2.2.6 spase://CDPP/NumericalData/AMDA/Cluster/Cluster3/STAFF/clust3-sta-pp prime parameters Cluster 3 Prime Parameter STAFF Data 2015-10-19T15:51:44Z The Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) experiment provides magnetic field power spectral density values parallel and perpendicular to the magnetic field and the electric field power spectral density values for several frequency ranges. For more details of the Cluster mission, the spacecraft, and its instruments, see the report Cluster: mission, payload and supporting activities, March 1993, ESA SP-1159, and the included article The STAFF (Spatio-Temporal Analysis of Field Fluctuations) Experiment for the Cluster Mission, by N. Cornilleau-Wehrlin et al., from which this information was obtained. ESA, Nicole Cornilleau-Wehrlin spase://SMWG/Person/Nicole.Cornilleau-Wehrlin PrincipalInvestigator spase://SMWG/Person/Elena.Budnik TechnicalContact NSSDC Master Catalog listing for Cluster II Samba Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-09 This site provides information concerning the Cluster II Samba Spatio-Temporal Analysis of Magnetic Field Fluctuations Instrument. spase://SMWG/Repository/CDPP/AMDA Online Open AMDA at CDPP http://amda.cdpp.eu NetCDF NASA, Nicole Cornilleau-Wehrlin CSDS-CNES Calibrated Cluster II Samba Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) Data Calibrated spase://CDPP/Instrument/AMDA/Cluster-Samba/STAFF ElectricField MagneticField Waves.Passive 2001-01-09T04:39:20Z 2012-12-31T23:59:47Z PT4S 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 4 second magnetosphere auroral region polar cap cusp bow shock solar wind magnetosheath Cluster magnetotail lobe Magnetic Field Spectral Power (1-10 Hz) c3_sta_f1 Cluster II Samba Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) magnetic field spectral power as measured by the onboard Cluster Fluxgate Magnetometer (FGM) in the 1-10 Hz (f1) frequency range at spin time resolution phys.flux.density;phys.magField PT4S nT^2 Hz^-1 1.0e-18>T^2 Hz^-1 TimeSeries 2 Magnetic Field Spectral Power Parallel to Bo (1-10 Hz) 1 c3_sta_f1(0) 1.0000e-7 100 B_par_f1 1.0000e-6 1 Magnetic Field Spectral Power Perpendicular to Bo (1-10 Hz) 2 c3_sta_f1(1) 1.0000e-7 100 B_perp_f1 1.0000e-6 1 -1.0000e+31 Scalar Magnetic 1 10 Hz Magnetic Field Spectral Power (10-180 Hz) c3_sta_f2 Cluster II Samba Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) magnetic field spectral power as measured by the onboard Cluster Fluxgate Magnetometer (FGM) in the 10-180 Hz (f2) frequency range at spin time resolution phys.flux.density;phys.magField PT4S nT^2 Hz^-1 1.0e-18>T^2 Hz^-1 TimeSeries 2 Magnetic Field Spectral Power Parallel to Bo (10-180 Hz) 1 c3_sta_f2(0) 1.0000e-9 1 B_par_f2 1.0000e-6 1 Magnetic Field Spectral Power Perpendicular to Bo (10-180 Hz) 2 c3_sta_f2(1) 1.0000e-9 1 B_perp_f2 1.0000e-6 1 -1.0000e+31 Scalar Magnetic 10 180 Hz Magnetic Field Spectral Power (180-4000 Hz) c3_sta_f3 Cluster II Samba Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) magnetic field spectral power as measured by the onboard Cluster Fluxgate Magnetometer (FGM) in the 180-4000 Hz (f3) frequency range at spin time resolution phys.flux.density;phys.magField PT4S nT^2 Hz^-1 1.0e-18>T^2 Hz^-1 TimeSeries 2 Magnetic Field Spectral Power Parallel to Bo (180-4000 Hz) 1 c3_sta_f3(0) 1.0000e-11 0.0010 B_par_f3 1.0000e-6 1 Magnetic Field Spectral Power Perpendicular to Bo (180-4000 Hz) 2 c3_sta_f3(1) 1.0000e-9 1 B_perp_f3 1.0000e-6 1 -1.0000e+31 Scalar Magnetic 1 10 Hz Electric Field Spectral Power (10-180 Hz) c3_stae_f2 Cluster II Samba 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 phys.flux.density;phys.electField PT4S V^2 m^-2 Hz^-1 1.0>V^2 m^-2 Hz^-1 TimeSeries E_pow_f2 1.0000e-13 1.0000e-5 1.0000e-14 1.0000e-4 -1.0000e+31 Scalar Electric 10 180 Hz Electric Field Spectral Power (180-4000 Hz) c3_stae_f3 Cluster II Samba 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 phys.flux.density;phys.electField PT4S V^2 m^-2 Hz^-1 1.0>V^2 m^-2 Hz^-1 TimeSeries E_pow_f3 1.0000e-14 1.0000e-7 1.0000e-15 1.0000e-6 -1.0000e+31 Scalar Electric 180 4000 Hz