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
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... ... @@ -5,22 +5,37 @@
5 5 <ResourceID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/STAFF</ResourceID>
6 6 <ResourceHeader>
7 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 17 <Contact>
12   - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID>
  18 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
13 19 <Role>PrincipalInvestigator</Role>
14 20 </Contact>
15 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 27 <Name>NSSDC's Master Catalog</Name>
17 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 30 </InformationURL>
20 31 <PriorID>spase://SMWG/Instrument/Cluster2-Rumba/STAFF</PriorID>
21 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 39 <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Rumba</ObservatoryID>
25 40 </Instrument>
26 41 </Spase>
... ...
Instrument/AMDA/Cluster-Salsa/STAFF.xml
  Diff comments   View file @a128b91
... ... @@ -6,21 +6,36 @@
6 6 <ResourceHeader>
7 7 <ResourceName>STAFF</ResourceName>
8 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 17 <Contact>
12   - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID>
  18 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
13 19 <Role>PrincipalInvestigator</Role>
14 20 </Contact>
15 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 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 30 </InformationURL>
20 31 <PriorID>spase://SMWG/Instrument/Cluster2-Salsa/STAFF</PriorID>
21 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 39 <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Salsa</ObservatoryID>
25 40 </Instrument>
26 41 </Spase>
... ...
Instrument/AMDA/Cluster-Samba/STAFF.xml
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... ... @@ -6,21 +6,37 @@
6 6 <ResourceHeader>
7 7 <ResourceName>STAFF</ResourceName>
8 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 17 <Contact>
12   - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID>
  18 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
13 19 <Role>PrincipalInvestigator</Role>
14 20 </Contact>
15 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 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 30 </InformationURL>
20 31 <PriorID>spase://SMWG/Instrument/Cluster2-Samba/STAFF</PriorID>
21 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 40 <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Samba</ObservatoryID>
25 41 </Instrument>
26 42 </Spase>
... ...
Instrument/AMDA/Cluster-Tango/STAFF.xml
  Diff comments   View file @a128b91
... ... @@ -6,21 +6,36 @@
6 6 <ResourceHeader>
7 7 <ResourceName>STAFF</ResourceName>
8 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 17 <Contact>
12   - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID>
  18 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
13 19 <Role>PrincipalInvestigator</Role>
14 20 </Contact>
15 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 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 30 </InformationURL>
20 31 <PriorID>spase://SMWG/Instrument/Cluster2-Tango/STAFF</PriorID>
21 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 39 <ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Tango</ObservatoryID>
25 40 </Instrument>
26 41 </Spase>
... ...
NumericalData/AMDA/ACE/MFI/ace-mag-real.xml
  Diff comments   View file @a128b91
... ... @@ -51,7 +51,7 @@
51 51 <TemporalDescription>
52 52 <TimeSpan>
53 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 55 </TimeSpan>
56 56 <Cadence>PT60S</Cadence>
57 57 </TemporalDescription>
... ...
NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml
  Diff comments   View file @a128b91
... ... @@ -44,7 +44,7 @@
44 44 <TemporalDescription>
45 45 <TimeSpan>
46 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 48 </TimeSpan>
49 49 <Cadence>PT60S</Cadence>
50 50 </TemporalDescription>
... ...
