diff --git a/Instrument/AMDA/Cluster-Rumba/FGM.xml b/Instrument/AMDA/Cluster-Rumba/FGM.xml
index cddcf45..67514d0 100644
--- a/Instrument/AMDA/Cluster-Rumba/FGM.xml
+++ b/Instrument/AMDA/Cluster-Rumba/FGM.xml
@@ -5,14 +5,19 @@
<ResourceID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/FGM</ResourceID>
<ResourceHeader>
<ResourceName>FGM</ResourceName>
- <AlternateName>Fluxgate Magnetometer (FGM)</AlternateName>
- <ReleaseDate>2011-02-04T15:37:46Z</ReleaseDate>
- <Description>This instrument (FGM: Fluxgate Magnetometer) consists of two tri-axial fluxgate magnetometers mounted on one of the two 5 m radial booms, plus a data processing unit (DPU) on the main equipment platform. The magnetometer boom lies in the spacecraft spin plane, with the outboard sensor at the boom tip and the inboard sensor mounted 1.5 m inboard from the tip, to minimize the importance of the spacecraft background magnetic field and its variations. The sensors are mounted such that the X axes are aligned with the spacecraft spin axis, and the other axes are in the spin plane. There are five sensitivity ranges, from +/- 256 nT to +/- 65,500 nT (used only to facilitate ground testing). Range switching can be automatic or by command. Calibration is done by introducing a known current step into the feedback loop of the sensors. Telemetry allocation limits the normal output to about 20 vectors/s. For short periods at higher time resolution, data are stored at rates of up to 124.3 vectors/s in a memory block, the micro-structure analyzer (MSA). The MSA capacity is 32,000 vectors, more than 4 minutes of data at the highest sampling rate. This memory is continually over-written until a special event is detected, when its contents are frozen and held for readout interleaved with the normal lower-resolution data. The DPU has dual redundancy, including two CPUs. The CPU convolves the full bandwidth data with a Gaussian digital filter to match the rate and bandwidth of the transmitted vectors to the available telemetry rate. Unfiltered vector data are sent at 64.35 ms intervals to all but one of the other experiments. The DPU has a number of stored algorithms for recognition of events of particular interest, to trigger the MSA. The objective is to identify such events as boundary crossings or shocks when the high-rate capability of the MSA for short periods could capture the detailed signature of the event. The algorithms were defined at an early stage, but resettable thresholds for the event triggers will enable optimization in flight. There are eight different telemetry operating modes of the instrument, corresponding to both normal and burst modes, with MSA readout rates of 0, 9, 12, or 120 vectors/s. 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 Cluster Magnetic Field Investigation: scientific objective and instrumentation,'' by A. Balogh et al., from which this information was obtained.</Description>
+ <AlternateName>Fluxgate Magnetometer</AlternateName>
+ <ReleaseDate>2016-11-04T15:37:46Z</ReleaseDate>
+ <Description>FGM (Fluxgate Magnetometer) consists of two tri-axial fluxgate magnetometers mounted on one of the two 5 m radial booms, plus a data processing unit (DPU) on the main equipment platform. The magnetometer boom lies in the spacecraft spin plane, with the outboard sensor at the boom tip and the inboard sensor mounted 1.5 m inboard from the tip, to minimize the importance of the spacecraft background magnetic field and its variations. The sensors are mounted such that the X axes are aligned with the spacecraft spin axis, and the other axes are in the spin plane. There are five sensitivity ranges, from +/- 256 nT to +/- 65,500 nT (used only to facilitate ground testing). Range switching can be automatic or by command. Calibration is done by introducing a known current step into the feedback loop of the sensors. Telemetry allocation limits the normal output to about 20 vectors/s.</Description>
