CDPP / CNES

Commit a128b91d4fa6ea541bbef07a2f73eef98e286e51

Authored by Elena.Budnik
1 parent 85e587dc
Exists in master and in 12 other branches amdadev, aschulz, autocommit, bepi_master, bepi_update, branch_q, cleanup_registry, cleanup_registry_master, cleanup_registry_merged, juice_jdc, juno_jade, soar

STAFF

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Instrument/AMDA/Cluster-Rumba/STAFF.xml
  Diff comments   View file @a128b91
@@ -5,22 +5,37 @@ @@ -5,22 +5,37 @@
5 <ResourceID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/STAFF</ResourceID> 5 <ResourceID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/STAFF</ResourceID>
6 <ResourceHeader> 6 <ResourceHeader>
7 <ResourceName>STAFF</ResourceName> 7 <ResourceName>STAFF</ResourceName>
8 - <AlternateName>Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF)</AlternateName>  
9 - <ReleaseDate>2011-02-04T15:37:47Z</ReleaseDate>  
10 - <Description>This experiment (STAFF: Spatio-Temporal Analysis of Field Fluctuations) is one of the five complementary experiments which form the Wave Experiment Consortium (WEC) on Cluster. STAFF consists of: (1) a triaxial boom-mounted search-coil magnetometer to measure the magnetic components of electromagnetic fluctuations (up to 4 KHz); and, (2) a spectrum analyzer to compute the 25 auto- and cross-correlation coefficients of the spectral matrix, using three magnetic and two electric components of the waves. The magnetic waveform (up to either 10 Hz or 180 Hz) is also transmitted. The Z-axis sensor is parallel to the spacecraft spin axis. Each sensor consists of a high-permeability core embedded inside two solenoids. The frequency response of the main winding is flattened by a secondary winding through a flux feedback effect, in the range 40--4000 Hz. Further, the secondary winding is used as a calibration loop to which an external AC signal is applied. In normal bit rate the wave-form data cover the 0.1--10 Hz frequency range, and the spectrum analyzer covers the range 8 Hz to 4 KHz. In high bit rate, the wave-form data cover 0.1--180 Hz and the spectrum analyzer covers 64 Hz to 4 KHz, using only the two highest frequency bands. 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. Other modes are also defined. The analysis will also use electric field waveform data from the EFW (part of WEC), and the hardware of the two instruments was designed to optimize correlation: low-pass filters are identical, sampling frequency is the same, and there is a synchronization signal for simultaneous sampling. The output signals of the STAFF magnetic preamplifiers are also sent to two other instruments: the WBD (part of WEC) and the EDI. Some of the magnetospheric structures to be studied are of small scale, and where the signature duration is of the order 1 s or less, the STAFF search coil data are complementary to those of the fluxgate magnetometer (FGM). 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.</Description> 8 + <AlternateName>Spatio-Temporal Analysis of Magnetic Field Fluctuations</AlternateName>
  9 + <ReleaseDate>2016-11-04T15:37:47Z</ReleaseDate>
  10 + <Description>STAFF is one of the five complementary experiments which form the Wave Experiment Consortium on Cluster. STAFF consists of:
  11 + * a triaxial boom-mounted search-coil magnetometer to measure the magnetic components of electromagnetic fluctuations (up to 4 KHz); and,
  12 + * a spectrum analyzer to compute the 25 auto- and cross-correlation coefficients of the spectral matrix, using three magnetic and two electric components of the waves.
  13 +
  14 + The magnetic waveform (up to either 10 Hz or 180 Hz) is also transmitted. The Z-axis sensor is parallel to the spacecraft spin axis.
  15 + Each sensor consists of a high-permeability core embedded inside two solenoids. The frequency response of the main winding is flattened by a secondary winding through a flux feedback effect, in the range 40--4000 Hz.</Description>
  16 + <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
11 <Contact> 17 <Contact>
12 - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID> 18 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
13 <Role>PrincipalInvestigator</Role> 19 <Role>PrincipalInvestigator</Role>
14 </Contact> 20 </Contact>
15 <InformationURL> 21 <InformationURL>
  22 + <Name>ESA web page</Name>
  23 + <URL>http://sci.esa.int/jump.cfm?oid=33024</URL>
  24 + <Description>STAFF</Description>
  25 + </InformationURL>
  26 + <InformationURL>
16 <Name>NSSDC's Master Catalog</Name> 27 <Name>NSSDC's Master Catalog</Name>
17 <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-045A&amp;ex=9</URL> 28 <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-045A&amp;ex=9</URL>
18 - <Description>Information about the Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) experiment on the Cluster 2/FM5 (Rumba) mission.</Description> 29 + <Description>Information about STAFF experiment on the Cluster 2/FM5 (Rumba) mission.</Description>
19 </InformationURL> 30 </InformationURL>
20 <PriorID>spase://SMWG/Instrument/Cluster2-Rumba/STAFF</PriorID> 31 <PriorID>spase://SMWG/Instrument/Cluster2-Rumba/STAFF</PriorID>
21 </ResourceHeader> 32 </ResourceHeader>
22 - <InstrumentType>Magnetometer</InstrumentType>  
23 - <InvestigationName>Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) on Cluster 2/FM5 (Rumba)</InvestigationName> 33 + <InstrumentType>SearchCoil</InstrumentType>
  34 + <InvestigationName></InvestigationName>
  35 + <OperatingSpan>
  36 + <StartDate>2000-12-01T00:00:00</StartDate>
  37 + <Note>Start of full orbit coverage: 2002-06-01T00:00:00</Note>
  38 + </OperatingSpan>
24 <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Rumba</ObservatoryID> 39 <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Rumba</ObservatoryID>
25 </Instrument> 40 </Instrument>
26 </Spase> 41 </Spase>
Instrument/AMDA/Cluster-Salsa/STAFF.xml
  Diff comments   View file @a128b91
@@ -6,21 +6,36 @@ @@ -6,21 +6,36 @@
6 <ResourceHeader> 6 <ResourceHeader>
7 <ResourceName>STAFF</ResourceName> 7 <ResourceName>STAFF</ResourceName>
8 <AlternateName>Spatio-Temporal Analysis of Magnetic Field Fluctuations</AlternateName> 8 <AlternateName>Spatio-Temporal Analysis of Magnetic Field Fluctuations</AlternateName>
9 - <ReleaseDate>2011-02-04T15:37:33Z</ReleaseDate>  
10 - <Description>This experiment (STAFF: Spatio-Temporal Analysis of Field Fluctuations) is one of the five complementary experiments which form the Wave Experiment Consortium (WEC) on Cluster. STAFF consists of: (1) a triaxial boom-mounted search-coil magnetometer to measure the magnetic components of electromagnetic fluctuations (up to 4 KHz); and, (2) a spectrum analyzer to compute the 25 auto- and cross-correlation coefficients of the spectral matrix, using three magnetic and two electric components of the waves. The magnetic waveform (up to either 10 Hz or 180 Hz) is also transmitted. The Z-axis sensor is parallel to the spacecraft spin axis. Each sensor consists of a high-permeability core embedded inside two solenoids. The frequency response of the main winding is flattened by a secondary winding through a flux feedback effect, in the range 40--4000 Hz. Further, the secondary winding is used as a calibration loop to which an external AC signal is applied. In normal bit rate the wave-form data cover the 0.1--10 Hz frequency range, and the spectrum analyzer covers the range 8 Hz to 4 KHz. In high bit rate, the wave-form data cover 0.1--180 Hz and the spectrum analyzer covers 64 Hz to 4 KHz, using only the two highest frequency bands. 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. Other modes are also defined. The analysis will also use electric field waveform data from the EFW (part of WEC), and the hardware of the two instruments was designed to optimize correlation: low-pass filters are identical, sampling frequency is the same, and there is a synchronization signal for simultaneous sampling. The output signals of the STAFF magnetic preamplifiers are also sent to two other instruments: the WBD (part of WEC) and the EDI. Some of the magnetospheric structures to be studied are of small scale, and where the signature duration is of the order 1 s or less, the STAFF search coil data are complementary to those of the fluxgate magnetometer (FGM). 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.</Description> 9 + <ReleaseDate>2016-11-04T15:37:47Z</ReleaseDate>
  10 + <Description>STAFF is one of the five complementary experiments which form the Wave Experiment Consortium on Cluster. STAFF consists of:
  11 + * a triaxial boom-mounted search-coil magnetometer to measure the magnetic components of electromagnetic fluctuations (up to 4 KHz); and,
  12 + * a spectrum analyzer to compute the 25 auto- and cross-correlation coefficients of the spectral matrix, using three magnetic and two electric components of the waves.
  13 +
  14 + The magnetic waveform (up to either 10 Hz or 180 Hz) is also transmitted. The Z-axis sensor is parallel to the spacecraft spin axis.
  15 + Each sensor consists of a high-permeability core embedded inside two solenoids. The frequency response of the main winding is flattened by a secondary winding through a flux feedback effect, in the range 40--4000 Hz.</Description>
  16 + <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
11 <Contact> 17 <Contact>
12 - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID> 18 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
13 <Role>PrincipalInvestigator</Role> 19 <Role>PrincipalInvestigator</Role>
14 </Contact> 20 </Contact>
15 <InformationURL> 21 <InformationURL>
  22 + <Name>ESA web page</Name>
  23 + <URL>http://sci.esa.int/jump.cfm?oid=33024</URL>
  24 + <Description>STAFF</Description>
  25 + </InformationURL>
  26 + <InformationURL>
16 <Name>NSSDC's Master Catalog</Name> 27 <Name>NSSDC's Master Catalog</Name>
17 - <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-041B&amp;ex=9</URL>  
18 - <Description>Information about the Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) experiment on the Cluster 2/FM6 (Salsa) mission.</Description> 28 + <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-045A&amp;ex=9</URL>
  29 + <Description>Information about STAFF experiment on the Cluster 2/FM6 (Salsa) mission.</Description>
19 </InformationURL> 30 </InformationURL>
20 <PriorID>spase://SMWG/Instrument/Cluster2-Salsa/STAFF</PriorID> 31 <PriorID>spase://SMWG/Instrument/Cluster2-Salsa/STAFF</PriorID>
21 </ResourceHeader> 32 </ResourceHeader>
22 - <InstrumentType>Magnetometer</InstrumentType>  
23 - <InvestigationName>Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) on Cluster 2/FM6 (Salsa)</InvestigationName> 33 + <InstrumentType>SearchCoil</InstrumentType>
  34 + <InvestigationName></InvestigationName>
  35 + <OperatingSpan>
  36 + <StartDate>2000-12-01T00:00:00</StartDate>
  37 + <Note>Start of full orbit coverage: 2002-06-01T00:00:00</Note>
  38 + </OperatingSpan>
24 <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Salsa</ObservatoryID> 39 <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Salsa</ObservatoryID>
25 </Instrument> 40 </Instrument>
26 </Spase> 41 </Spase>
Instrument/AMDA/Cluster-Samba/STAFF.xml
  Diff comments   View file @a128b91
@@ -6,21 +6,37 @@ @@ -6,21 +6,37 @@
6 <ResourceHeader> 6 <ResourceHeader>
7 <ResourceName>STAFF</ResourceName> 7 <ResourceName>STAFF</ResourceName>
8 <AlternateName>Spatio-Temporal Analysis of Magnetic Field Fluctuations</AlternateName> 8 <AlternateName>Spatio-Temporal Analysis of Magnetic Field Fluctuations</AlternateName>
9 - <ReleaseDate>2011-02-04T15:37:07Z</ReleaseDate>  
10 - <Description>This experiment (STAFF: Spatio-Temporal Analysis of Field Fluctuations) is one of the five complementary experiments which form the Wave Experiment Consortium (WEC) on Cluster. STAFF consists of: (1) a triaxial boom-mounted search-coil magnetometer to measure the magnetic components of electromagnetic fluctuations (up to 4 KHz); and, (2) a spectrum analyzer to compute the 25 auto- and cross-correlation coefficients of the spectral matrix, using three magnetic and two electric components of the waves. The magnetic waveform (up to either 10 Hz or 180 Hz) is also transmitted. The Z-axis sensor is parallel to the spacecraft spin axis. Each sensor consists of a high-permeability core embedded inside two solenoids. The frequency response of the main winding is flattened by a secondary winding through a flux feedback effect, in the range 40--4000 Hz. Further, the secondary winding is used as a calibration loop to which an external AC signal is applied. In normal bit rate the wave-form data cover the 0.1--10 Hz frequency range, and the spectrum analyzer covers the range 8 Hz to 4 KHz. In high bit rate, the wave-form data cover 0.1--180 Hz and the spectrum analyzer covers 64 Hz to 4 KHz, using only the two highest frequency bands. 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. Other modes are also defined. The analysis will also use electric field waveform data from the EFW (part of WEC), and the hardware of the two instruments was designed to optimize correlation: low-pass filters are identical, sampling frequency is the same, and there is a synchronization signal for simultaneous sampling. The output signals of the STAFF magnetic preamplifiers are also sent to two other instruments: the WBD (part of WEC) and the EDI. Some of the magnetospheric structures to be studied are of small scale, and where the signature duration is of the order 1 s or less, the STAFF search coil data are complementary to those of the fluxgate magnetometer (FGM). 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.</Description> 9 + <ReleaseDate>2016-11-04T15:37:47Z</ReleaseDate>
  10 + <Description>STAFF is one of the five complementary experiments which form the Wave Experiment Consortium on Cluster. STAFF consists of:
  11 + * a triaxial boom-mounted search-coil magnetometer to measure the magnetic components of electromagnetic fluctuations (up to 4 KHz); and,
  12 + * a spectrum analyzer to compute the 25 auto- and cross-correlation coefficients of the spectral matrix, using three magnetic and two electric components of the waves.