NumericalData/AMDA/Cluster/Cluster1/STAFF/clust1-sta-pp.xml
  Diff comments   View file @a128b91
... ... @@ -7,28 +7,29 @@
7 7 <ResourceName>prime parameters</ResourceName>
8 8 <AlternateName>Cluster 1 Prime Parameter STAFF Data</AlternateName>
9 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 18 </Description>
18   - <Acknowledgement>ESA, Nicole Cornilleau-Wehrlin</Acknowledgement>
  19 + <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
19 20 <Contact>
20   - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID>
  21 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
21 22 <Role>PrincipalInvestigator</Role>
22 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 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 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 33 </InformationURL>
33 34 </ResourceHeader>
34 35 <AccessInformation>
... ... @@ -39,14 +40,10 @@
39 40 <Name>AMDA at CDPP</Name>
40 41 <URL>http://amda.cdpp.eu</URL>
41 42 </AccessURL>
42   - <Format>NetCDF</Format>
43   - <Acknowledgement>NASA, Nicole Cornilleau-Wehrlin</Acknowledgement>
  43 + <Format>NetCDF</Format>
44 44 </AccessInformation>
45 45 <ProviderName>CSDS-CNES</ProviderName>
46 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 47 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/STAFF</InstrumentID>
51 48 <MeasurementType>ElectricField</MeasurementType>
52 49 <MeasurementType>MagneticField</MeasurementType>
... ... @@ -57,9 +54,9 @@
57 54 <StopDate>2012-12-31T23:59:48Z</StopDate>
58 55 </TimeSpan>
59 56 <Cadence>PT4S</Cadence>
60   - </TemporalDescription>
61   - <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
  57 + </TemporalDescription>
62 58 <ObservedRegion>Earth.Magnetosphere</ObservedRegion>
  59 + <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
63 60 <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion>
64 61 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion>
65 62 <ObservedRegion>Earth.Magnetosphere.Polar</ObservedRegion>
... ... @@ -81,11 +78,9 @@
81 78 <Keyword>magnetotail</Keyword>
82 79 <Keyword>lobe</Keyword>
83 80 <Parameter>
84   - <Name>Magnetic Field Spectral Density (1-10 Hz)</Name>
  81 + <Name>b spectral density (1-10 Hz)</Name>
85 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 84 </Description>
90 85 <Ucd>phys.flux.density;phys.magField</Ucd>
91 86 <Cadence>PT4S</Cadence>
... ... @@ -97,7 +92,7 @@
97 92 <Structure>
98 93 <Size>2</Size>
99 94 <Element>
100   - <Name>Magnetic Field Spectral Density Parallel to Bo (1-10 Hz)</Name>
  95 + <Name>parallel to b0</Name>
101 96 <Index>1</Index>
102 97 <ParameterKey>c1_sta_f1(0)</ParameterKey>
103 98 <ValidMin>1.0000e-7</ValidMin>
... ... @@ -109,7 +104,7 @@
109 104 </RenderingHints>
110 105 </Element>
111 106 <Element>
112   - <Name>Magnetic Field Spectral Density Perpendicular to Bo (1-10 Hz)</Name>
  107 + <Name>perpendicular to b0</Name>
113 108 <Index>2</Index>
114 109 <ParameterKey>c1_sta_f1(1)</ParameterKey>
115 110 <ValidMin>1.0000e-7</ValidMin>
... ... @@ -119,7 +114,7 @@
119 114 <ScaleMin>1.0000e-6</ScaleMin>
120 115 <ScaleMax>1</ScaleMax>
121 116 </RenderingHints>
122   - </Element>
  117 + </Element>
123 118 </Structure>
124 119 <FillValue>-1.0000e+31</FillValue>
125 120 <Field>
... ... @@ -134,11 +129,9 @@
134 129 </Parameter>
135 130  
136 131 <Parameter>
137   - <Name>Magnetic Field Spectral Density (10-180 Hz)</Name>
  132 + <Name>b spectral density (10-180 Hz)</Name>
138 133 <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)
142 135 </Description>
143 136 <Ucd>phys.flux.density;phys.magField</Ucd>
144 137 <Cadence>PT4S</Cadence>
... ... @@ -150,7 +143,7 @@
150 143 <Structure>
151 144 <Size>2</Size>
152 145 <Element>
153   - <Name>Magnetic Field Spectral Density Parallel to Bo (10-180 Hz)</Name>
  146 + <Name>parallel to b0</Name>
154 147 <Index>1</Index>
155 148 <ParameterKey>c1_sta_f2(0)</ParameterKey>
156 149 <ValidMin>1.0000e-9</ValidMin>
... ... @@ -162,7 +155,7 @@
162 155 </RenderingHints>
163 156 </Element>
164 157 <Element>
165   - <Name>Magnetic Field Spectral Density Perpendicular to Bo (10-180 Hz)</Name>
  158 + <Name>perpendicular to b0</Name>
166 159 <Index>2</Index>
167 160 <ParameterKey>c1_sta_f2(1)</ParameterKey>
168 161 <ValidMin>1.0000e-9</ValidMin>
... ... @@ -186,11 +179,9 @@
186 179 </Field>
187 180 </Parameter>
188 181 <Parameter>
189   - <Name>Magnetic Field Spectral Density (180-4000 Hz)</Name>
  182 + <Name>b spectral density (180-4000 Hz)</Name>
190 183 <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)
194 185 </Description>
195 186 <Ucd>phys.flux.density;phys.magField</Ucd>
196 187 <Cadence>PT4S</Cadence>
... ... @@ -202,7 +193,7 @@
202 193 <Structure>
203 194 <Size>2</Size>
204 195 <Element>
205   - <Name>Magnetic Field Spectral Density Parallel to Bo (180-4000 Hz)</Name>
  196 + <Name>parallel to b0</Name>
206 197 <Index>1</Index>
207 198 <ParameterKey>c1_sta_f3(0)</ParameterKey>
208 199 <ValidMin>1.0000e-11</ValidMin>
... ... @@ -214,7 +205,7 @@
214 205 </RenderingHints>
215 206 </Element>
216 207 <Element>
217   - <Name>Magnetic Field Spectral Density Perpendicular to Bo (180-4000 Hz)</Name>
  208 + <Name>perpendicular to b0</Name>
218 209 <Index>2</Index>
219 210 <ParameterKey>c1_sta_f3(1)</ParameterKey>
220 211 <ValidMin>1.0000e-9</ValidMin>
... ... @@ -236,14 +227,11 @@
236 227 <Units>Hz</Units>
237 228 </FrequencyRange>
238 229 </Field>
239   - </Parameter>
240   -
  230 + </Parameter>
241 231 <Parameter>
242   - <Name>Electric Field Spectral Density (10-180 Hz)</Name>
  232 + <Name>e spectral density (10-180 Hz)</Name>
243 233 <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.