<Contact>
- <PersonID>spase://SMWG/Person/Andre.Balogh</PersonID>
+ <PersonID>spase://SMWG/Person/Chris.Carr</PersonID>
<Role>PrincipalInvestigator</Role>
</Contact>
<InformationURL>
+ <Name>ESA web page</Name>
+ <URL>http://sci.esa.int/jump.cfm?oid=33024</URL>
+ <Description>Fluxgate Magnetometer</Description>
+ </InformationURL>
+ <InformationURL>
<Name>NSSDC's Master Catalog</Name>
<URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-045A&ex=4</URL>
<Description>Information about the Fluxgate Magnetometer (FGM) experiment on the Cluster 2/FM5 (Rumba) mission.</Description>
@@ -20,7 +25,11 @@
<PriorID>spase://SMWG/Instrument/Cluster2-Rumba/FGM</PriorID>
</ResourceHeader>
<InstrumentType>Magnetometer</InstrumentType>
- <InvestigationName>Fluxgate Magnetometer (FGM) on Cluster 2/FM5 (Rumba)</InvestigationName>
+ <InvestigationName></InvestigationName>
+ <OperatingSpan>
+ <StartDate>2000-12-01T00:00:00</StartDate>
+ <Note>Start of full orbit coverage: 2002-06-01T00:00:00</Note>
+ </OperatingSpan>
<ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Rumba</ObservatoryID>
</Instrument>
</Spase>
diff --git a/Instrument/AMDA/Cluster-Salsa/FGM.xml b/Instrument/AMDA/Cluster-Salsa/FGM.xml
index 402524f..077f601 100644
--- a/Instrument/AMDA/Cluster-Salsa/FGM.xml
+++ b/Instrument/AMDA/Cluster-Salsa/FGM.xml
@@ -6,21 +6,30 @@
<ResourceHeader>
<ResourceName>FGM</ResourceName>
<AlternateName>Fluxgate Magnetometer</AlternateName>
- <ReleaseDate>2011-02-04T15:37:33Z</ReleaseDate>
- <Description>This instrument (FGM: Fluxgate Magnetometer) consists of two tri-axial fluxgate magnetometers mounted on one of the two 5 m radial booms, plus a data processing unit (DPU) on the main equipment platform. The magnetometer boom lies in the spacecraft spin plane, with the outboard sensor at the boom tip and the inboard sensor mounted 1.5 m inboard from the tip, to minimize the importance of the spacecraft background magnetic field and its variations. The sensors are mounted such that the X axes are aligned with the spacecraft spin axis, and the other axes are in the spin plane. There are five sensitivity ranges, from +/- 256 nT to +/- 65,500 nT (used only to facilitate ground testing). Range switching can be automatic or by command. Calibration is done by introducing a known current step into the feedback loop of the sensors. Telemetry allocation limits the normal output to about 20 vectors/s. For short periods at higher time resolution, data are stored at rates of up to 124.3 vectors/s in a memory block, the micro-structure analyzer (MSA). The MSA capacity is 32,000 vectors, more than 4 minutes of data at the highest sampling rate. This memory is continually over-written until a special event is detected, when its contents are frozen and held for readout interleaved with the normal lower-resolution data. The DPU has dual redundancy, including two CPUs. The CPU convolves the full bandwidth data with a Gaussian digital filter to match the rate and bandwidth of the transmitted vectors to the available telemetry rate. Unfiltered vector data are sent at 64.35 ms intervals to all but one of the other experiments. The DPU has a number of stored algorithms for recognition of events of particular interest, to trigger the MSA. The objective is to identify such events as boundary crossings or shocks when the high-rate capability of the MSA for short periods could capture the detailed signature of the event. The algorithms were defined at an early stage, but resettable thresholds for the event triggers will enable optimization in flight. There are eight different telemetry operating modes of the instrument, corresponding to both normal and burst modes, with MSA readout rates of 0, 9, 12, or 120 vectors/s. 