  13 +
  14 + The magnetic waveform (up to either 10 Hz or 180 Hz) is also transmitted. The Z-axis sensor is parallel to the spacecraft spin axis.
  15 + Each sensor consists of a high-permeability core embedded inside two solenoids. The frequency response of the main winding is flattened by a secondary winding through a flux feedback effect, in the range 40--4000 Hz.</Description>
  16 + <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
11 <Contact> 17 <Contact>
12 - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID> 18 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
13 <Role>PrincipalInvestigator</Role> 19 <Role>PrincipalInvestigator</Role>
14 </Contact> 20 </Contact>
15 <InformationURL> 21 <InformationURL>
  22 + <Name>ESA web page</Name>
  23 + <URL>http://sci.esa.int/jump.cfm?oid=33024</URL>
  24 + <Description>STAFF</Description>
  25 + </InformationURL>
  26 + <InformationURL>
16 <Name>NSSDC's Master Catalog</Name> 27 <Name>NSSDC's Master Catalog</Name>
17 - <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-041A&amp;ex=9</URL>  
18 - <Description>Information about the Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) experiment on the Cluster 2/FM7 (Samba) mission.</Description> 28 + <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-045A&amp;ex=9</URL>
  29 + <Description>Information about STAFF experiment on the Cluster 2/FM7 (Samba) mission.</Description>
19 </InformationURL> 30 </InformationURL>
20 <PriorID>spase://SMWG/Instrument/Cluster2-Samba/STAFF</PriorID> 31 <PriorID>spase://SMWG/Instrument/Cluster2-Samba/STAFF</PriorID>
21 </ResourceHeader> 32 </ResourceHeader>
22 - <InstrumentType>Magnetometer</InstrumentType>  
23 - <InvestigationName>Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) on Cluster 2/FM7 (Samba)</InvestigationName> 33 + <InstrumentType>SearchCoil</InstrumentType>
  34 + <InvestigationName></InvestigationName>
  35 + <OperatingSpan>
  36 + <StartDate>2000-12-01T00:00:00</StartDate>
  37 + <Note>Start of full orbit coverage: 2002-06-01T00:00:00</Note>
  38 + <Note>C3 spacecraft tilt by 40ยฐ during one month: 2008-05-01T00:00:00</Note>
  39 + </OperatingSpan>
24 <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Samba</ObservatoryID> 40 <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Samba</ObservatoryID>
25 </Instrument> 41 </Instrument>
26 </Spase> 42 </Spase>
Instrument/AMDA/Cluster-Tango/STAFF.xml
  Diff comments   View file @a128b91
@@ -6,21 +6,36 @@ @@ -6,21 +6,36 @@
6 <ResourceHeader> 6 <ResourceHeader>
7 <ResourceName>STAFF</ResourceName> 7 <ResourceName>STAFF</ResourceName>
8 <AlternateName>Spatio-Temporal Analysis of Magnetic Field Fluctuations</AlternateName> 8 <AlternateName>Spatio-Temporal Analysis of Magnetic Field Fluctuations</AlternateName>
9 - <ReleaseDate>2011-02-04T15:37:19Z</ReleaseDate>  
10 - <Description>This experiment (STAFF: Spatio-Temporal Analysis of Field Fluctuations) is one of the five complementary experiments which form the Wave Experiment Consortium (WEC) on Cluster. STAFF consists of: (1) a triaxial boom-mounted search-coil magnetometer to measure the magnetic components of electromagnetic fluctuations (up to 4 KHz); and, (2) a spectrum analyzer to compute the 25 auto- and cross-correlation coefficients of the spectral matrix, using three magnetic and two electric components of the waves. The magnetic waveform (up to either 10 Hz or 180 Hz) is also transmitted. The Z-axis sensor is parallel to the spacecraft spin axis. Each sensor consists of a high-permeability core embedded inside two solenoids. The frequency response of the main winding is flattened by a secondary winding through a flux feedback effect, in the range 40--4000 Hz. Further, the secondary winding is used as a calibration loop to which an external AC signal is applied. In normal bit rate the wave-form data cover the 0.1--10 Hz frequency range, and the spectrum analyzer covers the range 8 Hz to 4 KHz. In high bit rate, the wave-form data cover 0.1--180 Hz and the spectrum analyzer covers 64 Hz to 4 KHz, using only the two highest frequency bands. 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. Other modes are also defined. The analysis will also use electric field waveform data from the EFW (part of WEC), and the hardware of the two instruments was designed to optimize correlation: low-pass filters are identical, sampling frequency is the same, and there is a synchronization signal for simultaneous sampling. The output signals of the STAFF magnetic preamplifiers are also sent to two other instruments: the WBD (part of WEC) and the EDI. Some of the magnetospheric structures to be studied are of small scale, and where the signature duration is of the order 1 s or less, the STAFF search coil data are complementary to those of the fluxgate magnetometer (FGM). 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.</Description> 9 + <ReleaseDate>2016-11-04T15:37:47Z</ReleaseDate>
  10 + <Description>STAFF is one of the five complementary experiments which form the Wave Experiment Consortium on Cluster. STAFF consists of:
  11 + * a triaxial boom-mounted search-coil magnetometer to measure the magnetic components of electromagnetic fluctuations (up to 4 KHz); and,
  12 + * a spectrum analyzer to compute the 25 auto- and cross-correlation coefficients of the spectral matrix, using three magnetic and two electric components of the waves.
  13 +
  14 + The magnetic waveform (up to either 10 Hz or 180 Hz) is also transmitted. The Z-axis sensor is parallel to the spacecraft spin axis.
  15 + Each sensor consists of a high-permeability core embedded inside two solenoids. The frequency response of the main winding is flattened by a secondary winding through a flux feedback effect, in the range 40--4000 Hz.</Description>
  16 + <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
11 <Contact> 17 <Contact>
12 - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID> 18 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
13 <Role>PrincipalInvestigator</Role> 19 <Role>PrincipalInvestigator</Role>
14 </Contact> 20 </Contact>
15 <InformationURL> 21 <InformationURL>
  22 + <Name>ESA web page</Name>
  23 + <URL>http://sci.esa.int/jump.cfm?oid=33024</URL>
  24 + <Description>STAFF</Description>
  25 + </InformationURL>
  26 + <InformationURL>
16 <Name>NSSDC's Master Catalog</Name> 27 <Name>NSSDC's Master Catalog</Name>
17 - <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-045B&amp;ex=9</URL>  
18 - <Description>Information about the Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) experiment on the Cluster 2/FM8 (Tango) mission.</Description> 28 + <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-045A&amp;ex=9</URL>
  29 + <Description>Information about STAFF experiment on the Cluster 2/FM8 (Tango) mission.</Description>
19 </InformationURL> 30 </InformationURL>
20 <PriorID>spase://SMWG/Instrument/Cluster2-Tango/STAFF</PriorID> 31 <PriorID>spase://SMWG/Instrument/Cluster2-Tango/STAFF</PriorID>
21 </ResourceHeader> 32 </ResourceHeader>
22 - <InstrumentType>Magnetometer</InstrumentType>  
23 - <InvestigationName>Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) on Cluster 2/FM8 (Tango)</InvestigationName> 33 + <InstrumentType>SearchCoil</InstrumentType>
  34 + <InvestigationName></InvestigationName>
  35 + <OperatingSpan>
  36 + <StartDate>2000-12-01T00:00:00</StartDate>
  37 + <Note>Start of full orbit coverage: 2002-06-01T00:00:00</Note>
  38 + </OperatingSpan>
24 <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Tango</ObservatoryID> 39 <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Tango</ObservatoryID>
25 </Instrument> 40 </Instrument>
26 </Spase> 41 </Spase>
NumericalData/AMDA/ACE/MFI/ace-mag-real.xml
  Diff comments   View file @a128b91
@@ -51,7 +51,7 @@ @@ -51,7 +51,7 @@
51 <TemporalDescription> 51 <TemporalDescription>
52 <TimeSpan> 52 <TimeSpan>
53 <StartDate>2014-01-06T00:00:00Z</StartDate> 53 <StartDate>2014-01-06T00:00:00Z</StartDate>
54 - <StopDate>2016-11-10T00:59:59Z</StopDate> 54 + <StopDate>2016-11-21T00:59:59Z</StopDate>
55 </TimeSpan> 55 </TimeSpan>
56 <Cadence>PT60S</Cadence> 56 <Cadence>PT60S</Cadence>
57 </TemporalDescription> 57 </TemporalDescription>
NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml
  Diff comments   View file @a128b91
@@ -44,7 +44,7 @@ @@ -44,7 +44,7 @@
44 <TemporalDescription> 44 <TemporalDescription>
45 <TimeSpan> 45 <TimeSpan>
46 <StartDate>2014-01-06T00:00:00Z</StartDate> 46 <StartDate>2014-01-06T00:00:00Z</StartDate>
47 - <StopDate>2016-11-10T00:59:59Z</StopDate> 47 + <StopDate>2016-11-21T00:59:59Z</StopDate>
48 </TimeSpan> 48 </TimeSpan>
49 <Cadence>PT60S</Cadence> 49 <Cadence>PT60S</Cadence>
50 </TemporalDescription> 50 </TemporalDescription>
NumericalData/AMDA/Cluster/Cluster1/STAFF/clust1-sta-pp.xml
  Diff comments   View file @a128b91
@@ -7,28 +7,29 @@ @@ -7,28 +7,29 @@
7 <ResourceName>prime parameters</ResourceName> 7 <ResourceName>prime parameters</ResourceName>
8 <AlternateName>Cluster 1 Prime Parameter STAFF Data</AlternateName> 8 <AlternateName>Cluster 1 Prime Parameter STAFF Data</AlternateName>
9 <ReleaseDate>2015-10-19T16:14:44Z</ReleaseDate> 9 <ReleaseDate>2015-10-19T16:14:44Z</ReleaseDate>
10 - <Description>The Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) experiment provides  
11 - magnetic field power spectral density values parallel and perpendicular to the magnetic field and  
12 - the electric field power spectral density values for several frequency ranges.  
