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      "name": "Cluster-Rumba Spatio-Temporal Analysis of Field Fluctuations (STAFF) Data at the ESA Cluster Science Archive",
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    "identifier": "spase://ESA/NumericalData/Cluster-Rumba/STAFF/CSA/PT0.125S",
        
    "creditText": "Dr. Nicole.Cornilleau-Wehrlin, the STAFF team and the ESA Cluster Active Archive",
    "description": "Magnetic field and electric field data products from the Cluster Spatio-Temporal Analysis of Field Fluctuations (STAFF) available from the Cluster Active Archive include: Level 2 calibrated data -- STAFF Waveform Analyzer (STAFF-SC) Complex Spectra of the magnetic field in GSE coordinates (normal mode, up to 12.5 Hz and burst mode up to 225 Hz) with a time resolution of 10 second and a frequency resolution of 0.1 Hz; STAFF-SC Calibrated Magnetic Field WaveForm in ISR2 coordinates (normal mode, 25 Hz sampling and burst mode, 450 Hz sampling); STAFF Spectrum Analyzer (STAFF-SA) Spectral Matrix (8 Hz to 4 KHz) which is the cross-product of the magnetic and electric fileds values computed on-board the spacecraft with time resolutions of 4 seconds and 1 second; and Power Spectral Density (8 Hz to 4 KHz) with time resolutions of 1, 0.125 and 0.25 second.  Level 3 value-added products include STAFF-SA Polarization and Propagation Parameters (8 Hz to 4 KHz).  In the base mode in normal bit rate the auto-spectra are averaged over 1 s, and the complete 25-component matrix is averaged over 4 s for five components. In high bit rate, only the two highest frequency bands are analyzed. In the fast modes, time resolution is 1 s for the cross-spectra, and either 0.125 s or 0.25 s for the auto-spectra.  The physical units for magnetic field spectral power are nT^2 Hz^-1, and electric field spectral power, V^2 m^-2 Hz^-1.  Ancillary data included preliminary spectra, uncalibrated waveform, caveats, and calibration information.  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.",
    "abstract": "Magnetic field and electric field data products from the Cluster Spatio-Temporal Analysis of Field Fluctuations (STAFF) available from the Cluster Active Archive include: Level 2 calibrated data -- STAFF Waveform Analyzer (STAFF-SC) Complex Spectra of the magnetic field in GSE coordinates (normal mode, up to 12.5 Hz and burst mode up to 225 Hz) with a time resolution of 10 second and a frequency resolution of 0.1 Hz; STAFF-SC Calibrated Magnetic Field WaveForm in ISR2 coordinates (normal mode, 25 Hz sampling and burst mode, 450 Hz sampling); STAFF Spectrum Analyzer (STAFF-SA) Spectral Matrix (8 Hz to 4 KHz) which is the cross-product of the magnetic and electric fileds values computed on-board the spacecraft with time resolutions of 4 seconds and 1 second; and Power Spectral Density (8 Hz to 4 KHz) with time resolutions of 1, 0.125 and 0.25 second.  Level 3 value-added products include STAFF-SA Polarization and Propagation Parameters (8 Hz to 4 KHz).  In the base mode in normal bit rate the auto-spectra are averaged over 1 s, and the complete 25-component matrix is averaged over 4 s for five components. In high bit rate, only the two highest frequency bands are analyzed. In the fast modes, time resolution is 1 s for the cross-spectra, and either 0.125 s or 0.25 s for the auto-spectra.  The physical units for magnetic field spectral power are nT^2 Hz^-1, and electric field spectral power, V^2 m^-2 Hz^-1.  Ancillary data included preliminary spectra, uncalibrated waveform, caveats, and calibration information.  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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        <div class="header">
            <div class="middle">HDPWS</div>
        </div>
        <div class="page">
            <div class="spase">
                <div class="abstract">
                    <div class="access">
                        <p class="box-title">
                    Data Access
                </p>
                        <ul class="list">
                            <li class="list">
                                <a target="_blank" href="https://www.cosmos.esa.int/">Access to files at the Cluster Science Archive (CSA)</a>
                            </li>
                        </ul>
                    </div>
                    <div class="citation inset">
                        <h1>
                            <a name="spase://ESA/NumericalData/Cluster-Rumba/STAFF/CSA/PT0.125S">Cluster-Rumba Spatio-Temporal Analysis of Field Fluctuations (STAFF) Data at the ESA Cluster Science Archive</a>
                        </h1>
                        <p>
                            <div class="term">ResourceID</div>
                            <div class="definition">spase://ESA/NumericalData/Cluster-Rumba/STAFF/CSA/PT0.125S</div>
                        </p>
                        <p>
                            <div class="term">Description</div>