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 Cluster Magnetic Field Investigation: scientific objective and instrumentation,'' by A. Balogh et al., from which this information was obtained.</Description>
+ <ReleaseDate>2016-11-04T15:37:46Z</ReleaseDate>
+ <Description>FGM (Fluxgate Magnetometer) consists of two tri-axial fluxgate magnetometers mounted on one of the two 5 m radial booms, plus a data processing unit (DPU) on the main equipment platform. The magnetometer boom lies in the spacecraft spin plane, with the outboard sensor at the boom tip and the inboard sensor mounted 1.5 m inboard from the tip, to minimize the importance of the spacecraft background magnetic field and its variations. The sensors are mounted such that the X axes are aligned with the spacecraft spin axis, and the other axes are in the spin plane. There are five sensitivity ranges, from +/- 256 nT to +/- 65,500 nT (used only to facilitate ground testing). Range switching can be automatic or by command. Calibration is done by introducing a known current step into the feedback loop of the sensors. Telemetry allocation limits the normal output to about 20 vectors/s.</Description>
<Contact>
- <PersonID>spase://SMWG/Person/Andre.Balogh</PersonID>
+ <PersonID>spase://SMWG/Person/Chris.Carr</PersonID>
<Role>PrincipalInvestigator</Role>
</Contact>
<InformationURL>
+ <Name>ESA web page</Name>
+ <URL>http://sci.esa.int/jump.cfm?oid=33024</URL>
+ <Description>Fluxgate Magnetometer</Description>
+ </InformationURL>
+ <InformationURL>
<Name>NSSDC's Master Catalog</Name>
- <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-041B&ex=4</URL>
+ <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-045A&ex=4</URL>
<Description>Information about the Fluxgate Magnetometer (FGM) experiment on the Cluster 2/FM6 (Salsa) mission.</Description>
</InformationURL>
<PriorID>spase://SMWG/Instrument/Cluster2-Salsa/FGM</PriorID>
</ResourceHeader>
<InstrumentType>Magnetometer</InstrumentType>
- <InvestigationName>Fluxgate Magnetometer (FGM) on Cluster 2/FM6 (Salsa)</InvestigationName>
+ <InvestigationName></InvestigationName>
+ <OperatingSpan>
+ <StartDate>2000-12-01T00:00:00</StartDate>
+ <Note>Start of full orbit coverage: 2002-06-01T00:00:00</Note>
+ </OperatingSpan>
<ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Salsa</ObservatoryID>
</Instrument>
</Spase>
diff --git a/Instrument/AMDA/Cluster-Samba/FGM.xml b/Instrument/AMDA/Cluster-Samba/FGM.xml
index 67962c0..6b9650c 100644
--- a/Instrument/AMDA/Cluster-Samba/FGM.xml
+++ b/Instrument/AMDA/Cluster-Samba/FGM.xml
@@ -6,21 +6,31 @@
<ResourceHeader>
<ResourceName>FGM</ResourceName>
<AlternateName>Fluxgate Magnetometer</AlternateName>
- <ReleaseDate>2011-02-04T15:37:07Z</ReleaseDate>