13 - For more details of the Cluster mission, the spacecraft, and its instruments, see the report  
14 - Cluster: mission, payload and supporting activities, March 1993, ESA SP-1159,  
15 - and the included article The STAFF (Spatio-Temporal Analysis of Field Fluctuations) Experiment  
16 - for the Cluster Mission, by N. Cornilleau-Wehrlin et al., from which this information was obtained. 10 + <Description>
  11 + 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.
  12 +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.
  13 +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.
  14 +The Spectrum Analyser can work in different modes, in Burst Mode the analysis is performed in
  15 +the frequency range 64 Hz - 4 kHz.
  16 +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.
  17 +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.
17 </Description> 18 </Description>
18 - <Acknowledgement>ESA, Nicole Cornilleau-Wehrlin</Acknowledgement> 19 + <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
19 <Contact> 20 <Contact>
20 - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID> 21 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
21 <Role>PrincipalInvestigator</Role> 22 <Role>PrincipalInvestigator</Role>
22 </Contact> 23 </Contact>
23 - <Contact>  
24 - <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>  
25 - <Role>TechnicalContact</Role>  
26 - </Contact> 24 + <InformationURL>
  25 + <Name>ESA web page</Name>
  26 + <URL>http://www.cosmos.esa.int/web/csa/documentation</URL>
  27 + <Description>This site contains STAFF data documentation</Description>
  28 + </InformationURL>
27 <InformationURL> 29 <InformationURL>
28 - <Name>NSSDC Master Catalog listing for Cluster II Rumba Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF)</Name> 30 + <Name>NSSDC Master Catalog listing for Cluster II Rumba STAFF</Name>
29 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-09</URL> 31 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-09</URL>
30 - <Description>This site provides information concerning the Cluster II Rumba Spatio-Temporal  
31 - Analysis of Magnetic Field Fluctuations Instrument.</Description> 32 + <Description>This site provides information concerning the Cluster STAFF Instrument.</Description>
32 </InformationURL> 33 </InformationURL>
33 </ResourceHeader> 34 </ResourceHeader>
34 <AccessInformation> 35 <AccessInformation>
@@ -39,14 +40,10 @@ @@ -39,14 +40,10 @@
39 <Name>AMDA at CDPP</Name> 40 <Name>AMDA at CDPP</Name>
40 <URL>http://amda.cdpp.eu</URL> 41 <URL>http://amda.cdpp.eu</URL>
41 </AccessURL> 42 </AccessURL>
42 - <Format>NetCDF</Format>  
43 - <Acknowledgement>NASA, Nicole Cornilleau-Wehrlin</Acknowledgement> 43 + <Format>NetCDF</Format>
44 </AccessInformation> 44 </AccessInformation>
45 <ProviderName>CSDS-CNES</ProviderName> 45 <ProviderName>CSDS-CNES</ProviderName>
46 <ProcessingLevel>Calibrated</ProcessingLevel> 46 <ProcessingLevel>Calibrated</ProcessingLevel>
47 - <ProviderResourceName>Cluster II Rumba Prime Parameter Spatio-Temporal Analysis of  
48 - Magnetic Field Fluctuations (STAFF) Data</ProviderResourceName>  
49 - <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>  
50 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/STAFF</InstrumentID> 47 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/STAFF</InstrumentID>
51 <MeasurementType>ElectricField</MeasurementType> 48 <MeasurementType>ElectricField</MeasurementType>
52 <MeasurementType>MagneticField</MeasurementType> 49 <MeasurementType>MagneticField</MeasurementType>
@@ -57,9 +54,9 @@ @@ -57,9 +54,9 @@
57 <StopDate>2012-12-31T23:59:48Z</StopDate> 54 <StopDate>2012-12-31T23:59:48Z</StopDate>
58 </TimeSpan> 55 </TimeSpan>
59 <Cadence>PT4S</Cadence> 56 <Cadence>PT4S</Cadence>
60 - </TemporalDescription>  
61 - <ObservedRegion>Earth.Magnetosheath</ObservedRegion> 57 + </TemporalDescription>
62 <ObservedRegion>Earth.Magnetosphere</ObservedRegion> 58 <ObservedRegion>Earth.Magnetosphere</ObservedRegion>
  59 + <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
63 <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion> 60 <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion>
64 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion> 61 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion>
65 <ObservedRegion>Earth.Magnetosphere.Polar</ObservedRegion> 62 <ObservedRegion>Earth.Magnetosphere.Polar</ObservedRegion>
@@ -81,11 +78,9 @@ @@ -81,11 +78,9 @@
81 <Keyword>magnetotail</Keyword> 78 <Keyword>magnetotail</Keyword>
82 <Keyword>lobe</Keyword> 79 <Keyword>lobe</Keyword>
83 <Parameter> 80 <Parameter>
84 - <Name>Magnetic Field Spectral Density (1-10 Hz)</Name> 81 + <Name>b spectral density (1-10 Hz)</Name>
85 <ParameterKey>c1_sta_f1</ParameterKey> 82 <ParameterKey>c1_sta_f1</ParameterKey>
86 - <Description>Cluster II Rumba Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
87 - Fluctuations (STAFF) magnetic field spectral power as measured by the onboard Cluster  
88 - Fluxgate Magnetometer (FGM) in the 1-10 Hz (f1) frequency range at spin time resolution 83 + <Description>Magnetic field spectral power in the 1-10 Hz (f1) at spin time resolution (parallel and perp components)
89 </Description> 84 </Description>
90 <Ucd>phys.flux.density;phys.magField</Ucd> 85 <Ucd>phys.flux.density;phys.magField</Ucd>
91 <Cadence>PT4S</Cadence> 86 <Cadence>PT4S</Cadence>
@@ -97,7 +92,7 @@ @@ -97,7 +92,7 @@
97 <Structure> 92 <Structure>
98 <Size>2</Size> 93 <Size>2</Size>
99 <Element> 94 <Element>
100 - <Name>Magnetic Field Spectral Density Parallel to Bo (1-10 Hz)</Name> 95 + <Name>parallel to b0</Name>
101 <Index>1</Index> 96 <Index>1</Index>
102 <ParameterKey>c1_sta_f1(0)</ParameterKey> 97 <ParameterKey>c1_sta_f1(0)</ParameterKey>
103 <ValidMin>1.0000e-7</ValidMin> 98 <ValidMin>1.0000e-7</ValidMin>
@@ -109,7 +104,7 @@ @@ -109,7 +104,7 @@
109 </RenderingHints> 104 </RenderingHints>
110 </Element> 105 </Element>
111 <Element> 106 <Element>
112 - <Name>Magnetic Field Spectral Density Perpendicular to Bo (1-10 Hz)</Name> 107 + <Name>perpendicular to b0</Name>
113 <Index>2</Index> 108 <Index>2</Index>
114 <ParameterKey>c1_sta_f1(1)</ParameterKey> 109 <ParameterKey>c1_sta_f1(1)</ParameterKey>
115 <ValidMin>1.0000e-7</ValidMin> 110 <ValidMin>1.0000e-7</ValidMin>
@@ -119,7 +114,7 @@ @@ -119,7 +114,7 @@
119 <ScaleMin>1.0000e-6</ScaleMin> 114 <ScaleMin>1.0000e-6</ScaleMin>
120 <ScaleMax>1</ScaleMax> 115 <ScaleMax>1</ScaleMax>
121 </RenderingHints> 116 </RenderingHints>
122 - </Element> 117 + </Element>
123 </Structure> 118 </Structure>
124 <FillValue>-1.0000e+31</FillValue> 119 <FillValue>-1.0000e+31</FillValue>
125 <Field> 120 <Field>
@@ -134,11 +129,9 @@ @@ -134,11 +129,9 @@
134 </Parameter> 129 </Parameter>
135 130
136 <Parameter> 131 <Parameter>
137 - <Name>Magnetic Field Spectral Density (10-180 Hz)</Name> 132 + <Name>b spectral density (10-180 Hz)</Name>
138 <ParameterKey>c1_sta_f2</ParameterKey> 133 <ParameterKey>c1_sta_f2</ParameterKey>
139 - <Description>Cluster II Rumba Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
140 - Fluctuations (STAFF) magnetic field spectral power as measured by the onboard Cluster  
141 - Fluxgate Magnetometer (FGM) in the 10-180 Hz (f2) frequency range at spin time resolution 134 + <Description>Magnetic field spectral power in the 10-180 Hz (f2) at spin time resolution (parallel and perp components)
142 </Description> 135 </Description>
143 <Ucd>phys.flux.density;phys.magField</Ucd> 136 <Ucd>phys.flux.density;phys.magField</Ucd>
144 <Cadence>PT4S</Cadence> 137 <Cadence>PT4S</Cadence>
@@ -150,7 +143,7 @@ @@ -150,7 +143,7 @@
150 <Structure> 143 <Structure>
151 <Size>2</Size> 144 <Size>2</Size>
152 <Element> 145 <Element>
153 - <Name>Magnetic Field Spectral Density Parallel to Bo (10-180 Hz)</Name> 146 + <Name>parallel to b0</Name>
154 <Index>1</Index> 147 <Index>1</Index>
155 <ParameterKey>c1_sta_f2(0)</ParameterKey> 148 <ParameterKey>c1_sta_f2(0)</ParameterKey>
156 <ValidMin>1.0000e-9</ValidMin> 149 <ValidMin>1.0000e-9</ValidMin>
@@ -162,7 +155,7 @@ @@ -162,7 +155,7 @@
162 </RenderingHints> 155 </RenderingHints>
163 </Element> 156 </Element>
164 <Element> 157 <Element>
165 - <Name>Magnetic Field Spectral Density Perpendicular to Bo (10-180 Hz)</Name> 158 + <Name>perpendicular to b0</Name>
166 <Index>2</Index> 159 <Index>2</Index>
167 <ParameterKey>c1_sta_f2(1)</ParameterKey> 160 <ParameterKey>c1_sta_f2(1)</ParameterKey>
168 <ValidMin>1.0000e-9</ValidMin> 161 <ValidMin>1.0000e-9</ValidMin>
@@ -186,11 +179,9 @@ @@ -186,11 +179,9 @@
186 </Field> 179 </Field>
187 </Parameter> 180 </Parameter>
188 <Parameter> 181 <Parameter>
189 - <Name>Magnetic Field Spectral Density (180-4000 Hz)</Name> 182 + <Name>b spectral density (180-4000 Hz)</Name>
190 <ParameterKey>c1_sta_f3</ParameterKey> 183 <ParameterKey>c1_sta_f3</ParameterKey>
191 - <Description>Cluster II Rumba Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
192 - Fluctuations (STAFF) magnetic field spectral power as measured by the onboard Cluster  
193 - Fluxgate Magnetometer (FGM) in the 180-4000 Hz (f3) frequency range at spin time resolution 184 + <Description> Magnetic field spectral power in the 80-4000 Hz (f3) at spin time resolution (parallel and perp components)
194 </Description> 185 </Description>
195 <Ucd>phys.flux.density;phys.magField</Ucd> 186 <Ucd>phys.flux.density;phys.magField</Ucd>
196 <Cadence>PT4S</Cadence> 187 <Cadence>PT4S</Cadence>
@@ -202,7 +193,7 @@ @@ -202,7 +193,7 @@
202 <Structure> 193 <Structure>
203 <Size>2</Size> 194 <Size>2</Size>
204 <Element> 195 <Element>
205 - <Name>Magnetic Field Spectral Density Parallel to Bo (180-4000 Hz)</Name> 196 + <Name>parallel to b0</Name>
206 <Index>1</Index> 197 <Index>1</Index>
207 <ParameterKey>c1_sta_f3(0)</ParameterKey> 198 <ParameterKey>c1_sta_f3(0)</ParameterKey>
208 <ValidMin>1.0000e-11</ValidMin> 199 <ValidMin>1.0000e-11</ValidMin>
@@ -214,7 +205,7 @@ @@ -214,7 +205,7 @@
214 </RenderingHints> 205 </RenderingHints>
215 </Element> 206 </Element>
216 <Element> 207 <Element>
217 - <Name>Magnetic Field Spectral Density Perpendicular to Bo (180-4000 Hz)</Name> 208 + <Name>perpendicular to b0</Name>
218 <Index>2</Index> 209 <Index>2</Index>
219 <ParameterKey>c1_sta_f3(1)</ParameterKey> 210 <ParameterKey>c1_sta_f3(1)</ParameterKey>
220 <ValidMin>1.0000e-9</ValidMin> 211 <ValidMin>1.0000e-9</ValidMin>
@@ -236,14 +227,11 @@ @@ -236,14 +227,11 @@
236 <Units>Hz</Units> 227 <Units>Hz</Units>
237 </FrequencyRange> 228 </FrequencyRange>
238 </Field> 229 </Field>
239 - </Parameter>  
240 - 230 + </Parameter>
241 <Parameter> 231 <Parameter>
242 - <Name>Electric Field Spectral Density (10-180 Hz)</Name> 232 + <Name>e spectral density (10-180 Hz)</Name>
243 <ParameterKey>c1_stae_f2</ParameterKey> 233 <ParameterKey>c1_stae_f2</ParameterKey>
244 - <Description>Cluster II Rumba Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
245 - Fluctuations (STAFF) electric field spectral power in the 10-180 Hz (f2)  
246 - frequency range at spin time resolution 234 + <Description> Electric field spectral power in the 10-180 Hz (f2) frequency range at spin time resolution.
