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Cluster 2 - STAFF - prime parameters

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/Cluster/Cluster2/STAFF/clust2-sta-pp

Description
The STAFF Spectrum Analyser (SA) combines the 3 magnetic components of the waves with the two electric components measured by the EFW experiment to calculate in real time the 5x5 Hermitian cross-spectral matrix at 27 frequencies distributed logarithmically in the frequency range 8 Hz to 4 kHz. The components in the spin plane are despun onboard. The five auto-spectral power estimates are obtained with a dynamic range of approximately 100 dB and an average amplitude resolution of 0.38 dB. The 10 cross-spectral power estimates are normalised to give the coherence. The precision of the phase depends upon the magnitude of the coherence: for a signal with magnitude in the highest bin, it is approximately 5 degree close to 0 degree, 180 degree, and +/- 90 degree, increasing to about 10 degree midway between these angles. The Spectrum Analyser can work in different modes, in Burst Mode the analysis is performed in the frequency range 64 Hz - 4 kHz. This dataset contains preliminary spin resolution measurements of the magnetic field spectral density and electric field spectral density from the STAFF Spectrum Analyser experiment on the Cluster C1 spacecraft. These data have been converted into Cluster Exchange Format from the orignal Cluster Science Data System Common Data Format (CDF) Prime Parameter files that were made available through the Cluster Science Data System.