- <Description>This instrument (FGM: Fluxgate Magnetometer) consists of two tri-axial fluxgate magnetometers mounted on one of the two 5 m radial booms, plus a data processing unit (DPU) on the main equipment platform. The magnetometer boom lies in the spacecraft spin plane, with the outboard sensor at the boom tip and the inboard sensor mounted 1.5 m inboard from the tip, to minimize the importance of the spacecraft background magnetic field and its variations. The sensors are mounted such that the X axes are aligned with the spacecraft spin axis, and the other axes are in the spin plane. There are five sensitivity ranges, from +/- 256 nT to +/- 65,500 nT (used only to facilitate ground testing). Range switching can be automatic or by command. Calibration is done by introducing a known current step into the feedback loop of the sensors. Telemetry allocation limits the normal output to about 20 vectors/s. For short periods at higher time resolution, data are stored at rates of up to 124.3 vectors/s in a memory block, the micro-structure analyzer (MSA). The MSA capacity is 32,000 vectors, more than 4 minutes of data at the highest sampling rate. This memory is continually over-written until a special event is detected, when its contents are frozen and held for readout interleaved with the normal lower-resolution data. The DPU has dual redundancy, including two CPUs. The CPU convolves the full bandwidth data with a Gaussian digital filter to match the rate and bandwidth of the transmitted vectors to the available telemetry rate. Unfiltered vector data are sent at 64.35 ms intervals to all but one of the other experiments. The DPU has a number of stored algorithms for recognition of events of particular interest, to trigger the MSA. The objective is to identify such events as boundary crossings or shocks when the high-rate capability of the MSA for short periods could capture the detailed signature of the event. The algorithms were defined at an early stage, but resettable thresholds for the event triggers will enable optimization in flight. There are eight different telemetry operating modes of the instrument, corresponding to both normal and burst modes, with MSA readout rates of 0, 9, 12, or 120 vectors/s. 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 Cluster Magnetic Field Investigation: scientific objective and instrumentation,'' by A. Balogh et al., from which this information was obtained.</Description>
+ <ReleaseDate>2016-11-04T15:37:46Z</ReleaseDate>
+ <Description>FGM (Fluxgate Magnetometer) consists of two tri-axial fluxgate magnetometers mounted on one of the two 5 m radial booms, plus a data processing unit (DPU) on the main equipment platform. The magnetometer boom lies in the spacecraft spin plane, with the outboard sensor at the boom tip and the inboard sensor mounted 1.5 m inboard from the tip, to minimize the importance of the spacecraft background magnetic field and its variations. The sensors are mounted such that the X axes are aligned with the spacecraft spin axis, and the other axes are in the spin plane. There are five sensitivity ranges, from +/- 256 nT to +/- 65,500 nT (used only to facilitate ground testing). Range switching can be automatic or by command. Calibration is done by introducing a known current step into the feedback loop of the sensors. Telemetry allocation limits the normal output to about 20 vectors/s.</Description>
<Contact>
- <PersonID>spase://SMWG/Person/Andre.Balogh</PersonID>
+ <PersonID>spase://SMWG/Person/Chris.Carr</PersonID>
<Role>PrincipalInvestigator</Role>
</Contact>
<InformationURL>
+ <Name>ESA web page</Name>
+ <URL>http://sci.esa.int/jump.cfm?oid=33024</URL>
+ <Description>Fluxgate Magnetometer</Description>
+ </InformationURL>
+ <InformationURL>
<Name>NSSDC's Master Catalog</Name>
- <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-041A&ex=4</URL>
+ <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-045A&ex=4</URL>
<Description>Information about the Fluxgate Magnetometer (FGM) experiment on the Cluster 2/FM7 (Samba) mission.</Description>
</InformationURL>
<PriorID>spase://SMWG/Instrument/Cluster2-Samba/FGM</PriorID>
</ResourceHeader>
<InstrumentType>Magnetometer</InstrumentType>