247 235 </Description>
248 236 <Ucd>phys.flux.density;phys.electField</Ucd>
249 237 <Cadence>PT4S</Cadence>
... ... @@ -269,11 +257,9 @@
269 257 </Field>
270 258 </Parameter>
271 259 <Parameter>
272   - <Name>Electric Field Spectral Density (180-4000 Hz)</Name>
  260 + <Name>e spectral density (180-4000 Hz)</Name>
273 261 <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.
277 263 </Description>
278 264 <Ucd>phys.flux.density;phys.electField</Ucd>
279 265 <Cadence>PT4S</Cadence>
... ...
NumericalData/AMDA/Cluster/Cluster2/STAFF/clust2-sta-pp.xml
  Diff comments   View file @a128b91
... ... @@ -6,30 +6,31 @@
6 6 <ResourceHeader>
7 7 <ResourceName>prime parameters</ResourceName>
8 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 18 </Description>
18   - <Acknowledgement>ESA, Nicole Cornilleau-Wehrlin</Acknowledgement>
  19 + <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
19 20 <Contact>
20   - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID>
  21 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
21 22 <Role>PrincipalInvestigator</Role>
22 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 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 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 34 </ResourceHeader>
34 35 <AccessInformation>
35 36 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
... ... @@ -39,15 +40,11 @@
39 40 <Name>AMDA at CDPP</Name>
40 41 <URL>http://amda.cdpp.eu</URL>
41 42 </AccessURL>
42   - <Format>NetCDF</Format>
43   - <Acknowledgement>NASA, Nicole Cornilleau-Wehrlin</Acknowledgement>
  43 + <Format>NetCDF</Format>
44 44 </AccessInformation>
45 45 <ProviderName>CSDS-CNES</ProviderName>
46 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 48 <MeasurementType>ElectricField</MeasurementType>
52 49 <MeasurementType>MagneticField</MeasurementType>
53 50 <MeasurementType>Waves.Passive</MeasurementType>
... ... @@ -57,9 +54,9 @@
57 54 <StopDate>2012-12-31T23:59:46Z</StopDate>
58 55 </TimeSpan>
59 56 <Cadence>PT4S</Cadence>
60   - </TemporalDescription>
61   - <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
  57 + </TemporalDescription>
62 58 <ObservedRegion>Earth.Magnetosphere</ObservedRegion>
  59 + <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
63 60 <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion>
64 61 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion>
65 62 <ObservedRegion>Earth.Magnetosphere.Polar</ObservedRegion>
... ... @@ -79,25 +76,23 @@
79 76 <Keyword>magnetosheath</Keyword>
80 77 <Keyword>Cluster</Keyword>
81 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 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 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 93 <Size>2</Size>
99 94 <Element>
100   - <Name>Magnetic Field Spectral Power Parallel to Bo (1-10 Hz)</Name>
  95 + <Name>parallel to b0</Name>
101 96 <Index>1</Index>
102 97 <ParameterKey>c2_sta_f1(0)</ParameterKey>
103 98 <ValidMin>1.0000e-7</ValidMin>
... ... @@ -109,7 +104,7 @@
109 104 </RenderingHints>
110 105 </Element>
111 106 <Element>
112   - <Name>Magnetic Field Spectral Power Perpendicular to Bo (1-10 Hz)</Name>
  107 + <Name>perpendicular to b0</Name>
113 108 <Index>2</Index>