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Version:2.4.1

NumericalData

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/Cluster/Cluster2/STAFF/clust2-sta-pp
ResourceHeader
ResourceName
Cluster 2 - STAFF - prime parameters
AlternateName
Cluster 2 Prime Parameter STAFF Data
ReleaseDate
2013-05-03 12:17:15Z
Description
The STAFF Spectrum Analyser (SA) combines the 3 magnetic components of the waves with the two electric components measured by the EFW experiment to calculate in real time the 5x5 Hermitian cross-spectral matrix at 27 frequencies distributed logarithmically in the frequency range 8 Hz to 4 kHz. The components in the spin plane are despun onboard. The five auto-spectral power estimates are obtained with a dynamic range of approximately 100 dB and an average amplitude resolution of 0.38 dB. The 10 cross-spectral power estimates are normalised to give the coherence. The precision of the phase depends upon the magnitude of the coherence: for a signal with magnitude in the highest bin, it is approximately 5 degree close to 0 degree, 180 degree, and +/- 90 degree, increasing to about 10 degree midway between these angles. The Spectrum Analyser can work in different modes, in Burst Mode the analysis is performed in the frequency range 64 Hz - 4 kHz. This dataset contains preliminary spin resolution measurements of the magnetic field spectral density and electric field spectral density from the STAFF Spectrum Analyser experiment on the Cluster C1 spacecraft. These data have been converted into Cluster Exchange Format from the orignal Cluster Science Data System Common Data Format (CDF) Prime Parameter files that were made available through the Cluster Science Data System.
Acknowledgement
Principal Investigator: Patrick Canu
Contacts
Role Person StartDate StopDate Note
1. PrincipalInvestigator spase://SMWG/Person/Patrick.Canu
InformationURL
Name
ESA web page
URL
http://www.cosmos.esa.int/web/csa/documentation
Description
This site contains STAFF data documentation
InformationURL
Name
NSSDC Master Catalog listing for Cluster II Salsa STAFF
URL
http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-09
Description
This site provides information concerning the Cluster STAFF Instrument.
AccessInformation
RepositoryID
spase://SMWG/Repository/CDPP/AMDA
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA HAPI Server
URL
https://amda.irap.omp.eu/service/hapi
Style
HAPI
ProductKey
clust2-sta-pp
Description
Web Service to this product using the HAPI interface.
Format
CSV
Acknowledgement
Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.
AccessInformation
RepositoryID
spase://SMWG/Repository/CDPP/AMDA
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA Web application
URL
https://amda.cdpp.eu
Description
Access to Data via CDPP/AMDA Web application.
Format
CSV
Format
VOTable
Format
CDF
Format
PNG
Acknowledgement
Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.
ProcessingLevel
Calibrated
ProviderName
CSDS-CNES
InstrumentIDs
spase://CNES/Instrument/CDPP-AMDA/Cluster2/STAFF
MeasurementType
ElectricField
MeasurementType
MagneticField
MeasurementType
Waves.Passive
TemporalDescription
TimeSpan
StartDate
2001-01-09 15:10:02Z
StopDate
2012-12-31 23:59:46Z
Cadence
PT4S
ObservedRegion
Earth.Magnetosphere
ObservedRegion
Earth.Magnetosheath
ObservedRegion
Earth.Magnetosphere.Magnetotail
ObservedRegion
Earth.Magnetosphere.Main
ObservedRegion
Earth.Magnetosphere.Polar
ObservedRegion
Earth.Magnetosphere.RadiationBelt
ObservedRegion
Earth.NearSurface.AuroralRegion
ObservedRegion
Earth.NearSurface.Ionosphere
ObservedRegion
Earth.NearSurface.Plasmasphere
ObservedRegion
Earth.NearSurface.PolarCap
ObservedRegion
Heliosphere.NearEarth
Keywords
4 second
magnetosphere
auroral region
polar cap
cusp
bow shock
solar wind
magnetosheath
Cluster
magnetotail
lobe
Parameter #1
Name
b spectral density (1-10 Hz)
ParameterKey
c2_sta_f1
Description
Magnetic field spectral power in the 1-10 Hz (f1) at spin time resolution (parallel and perp components)
UCD
phys.magField
Cadence
PT4S
Units
nT^2 Hz^-1
UnitsConversion
1.0e-18>T^2 Hz^-1
RenderingHints
DisplayType
TimeSeries
Structure
Size
2
Element
Name
parallel to b0
Index
1
ParameterKey
c2_sta_f1(0)
ValidMin
1.0000e-7
ValidMax
100
RenderingHints
AxisLabel
B_par_f1
ScaleMin
1.0000e-6
ScaleMax
1
Element
Name
perpendicular to b0
Index
2
ParameterKey
c2_sta_f1(1)
ValidMin
1.0000e-7
ValidMax
100
RenderingHints
AxisLabel
B_perp_f1
ScaleMin
1.0000e-6
ScaleMax
1
FillValue
-1.0000e+31
Field
Qualifier
Scalar
FieldQuantity
Magnetic
FrequencyRange
Low
1
High
10
Units
Hz
Parameter #2
Name
b spectral density (10-180 Hz)
ParameterKey
c2_sta_f2
Description
Magnetic field spectral power in the 10-180 Hz (f2) at spin time resolution (parallel and perp components)
UCD
phys.magField
Cadence
PT4S
Units
nT^2 Hz^-1
UnitsConversion
1.0e-18>T^2 Hz^-1
RenderingHints
DisplayType
TimeSeries
Structure
Size
2
Element
Name
parallel to b0
Index
1
ParameterKey
c2_sta_f2(0)
ValidMin
1.0000e-9
ValidMax
1
RenderingHints
AxisLabel
B_par_f2
ScaleMin
1.0000e-6
ScaleMax
1
Element
Name
perpendicular to b0
Index
2
ParameterKey
c2_sta_f2(1)
ValidMin
1.0000e-9
ValidMax
1
RenderingHints
AxisLabel
B_perp_f2
ScaleMin
1.0000e-6
ScaleMax
1
FillValue
-1.0000e+31
Field
Qualifier
Scalar
FieldQuantity
Magnetic
FrequencyRange
Low
10
High
180
Units
Hz
Parameter #3
Name
b spectral density (180-4000 Hz)
ParameterKey
c2_sta_f3
Description
Magnetic field spectral power in the 80-4000 Hz (f3) at spin time resolution (parallel and perp components)
UCD
phys.magField
Cadence
PT4S
Units
nT^2 Hz^-1
UnitsConversion
1.0e-18>T^2 Hz^-1
RenderingHints
DisplayType
TimeSeries
Structure
Size
2
Element
Name
parallel to b0
Index
1
ParameterKey
c2_sta_f3(0)
ValidMin
1.0000e-11
ValidMax
0.0010
RenderingHints
AxisLabel
B_par_f3
ScaleMin
1.0000e-6
ScaleMax
1
Element
Name
perpendicular to b0
Index
2
ParameterKey
c2_sta_f3(1)
ValidMin
1.0000e-9
ValidMax
1
RenderingHints
AxisLabel
B_perp_f3
ScaleMin
1.0000e-6
ScaleMax
1
FillValue
-1.0000e+31
Field
Qualifier
Scalar
FieldQuantity
Magnetic
FrequencyRange
Low
1
High
10
Units
Hz
Parameter #4
Name
e spectral density (10-180 Hz)
ParameterKey
c2_stae_f2
Description
Electric field spectral power in the 10-180 Hz (f2) frequency range at spin time resolution.
UCD
phys.electField
Cadence
PT4S
Units
V^2 m^-2 Hz^-1
UnitsConversion
1.0>V^2 m^-2 Hz^-1
RenderingHints
DisplayType
TimeSeries
AxisLabel
E_pow_f2
ScaleMin
1.0000e-13
ScaleMax
1.0000e-5
ValidMin
1.0000e-14
ValidMax
1.0000e-4
FillValue
-1.0000e+31
Field
Qualifier
Scalar
FieldQuantity
Electric
FrequencyRange
Low
10
High
180
Units
Hz
Parameter #5
Name
e spectral density (180-4000 Hz)
ParameterKey
c2_stae_f3
Description
Electric field spectral power in the 180-4000 Hz (f3) frequency range at spin time resolution.
UCD
phys.electField
Cadence
PT4S
Units
V^2 m^-2 Hz^-1
UnitsConversion
1.0>V^2 m^-2 Hz^-1
RenderingHints
DisplayType
TimeSeries
AxisLabel
E_pow_f3
ScaleMin
1.0000e-14
ScaleMax
1.0000e-7
ValidMin
1.0000e-15
ValidMax
1.0000e-6
FillValue
-1.0000e+31
Field
Qualifier
Scalar
FieldQuantity
Electric
FrequencyRange
Low
180
High
4000
Units
Hz
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Last Updated: 2013-05-03