- <InvestigationName>Fluxgate Magnetometer (FGM) on Cluster 2/FM7 (Samba)</InvestigationName>
+ <InvestigationName></InvestigationName>
+ <OperatingSpan>
+ <StartDate>2000-12-01T00:00:00</StartDate>
+ <Note>Start of full orbit coverage: 2002-06-01T00:00:00</Note>
+ <Note>C3 spacecraft tilt by 40° during one month: 2008-05-01T00:00:00</Note>
+ </OperatingSpan>
<ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Samba</ObservatoryID>
</Instrument>
</Spase>
diff --git a/Instrument/AMDA/Cluster-Tango/FGM.xml b/Instrument/AMDA/Cluster-Tango/FGM.xml
index 76667e8..f0d0df9 100644
--- a/Instrument/AMDA/Cluster-Tango/FGM.xml
+++ b/Instrument/AMDA/Cluster-Tango/FGM.xml
@@ -6,21 +6,30 @@
<ResourceHeader>
<ResourceName>FGM</ResourceName>
<AlternateName>Fluxgate Magnetometer</AlternateName>
- <ReleaseDate>2011-02-04T15:37:19Z</ReleaseDate>
- <Description>This instrument (FGM: Fluxgate Magnetometer) consists of two tri-axial fluxgate magnetometers mounted on one of the two 5 m radial booms, plus a data processing unit (DPU) on the main equipment platform. The magnetometer boom lies in the spacecraft spin plane, with the outboard sensor at the boom tip and the inboard sensor mounted 1.5 m inboard from the tip, to minimize the importance of the spacecraft background magnetic field and its variations. The sensors are mounted such that the X axes are aligned with the spacecraft spin axis, and the other axes are in the spin plane. There are five sensitivity ranges, from +/- 256 nT to +/- 65,500 nT (used only to facilitate ground testing). Range switching can be automatic or by command. Calibration is done by introducing a known current step into the feedback loop of the sensors. Telemetry allocation limits the normal output to about 20 vectors/s. For short periods at higher time resolution, data are stored at rates of up to 124.3 vectors/s in a memory block, the micro-structure analyzer (MSA). The MSA capacity is 32,000 vectors, more than 4 minutes of data at the highest sampling rate. This memory is continually over-written until a special event is detected, when its contents are frozen and held for readout interleaved with the normal lower-resolution data. The DPU has dual redundancy, including two CPUs. The CPU convolves the full bandwidth data with a Gaussian digital filter to match the rate and bandwidth of the transmitted vectors to the available telemetry rate. Unfiltered vector data are sent at 64.35 ms intervals to all but one of the other experiments. The DPU has a number of stored algorithms for recognition of events of particular interest, to trigger the MSA. The objective is to identify such events as boundary crossings or shocks when the high-rate capability of the MSA for short periods could capture the detailed signature of the event. The algorithms were defined at an early stage, but resettable thresholds for the event triggers will enable optimization in flight. There are eight different telemetry operating modes of the instrument, corresponding to both normal and burst modes, with MSA readout rates of 0, 9, 12, or 120 vectors/s. 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 Cluster Magnetic Field Investigation: scientific objective and instrumentation,'' by A. Balogh et al., from which this information was obtained.</Description>
+ <ReleaseDate>2016-11-04T15:37:46Z</ReleaseDate>