                            <div class="definition">Magnetic field and electric field data products from the Cluster Spatio-Temporal Analysis of Field Fluctuations (STAFF) available from the Cluster Active Archive include: Level 2 calibrated data -- STAFF Waveform Analyzer (STAFF-SC) Complex Spectra of the magnetic field in GSE coordinates (normal mode, up to 12.5 Hz and burst mode up to 225 Hz) with a time resolution of 10 second and a frequency resolution of 0.1 Hz; STAFF-SC Calibrated Magnetic Field WaveForm in ISR2 coordinates (normal mode, 25 Hz sampling and burst mode, 450 Hz sampling); STAFF Spectrum Analyzer (STAFF-SA) Spectral Matrix (8 Hz to 4 KHz) which is the cross-product of the magnetic and electric fileds values computed on-board the spacecraft with time resolutions of 4 seconds and 1 second; and Power Spectral Density (8 Hz to 4 KHz) with time resolutions of 1, 0.125 and 0.25 second.  Level 3 value-added products include STAFF-SA Polarization and Propagation Parameters (8 Hz to 4 KHz).  In the base mode in normal bit rate the auto-spectra are averaged over 1 s, and the complete 25-component matrix is averaged over 4 s for five components. In high bit rate, only the two highest frequency bands are analyzed. In the fast modes, time resolution is 1 s for the cross-spectra, and either 0.125 s or 0.25 s for the auto-spectra.  The physical units for magnetic field spectral power are nT^2 Hz^-1, and electric field spectral power, V^2 m^-2 Hz^-1.  Ancillary data included preliminary spectra, uncalibrated waveform, caveats, and calibration information.  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.</div>
                        </p>
                        <p/>
                    </div>
                </div>
                <div>
                    <p class="right">
                        <a target="_blank" href="/WS/hdp/1/Spase?ResourceID=spase://ESA/NumericalData/Cluster-Rumba/STAFF/CSA/PT0.125S&amp;Format=spase_xml" download="PT0.125S.xml">View XML</a> |
              <a target="_blank" href="https://spase-editor.heliocloud.org/?edit=https://heliophysicsdata.gsfc.nasa.gov/WS/hdp/1/Spase?ResourceID=spase://ESA/NumericalData/Cluster-Rumba/STAFF/CSA/PT0.125S&amp;Format=spase_xml">Edit</a>
                    </p>
                    <h1 class="detail">Details</h1>
                </div>
                <div>
                    <div class="product">
                        <p class="version">Version:2.3.0</p>
                        <h1>NumericalData</h1>
                        <div class="term">ResourceID</div>
                        <div class="definition">spase://ESA/NumericalData/Cluster-Rumba/STAFF/CSA/PT0.125S</div>
                        <div class="term">ResourceHeader</div>
                        <div class="definition">
                            <div class="term">ResourceName</div>
                            <div class="definition">Cluster-Rumba Spatio-Temporal Analysis of Field Fluctuations (STAFF) Data at the ESA Cluster Science Archive</div>
                            <div class="term">AlternateName</div>
                            <div class="definition">Cluster 2 Rumba Spatio-Temporal Analysis of Field Fluctuations (STAFF) Data at the ESA Cluster Active Archive</div>
                            <div class="term">ReleaseDate</div>
                            <div class="definition">2019-05-05 12:34:56Z</div>
                            <div class="term">Description</div>
                            <div class="definition">Magnetic field and electric field data products from the Cluster Spatio-Temporal Analysis of Field Fluctuations (STAFF) available from the Cluster Active Archive include: Level 2 calibrated data -- STAFF Waveform Analyzer (STAFF-SC) Complex Spectra of the magnetic field in GSE coordinates (normal mode, up to 12.5 Hz and burst mode up to 225 Hz) with a time resolution of 10 second and a frequency resolution of 0.1 Hz; STAFF-SC Calibrated Magnetic Field WaveForm in ISR2 coordinates (normal mode, 25 Hz sampling and burst mode, 450 Hz sampling); STAFF Spectrum Analyzer (STAFF-SA) Spectral Matrix (8 Hz to 4 KHz) which is the cross-product of the magnetic and electric fileds values computed on-board the spacecraft with time resolutions of 4 seconds and 1 second; and Power Spectral Density (8 Hz to 4 KHz) with time resolutions of 1, 0.125 and 0.25 second.  Level 3 value-added products include STAFF-SA Polarization and Propagation Parameters (8 Hz to 4 KHz).  In the base mode in normal bit rate the auto-spectra are averaged over 1 s, and the complete 25-component matrix is averaged over 4 s for five components. In high bit rate, only the two highest frequency bands are analyzed. In the fast modes, time resolution is 1 s for the cross-spectra, and either 0.125 s or 0.25 s for the auto-spectra.  The physical units for magnetic field spectral power are nT^2 Hz^-1, and electric field spectral power, V^2 m^-2 Hz^-1.  Ancillary data included preliminary spectra, uncalibrated waveform, caveats, and calibration information.  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.</div>