114 109 <ParameterKey>c2_sta_f1(1)</ParameterKey>
115 110 <ValidMin>1.0000e-7</ValidMin>
... ... @@ -119,7 +114,7 @@
119 114 <ScaleMin>1.0000e-6</ScaleMin>
120 115 <ScaleMax>1</ScaleMax>
121 116 </RenderingHints>
122   - </Element>
  117 + </Element>
123 118 </Structure>
124 119 <FillValue>-1.0000e+31</FillValue>
125 120 <Field>
... ... @@ -132,12 +127,11 @@
132 127 </FrequencyRange>
133 128 </Field>
134 129 </Parameter>
  130 +
135 131 <Parameter>
136   - <Name>Magnetic Field Spectral Power (10-180 Hz)</Name>
  132 + <Name>b spectral density (10-180 Hz)</Name>
137 133 <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)
141 135 </Description>
142 136 <Ucd>phys.flux.density;phys.magField</Ucd>
143 137 <Cadence>PT4S</Cadence>
... ... @@ -149,7 +143,7 @@
149 143 <Structure>
150 144 <Size>2</Size>
151 145 <Element>
152   - <Name>Magnetic Field Spectral Power Parallel to Bo (10-180 Hz)</Name>
  146 + <Name>parallel to b0</Name>
153 147 <Index>1</Index>
154 148 <ParameterKey>c2_sta_f2(0)</ParameterKey>
155 149 <ValidMin>1.0000e-9</ValidMin>
... ... @@ -161,7 +155,7 @@
161 155 </RenderingHints>
162 156 </Element>
163 157 <Element>
164   - <Name>Magnetic Field Spectral Power Perpendicular to Bo (10-180 Hz)</Name>
  158 + <Name>perpendicular to b0</Name>
165 159 <Index>2</Index>
166 160 <ParameterKey>c2_sta_f2(1)</ParameterKey>
167 161 <ValidMin>1.0000e-9</ValidMin>
... ... @@ -185,11 +179,9 @@
185 179 </Field>
186 180 </Parameter>
187 181 <Parameter>
188   - <Name>Magnetic Field Spectral Power (180-4000 Hz)</Name>
  182 + <Name>b spectral density (180-4000 Hz)</Name>
189 183 <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)
193 185 </Description>
194 186 <Ucd>phys.flux.density;phys.magField</Ucd>
195 187 <Cadence>PT4S</Cadence>
... ... @@ -201,7 +193,7 @@
201 193 <Structure>
202 194 <Size>2</Size>
203 195 <Element>
204   - <Name>Magnetic Field Spectral Power Parallel to Bo (180-4000 Hz)</Name>
  196 + <Name>parallel to b0</Name>
205 197 <Index>1</Index>
206 198 <ParameterKey>c2_sta_f3(0)</ParameterKey>
207 199 <ValidMin>1.0000e-11</ValidMin>
... ... @@ -213,7 +205,7 @@
213 205 </RenderingHints>
214 206 </Element>
215 207 <Element>
216   - <Name>Magnetic Field Spectral Power Perpendicular to Bo (180-4000 Hz)</Name>
  208 + <Name>perpendicular to b0</Name>
217 209 <Index>2</Index>
218 210 <ParameterKey>c2_sta_f3(1)</ParameterKey>
219 211 <ValidMin>1.0000e-9</ValidMin>
... ... @@ -235,13 +227,11 @@
235 227 <Units>Hz</Units>
236 228 </FrequencyRange>
237 229 </Field>
238   - </Parameter>
  230 + </Parameter>
239 231 <Parameter>
240   - <Name>Electric Field Spectral Power (10-180 Hz)</Name>
  232 + <Name>e spectral density (10-180 Hz)</Name>
241 233 <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.
245 235 </Description>
246 236 <Ucd>phys.flux.density;phys.electField</Ucd>
247 237 <Cadence>PT4S</Cadence>
... ... @@ -267,11 +257,9 @@
267 257 </Field>
268 258 </Parameter>
269 259 <Parameter>
270   - <Name>Electric Field Spectral Power (180-4000 Hz)</Name>
  260 + <Name>e spectral density (180-4000 Hz)</Name>
271 261 <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.
275 263 </Description>
276 264 <Ucd>phys.flux.density;phys.electField</Ucd>
277 265 <Cadence>PT4S</Cadence>
... ...