+ <Description>FGM (Fluxgate Magnetometer) consists of two tri-axial fluxgate magnetometers mounted on one of the two 5 m radial booms, plus a data processing unit (DPU) on the main equipment platform. The magnetometer boom lies in the spacecraft spin plane, with the outboard sensor at the boom tip and the inboard sensor mounted 1.5 m inboard from the tip, to minimize the importance of the spacecraft background magnetic field and its variations. The sensors are mounted such that the X axes are aligned with the spacecraft spin axis, and the other axes are in the spin plane. There are five sensitivity ranges, from +/- 256 nT to +/- 65,500 nT (used only to facilitate ground testing). Range switching can be automatic or by command. Calibration is done by introducing a known current step into the feedback loop of the sensors. Telemetry allocation limits the normal output to about 20 vectors/s.</Description>
<Contact>
- <PersonID>spase://SMWG/Person/Andre.Balogh</PersonID>
+ <PersonID>spase://SMWG/Person/Chris.Carr</PersonID>
<Role>PrincipalInvestigator</Role>
</Contact>
<InformationURL>
+ <Name>ESA web page</Name>
+ <URL>http://sci.esa.int/jump.cfm?oid=33024</URL>
+ <Description>Fluxgate Magnetometer</Description>
+ </InformationURL>
+ <InformationURL>
<Name>NSSDC's Master Catalog</Name>
- <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-045B&ex=4</URL>
+ <URL>http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=2000-045A&ex=4</URL>
<Description>Information about the Fluxgate Magnetometer (FGM) experiment on the Cluster 2/FM8 (Tango) mission.</Description>
</InformationURL>
<PriorID>spase://SMWG/Instrument/Cluster2-Tango/FGM</PriorID>
</ResourceHeader>
<InstrumentType>Magnetometer</InstrumentType>
- <InvestigationName>Fluxgate Magnetometer (FGM) on Cluster 2/FM8 (Tango)</InvestigationName>
+ <InvestigationName></InvestigationName>
+ <OperatingSpan>
+ <StartDate>2000-12-01T00:00:00</StartDate>
+ <Note>Start of full orbit coverage: 2002-06-01T00:00:00</Note>
+ </OperatingSpan>
<ObservatoryID>spase://CDPP/Observatory/AMDA/Cluster-Tango</ObservatoryID>
</Instrument>
</Spase>
diff --git a/NumericalData/AMDA/Cluster/Cluster1/FGM/clust1-fgm-prp.xml b/NumericalData/AMDA/Cluster/Cluster1/FGM/clust1-fgm-prp.xml
index f0f9ce2..af701c9 100644
--- a/NumericalData/AMDA/Cluster/Cluster1/FGM/clust1-fgm-prp.xml
+++ b/NumericalData/AMDA/Cluster/Cluster1/FGM/clust1-fgm-prp.xml
@@ -6,14 +6,19 @@
<ResourceHeader>
<ResourceName>4 sec (spin)</ResourceName>
<AlternateName>Cluster 1 Spin Resolution FGM Data</AlternateName>
- <ReleaseDate>2015-10-16T16:14:00Z</ReleaseDate>
- <Description>This dataset contains spin resolution measurements of the magnetic field vector from the fluxgate magnetometer (FGM) instrument
- on the Cluster Rumba spacecraft.</Description>
- <Acknowledgement>NASA, Andre Balogh, Elizabeth E. Lucek</Acknowledgement>
+ <ReleaseDate>2016-10-16T16:14:00Z</ReleaseDate>
+ <Description>This dataset contains spin resolution (~4s) measurements of the magnetic field vector from the fluxgate magnetometer (FGM) instrument
+ on the Cluster1 spacecraft.</Description>
+ <Acknowledgement>Principal Investigator: Chris Carr</Acknowledgement>
<Contact>
- <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
- <Role>TechnicalContact</Role>
- </Contact>
+ <PersonID>spase://SMWG/Person/Chris.Carr</PersonID>
+ <Role>PrincipalInvestigator</Role>
+ </Contact>
+ <InformationURL>
+ <Name>ESA web page</Name>
+ <URL>http://www.cosmos.esa.int/web/csa/documentation</URL>
+ <Description>This site contains FGM data documentation</Description>
+ </InformationURL>
<InformationURL>
<Name>NSSDC Master Catalog listing for Cluster Rumba Fluxgate Magnetometer (FGM)</Name>
<URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-04</URL>
@@ -28,12 +33,11 @@
<Name>AMDA at CDPP</Name>
<URL>http://amda.cdpp.eu</URL>
</AccessURL>
- <Format>NetCDF</Format>
- <Acknowledgement>NASA, Andre Balogh, Elizabeth E. Lucek</Acknowledgement>