247 </Description> 235 </Description>
248 <Ucd>phys.flux.density;phys.electField</Ucd> 236 <Ucd>phys.flux.density;phys.electField</Ucd>
249 <Cadence>PT4S</Cadence> 237 <Cadence>PT4S</Cadence>
@@ -269,11 +257,9 @@ @@ -269,11 +257,9 @@
269 </Field> 257 </Field>
270 </Parameter> 258 </Parameter>
271 <Parameter> 259 <Parameter>
272 - <Name>Electric Field Spectral Density (180-4000 Hz)</Name> 260 + <Name>e spectral density (180-4000 Hz)</Name>
273 <ParameterKey>c1_stae_f3</ParameterKey> 261 <ParameterKey>c1_stae_f3</ParameterKey>
274 - <Description>Cluster II Rumba Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
275 - Fluctuations (STAFF) electric field spectral power in the 180-4000 Hz (f3)  
276 - frequency range at spin time resolution 262 + <Description>Electric field spectral power in the 180-4000 Hz (f3) frequency range at spin time resolution.
277 </Description> 263 </Description>
278 <Ucd>phys.flux.density;phys.electField</Ucd> 264 <Ucd>phys.flux.density;phys.electField</Ucd>
279 <Cadence>PT4S</Cadence> 265 <Cadence>PT4S</Cadence>
NumericalData/AMDA/Cluster/Cluster2/STAFF/clust2-sta-pp.xml
  Diff comments   View file @a128b91
@@ -6,30 +6,31 @@ @@ -6,30 +6,31 @@
6 <ResourceHeader> 6 <ResourceHeader>
7 <ResourceName>prime parameters</ResourceName> 7 <ResourceName>prime parameters</ResourceName>
8 <AlternateName>Cluster 2 Prime Parameter STAFF Data</AlternateName> 8 <AlternateName>Cluster 2 Prime Parameter STAFF Data</AlternateName>
9 - <ReleaseDate>2015-10-19T17:51:44Z</ReleaseDate>  
10 - <Description>The Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) experiment provides  
11 - magnetic field power spectral density values parallel and perpendicular to the magnetic field and  
12 - the electric field power spectral density values for several frequency ranges.  
13 - For more details of the Cluster mission, the spacecraft, and its instruments, see the report  
14 - Cluster: mission, payload and supporting activities, March 1993, ESA SP-1159,  
15 - and the included article The STAFF (Spatio-Temporal Analysis of Field Fluctuations) Experiment  
16 - for the Cluster Mission, by N. Cornilleau-Wehrlin et al., from which this information was obtained. 9 + <ReleaseDate>2015-10-19T16:14:44Z</ReleaseDate>
  10 + <Description>
  11 + 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.
  12 +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.
  13 +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.
  14 +The Spectrum Analyser can work in different modes, in Burst Mode the analysis is performed in
  15 +the frequency range 64 Hz - 4 kHz.
  16 +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.
  17 +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.
17 </Description> 18 </Description>
18 - <Acknowledgement>ESA, Nicole Cornilleau-Wehrlin</Acknowledgement> 19 + <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
19 <Contact> 20 <Contact>
20 - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID> 21 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
21 <Role>PrincipalInvestigator</Role> 22 <Role>PrincipalInvestigator</Role>
22 </Contact> 23 </Contact>
23 - <Contact>  
24 - <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>  
25 - <Role>TechnicalContact</Role>  
26 - </Contact> 24 + <InformationURL>
  25 + <Name>ESA web page</Name>
  26 + <URL>http://www.cosmos.esa.int/web/csa/documentation</URL>
  27 + <Description>This site contains STAFF data documentation</Description>
  28 + </InformationURL>
27 <InformationURL> 29 <InformationURL>
28 - <Name>NSSDC Master Catalog listing for Cluster II Salsa Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF)</Name> 30 + <Name>NSSDC Master Catalog listing for Cluster II Samba STAFF</Name>
29 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-09</URL> 31 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-09</URL>
30 - <Description>This site provides information concerning the Cluster II Salsa Spatio-Temporal  
31 - Analysis of Magnetic Field Fluctuations Instrument.</Description>  
32 - </InformationURL> 32 + <Description>This site provides information concerning the Cluster STAFF Instrument.</Description>
  33 + </InformationURL>
33 </ResourceHeader> 34 </ResourceHeader>
34 <AccessInformation> 35 <AccessInformation>
35 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID> 36 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
@@ -39,15 +40,11 @@ @@ -39,15 +40,11 @@
39 <Name>AMDA at CDPP</Name> 40 <Name>AMDA at CDPP</Name>
40 <URL>http://amda.cdpp.eu</URL> 41 <URL>http://amda.cdpp.eu</URL>
41 </AccessURL> 42 </AccessURL>
42 - <Format>NetCDF</Format>  
43 - <Acknowledgement>NASA, Nicole Cornilleau-Wehrlin</Acknowledgement> 43 + <Format>NetCDF</Format>
44 </AccessInformation> 44 </AccessInformation>
45 <ProviderName>CSDS-CNES</ProviderName> 45 <ProviderName>CSDS-CNES</ProviderName>
46 <ProcessingLevel>Calibrated</ProcessingLevel> 46 <ProcessingLevel>Calibrated</ProcessingLevel>
47 - <ProviderResourceName>Cluster II Salsa Prime Parameter Spatio-Temporal Analysis of  
48 - Magnetic Field Fluctuations (STAFF) Data</ProviderResourceName>  
49 - <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>  
50 - <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Salsa/STAFF</InstrumentID> 47 + <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/STAFF</InstrumentID>
51 <MeasurementType>ElectricField</MeasurementType> 48 <MeasurementType>ElectricField</MeasurementType>
52 <MeasurementType>MagneticField</MeasurementType> 49 <MeasurementType>MagneticField</MeasurementType>
53 <MeasurementType>Waves.Passive</MeasurementType> 50 <MeasurementType>Waves.Passive</MeasurementType>
@@ -57,9 +54,9 @@ @@ -57,9 +54,9 @@
57 <StopDate>2012-12-31T23:59:46Z</StopDate> 54 <StopDate>2012-12-31T23:59:46Z</StopDate>
58 </TimeSpan> 55 </TimeSpan>
59 <Cadence>PT4S</Cadence> 56 <Cadence>PT4S</Cadence>
60 - </TemporalDescription>  
61 - <ObservedRegion>Earth.Magnetosheath</ObservedRegion> 57 + </TemporalDescription>
62 <ObservedRegion>Earth.Magnetosphere</ObservedRegion> 58 <ObservedRegion>Earth.Magnetosphere</ObservedRegion>
  59 + <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
63 <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion> 60 <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion>
64 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion> 61 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion>
65 <ObservedRegion>Earth.Magnetosphere.Polar</ObservedRegion> 62 <ObservedRegion>Earth.Magnetosphere.Polar</ObservedRegion>
@@ -79,25 +76,23 @@ @@ -79,25 +76,23 @@
79 <Keyword>magnetosheath</Keyword> 76 <Keyword>magnetosheath</Keyword>
80 <Keyword>Cluster</Keyword> 77 <Keyword>Cluster</Keyword>
81 <Keyword>magnetotail</Keyword> 78 <Keyword>magnetotail</Keyword>
82 - <Keyword>lobe</Keyword>  
83 - <Parameter>  
84 - <Name>Magnetic Field Spectral Power (1-10 Hz)</Name> 79 + <Keyword>lobe</Keyword>
  80 + <Parameter>
  81 + <Name>b spectral density (1-10 Hz)</Name>
85 <ParameterKey>c2_sta_f1</ParameterKey> 82 <ParameterKey>c2_sta_f1</ParameterKey>
86 - <Description>Cluster II Salsa Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
87 - Fluctuations (STAFF) magnetic field spectral power as measured by the onboard Cluster  
88 - Fluxgate Magnetometer (FGM) in the 1-10 Hz (f1) frequency range at spin time resolution 83 + <Description>Magnetic field spectral power in the 1-10 Hz (f1) at spin time resolution (parallel and perp components)
89 </Description> 84 </Description>
90 - <Ucd>phys.flux.density;phys.magField</Ucd>  
91 - <Cadence>PT4S</Cadence>  
92 - <Units>nT^2 Hz^-1</Units>  
93 - <UnitsConversion>1.0e-18&gt;T^2 Hz^-1</UnitsConversion>  
94 - <RenderingHints>  
95 - <DisplayType>TimeSeries</DisplayType>  
96 - </RenderingHints>  
97 - <Structure> 85 + <Ucd>phys.flux.density;phys.magField</Ucd>
  86 + <Cadence>PT4S</Cadence>
  87 + <Units>nT^2 Hz^-1</Units>
  88 + <UnitsConversion>1.0e-18&gt;T^2 Hz^-1</UnitsConversion>
  89 + <RenderingHints>
  90 + <DisplayType>TimeSeries</DisplayType>
  91 + </RenderingHints>
  92 + <Structure>
98 <Size>2</Size> 93 <Size>2</Size>
99 <Element> 94 <Element>
100 - <Name>Magnetic Field Spectral Power Parallel to Bo (1-10 Hz)</Name> 95 + <Name>parallel to b0</Name>