NumericalData/AMDA/Cluster/Cluster3/STAFF/clust3-sta-pp.xml
  Diff comments   View file @a128b91
... ... @@ -6,30 +6,31 @@
6 6 <ResourceHeader>
7 7 <ResourceName>prime parameters</ResourceName>
8 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 18 </Description>
18   - <Acknowledgement>ESA, Nicole Cornilleau-Wehrlin</Acknowledgement>
  19 + <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
19 20 <Contact>
20   - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID>
  21 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
21 22 <Role>PrincipalInvestigator</Role>
22 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 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 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 34 </ResourceHeader>
34 35 <AccessInformation>
35 36 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
... ... @@ -39,14 +40,10 @@
39 40 <Name>AMDA at CDPP</Name>
40 41 <URL>http://amda.cdpp.eu</URL>
41 42 </AccessURL>
42   - <Format>NetCDF</Format>
43   - <Acknowledgement>NASA, Nicole Cornilleau-Wehrlin</Acknowledgement>
  43 + <Format>NetCDF</Format>
44 44 </AccessInformation>
45 45 <ProviderName>CSDS-CNES</ProviderName>
46 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 47 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Samba/STAFF</InstrumentID>
51 48 <MeasurementType>ElectricField</MeasurementType>
52 49 <MeasurementType>MagneticField</MeasurementType>
... ... @@ -57,9 +54,9 @@
57 54 <StopDate>2012-12-31T23:59:47Z</StopDate>
58 55 </TimeSpan>
59 56 <Cadence>PT4S</Cadence>
60   - </TemporalDescription>
61   - <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
  57 + </TemporalDescription>
62 58 <ObservedRegion>Earth.Magnetosphere</ObservedRegion>
  59 + <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
63 60 <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion>
64 61 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion>
65 62 <ObservedRegion>Earth.Magnetosphere.Polar</ObservedRegion>
... ... @@ -79,13 +76,11 @@
79 76 <Keyword>magnetosheath</Keyword>
80 77 <Keyword>Cluster</Keyword>
81 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 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 84 </Description>
90 85 <Ucd>phys.flux.density;phys.magField</Ucd>
91 86 <Cadence>PT4S</Cadence>
... ... @@ -94,10 +89,10 @@
94 89 <RenderingHints>
95 90 <DisplayType>TimeSeries</DisplayType>
96 91 </RenderingHints>
97   - <Structure>
  92 + <Structure>
98 93 <Size>2</Size>
99 94 <Element>
100   - <Name>Magnetic Field Spectral Power Parallel to Bo (1-10 Hz)</Name>
  95 + <Name>parallel to b0</Name>
101 96 <Index>1</Index>
102 97 <ParameterKey>c3_sta_f1(0)</ParameterKey>
103 98 <ValidMin>1.0000e-7</ValidMin>
... ... @@ -109,7 +104,7 @@
109 104 </RenderingHints>
110 105 </Element>
111 106 <Element>
112   - <Name>Magnetic Field Spectral Power Perpendicular to Bo (1-10 Hz)</Name>
  107 + <Name>perpendicular to b0</Name>
113 108 <Index>2</Index>
114 109 <ParameterKey>c3_sta_f1(1)</ParameterKey>
115 110 <ValidMin>1.0000e-7</ValidMin>
... ... @@ -119,7 +114,7 @@
119 114 <ScaleMin>1.0000e-6</ScaleMin>
120 115 <ScaleMax>1</ScaleMax>
121 116 </RenderingHints>
122   - </Element>
  117 + </Element>
123 118 </Structure>
124 119 <FillValue>-1.0000e+31</FillValue>
125 120 <Field>
... ... @@ -132,12 +127,11 @@
132 127 </FrequencyRange>
133 128 </Field>
134 129 </Parameter>
  130 +
135 131 <Parameter>
136   - <Name>Magnetic Field Spectral Power (10-180 Hz)</Name>
  132 + <Name>b spectral density (10-180 Hz)</Name>
137 133 <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)
141 135 </Description>
142 136 <Ucd>phys.flux.density;phys.magField</Ucd>
143 137 <Cadence>PT4S</Cadence>
... ... @@ -149,7 +143,7 @@
149 143 <Structure>
150 144 <Size>2</Size>
151 145 <Element>
152   - <Name>Magnetic Field Spectral Power Parallel to Bo (10-180 Hz)</Name>
  146 + <Name>parallel to b0</Name>
153 147 <Index>1</Index>
154 148 <ParameterKey>c3_sta_f2(0)</ParameterKey>