                            <div class="term">Acknowledgement</div>
                            <div class="definition">Dr. Nicole.Cornilleau-Wehrlin, the STAFF team and the ESA Cluster Active Archive</div>
                            <div class="term">Contacts</div>
                            <div class="definition">
                                <table class="nested" cellspacing="0">
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                                        <th/>
                                        <th class="center">Role</th>
                                        <th class="center">Person</th>
                                        <th class="center">StartDate</th>
                                        <th class="center">StopDate</th>
                                        <th class="center">Note</th>
                                    </tr>
                                    <tbody>
                                        <tr>
                                            <td>1.</td>
                                            <td>PrincipalInvestigator</td>
                                            <td>
                                                <a target="_blank" href="https://spase-metadata.org/SMWG/Person/Nicole.Cornilleau-Wehrlin.html">spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</a>
                                            </td>
                                            <td/>
                                            <td/>
                                            <td/>
                                        </tr>
                                        <tr>
                                            <td>2.</td>
                                            <td>ProjectScientist</td>
                                            <td>
                                                <a target="_blank" href="https://spase-metadata.org/SMWG/Person/Melvyn.L.Goldstein.html">spase://SMWG/Person/Melvyn.L.Goldstein</a>
                                            </td>
                                            <td/>
                                            <td/>
                                            <td/>
                                        </tr>
                                    </tbody>
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                            </div>
                            <div class="definition">
                                <p/>
                                <p/>
                            </div>
                            <div class="term">InformationURL</div>
                            <div class="definition">
                                <div class="term">Name</div>
                                <div class="definition">NSSDC Master Catalog listing for Cluster II Rumba Spatio-Temporal Analysis of Field Fluctuations(STAFF)</div>
                                <div class="term">URL</div>
                                <div class="definition">
                                    <a target="_blank" href="https://nssdc.gsfc.nasa.gov/nmc/experiment/display.action?id=2000-045A-09">https://nssdc.gsfc.nasa.gov/nmc/experiment/display.action?id=2000-045A-09</a>
                                </div>
                                <div class="term">Description</div>
                                <div class="definition">This site provides information concerning the Cluster II Rumba Spatio-Temporal Analysis of Field Fluctuations (STAFF) Instrument.</div>
                            </div>
                            <div class="term">InformationURL</div>
                            <div class="definition">
                                <div class="term">Name</div>
                                <div class="definition">Cluster Science Archive (CSA) Documentation</div>
                                <div class="term">URL</div>
                                <div class="definition">
                                    <a target="_blank" href="https://www.cosmos.esa.int/?project=CLUSTER&amp;page=caa_documentation">https://www.cosmos.esa.int/?project=CLUSTER&amp;page=caa_documentation</a>
                                </div>
                                <div class="term">Description</div>
                                <div class="definition">CAA Instrument User Guides, Calibration Reports and ICDS.</div>
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                            <div class="term">Association</div>
                            <div class="definition">
                                <div class="term">AssociationID</div>
                                <div class="definition">
                                    <a href="https://spase-metadata.org/SMWG/Observatory/Cluster-Rumba.html">spase://SMWG/Observatory/Cluster-Rumba</a>
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                                <div class="term">AssociationType</div>
                                <div class="definition">ObservedBy</div>