101 <Index>1</Index> 96 <Index>1</Index>
102 <ParameterKey>c2_sta_f1(0)</ParameterKey> 97 <ParameterKey>c2_sta_f1(0)</ParameterKey>
103 <ValidMin>1.0000e-7</ValidMin> 98 <ValidMin>1.0000e-7</ValidMin>
@@ -109,7 +104,7 @@ @@ -109,7 +104,7 @@
109 </RenderingHints> 104 </RenderingHints>
110 </Element> 105 </Element>
111 <Element> 106 <Element>
112 - <Name>Magnetic Field Spectral Power Perpendicular to Bo (1-10 Hz)</Name> 107 + <Name>perpendicular to b0</Name>
113 <Index>2</Index> 108 <Index>2</Index>
114 <ParameterKey>c2_sta_f1(1)</ParameterKey> 109 <ParameterKey>c2_sta_f1(1)</ParameterKey>
115 <ValidMin>1.0000e-7</ValidMin> 110 <ValidMin>1.0000e-7</ValidMin>
@@ -119,7 +114,7 @@ @@ -119,7 +114,7 @@
119 <ScaleMin>1.0000e-6</ScaleMin> 114 <ScaleMin>1.0000e-6</ScaleMin>
120 <ScaleMax>1</ScaleMax> 115 <ScaleMax>1</ScaleMax>
121 </RenderingHints> 116 </RenderingHints>
122 - </Element> 117 + </Element>
123 </Structure> 118 </Structure>
124 <FillValue>-1.0000e+31</FillValue> 119 <FillValue>-1.0000e+31</FillValue>
125 <Field> 120 <Field>
@@ -132,12 +127,11 @@ @@ -132,12 +127,11 @@
132 </FrequencyRange> 127 </FrequencyRange>
133 </Field> 128 </Field>
134 </Parameter> 129 </Parameter>
  130 +
135 <Parameter> 131 <Parameter>
136 - <Name>Magnetic Field Spectral Power (10-180 Hz)</Name> 132 + <Name>b spectral density (10-180 Hz)</Name>
137 <ParameterKey>c2_sta_f2</ParameterKey> 133 <ParameterKey>c2_sta_f2</ParameterKey>
138 - <Description>Cluster II Salsa Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
139 - Fluctuations (STAFF) magnetic field spectral power as measured by the onboard Cluster  
140 - Fluxgate Magnetometer (FGM) in the 10-180 Hz (f2) frequency range at spin time resolution 134 + <Description>Magnetic field spectral power in the 10-180 Hz (f2) at spin time resolution (parallel and perp components)
141 </Description> 135 </Description>
142 <Ucd>phys.flux.density;phys.magField</Ucd> 136 <Ucd>phys.flux.density;phys.magField</Ucd>
143 <Cadence>PT4S</Cadence> 137 <Cadence>PT4S</Cadence>
@@ -149,7 +143,7 @@ @@ -149,7 +143,7 @@
149 <Structure> 143 <Structure>
150 <Size>2</Size> 144 <Size>2</Size>
151 <Element> 145 <Element>
152 - <Name>Magnetic Field Spectral Power Parallel to Bo (10-180 Hz)</Name> 146 + <Name>parallel to b0</Name>
153 <Index>1</Index> 147 <Index>1</Index>
154 <ParameterKey>c2_sta_f2(0)</ParameterKey> 148 <ParameterKey>c2_sta_f2(0)</ParameterKey>
155 <ValidMin>1.0000e-9</ValidMin> 149 <ValidMin>1.0000e-9</ValidMin>
@@ -161,7 +155,7 @@ @@ -161,7 +155,7 @@
161 </RenderingHints> 155 </RenderingHints>
162 </Element> 156 </Element>
163 <Element> 157 <Element>
164 - <Name>Magnetic Field Spectral Power Perpendicular to Bo (10-180 Hz)</Name> 158 + <Name>perpendicular to b0</Name>
165 <Index>2</Index> 159 <Index>2</Index>
166 <ParameterKey>c2_sta_f2(1)</ParameterKey> 160 <ParameterKey>c2_sta_f2(1)</ParameterKey>
167 <ValidMin>1.0000e-9</ValidMin> 161 <ValidMin>1.0000e-9</ValidMin>
@@ -185,11 +179,9 @@ @@ -185,11 +179,9 @@
185 </Field> 179 </Field>
186 </Parameter> 180 </Parameter>
187 <Parameter> 181 <Parameter>
188 - <Name>Magnetic Field Spectral Power (180-4000 Hz)</Name> 182 + <Name>b spectral density (180-4000 Hz)</Name>
189 <ParameterKey>c2_sta_f3</ParameterKey> 183 <ParameterKey>c2_sta_f3</ParameterKey>
190 - <Description>Cluster II Salsa Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
191 - Fluctuations (STAFF) magnetic field spectral power as measured by the onboard Cluster  
192 - Fluxgate Magnetometer (FGM) in the 180-4000 Hz (f3) frequency range at spin time resolution 184 + <Description> Magnetic field spectral power in the 80-4000 Hz (f3) at spin time resolution (parallel and perp components)
193 </Description> 185 </Description>
194 <Ucd>phys.flux.density;phys.magField</Ucd> 186 <Ucd>phys.flux.density;phys.magField</Ucd>
195 <Cadence>PT4S</Cadence> 187 <Cadence>PT4S</Cadence>
@@ -201,7 +193,7 @@ @@ -201,7 +193,7 @@
201 <Structure> 193 <Structure>
202 <Size>2</Size> 194 <Size>2</Size>
203 <Element> 195 <Element>
204 - <Name>Magnetic Field Spectral Power Parallel to Bo (180-4000 Hz)</Name> 196 + <Name>parallel to b0</Name>
205 <Index>1</Index> 197 <Index>1</Index>
206 <ParameterKey>c2_sta_f3(0)</ParameterKey> 198 <ParameterKey>c2_sta_f3(0)</ParameterKey>
207 <ValidMin>1.0000e-11</ValidMin> 199 <ValidMin>1.0000e-11</ValidMin>
@@ -213,7 +205,7 @@ @@ -213,7 +205,7 @@
213 </RenderingHints> 205 </RenderingHints>
214 </Element> 206 </Element>
215 <Element> 207 <Element>
216 - <Name>Magnetic Field Spectral Power Perpendicular to Bo (180-4000 Hz)</Name> 208 + <Name>perpendicular to b0</Name>
217 <Index>2</Index> 209 <Index>2</Index>
218 <ParameterKey>c2_sta_f3(1)</ParameterKey> 210 <ParameterKey>c2_sta_f3(1)</ParameterKey>
219 <ValidMin>1.0000e-9</ValidMin> 211 <ValidMin>1.0000e-9</ValidMin>
@@ -235,13 +227,11 @@ @@ -235,13 +227,11 @@
235 <Units>Hz</Units> 227 <Units>Hz</Units>
236 </FrequencyRange> 228 </FrequencyRange>
237 </Field> 229 </Field>
238 - </Parameter> 230 + </Parameter>
239 <Parameter> 231 <Parameter>
240 - <Name>Electric Field Spectral Power (10-180 Hz)</Name> 232 + <Name>e spectral density (10-180 Hz)</Name>
241 <ParameterKey>c2_stae_f2</ParameterKey> 233 <ParameterKey>c2_stae_f2</ParameterKey>
242 - <Description>Cluster II Salsa Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
243 - Fluctuations (STAFF) electric field spectral power in the 10-180 Hz (f2)  
244 - frequency range at spin time resolution 234 + <Description> Electric field spectral power in the 10-180 Hz (f2) frequency range at spin time resolution.
245 </Description> 235 </Description>
246 <Ucd>phys.flux.density;phys.electField</Ucd> 236 <Ucd>phys.flux.density;phys.electField</Ucd>
247 <Cadence>PT4S</Cadence> 237 <Cadence>PT4S</Cadence>
@@ -267,11 +257,9 @@ @@ -267,11 +257,9 @@
267 </Field> 257 </Field>
268 </Parameter> 258 </Parameter>
269 <Parameter> 259 <Parameter>
270 - <Name>Electric Field Spectral Power (180-4000 Hz)</Name> 260 + <Name>e spectral density (180-4000 Hz)</Name>
271 <ParameterKey>c2_stae_f3</ParameterKey> 261 <ParameterKey>c2_stae_f3</ParameterKey>
272 - <Description>Cluster II Salsa Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
273 - Fluctuations (STAFF) electric field spectral power in the 180-4000 Hz (f3)  
274 - frequency range at spin time resolution 262 + <Description>Electric field spectral power in the 180-4000 Hz (f3) frequency range at spin time resolution.
275 </Description> 263 </Description>
276 <Ucd>phys.flux.density;phys.electField</Ucd> 264 <Ucd>phys.flux.density;phys.electField</Ucd>
277 <Cadence>PT4S</Cadence> 265 <Cadence>PT4S</Cadence>
NumericalData/AMDA/Cluster/Cluster3/STAFF/clust3-sta-pp.xml
  Diff comments   View file @a128b91
@@ -6,30 +6,31 @@ @@ -6,30 +6,31 @@
6 <ResourceHeader> 6 <ResourceHeader>
7 <ResourceName>prime parameters</ResourceName> 7 <ResourceName>prime parameters</ResourceName>
8 <AlternateName>Cluster 3 Prime Parameter STAFF Data</AlternateName> 8 <AlternateName>Cluster 3 Prime Parameter STAFF Data</AlternateName>
9 - <ReleaseDate>2015-10-19T15:51:44Z</ReleaseDate>  
10 - <Description>The Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) experiment provides  
11 - magnetic field power spectral density values parallel and perpendicular to the magnetic field and  
12 - the electric field power spectral density values for several frequency ranges.  
13 - For more details of the Cluster mission, the spacecraft, and its instruments, see the report  
14 - Cluster: mission, payload and supporting activities, March 1993, ESA SP-1159,  
15 - and the included article The STAFF (Spatio-Temporal Analysis of Field Fluctuations) Experiment  
16 - for the Cluster Mission, by N. Cornilleau-Wehrlin et al., from which this information was obtained. 9 + <ReleaseDate>2015-10-19T16:14:44Z</ReleaseDate>
  10 + <Description>
  11 + 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.
  12 +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.
  13 +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.
  14 +The Spectrum Analyser can work in different modes, in Burst Mode the analysis is performed in
  15 +the frequency range 64 Hz - 4 kHz.
  16 +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.
  17 +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.