155 149 <ValidMin>1.0000e-9</ValidMin>
... ... @@ -161,7 +155,7 @@
161 155 </RenderingHints>
162 156 </Element>
163 157 <Element>
164   - <Name>Magnetic Field Spectral Power Perpendicular to Bo (10-180 Hz)</Name>
  158 + <Name>perpendicular to b0</Name>
165 159 <Index>2</Index>
166 160 <ParameterKey>c3_sta_f2(1)</ParameterKey>
167 161 <ValidMin>1.0000e-9</ValidMin>
... ... @@ -185,11 +179,9 @@
185 179 </Field>
186 180 </Parameter>
187 181 <Parameter>
188   - <Name>Magnetic Field Spectral Power (180-4000 Hz)</Name>
  182 + <Name>b spectral density (180-4000 Hz)</Name>
189 183 <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)
193 185 </Description>
194 186 <Ucd>phys.flux.density;phys.magField</Ucd>
195 187 <Cadence>PT4S</Cadence>
... ... @@ -201,7 +193,7 @@
201 193 <Structure>
202 194 <Size>2</Size>
203 195 <Element>
204   - <Name>Magnetic Field Spectral Power Parallel to Bo (180-4000 Hz)</Name>
  196 + <Name>parallel to b0</Name>
205 197 <Index>1</Index>
206 198 <ParameterKey>c3_sta_f3(0)</ParameterKey>
207 199 <ValidMin>1.0000e-11</ValidMin>
... ... @@ -213,7 +205,7 @@
213 205 </RenderingHints>
214 206 </Element>
215 207 <Element>
216   - <Name>Magnetic Field Spectral Power Perpendicular to Bo (180-4000 Hz)</Name>
  208 + <Name>perpendicular to b0</Name>
217 209 <Index>2</Index>
218 210 <ParameterKey>c3_sta_f3(1)</ParameterKey>
219 211 <ValidMin>1.0000e-9</ValidMin>
... ... @@ -235,13 +227,11 @@
235 227 <Units>Hz</Units>
236 228 </FrequencyRange>
237 229 </Field>
238   - </Parameter>
  230 + </Parameter>
239 231 <Parameter>
240   - <Name>Electric Field Spectral Power (10-180 Hz)</Name>
  232 + <Name>e spectral density (10-180 Hz)</Name>
241 233 <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.
245 235 </Description>
246 236 <Ucd>phys.flux.density;phys.electField</Ucd>
247 237 <Cadence>PT4S</Cadence>
... ... @@ -267,11 +257,9 @@
267 257 </Field>
268 258 </Parameter>
269 259 <Parameter>
270   - <Name>Electric Field Spectral Power (180-4000 Hz)</Name>
  260 + <Name>e spectral density (180-4000 Hz)</Name>
271 261 <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.
275 263 </Description>
276 264 <Ucd>phys.flux.density;phys.electField</Ucd>
277 265 <Cadence>PT4S</Cadence>
... ...
NumericalData/AMDA/Cluster/Cluster4/STAFF/clust4-sta-pp.xml
  Diff comments   View file @a128b91
... ... @@ -6,30 +6,31 @@
6 6 <ResourceHeader>
7 7 <ResourceName>prime parameters</ResourceName>
8 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 18 </Description>
18   - <Acknowledgement>ESA, Nicole Cornilleau-Wehrlin</Acknowledgement>
  19 + <Acknowledgement>Principal Investigator: Patrick Canu</Acknowledgement>
19 20 <Contact>
20   - <PersonID>spase://SMWG/Person/Nicole.Cornilleau-Wehrlin</PersonID>
  21 + <PersonID>spase://SMWG/Person/Patrick.Canu</PersonID>
21 22 <Role>PrincipalInvestigator</Role>
22 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 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 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 34 </ResourceHeader>
34 35 <AccessInformation>
35 36 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
... ... @@ -39,14 +40,10 @@
39 40 <Name>AMDA at CDPP</Name>
40 41 <URL>http://amda.cdpp.eu</URL>
41 42 </AccessURL>
42   - <Format>NetCDF</Format>
43   - <Acknowledgement/>
  43 + <Format>NetCDF</Format>
44 44 </AccessInformation>
45 45 <ProviderName>CSDS-CNES</ProviderName>
46 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 47 <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Tango/STAFF</InstrumentID>
51 48 <MeasurementType>ElectricField</MeasurementType>
52 49 <MeasurementType>MagneticField</MeasurementType>
... ... @@ -57,9 +54,9 @@
57 54 <StopDate>2012-12-31T23:59:45Z</StopDate>
58 55 </TimeSpan>
59 56 <Cadence>PT4S</Cadence>
60   - </TemporalDescription>
61   - <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
  57 + </TemporalDescription>
62 58 <ObservedRegion>Earth.Magnetosphere</ObservedRegion>