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                            <div class="term">PriorIDs</div>
                            <div class="definition">spase://VSPO/NumericalData/Cluster-Rumba/STAFF/CSA/PT0.125S</div>
                        </div>
                        <div class="term">AccessInformation</div>
                        <div class="definition">
                            <div class="term">RepositoryID</div>
                            <div class="definition">
                                <a href="https://spase-metadata.org/SMWG/Repository/CSA.html">spase://SMWG/Repository/CSA</a>
                            </div>
                            <div class="term">Availability</div>
                            <div class="definition">Online</div>
                            <div class="term">AccessRights</div>
                            <div class="definition">Open</div>
                            <div class="term">AccessURL</div>
                            <div class="definition">
                                <div class="term">Name</div>
                                <div class="definition">Access to files at the Cluster Science Archive (CSA)</div>
                                <div class="term">URL</div>
                                <div class="definition">
                                    <a target="_blank" href="https://www.cosmos.esa.int/">https://www.cosmos.esa.int/</a>
                                </div>
                                <div class="term">Description</div>
                                <div class="definition">Cluster II Rumba Spatio-Temporal Analysis of Field Fluctuations (STAFF) data. It's open access but registration is required.</div>
                            </div>
                            <div class="term">Format</div>
                            <div class="definition">CEF</div>
                        </div>
                        <div class="term">ProcessingLevel</div>
                        <div class="definition">Calibrated</div>
                        <div class="term">InstrumentIDs</div>
                        <div class="definition">
                            <a target="_blank" href="https://spase-metadata.org/SMWG/Instrument/Cluster-Rumba/STAFF.html">spase://SMWG/Instrument/Cluster-Rumba/STAFF</a>
                        </div>
                        <div class="term">MeasurementType</div>
                        <div class="definition">MagneticField</div>
                        <div class="term">MeasurementType</div>
                        <div class="definition">ElectricField</div>
                        <div class="term">TemporalDescription</div>
                        <div class="definition">
                            <div class="term">TimeSpan</div>
                            <div class="definition">
                                <div class="term">StartDate</div>
                                <div class="definition">2001-01-01 00:00:00.000</div>
                                <div class="term">RelativeStopDate</div>
                                <div class="definition">-P8M</div>
                            </div>
                            <div class="term">Cadence</div>
                            <div class="definition">PT0.125S</div>
                        </div>
                        <div class="term">ObservedRegion</div>
                        <div class="definition">Earth.Magnetosheath</div>
                        <div class="term">ObservedRegion</div>
                        <div class="definition">Earth.Magnetosphere</div>
                        <div class="term">ObservedRegion</div>
                        <div class="definition">Earth.Magnetosphere.Magnetotail</div>
                        <div class="term">ObservedRegion</div>
                        <div class="definition">Earth.Magnetosphere.Main</div>
                        <div class="term">ObservedRegion</div>
                        <div class="definition">Earth.Magnetosphere.Polar</div>
                        <div class="term">ObservedRegion</div>
                        <div class="definition">Earth.Magnetosphere.RadiationBelt</div>
                        <div class="term">ObservedRegion</div>
                        <div class="definition">Earth.NearSurface.AuroralRegion</div>
                        <div class="term">ObservedRegion</div>
                        <div class="definition">Earth.NearSurface.Ionosphere</div>
                        <div class="term">ObservedRegion</div>
                        <div class="definition">Earth.NearSurface.Plasmasphere</div>
                        <div class="term">ObservedRegion</div>
                        <div class="definition">Earth.NearSurface.PolarCap</div>
                        <div class="term">ObservedRegion</div>
                        <div class="definition">Heliosphere.NearEarth</div>
                    </div>
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