17 </Description> 18 </Description>
18 - <Acknowledgement>ESA, Nicole Cornilleau-Wehrlin</Acknowledgement> 19 + <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
19 <Contact> 20 <Contact>
20 - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID> 21 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
21 <Role>PrincipalInvestigator</Role> 22 <Role>PrincipalInvestigator</Role>
22 </Contact> 23 </Contact>
23 - <Contact>  
24 - <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>  
25 - <Role>TechnicalContact</Role>  
26 - </Contact> 24 + <InformationURL>
  25 + <Name>ESA web page</Name>
  26 + <URL>http://www.cosmos.esa.int/web/csa/documentation</URL>
  27 + <Description>This site contains STAFF data documentation</Description>
  28 + </InformationURL>
27 <InformationURL> 29 <InformationURL>
28 - <Name>NSSDC Master Catalog listing for Cluster II Samba Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF)</Name> 30 + <Name>NSSDC Master Catalog listing for Cluster II Samba STAFF</Name>
29 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-09</URL> 31 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-09</URL>
30 - <Description>This site provides information concerning the Cluster II Samba Spatio-Temporal  
31 - Analysis of Magnetic Field Fluctuations Instrument.</Description>  
32 - </InformationURL> 32 + <Description>This site provides information concerning the Cluster STAFF Instrument.</Description>
  33 + </InformationURL>
33 </ResourceHeader> 34 </ResourceHeader>
34 <AccessInformation> 35 <AccessInformation>
35 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID> 36 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
@@ -39,14 +40,10 @@ @@ -39,14 +40,10 @@
39 <Name>AMDA at CDPP</Name> 40 <Name>AMDA at CDPP</Name>
40 <URL>http://amda.cdpp.eu</URL> 41 <URL>http://amda.cdpp.eu</URL>
41 </AccessURL> 42 </AccessURL>
42 - <Format>NetCDF</Format>  
43 - <Acknowledgement>NASA, Nicole Cornilleau-Wehrlin</Acknowledgement> 43 + <Format>NetCDF</Format>
44 </AccessInformation> 44 </AccessInformation>
45 <ProviderName>CSDS-CNES</ProviderName> 45 <ProviderName>CSDS-CNES</ProviderName>
46 <ProcessingLevel>Calibrated</ProcessingLevel> 46 <ProcessingLevel>Calibrated</ProcessingLevel>
47 - <ProviderResourceName>Cluster II Samba Prime Parameter Spatio-Temporal Analysis of  
48 - Magnetic Field Fluctuations (STAFF) Data</ProviderResourceName>  
49 - <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>  
50 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Samba/STAFF</InstrumentID> 47 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Samba/STAFF</InstrumentID>
51 <MeasurementType>ElectricField</MeasurementType> 48 <MeasurementType>ElectricField</MeasurementType>
52 <MeasurementType>MagneticField</MeasurementType> 49 <MeasurementType>MagneticField</MeasurementType>
@@ -57,9 +54,9 @@ @@ -57,9 +54,9 @@
57 <StopDate>2012-12-31T23:59:47Z</StopDate> 54 <StopDate>2012-12-31T23:59:47Z</StopDate>
58 </TimeSpan> 55 </TimeSpan>
59 <Cadence>PT4S</Cadence> 56 <Cadence>PT4S</Cadence>
60 - </TemporalDescription>  
61 - <ObservedRegion>Earth.Magnetosheath</ObservedRegion> 57 + </TemporalDescription>
62 <ObservedRegion>Earth.Magnetosphere</ObservedRegion> 58 <ObservedRegion>Earth.Magnetosphere</ObservedRegion>
  59 + <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
63 <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion> 60 <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion>
64 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion> 61 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion>
65 <ObservedRegion>Earth.Magnetosphere.Polar</ObservedRegion> 62 <ObservedRegion>Earth.Magnetosphere.Polar</ObservedRegion>
@@ -79,13 +76,11 @@ @@ -79,13 +76,11 @@
79 <Keyword>magnetosheath</Keyword> 76 <Keyword>magnetosheath</Keyword>
80 <Keyword>Cluster</Keyword> 77 <Keyword>Cluster</Keyword>
81 <Keyword>magnetotail</Keyword> 78 <Keyword>magnetotail</Keyword>
82 - <Keyword>lobe</Keyword>  
83 - <Parameter>  
84 - <Name>Magnetic Field Spectral Power (1-10 Hz)</Name> 79 + <Keyword>lobe</Keyword>
  80 + <Parameter>
  81 + <Name>b spectral density (1-10 Hz)</Name>
85 <ParameterKey>c3_sta_f1</ParameterKey> 82 <ParameterKey>c3_sta_f1</ParameterKey>
86 - <Description>Cluster II Samba Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
87 - Fluctuations (STAFF) magnetic field spectral power as measured by the onboard Cluster  
88 - Fluxgate Magnetometer (FGM) in the 1-10 Hz (f1) frequency range at spin time resolution 83 + <Description>Magnetic field spectral power in the 1-10 Hz (f1) at spin time resolution (parallel and perp components)
89 </Description> 84 </Description>
90 <Ucd>phys.flux.density;phys.magField</Ucd> 85 <Ucd>phys.flux.density;phys.magField</Ucd>
91 <Cadence>PT4S</Cadence> 86 <Cadence>PT4S</Cadence>
@@ -94,10 +89,10 @@ @@ -94,10 +89,10 @@
94 <RenderingHints> 89 <RenderingHints>
95 <DisplayType>TimeSeries</DisplayType> 90 <DisplayType>TimeSeries</DisplayType>
96 </RenderingHints> 91 </RenderingHints>
97 - <Structure> 92 + <Structure>
98 <Size>2</Size> 93 <Size>2</Size>
99 <Element> 94 <Element>
100 - <Name>Magnetic Field Spectral Power Parallel to Bo (1-10 Hz)</Name> 95 + <Name>parallel to b0</Name>
101 <Index>1</Index> 96 <Index>1</Index>
102 <ParameterKey>c3_sta_f1(0)</ParameterKey> 97 <ParameterKey>c3_sta_f1(0)</ParameterKey>
103 <ValidMin>1.0000e-7</ValidMin> 98 <ValidMin>1.0000e-7</ValidMin>
@@ -109,7 +104,7 @@ @@ -109,7 +104,7 @@
109 </RenderingHints> 104 </RenderingHints>
110 </Element> 105 </Element>
111 <Element> 106 <Element>
112 - <Name>Magnetic Field Spectral Power Perpendicular to Bo (1-10 Hz)</Name> 107 + <Name>perpendicular to b0</Name>
113 <Index>2</Index> 108 <Index>2</Index>
114 <ParameterKey>c3_sta_f1(1)</ParameterKey> 109 <ParameterKey>c3_sta_f1(1)</ParameterKey>
115 <ValidMin>1.0000e-7</ValidMin> 110 <ValidMin>1.0000e-7</ValidMin>
@@ -119,7 +114,7 @@ @@ -119,7 +114,7 @@
119 <ScaleMin>1.0000e-6</ScaleMin> 114 <ScaleMin>1.0000e-6</ScaleMin>
120 <ScaleMax>1</ScaleMax> 115 <ScaleMax>1</ScaleMax>
121 </RenderingHints> 116 </RenderingHints>
122 - </Element> 117 + </Element>
123 </Structure> 118 </Structure>
124 <FillValue>-1.0000e+31</FillValue> 119 <FillValue>-1.0000e+31</FillValue>
125 <Field> 120 <Field>
@@ -132,12 +127,11 @@ @@ -132,12 +127,11 @@
132 </FrequencyRange> 127 </FrequencyRange>
133 </Field> 128 </Field>
134 </Parameter> 129 </Parameter>
  130 +
135 <Parameter> 131 <Parameter>
136 - <Name>Magnetic Field Spectral Power (10-180 Hz)</Name> 132 + <Name>b spectral density (10-180 Hz)</Name>
137 <ParameterKey>c3_sta_f2</ParameterKey> 133 <ParameterKey>c3_sta_f2</ParameterKey>
138 - <Description>Cluster II Samba Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
139 - Fluctuations (STAFF) magnetic field spectral power as measured by the onboard Cluster  
140 - Fluxgate Magnetometer (FGM) in the 10-180 Hz (f2) frequency range at spin time resolution 134 + <Description>Magnetic field spectral power in the 10-180 Hz (f2) at spin time resolution (parallel and perp components)
141 </Description> 135 </Description>
142 <Ucd>phys.flux.density;phys.magField</Ucd> 136 <Ucd>phys.flux.density;phys.magField</Ucd>
143 <Cadence>PT4S</Cadence> 137 <Cadence>PT4S</Cadence>
@@ -149,7 +143,7 @@ @@ -149,7 +143,7 @@
149 <Structure> 143 <Structure>
150 <Size>2</Size> 144 <Size>2</Size>
151 <Element> 145 <Element>
152 - <Name>Magnetic Field Spectral Power Parallel to Bo (10-180 Hz)</Name> 146 + <Name>parallel to b0</Name>
153 <Index>1</Index> 147 <Index>1</Index>
154 <ParameterKey>c3_sta_f2(0)</ParameterKey> 148 <ParameterKey>c3_sta_f2(0)</ParameterKey>
155 <ValidMin>1.0000e-9</ValidMin> 149 <ValidMin>1.0000e-9</ValidMin>
@@ -161,7 +155,7 @@ @@ -161,7 +155,7 @@
161 </RenderingHints> 155 </RenderingHints>
162 </Element> 156 </Element>
163 <Element> 157 <Element>
164 - <Name>Magnetic Field Spectral Power Perpendicular to Bo (10-180 Hz)</Name> 158 + <Name>perpendicular to b0</Name>
165 <Index>2</Index> 159 <Index>2</Index>
166 <ParameterKey>c3_sta_f2(1)</ParameterKey> 160 <ParameterKey>c3_sta_f2(1)</ParameterKey>
167 <ValidMin>1.0000e-9</ValidMin> 161 <ValidMin>1.0000e-9</ValidMin>
@@ -185,11 +179,9 @@ @@ -185,11 +179,9 @@
185 </Field> 179 </Field>
186 </Parameter> 180 </Parameter>
187 <Parameter> 181 <Parameter>
188 - <Name>Magnetic Field Spectral Power (180-4000 Hz)</Name> 182 + <Name>b spectral density (180-4000 Hz)</Name>
189 <ParameterKey>c3_sta_f3</ParameterKey> 183 <ParameterKey>c3_sta_f3</ParameterKey>
190 - <Description>Cluster II Samba Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
191 - Fluctuations (STAFF) magnetic field spectral power as measured by the onboard Cluster  
192 - Fluxgate Magnetometer (FGM) in the 180-4000 Hz (f3) frequency range at spin time resolution 184 + <Description> Magnetic field spectral power in the 80-4000 Hz (f3) at spin time resolution (parallel and perp components)
193 </Description> 185 </Description>
194 <Ucd>phys.flux.density;phys.magField</Ucd> 186 <Ucd>phys.flux.density;phys.magField</Ucd>
195 <Cadence>PT4S</Cadence> 187 <Cadence>PT4S</Cadence>
@@ -201,7 +193,7 @@ @@ -201,7 +193,7 @@
201 <Structure> 193 <Structure>
202 <Size>2</Size> 194 <Size>2</Size>
203 <Element> 195 <Element>
204 - <Name>Magnetic Field Spectral Power Parallel to Bo (180-4000 Hz)</Name> 196 + <Name>parallel to b0</Name>
205 <Index>1</Index> 197 <Index>1</Index>
206 <ParameterKey>c3_sta_f3(0)</ParameterKey> 198 <ParameterKey>c3_sta_f3(0)</ParameterKey>
207 <ValidMin>1.0000e-11</ValidMin> 199 <ValidMin>1.0000e-11</ValidMin>
@@ -213,7 +205,7 @@ @@ -213,7 +205,7 @@
213 </RenderingHints> 205 </RenderingHints>
214 </Element> 206 </Element>
215 <Element> 207 <Element>
216 - <Name>Magnetic Field Spectral Power Perpendicular to Bo (180-4000 Hz)</Name> 208 + <Name>perpendicular to b0</Name>
217 <Index>2</Index> 209 <Index>2</Index>
218 <ParameterKey>c3_sta_f3(1)</ParameterKey> 210 <ParameterKey>c3_sta_f3(1)</ParameterKey>
219 <ValidMin>1.0000e-9</ValidMin> 211 <ValidMin>1.0000e-9</ValidMin>
@@ -235,13 +227,11 @@ @@ -235,13 +227,11 @@
235 <Units>Hz</Units> 227 <Units>Hz</Units>
236 </FrequencyRange> 228 </FrequencyRange>
237 </Field> 229 </Field>
238 - </Parameter> 230 + </Parameter>
239 <Parameter> 231 <Parameter>
240 - <Name>Electric Field Spectral Power (10-180 Hz)</Name> 232 + <Name>e spectral density (10-180 Hz)</Name>
241 <ParameterKey>c3_stae_f2</ParameterKey> 233 <ParameterKey>c3_stae_f2</ParameterKey>
242 - <Description>Cluster II Samba Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
243 - Fluctuations (STAFF) electric field spectral power in the 10-180 Hz (f2)  
244 - frequency range at spin time resolution 234 + <Description> Electric field spectral power in the 10-180 Hz (f2) frequency range at spin time resolution.
245 </Description> 235 </Description>
246 <Ucd>phys.flux.density;phys.electField</Ucd> 236 <Ucd>phys.flux.density;phys.electField</Ucd>
247 <Cadence>PT4S</Cadence> 237 <Cadence>PT4S</Cadence>
@@ -267,11 +257,9 @@ @@ -267,11 +257,9 @@
267 </Field> 257 </Field>
268 </Parameter> 258 </Parameter>
269 <Parameter> 259 <Parameter>
270 - <Name>Electric Field Spectral Power (180-4000 Hz)</Name> 260 + <Name>e spectral density (180-4000 Hz)</Name>
271 <ParameterKey>c3_stae_f3</ParameterKey> 261 <ParameterKey>c3_stae_f3</ParameterKey>
272 - <Description>Cluster II Samba Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
273 - Fluctuations (STAFF) electric field spectral power in the 180-4000 Hz (f3)  
274 - frequency range at spin time resolution 262 + <Description>Electric field spectral power in the 180-4000 Hz (f3) frequency range at spin time resolution.
