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Cluster-Samba Electron Drift Instrument (EDI) Data at the ESA Cluster Science Archive

(2025). Cluster-Samba Electron Drift Instrument (EDI) Data at the ESA Cluster Science Archive [Data set]. European Space Astronomy Centre. https://doi.org/10.48322/rwbc-0g86. Accessed on .

Note: Proper references, including those in BibTex or other formats, should include the "Accessed on date" as shown above to identify the version of the resource being cited in a given publication.

ResourceID
spase://NASA/NumericalData/Cluster-Samba/EDI/CSA/PT0.0625S

Description

The Electron Drift Instrument (EDI) data products from the Cluster spacecraft in three main categories: (1) Electron enegergies measured between 0.5 and 1.0 keV for the Windshield Wiper mode: time series of the three components of the electron drift velocity and of the three components of the electric field in Cartesian GSE coordinate system (corrected for spacecraft motion) with different qualities and time resolution at 1-4 sec (PP, PPP, MPD); (2) Ambient electron measurements at fixed enegeris of 0.5 or 1.0 keV: time series of electron counts normally at 16 ms for the three pitch angles 0 deg, 90 deg, 180 deg, the detector look direction in the spacecraft frame and in GSE and the status for AE mode; and (3) Overview plot of the main parameters for both modes for every 3 h for one reference spacecraft (usually Cluster III). Besides the main products, there also are raw data and auxiliary data. Raw data consist of merged science files (MSF) that are obtained by merging the housekeeping and science (burst (BM) and normal (NM) mode) telemetry files. They are in binary format. Auxiliary are either data used internally by the main data production software or data dedicated to intercalibration or time-interval lists of the EDI operation modes. For more details, see "The Cluster Active Archive: Studying the Earth's Space Plasma Environment", edited by Dr. Harri Laakso, Matthew G. T. T. Taylor, C. Philippe Escoubet, from which this information was obtained.

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Details

Version:2.7.1

MetadataRightsList

Rights
SchemeURI
https://spdx.org/licenses/
RightsIdentifierScheme
SPDX
RightsIdentifier
CC0-1.0
RightsURI
https://spdx.org/licenses/CC0-1.0.html
RightsName
Creative Commons Zero v1.0 Universal
Note
CC0 1.0 Universal is the Creative Commons license applicable to all publicly available SPASE metadata descriptions

Version:2.7.1

NumericalData

ResourceID
spase://NASA/NumericalData/Cluster-Samba/EDI/CSA/PT0.0625S
NamingAuthority
NASA
ResourceType
NumericalData
ResourceHeader
ResourceName
Cluster-Samba Electron Drift Instrument (EDI) Data at the ESA Cluster Science Archive
AlternateName
Cluster 2 Samba Electron Drift Instrument (EDI) Data at the ESA Cluster Active Archive
DOI
https://doi.org/10.48322/rwbc-0g86
ReleaseDate
2025-12-04 13:29:02Z
RevisionHistory
RevisionEvent
ReleaseDate
2021-02-12 20:40:18Z
Note
Only known prior ReleaseDate of the metadata
RevisionEvent
ReleaseDate
2025-11-14 16:01:46Z
Note
Added PublicationInfo. Added ResourceType and NamingAuthority. Changed http to https in top-level schemaLocation attribute. Fixed version number separator in top-level schemaLocation attribute. Matched version number in schemaLocation attribute to updated value in Version tag. ZCB
RevisionEvent
ReleaseDate
2025-12-04 13:29:02Z
Note
Added MetadataRightsList. Updated to 2.7.1. ZCB
Description

The Electron Drift Instrument (EDI) data products from the Cluster spacecraft in three main categories: (1) Electron enegergies measured between 0.5 and 1.0 keV for the Windshield Wiper mode: time series of the three components of the electron drift velocity and of the three components of the electric field in Cartesian GSE coordinate system (corrected for spacecraft motion) with different qualities and time resolution at 1-4 sec (PP, PPP, MPD); (2) Ambient electron measurements at fixed enegeris of 0.5 or 1.0 keV: time series of electron counts normally at 16 ms for the three pitch angles 0 deg, 90 deg, 180 deg, the detector look direction in the spacecraft frame and in GSE and the status for AE mode; and (3) Overview plot of the main parameters for both modes for every 3 h for one reference spacecraft (usually Cluster III). Besides the main products, there also are raw data and auxiliary data. Raw data consist of merged science files (MSF) that are obtained by merging the housekeeping and science (burst (BM) and normal (NM) mode) telemetry files. They are in binary format. Auxiliary are either data used internally by the main data production software or data dedicated to intercalibration or time-interval lists of the EDI operation modes. For more details, see "The Cluster Active Archive: Studying the Earth's Space Plasma Environment", edited by Dr. Harri Laakso, Matthew G. T. T. Taylor, C. Philippe Escoubet, from which this information was obtained.

Acknowledgement
Goetz Paschmann and the Cluster Active Archive
PublicationInfo
Authors
Paschmann, Goetz
PublicationDate
2025-11-14 16:01:46Z
PublishedBy
European Space Astronomy Centre
Contacts
RolePersonStartDateStopDateNote
1.PrincipalInvestigatorspase://SMWG/Person/Goetz.Paschmann
2.ProjectScientistspase://SMWG/Person/Melvyn.L.Goldstein
InformationURL
Name
NSSDC Master Catalog listing for Cluster II Samba Electron Drift Instrument (EDI)
URL
Description

This site provides information concerning the Cluster II Samba Electron Drift Instrument.

InformationURL
Name
Cluster Science Archive (CSA) Documentation
URL
Description

CAA Instrument User Guides, Calibration Reports and ICDS.

Association
AssociationID
AssociationType
ObservedBy
PriorIDs
spase://VSPO/NumericalData/Cluster-Samba/EDI/CSA/PT0.0625S
spase://ESA/NumericalData/Cluster-Samba/EDI/CSA/PT0.0625S
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
Access to files at the Cluster Science Archive (CSA)
URL
Description

Cluster II Samba Electron Drift Instrument (EDI) data; open access but registration is required.

Format
CEF
ProcessingLevel
Calibrated
InstrumentIDs
MeasurementType
ElectricField
TemporalDescription
TimeSpan
StartDate
2001-01-30 00:00:00.000
RelativeStopDate
-P3M
Cadence
PT0.0625S
ObservedRegion
Earth.Magnetosheath
ObservedRegion
Earth.Magnetosphere
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
Caveats
The measured electron drift velocity cannot always be separated into the electric-field and magnetic gradient induced parts; in such cases the computed electric fields are subject to contamination by magnetic gradient effects. The raw-data counts have to be corrected for the angular dependence of the efficiency. The status byte and the AEC-files must be used as described above. Ambient electron data are available since October 2004 on C1, C2 and C3, see CLIST files for time intervals. The EDI instrument on C2 is working only in ambient mode.