+ <Format>NetCDF</Format>
</AccessInformation>
<ProviderName>CSA</ProviderName>
<ProcessingLevel>Calibrated</ProcessingLevel>
- <ProviderResourceName>Cluster Rumba Spin Resolution Fluxgate Magnetometer (FGM) Data</ProviderResourceName>
+ <ProviderResourceName>C1_CP_FGM_SPIN</ProviderResourceName>
<ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
<InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Rumba/FGM</InstrumentID>
<MeasurementType>MagneticField</MeasurementType>
@@ -58,7 +62,7 @@
<Parameter>
<Name>b_gse</Name>
<ParameterKey>c1_b_gse</ParameterKey>
- <Description>Cluster Rumba Fluxgate Magnetometer magnetic field vector at spin time resolution</Description>
+ <Description>FGM: magnetic field vector (3 GSE components), 4s resolution</Description>
<Ucd>phys.magField</Ucd>
<Cadence>PT4S</Cadence>
<Units>nT</Units>
@@ -100,7 +104,7 @@
<Parameter>
<Name>b_gsm</Name>
<ParameterKey>c1_b_gsm</ParameterKey>
- <Description>Cluster Rumba Fluxgate Magnetometer magnetic field vector at spin time resolution</Description>
+ <Description>FGM: magnetic field vector (3 GSM components), 4s resolution</Description>
<Ucd>phys.magField</Ucd>
<Cadence>PT4S</Cadence>
<Units>nT</Units>
@@ -142,7 +146,7 @@
<Parameter>
<Name>|b|</Name>
<ParameterKey>c1_btot</ParameterKey>
- <Description>Cluster Rumba Fluxgate Magnetometer magnetic field magnitude at spin time resolution</Description>
+ <Description>FGM: magnetic field vector magnitude</Description>
<Ucd>phys.magField</Ucd>
<Cadence>PT4S</Cadence>
<Units>nT</Units>
diff --git a/NumericalData/AMDA/Cluster/Cluster2/FGM/clust2-fgm-prp.xml b/NumericalData/AMDA/Cluster/Cluster2/FGM/clust2-fgm-prp.xml
index 67c6a3c..eb91f83 100644
--- a/NumericalData/AMDA/Cluster/Cluster2/FGM/clust2-fgm-prp.xml
+++ b/NumericalData/AMDA/Cluster/Cluster2/FGM/clust2-fgm-prp.xml
@@ -6,16 +6,21 @@
<ResourceHeader>
<ResourceName>4 sec (spin)</ResourceName>
<AlternateName>Cluster 2 Spin Resolution FGM Data</AlternateName>
- <ReleaseDate>2015-10-19T00:00:00Z</ReleaseDate>
- <Description>This dataset contains spin resolution measurements of the magnetic field vector from the fluxgate magnetometer (FGM) instrument
- on the Cluster Rumba spacecraft.</Description>
- <Acknowledgement>NASA, Andre Balogh, Elizabeth E. Lucek</Acknowledgement>
+ <ReleaseDate>2016-10-16T16:14:00Z</ReleaseDate>
+ <Description>This dataset contains spin resolution (~4s) measurements of the magnetic field vector from the fluxgate magnetometer (FGM) instrument
+ on the Cluster2 spacecraft.</Description>
+ <Acknowledgement>Principal Investigator: Chris Carr</Acknowledgement>
<Contact>
- <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
- <Role>TechnicalContact</Role>
- </Contact>
+ <PersonID>spase://SMWG/Person/Chris.Carr</PersonID>
+ <Role>PrincipalInvestigator</Role>
+ </Contact>
<InformationURL>
- <Name>NSSDC Master Catalog listing for Cluster Rumba Fluxgate Magnetometer (FGM)</Name>
+ <Name>ESA web page</Name>
+ <URL>http://www.cosmos.esa.int/web/csa/documentation</URL>
+ <Description>This site contains FGM data documentation</Description>
+ </InformationURL>
+ <InformationURL>
+ <Name>NSSDC Master Catalog listing for Cluster Salsa Fluxgate Magnetometer (FGM)</Name>
<URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-04</URL>
<Description>This site provides information concerning the Cluster Salsa Fluxgate Magnetometer Instrument.</Description>
</InformationURL>
@@ -28,12 +33,11 @@
<Name>AMDA at CDPP</Name>
<URL>http://amda.cdpp.eu</URL>
</AccessURL>
- <Format>NetCDF</Format>
- <Acknowledgement>NASA, Andre Balogh, Elizabeth E. Lucek</Acknowledgement>
+ <Format>NetCDF</Format>
</AccessInformation>