275 </Description> 263 </Description>
276 <Ucd>phys.flux.density;phys.electField</Ucd> 264 <Ucd>phys.flux.density;phys.electField</Ucd>
277 <Cadence>PT4S</Cadence> 265 <Cadence>PT4S</Cadence>
NumericalData/AMDA/Cluster/Cluster4/STAFF/clust4-sta-pp.xml
  Diff comments   View file @a128b91
@@ -6,30 +6,31 @@ @@ -6,30 +6,31 @@
6 <ResourceHeader> 6 <ResourceHeader>
7 <ResourceName>prime parameters</ResourceName> 7 <ResourceName>prime parameters</ResourceName>
8 <AlternateName>Cluster 4 Prime Parameter STAFF Data</AlternateName> 8 <AlternateName>Cluster 4 Prime Parameter STAFF Data</AlternateName>
9 - <ReleaseDate>2015-10-16T17:51:44Z</ReleaseDate>  
10 - <Description>The Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) experiment provides  
11 - magnetic field power spectral density values parallel and perpendicular to the magnetic field and  
12 - the electric field power spectral density values for several frequency ranges.  
13 - For more details of the Cluster mission, the spacecraft, and its instruments, see the report  
14 - Cluster: mission, payload and supporting activities, March 1993, ESA SP-1159,  
15 - and the included article The STAFF (Spatio-Temporal Analysis of Field Fluctuations) Experiment  
16 - for the Cluster Mission, by N. Cornilleau-Wehrlin et al., from which this information was obtained. 9 + <ReleaseDate>2015-10-19T16:14:44Z</ReleaseDate>
  10 + <Description>
  11 + 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.
  12 +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.
  13 +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.
  14 +The Spectrum Analyser can work in different modes, in Burst Mode the analysis is performed in
  15 +the frequency range 64 Hz - 4 kHz.
  16 +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.
  17 +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.
17 </Description> 18 </Description>
18 - <Acknowledgement>ESA, Nicole Cornilleau-Wehrlin</Acknowledgement> 19 + <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
19 <Contact> 20 <Contact>
20 - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID> 21 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
21 <Role>PrincipalInvestigator</Role> 22 <Role>PrincipalInvestigator</Role>
22 </Contact> 23 </Contact>
23 - <Contact>  
24 - <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>  
25 - <Role>TechnicalContact</Role>  
26 - </Contact> 24 + <InformationURL>
  25 + <Name>ESA web page</Name>
  26 + <URL>http://www.cosmos.esa.int/web/csa/documentation</URL>
  27 + <Description>This site contains STAFF data documentation</Description>
  28 + </InformationURL>
27 <InformationURL> 29 <InformationURL>
28 - <Name>NSSDC Master Catalog listing for Cluster II Tango Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF)</Name> 30 + <Name>NSSDC Master Catalog listing for Cluster II Tango STAFF</Name>
29 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-09</URL> 31 <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-09</URL>
30 - <Description>This site provides information concerning the Cluster II Tango Spatio-Temporal  
31 - Analysis of Magnetic Field Fluctuations Instrument.</Description>  
32 - </InformationURL> 32 + <Description>This site provides information concerning the Cluster STAFF Instrument.</Description>
  33 + </InformationURL>
33 </ResourceHeader> 34 </ResourceHeader>
34 <AccessInformation> 35 <AccessInformation>
35 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID> 36 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
@@ -39,14 +40,10 @@ @@ -39,14 +40,10 @@
39 <Name>AMDA at CDPP</Name> 40 <Name>AMDA at CDPP</Name>
40 <URL>http://amda.cdpp.eu</URL> 41 <URL>http://amda.cdpp.eu</URL>
41 </AccessURL> 42 </AccessURL>
42 - <Format>NetCDF</Format>  
43 - <Acknowledgement/> 43 + <Format>NetCDF</Format>
44 </AccessInformation> 44 </AccessInformation>
45 <ProviderName>CSDS-CNES</ProviderName> 45 <ProviderName>CSDS-CNES</ProviderName>
46 <ProcessingLevel>Calibrated</ProcessingLevel> 46 <ProcessingLevel>Calibrated</ProcessingLevel>
47 - <ProviderResourceName>Cluster II Tango Prime Parameter Spatio-Temporal Analysis of  
48 - Magnetic Field Fluctuations (STAFF) Data</ProviderResourceName>  
49 - <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>  
50 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Tango/STAFF</InstrumentID> 47 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Tango/STAFF</InstrumentID>
51 <MeasurementType>ElectricField</MeasurementType> 48 <MeasurementType>ElectricField</MeasurementType>
52 <MeasurementType>MagneticField</MeasurementType> 49 <MeasurementType>MagneticField</MeasurementType>
@@ -57,9 +54,9 @@ @@ -57,9 +54,9 @@
57 <StopDate>2012-12-31T23:59:45Z</StopDate> 54 <StopDate>2012-12-31T23:59:45Z</StopDate>
58 </TimeSpan> 55 </TimeSpan>
59 <Cadence>PT4S</Cadence> 56 <Cadence>PT4S</Cadence>
60 - </TemporalDescription>  
61 - <ObservedRegion>Earth.Magnetosheath</ObservedRegion> 57 + </TemporalDescription>
62 <ObservedRegion>Earth.Magnetosphere</ObservedRegion> 58 <ObservedRegion>Earth.Magnetosphere</ObservedRegion>
  59 + <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
63 <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion> 60 <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion>
64 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion> 61 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion>
65 <ObservedRegion>Earth.Magnetosphere.Polar</ObservedRegion> 62 <ObservedRegion>Earth.Magnetosphere.Polar</ObservedRegion>
@@ -79,13 +76,11 @@ @@ -79,13 +76,11 @@
79 <Keyword>magnetosheath</Keyword> 76 <Keyword>magnetosheath</Keyword>
80 <Keyword>Cluster</Keyword> 77 <Keyword>Cluster</Keyword>
81 <Keyword>magnetotail</Keyword> 78 <Keyword>magnetotail</Keyword>
82 - <Keyword>lobe</Keyword>  
83 - <Parameter>  
84 - <Name>Magnetic Field Spectral Power (1-10 Hz)</Name> 79 + <Keyword>lobe</Keyword>
  80 + <Parameter>
  81 + <Name>b spectral density (1-10 Hz)</Name>
85 <ParameterKey>c4_sta_f1</ParameterKey> 82 <ParameterKey>c4_sta_f1</ParameterKey>
86 - <Description>Cluster II Tango Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
87 - Fluctuations (STAFF) magnetic field spectral power as measured by the onboard Cluster  
88 - Fluxgate Magnetometer (FGM) in the 1-10 Hz (f1) frequency range at spin time resolution 83 + <Description>Magnetic field spectral power in the 1-10 Hz (f1) at spin time resolution (parallel and perp components)
89 </Description> 84 </Description>
90 <Ucd>phys.flux.density;phys.magField</Ucd> 85 <Ucd>phys.flux.density;phys.magField</Ucd>
91 <Cadence>PT4S</Cadence> 86 <Cadence>PT4S</Cadence>
@@ -94,10 +89,10 @@ @@ -94,10 +89,10 @@
94 <RenderingHints> 89 <RenderingHints>
95 <DisplayType>TimeSeries</DisplayType> 90 <DisplayType>TimeSeries</DisplayType>
96 </RenderingHints> 91 </RenderingHints>
97 - <Structure> 92 + <Structure>
98 <Size>2</Size> 93 <Size>2</Size>
99 <Element> 94 <Element>
100 - <Name>Magnetic Field Spectral Power Parallel to Bo (1-10 Hz)</Name> 95 + <Name>parallel to b0</Name>
101 <Index>1</Index> 96 <Index>1</Index>
102 <ParameterKey>c4_sta_f1(0)</ParameterKey> 97 <ParameterKey>c4_sta_f1(0)</ParameterKey>
103 <ValidMin>1.0000e-7</ValidMin> 98 <ValidMin>1.0000e-7</ValidMin>
@@ -109,7 +104,7 @@ @@ -109,7 +104,7 @@
109 </RenderingHints> 104 </RenderingHints>
110 </Element> 105 </Element>
111 <Element> 106 <Element>
112 - <Name>Magnetic Field Spectral Power Perpendicular to Bo (1-10 Hz)</Name> 107 + <Name>perpendicular to b0</Name>
113 <Index>2</Index> 108 <Index>2</Index>
114 <ParameterKey>c4_sta_f1(1)</ParameterKey> 109 <ParameterKey>c4_sta_f1(1)</ParameterKey>
115 <ValidMin>1.0000e-7</ValidMin> 110 <ValidMin>1.0000e-7</ValidMin>
@@ -119,7 +114,7 @@ @@ -119,7 +114,7 @@
119 <ScaleMin>1.0000e-6</ScaleMin> 114 <ScaleMin>1.0000e-6</ScaleMin>
120 <ScaleMax>1</ScaleMax> 115 <ScaleMax>1</ScaleMax>
121 </RenderingHints> 116 </RenderingHints>
122 - </Element> 117 + </Element>
123 </Structure> 118 </Structure>
124 <FillValue>-1.0000e+31</FillValue> 119 <FillValue>-1.0000e+31</FillValue>
125 <Field> 120 <Field>
@@ -132,12 +127,11 @@ @@ -132,12 +127,11 @@
132 </FrequencyRange> 127 </FrequencyRange>
133 </Field> 128 </Field>
134 </Parameter> 129 </Parameter>
  130 +
135 <Parameter> 131 <Parameter>
136 - <Name>Magnetic Field Spectral Power (10-180 Hz)</Name> 132 + <Name>b spectral density (10-180 Hz)</Name>
137 <ParameterKey>c4_sta_f2</ParameterKey> 133 <ParameterKey>c4_sta_f2</ParameterKey>
138 - <Description>Cluster II Tango Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
139 - Fluctuations (STAFF) magnetic field spectral power as measured by the onboard Cluster  
140 - Fluxgate Magnetometer (FGM) in the 10-180 Hz (f2) frequency range at spin time resolution 134 + <Description>Magnetic field spectral power in the 10-180 Hz (f2) at spin time resolution (parallel and perp components)
141 </Description> 135 </Description>
142 <Ucd>phys.flux.density;phys.magField</Ucd> 136 <Ucd>phys.flux.density;phys.magField</Ucd>
143 <Cadence>PT4S</Cadence> 137 <Cadence>PT4S</Cadence>
@@ -149,7 +143,7 @@ @@ -149,7 +143,7 @@
