2.3.0 spase://ESA/NumericalData/Cluster-Salsa/STAFF/PrimeParameter/PT4S Cluster-Salsa Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) Data Cluster 2 Prime Parameter STAFF Data 2021-04-27T17:52:14Z 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. NASA, Nicole Cornilleau-Wehrlin spase://SMWG/Person/Nicole.Cornilleau-Wehrlin PrincipalInvestigator spase://SMWG/Person/Arne.Pedersen CoInvestigator spase://SMWG/Person/Les.J.C.Woolliscroft CoInvestigator spase://SMWG/Person/Donald.A.Gurnett CoInvestigator spase://SMWG/Person/Christopher.C.Harvey CoInvestigator spase://SMWG/Person/Georg.Gustafsson CoInvestigator spase://SMWG/Person/Daniel.Hubert CoInvestigator spase://SMWG/Person/P.Lefeuvre CoInvestigator spase://SMWG/Person/Robert.Manning CoInvestigator spase://SMWG/Person/Wlodek.Kofman CoInvestigator spase://SMWG/Person/James.M.Weygand MetadataContact NSSDC Master Catalog listing for Cluster II Salsa Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) https://nssdc.gsfc.nasa.gov/nmc/experiment/display.action?id=2000-041B-09 This site provides information concerning the Cluster II Salsa Spatio-Temporal Analysis of Magnetic Field Fluctuations Instrument. spase://SMWG/Observatory/Cluster-Salsa ObservedBy spase://VMO/NumericalData/Cluster2-Salsa/STAFF/PrimeParameter/4S spase://VMO/NumericalData/Cluster-Salsa/STAFF/PrimeParameter/4S spase://VSPO/NumericalData/Cluster-Salsa/STAFF/PrimeParameter/PT4S spase://SMWG/Repository/NASA/GSFC/SPDF/CDAWeb Online Open FTPS from SPDF (not with most browsers) ftps://spdf.gsfc.nasa.gov/pub/data/cluster/c2/pp/sta/ Cluster II Salsa Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) data HTTPS from SPDF https://spdf.gsfc.nasa.gov/pub/data/cluster/c2/pp/sta/ In CDF via HTTP from SPDF CDAWeb https://cdaweb.gsfc.nasa.gov/cgi-bin/eval2.cgi?dataset=C2_PP_STA&index=sp_phys C2_PP_STA CDF NASA, Nicole Cornilleau-Wehrlin spase://SMWG/Repository/NASA/GSFC/SPDF Online Open CDAWeb HAPI Server https://cdaweb.gsfc.nasa.gov/hapi C2_PP_STA Web Service to this product using the HAPI interface. CSV NASA, Nicole Cornilleau-Wehrlin Calibrated Cluster II Salsa Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) Data Calibrated 1 spase://SMWG/Instrument/Cluster-Salsa/STAFF ElectricField MagneticField Waves.Passive 2000-12-09T00:00:00 -P3M Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000 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 Half Sample Time Interval Half_interval__C2_PP_STA Half width of measurement interval PT4S ms -1.0000e+31 Other Universal Time Epoch__C2_PP_STA Universal Time in data cell: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000. Interval centered time tag PT4S ms 1.0e-3>s Epoch -1.0000e+31 Temporal Status Status__C2_PP_STA Cluster II Salsa Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) status at spin time resolution PT4S 0 255 255 Other Wave Experiment Consortium (WEC) Status State_wec__C2_PP_STA Cluster II Salsa Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) Wave Experiment Consortium (WEC) status at spin time resolution PT4S 0 255 255 Other Magnetic Field Spectral Power Parallel to Bo (0.3-10 Hz) B_par_f1__C2_PP_STA Cluster II Salsa 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 PT4S nT^2 Hz^-1 1.0e-18>T^2 Hz^-1 B_par_f1 1.0000e-6 1 1.0000e-7 100 -1.0000e+31 Scalar Magnetic 0.3 10 Hz Magnetic Field Spectral Power Parallel to Bo (10-180 Hz) B_par_f2__C2_PP_STA Cluster II Salsa 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 PT4S nT^2 Hz^-1 1.0e-18>T^2 Hz^-1 B_par_f2 1.0000e-7 0.1 1.0000e-9 1 -1.0000e+31 Scalar Magnetic 10 180 Hz Magnetic Field Spectral Power Parallel to Bo (180-4000 Hz) B_par_f3__C2_PP_STA Cluster II Salsa 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 PT4S nT^2 Hz^-1 1.0e-18>T^2 Hz^-1 B_par_f3 1.0000e-10 1.0000e-4 1.0000e-11 0.0010 -1.0000e+31 Scalar Magnetic 180 4000 Hz Magnetic Field Spectral Power Perpendicular to Bo (0.3-10 Hz) B_perp_f1__C2_PP_STA Cluster II Salsa 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 PT4S nT^2 Hz^-1 1.0e-18>T^2 Hz^-1 B_perp_f1 1.0000e-6 1 1.0000e-7 100 -1.0000e+31 Scalar Magnetic 0.3 10 Hz Magnetic Field Spectral Power Perpendicular to Bo (10-180 Hz) B_perp_f2__C2_PP_STA Cluster II Salsa 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 PT4S nT^2 Hz^-1 1.0e-18>T^2 Hz^-1 B_perp_f2 1.0000e-7 0.1 1.0000e-9 1 -1.0000e+31 Scalar Magnetic 10 180 Hz Magnetic Field Spectral Power Perpendicular to Bo (180-4000 Hz) B_perp_f3__C2_PP_STA Cluster II Salsa 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 PT4S nT^2 Hz^-1 1.0e-18>T^2 Hz^-1 B_perp_f3 1.0000e-10 1.0000e-4 1.0000e-11 0.0010 -1.0000e+31 Scalar Magnetic 180 4000 Hz Electric Field Spectral Power (10-180 Hz) E_pow_f2__C2_PP_STA Cluster II Salsa 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 PT4S V^2 m^-2 Hz^-1 1.0>V^2 m^-2 Hz^-1 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) E_pow_f3__C2_PP_STA Cluster II Salsa 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 PT4S V^2 m^-2 Hz^-1 1.0>V^2 m^-2 Hz^-1 E_pow_f3 1.0000e-14 1.0000e-7 1.0000e-15 1.0000e-6 -1.0000e+31 Scalar Electric 180 4000 Hz