz (f2) frequency range at spin time resolution nT^2 Hz^-1 1.0e-18>T^2 Hz^-1 Perpendicular Magnetic 10 180 Hz Cluster 3 STAFF Magnetic Field Spectral Power Perpendicular to Bo (180-4000 Hz) Cluster 3 Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) magnetic field spectral power perpendicular to the mean magnetic field as measured by the onboard Cluster Fluxgate Magnetometer (FGM) in the 180-4000 Hz (f3) frequency range at spin time resolution nT^2 Hz^-1 1.0e-18>T^2 Hz^-1 Perpendicular Magnetic 180 4000 Hz Cluster 3 STAFF Electric Field Spectral Power (10-180 Hz) Cluster 3 Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) electric field spectral power in the 10-180 Hz (f2) frequency range at spin time resolution V^2 m^-2 Hz^-1 Scalar Electric 10 180 Hz Cluster 3 STAFF Electric Field Spectral Power (180-4000 Hz) Cluster 3 Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) electric field spectral power in the 180-4000 Hz (f3) frequency range at spin time resolution V^2 m^-2 Hz^-1 Scalar Electric 180 4000 Hz Cluster 3 STAFF Status Cluster 3 Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) status at spin time resolution Other