  59 + <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
63 60 <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion>
64 61 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion>
65 62 <ObservedRegion>Earth.Magnetosphere.Polar</ObservedRegion>
... ... @@ -79,13 +76,11 @@
79 76 <Keyword>magnetosheath</Keyword>
80 77 <Keyword>Cluster</Keyword>
81 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 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 84 </Description>
90 85 <Ucd>phys.flux.density;phys.magField</Ucd>
91 86 <Cadence>PT4S</Cadence>
... ... @@ -94,10 +89,10 @@
94 89 <RenderingHints>
95 90 <DisplayType>TimeSeries</DisplayType>
96 91 </RenderingHints>
97   - <Structure>
  92 + <Structure>
98 93 <Size>2</Size>
99 94 <Element>
100   - <Name>Magnetic Field Spectral Power Parallel to Bo (1-10 Hz)</Name>
  95 + <Name>parallel to b0</Name>
101 96 <Index>1</Index>
102 97 <ParameterKey>c4_sta_f1(0)</ParameterKey>
103 98 <ValidMin>1.0000e-7</ValidMin>
... ... @@ -109,7 +104,7 @@
109 104 </RenderingHints>
110 105 </Element>
111 106 <Element>
112   - <Name>Magnetic Field Spectral Power Perpendicular to Bo (1-10 Hz)</Name>
  107 + <Name>perpendicular to b0</Name>
113 108 <Index>2</Index>
114 109 <ParameterKey>c4_sta_f1(1)</ParameterKey>
115 110 <ValidMin>1.0000e-7</ValidMin>
... ... @@ -119,7 +114,7 @@
119 114 <ScaleMin>1.0000e-6</ScaleMin>
120 115 <ScaleMax>1</ScaleMax>
121 116 </RenderingHints>
122   - </Element>
  117 + </Element>
123 118 </Structure>
124 119 <FillValue>-1.0000e+31</FillValue>
125 120 <Field>
... ... @@ -132,12 +127,11 @@
132 127 </FrequencyRange>
133 128 </Field>
134 129 </Parameter>
  130 +
135 131 <Parameter>
136   - <Name>Magnetic Field Spectral Power (10-180 Hz)</Name>
  132 + <Name>b spectral density (10-180 Hz)</Name>
137 133 <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)
141 135 </Description>
142 136 <Ucd>phys.flux.density;phys.magField</Ucd>
143 137 <Cadence>PT4S</Cadence>
... ... @@ -149,7 +143,7 @@
149 143 <Structure>
150 144 <Size>2</Size>
151 145 <Element>
152   - <Name>Magnetic Field Spectral Power Parallel to Bo (10-180 Hz)</Name>
  146 + <Name>parallel to b0</Name>
153 147 <Index>1</Index>
154 148 <ParameterKey>c4_sta_f2(0)</ParameterKey>
155 149 <ValidMin>1.0000e-9</ValidMin>
... ... @@ -161,7 +155,7 @@
161 155 </RenderingHints>
162 156 </Element>
163 157 <Element>
164   - <Name>Magnetic Field Spectral Power Perpendicular to Bo (10-180 Hz)</Name>
  158 + <Name>perpendicular to b0</Name>
165 159 <Index>2</Index>
166 160 <ParameterKey>c4_sta_f2(1)</ParameterKey>
167 161 <ValidMin>1.0000e-9</ValidMin>
... ... @@ -185,11 +179,9 @@
185 179 </Field>
186 180 </Parameter>
187 181 <Parameter>
188   - <Name>Magnetic Field Spectral Power (180-4000 Hz)</Name>
  182 + <Name>b spectral density (180-4000 Hz)</Name>
189 183 <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)
193 185 </Description>
194 186 <Ucd>phys.flux.density;phys.magField</Ucd>
195 187 <Cadence>PT4S</Cadence>
... ... @@ -201,7 +193,7 @@
201 193 <Structure>
202 194 <Size>2</Size>
203 195 <Element>
204   - <Name>Magnetic Field Spectral Power Parallel to Bo (180-4000 Hz)</Name>
  196 + <Name>parallel to b0</Name>
205 197 <Index>1</Index>
206 198 <ParameterKey>c4_sta_f3(0)</ParameterKey>
207 199 <ValidMin>1.0000e-11</ValidMin>
... ... @@ -213,7 +205,7 @@
213 205 </RenderingHints>
214 206 </Element>
215 207 <Element>
216   - <Name>Magnetic Field Spectral Power Perpendicular to Bo (180-4000 Hz)</Name>
  208 + <Name>perpendicular to b0</Name>
217 209 <Index>2</Index>
218 210 <ParameterKey>c4_sta_f3(1)</ParameterKey>
219 211 <ValidMin>1.0000e-9</ValidMin>
... ... @@ -235,13 +227,11 @@
235 227 <Units>Hz</Units>
236 228 </FrequencyRange>
237 229 </Field>
238   - </Parameter>
  230 + </Parameter>
239 231 <Parameter>
240   - <Name>Electric Field Spectral Power (10-180 Hz)</Name>
  232 + <Name>e spectral density (10-180 Hz)</Name>
241 233 <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.