149 <Structure> 143 <Structure>
150 <Size>2</Size> 144 <Size>2</Size>
151 <Element> 145 <Element>
152 - <Name>Magnetic Field Spectral Power Parallel to Bo (10-180 Hz)</Name> 146 + <Name>parallel to b0</Name>
153 <Index>1</Index> 147 <Index>1</Index>
154 <ParameterKey>c4_sta_f2(0)</ParameterKey> 148 <ParameterKey>c4_sta_f2(0)</ParameterKey>
155 <ValidMin>1.0000e-9</ValidMin> 149 <ValidMin>1.0000e-9</ValidMin>
@@ -161,7 +155,7 @@ @@ -161,7 +155,7 @@
161 </RenderingHints> 155 </RenderingHints>
162 </Element> 156 </Element>
163 <Element> 157 <Element>
164 - <Name>Magnetic Field Spectral Power Perpendicular to Bo (10-180 Hz)</Name> 158 + <Name>perpendicular to b0</Name>
165 <Index>2</Index> 159 <Index>2</Index>
166 <ParameterKey>c4_sta_f2(1)</ParameterKey> 160 <ParameterKey>c4_sta_f2(1)</ParameterKey>
167 <ValidMin>1.0000e-9</ValidMin> 161 <ValidMin>1.0000e-9</ValidMin>
@@ -185,11 +179,9 @@ @@ -185,11 +179,9 @@
185 </Field> 179 </Field>
186 </Parameter> 180 </Parameter>
187 <Parameter> 181 <Parameter>
188 - <Name>Magnetic Field Spectral Power (180-4000 Hz)</Name> 182 + <Name>b spectral density (180-4000 Hz)</Name>
189 <ParameterKey>c4_sta_f3</ParameterKey> 183 <ParameterKey>c4_sta_f3</ParameterKey>
190 - <Description>Cluster II Tango Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
191 - Fluctuations (STAFF) magnetic field spectral power as measured by the onboard Cluster  
192 - Fluxgate Magnetometer (FGM) in the 180-4000 Hz (f3) frequency range at spin time resolution 184 + <Description> Magnetic field spectral power in the 80-4000 Hz (f3) at spin time resolution (parallel and perp components)
193 </Description> 185 </Description>
194 <Ucd>phys.flux.density;phys.magField</Ucd> 186 <Ucd>phys.flux.density;phys.magField</Ucd>
195 <Cadence>PT4S</Cadence> 187 <Cadence>PT4S</Cadence>
@@ -201,7 +193,7 @@ @@ -201,7 +193,7 @@
201 <Structure> 193 <Structure>
202 <Size>2</Size> 194 <Size>2</Size>
203 <Element> 195 <Element>
204 - <Name>Magnetic Field Spectral Power Parallel to Bo (180-4000 Hz)</Name> 196 + <Name>parallel to b0</Name>
205 <Index>1</Index> 197 <Index>1</Index>
206 <ParameterKey>c4_sta_f3(0)</ParameterKey> 198 <ParameterKey>c4_sta_f3(0)</ParameterKey>
207 <ValidMin>1.0000e-11</ValidMin> 199 <ValidMin>1.0000e-11</ValidMin>
@@ -213,7 +205,7 @@ @@ -213,7 +205,7 @@
213 </RenderingHints> 205 </RenderingHints>
214 </Element> 206 </Element>
215 <Element> 207 <Element>
216 - <Name>Magnetic Field Spectral Power Perpendicular to Bo (180-4000 Hz)</Name> 208 + <Name>perpendicular to b0</Name>
217 <Index>2</Index> 209 <Index>2</Index>
218 <ParameterKey>c4_sta_f3(1)</ParameterKey> 210 <ParameterKey>c4_sta_f3(1)</ParameterKey>
219 <ValidMin>1.0000e-9</ValidMin> 211 <ValidMin>1.0000e-9</ValidMin>
@@ -235,13 +227,11 @@ @@ -235,13 +227,11 @@
235 <Units>Hz</Units> 227 <Units>Hz</Units>
236 </FrequencyRange> 228 </FrequencyRange>
237 </Field> 229 </Field>
238 - </Parameter> 230 + </Parameter>
239 <Parameter> 231 <Parameter>
240 - <Name>Electric Field Spectral Power (10-180 Hz)</Name> 232 + <Name>e spectral density (10-180 Hz)</Name>
241 <ParameterKey>c4_stae_f2</ParameterKey> 233 <ParameterKey>c4_stae_f2</ParameterKey>
242 - <Description>Cluster II Tango Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
243 - Fluctuations (STAFF) electric field spectral power in the 10-180 Hz (f2)  
244 - frequency range at spin time resolution 234 + <Description> Electric field spectral power in the 10-180 Hz (f2) frequency range at spin time resolution.
245 </Description> 235 </Description>
246 <Ucd>phys.flux.density;phys.electField</Ucd> 236 <Ucd>phys.flux.density;phys.electField</Ucd>
247 <Cadence>PT4S</Cadence> 237 <Cadence>PT4S</Cadence>
@@ -267,11 +257,9 @@ @@ -267,11 +257,9 @@
267 </Field> 257 </Field>
268 </Parameter> 258 </Parameter>
269 <Parameter> 259 <Parameter>
270 - <Name>Electric Field Spectral Power (180-4000 Hz)</Name> 260 + <Name>e spectral density (180-4000 Hz)</Name>
271 <ParameterKey>c4_stae_f3</ParameterKey> 261 <ParameterKey>c4_stae_f3</ParameterKey>
272 - <Description>Cluster II Tango Prime Parameter Spatio-Temporal Analysis of Magnetic Field  
273 - Fluctuations (STAFF) electric field spectral power in the 180-4000 Hz (f3)  
274 - frequency range at spin time resolution 262 + <Description>Electric field spectral power in the 180-4000 Hz (f3) frequency range at spin time resolution.
275 </Description> 263 </Description>
276 <Ucd>phys.flux.density;phys.electField</Ucd> 264 <Ucd>phys.flux.density;phys.electField</Ucd>
277 <Cadence>PT4S</Cadence> 265 <Cadence>PT4S</Cadence>
NumericalData/AMDA/Indices/Ground_Based/ground-based-dst.xml
  Diff comments   View file @a128b91
@@ -47,7 +47,7 @@ @@ -47,7 +47,7 @@
47 <TemporalDescription> 47 <TemporalDescription>
48 <TimeSpan> 48 <TimeSpan>
49 <StartDate>1970-01-01T00:00:00Z</StartDate> 49 <StartDate>1970-01-01T00:00:00Z</StartDate>
50 - <StopDate>2016-05-31T23:59:59Z</StopDate> 50 + <StopDate>2016-10-31T23:59:59Z</StopDate>
51 </TimeSpan> 51 </TimeSpan>
52 <Cadence>PT1H</Cadence></TemporalDescription> 52 <Cadence>PT1H</Cadence></TemporalDescription>
53 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion> 53 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion>
NumericalData/AMDA/MAVEN/EUV/mvn-euv-clb.xml
  Diff comments   View file @a128b91
@@ -45,7 +45,7 @@ @@ -45,7 +45,7 @@
45 <TemporalDescription> 45 <TemporalDescription>
46 <TimeSpan> 46 <TimeSpan>
47 <StartDate>2014-10-18T00:00:16Z</StartDate> 47 <StartDate>2014-10-18T00:00:16Z</StartDate>
48 - <StopDate>2016-05-15T00:00:00Z</StopDate> 48 + <StopDate>2016-08-15T00:00:00Z</StopDate>
49 </TimeSpan> 49 </TimeSpan>
50 <Cadence>PT60S</Cadence> 50 <Cadence>PT60S</Cadence>
51 </TemporalDescription> 51 </TemporalDescription>
NumericalData/AMDA/MAVEN/Ephemeris/maven-orb-marsobs.xml
  Diff comments   View file @a128b91
@@ -49,7 +49,7 @@ @@ -49,7 +49,7 @@
49 <TemporalDescription> 49 <TemporalDescription>
50 <TimeSpan> 50 <TimeSpan>
51 <StartDate>2014-06-01T00:00:00Z</StartDate> 51 <StartDate>2014-06-01T00:00:00Z</StartDate>
52 - <StopDate>2016-11-01T20:12:00Z</StopDate> 52 + <StopDate>2016-11-08T19:42:00Z</StopDate>
53 </TimeSpan> 53 </TimeSpan>
54 <Cadence>PT1M</Cadence> 54 <Cadence>PT1M</Cadence>
55 </TemporalDescription> 55 </TemporalDescription>
NumericalData/AMDA/MAVEN/MAG/mav-mag-pds.xml
  Diff comments   View file @a128b91
@@ -48,7 +48,7 @@ @@ -48,7 +48,7 @@
48 <TemporalDescription> 48 <TemporalDescription>
49 <TimeSpan> 49 <TimeSpan>
50 <StartDate>2014-10-10T00:00:00Z</StartDate> 50 <StartDate>2014-10-10T00:00:00Z</StartDate>
51 - <StopDate>2016-05-15T00:00:02Z</StopDate> 51 + <StopDate>2016-05-19T00:00:01Z</StopDate>
52 </TimeSpan> 52 </TimeSpan>
53 <Cadence>PT0.031S</Cadence> 53 <Cadence>PT0.031S</Cadence>
54 </TemporalDescription> 54 </TemporalDescription>
NumericalData/AMDA/MAVEN/STATIC/mavpds-sta-c0.xml
  Diff comments   View file @a128b91
@@ -44,7 +44,7 @@ @@ -44,7 +44,7 @@
44 <TemporalDescription> 44 <TemporalDescription>
45 <TimeSpan> 45 <TimeSpan>
46 <StartDate>2014-10-13T00:00:20Z</StartDate> 46 <StartDate>2014-10-13T00:00:20Z</StartDate>
47 - <StopDate>2016-05-15T00:00:19Z</StopDate> 47 + <StopDate>2016-08-15T00:00:06Z</StopDate>
48 </TimeSpan> 48 </TimeSpan>
49 <Cadence>PT4S</Cadence> 49 <Cadence>PT4S</Cadence>
50 </TemporalDescription> 50 </TemporalDescription>
NumericalData/AMDA/MAVEN/STATIC/mavpds-sta-c6.xml
  Diff comments   View file @a128b91
@@ -47,7 +47,7 @@ @@ -47,7 +47,7 @@
47 <TemporalDescription> 47 <TemporalDescription>
48 <TimeSpan> 48 <TimeSpan>
49 <StartDate>2014-10-13T00:00:04Z</StartDate> 49 <StartDate>2014-10-13T00:00:04Z</StartDate>
50 - <StopDate>2016-05-15T00:00:03Z</StopDate> 50 + <StopDate>2016-08-15T00:00:02Z</StopDate>
51 </TimeSpan> 51 </TimeSpan>
52 <Cadence>PT4S</Cadence> 52 <Cadence>PT4S</Cadence>
53 </TemporalDescription> 53 </TemporalDescription>
NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-momboard.xml
  Diff comments   View file @a128b91
@@ -48,7 +48,7 @@ @@ -48,7 +48,7 @@
48 <TemporalDescription> 48 <TemporalDescription>
49 <TimeSpan> 49 <TimeSpan>
50 <StartDate>2014-03-19T14:19:43Z</StartDate> 50 <StartDate>2014-03-19T14:19:43Z</StartDate>
51 - <StopDate>2016-05-15T00:00:45Z</StopDate> 51 + <StopDate>2016-08-15T00:01:00Z</StopDate>
52 </TimeSpan> 52 </TimeSpan>
53 <Cadence>PT4S</Cadence></TemporalDescription> 53 <Cadence>PT4S</Cadence></TemporalDescription>
54 <ObservedRegion>Mars</ObservedRegion> 54 <ObservedRegion>Mars</ObservedRegion>
NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-specboard.xml
  Diff comments   View file @a128b91
@@ -45,7 +45,7 @@ @@ -45,7 +45,7 @@
45 <TemporalDescription> 45 <TemporalDescription>
46 <TimeSpan> 46 <TimeSpan>
47 <StartDate>2014-03-19T14:20:43Z</StartDate> 47 <StartDate>2014-03-19T14:20:43Z</StartDate>
48 - <StopDate>2016-05-15T00:00:37Z</StopDate> 48 + <StopDate>2016-08-15T00:00:56Z</StopDate>
49 </TimeSpan> 49 </TimeSpan>
50 <Cadence>PT4S</Cadence></TemporalDescription> 50 <Cadence>PT4S</Cadence></TemporalDescription>
51 <ObservedRegion>Mars</ObservedRegion> 51 <ObservedRegion>Mars</ObservedRegion>