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.
Version:2.3.0
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.
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | PrincipalInvestigator | spase://SMWG/Person/Nicole.Cornilleau-Wehrlin | |||
| 2. | CoInvestigator | spase://SMWG/Person/Arne.Pedersen | |||
| 3. | CoInvestigator | spase://SMWG/Person/Les.J.C.Woolliscroft | |||
| 4. | CoInvestigator | spase://SMWG/Person/Donald.A.Gurnett | |||
| 5. | CoInvestigator | spase://SMWG/Person/Christopher.C.Harvey | |||
| 6. | CoInvestigator | spase://SMWG/Person/Georg.Gustafsson | |||
| 7. | CoInvestigator | spase://SMWG/Person/Daniel.Hubert | |||
| 8. | CoInvestigator | spase://SMWG/Person/P.Lefeuvre | |||
| 9. | CoInvestigator | spase://SMWG/Person/Robert.Manning | |||
| 10. | CoInvestigator | spase://SMWG/Person/Wlodek.Kofman | |||
| 11. | MetadataContact | spase://SMWG/Person/James.M.Weygand |
This site provides information concerning the Cluster II Rumba Spatio-Temporal Analysis of Magnetic Field Fluctuations Instrument.
Cluster II Rumba Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) data
In CDF via HTTP from SPDF
Web Service to this product using the HAPI interface.
Half width of measurement interval
Universal Time in data cell: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000.
Cluster II Rumba Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) status at spin time resolution
Cluster II Rumba Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) Wave Experiment Consortium (WEC) status at spin time resolution
Cluster II Rumba 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
Cluster II Rumba 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
Cluster II Rumba 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
Cluster II Rumba 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
Cluster II Rumba 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
Cluster II Rumba 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
Cluster II Rumba 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
Cluster II Rumba 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