245 235 </Description>
246 236 <Ucd>phys.flux.density;phys.electField</Ucd>
247 237 <Cadence>PT4S</Cadence>
... ... @@ -267,11 +257,9 @@
267 257 </Field>
268 258 </Parameter>
269 259 <Parameter>
270   - <Name>Electric Field Spectral Power (180-4000 Hz)</Name>
  260 + <Name>e spectral density (180-4000 Hz)</Name>
271 261 <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.
275 263 </Description>
276 264 <Ucd>phys.flux.density;phys.electField</Ucd>
277 265 <Cadence>PT4S</Cadence>
... ...
NumericalData/AMDA/Indices/Ground_Based/ground-based-dst.xml
  Diff comments   View file @a128b91
... ... @@ -47,7 +47,7 @@
47 47 <TemporalDescription>
48 48 <TimeSpan>
49 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 51 </TimeSpan>
52 52 <Cadence>PT1H</Cadence></TemporalDescription>
53 53 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion>
... ...
NumericalData/AMDA/MAVEN/EUV/mvn-euv-clb.xml
  Diff comments   View file @a128b91
... ... @@ -45,7 +45,7 @@
45 45 <TemporalDescription>
46 46 <TimeSpan>
47 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 49 </TimeSpan>
50 50 <Cadence>PT60S</Cadence>
51 51 </TemporalDescription>
... ...
NumericalData/AMDA/MAVEN/Ephemeris/maven-orb-marsobs.xml
  Diff comments   View file @a128b91
... ... @@ -49,7 +49,7 @@
49 49 <TemporalDescription>
50 50 <TimeSpan>
51 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 53 </TimeSpan>
54 54 <Cadence>PT1M</Cadence>
55 55 </TemporalDescription>
... ...
NumericalData/AMDA/MAVEN/MAG/mav-mag-pds.xml
  Diff comments   View file @a128b91
... ... @@ -48,7 +48,7 @@
48 48 <TemporalDescription>
49 49 <TimeSpan>
50 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 52 </TimeSpan>
53 53 <Cadence>PT0.031S</Cadence>
54 54 </TemporalDescription>
... ...
NumericalData/AMDA/MAVEN/STATIC/mavpds-sta-c0.xml
  Diff comments   View file @a128b91
... ... @@ -44,7 +44,7 @@
44 44 <TemporalDescription>
45 45 <TimeSpan>
46 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 48 </TimeSpan>
49 49 <Cadence>PT4S</Cadence>
50 50 </TemporalDescription>
... ...
NumericalData/AMDA/MAVEN/STATIC/mavpds-sta-c6.xml
  Diff comments   View file @a128b91
... ... @@ -47,7 +47,7 @@
47 47 <TemporalDescription>
48 48 <TimeSpan>
49 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 51 </TimeSpan>
52 52 <Cadence>PT4S</Cadence>
53 53 </TemporalDescription>
... ...
NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-momboard.xml
  Diff comments   View file @a128b91
... ... @@ -48,7 +48,7 @@
48 48 <TemporalDescription>
49 49 <TimeSpan>
50 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 52 </TimeSpan>
53 53 <Cadence>PT4S</Cadence></TemporalDescription>
54 54 <ObservedRegion>Mars</ObservedRegion>
... ...
NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-specboard.xml
  Diff comments   View file @a128b91
... ... @@ -45,7 +45,7 @@
45 45 <TemporalDescription>
46 46 <TimeSpan>
47 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 49 </TimeSpan>
50 50 <Cadence>PT4S</Cadence></TemporalDescription>
51 51 <ObservedRegion>Mars</ObservedRegion>
... ...