<ProviderName>CSA</ProviderName>
<ProcessingLevel>Calibrated</ProcessingLevel>
- <ProviderResourceName>Cluster Salsa Spin Resolution Fluxgate Magnetometer (FGM) Data</ProviderResourceName>
+ <ProviderResourceName>C2_CP_FGM_SPIN</ProviderResourceName>
<ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
<InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Salsa/FGM</InstrumentID>
<MeasurementType>MagneticField</MeasurementType>
@@ -58,7 +62,7 @@
<Parameter>
<Name>b_gse</Name>
<ParameterKey>c2_b_gse</ParameterKey>
- <Description>Cluster Salsa Fluxgate Magnetometer magnetic field vector at spin time resolution</Description>
+ <Description>FGM: magnetic field vector (3 GSE components), 4s resolution</Description>
<Ucd>phys.magField</Ucd>
<Cadence>PT4S</Cadence>
<Units>nT</Units>
@@ -100,7 +104,7 @@
<Parameter>
<Name>b_gsm</Name>
<ParameterKey>c2_b_gsm</ParameterKey>
- <Description>Cluster Salsa Fluxgate Magnetometer magnetic field vector at spin time resolution</Description>
+ <Description>FGM: magnetic field vector (3 GSM components), 4s resolution</Description>
<Ucd>phys.magField</Ucd>
<Cadence>PT4S</Cadence>
<Units>nT</Units>
@@ -142,7 +146,7 @@
<Parameter>
<Name>|b|</Name>
<ParameterKey>c2_btot</ParameterKey>
- <Description>Cluster Salsa Fluxgate Magnetometer magnetic field magnitude at spin time resolution</Description>
+ <Description>FGM: magnetic field vector magnitude</Description>
<Ucd>phys.magField</Ucd>
<Cadence>PT4S</Cadence>
<Units>nT</Units>
diff --git a/NumericalData/AMDA/Cluster/Cluster3/FGM/clust3-fgm-prp.xml b/NumericalData/AMDA/Cluster/Cluster3/FGM/clust3-fgm-prp.xml
index 6e25838..8e2cc84 100644
--- a/NumericalData/AMDA/Cluster/Cluster3/FGM/clust3-fgm-prp.xml
+++ b/NumericalData/AMDA/Cluster/Cluster3/FGM/clust3-fgm-prp.xml
@@ -6,16 +6,21 @@
<ResourceHeader>
<ResourceName>4 sec (spin)</ResourceName>
<AlternateName>Cluster 3 Spin Resolution FGM Data</AlternateName>
- <ReleaseDate>2015-10-19T00:00:00Z</ReleaseDate>
- <Description>This dataset contains spin resolution measurements of the magnetic field vector from the fluxgate magnetometer
- (FGM) instrument on the Cluster Rumba spacecraft.</Description>
- <Acknowledgement>NASA, Andre Balogh, Elizabeth E. Lucek</Acknowledgement>
+ <ReleaseDate>2016-10-16T16:14:00Z</ReleaseDate>
+ <Description>This dataset contains spin resolution (~4s) measurements of the magnetic field vector from the fluxgate magnetometer (FGM) instrument
+ on the Cluster3 spacecraft.</Description>
+ <Acknowledgement>Principal Investigator: Chris Carr</Acknowledgement>
<Contact>
- <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
- <Role>TechnicalContact</Role>
- </Contact>
+ <PersonID>spase://SMWG/Person/Chris.Carr</PersonID>
+ <Role>PrincipalInvestigator</Role>
+ </Contact>
<InformationURL>
- <Name>NSSDC Master Catalog listing for Cluster Rumba Fluxgate Magnetometer (FGM)</Name>
+ <Name>ESA web page</Name>
+ <URL>http://www.cosmos.esa.int/web/csa/documentation</URL>
+ <Description>This site contains FGM data documentation</Description>
+ </InformationURL>
+ <InformationURL>
+ <Name>NSSDC Master Catalog listing for Cluster Samba Fluxgate Magnetometer (FGM)</Name>
<URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-04</URL>
<Description>This site provides information concerning the Cluster Samba Fluxgate Magnetometer Instrument.</Description>
</InformationURL>
@@ -28,12 +33,11 @@
<Name>AMDA at CDPP</Name>
<URL>http://amda.cdpp.eu</URL>
</AccessURL>
- <Format>NetCDF</Format>
- <Acknowledgement>NASA, Andre Balogh, Elizabeth E. Lucek</Acknowledgement>
+ <Format>NetCDF</Format>
</AccessInformation>
<ProviderName>CSA</ProviderName>
<ProcessingLevel>Calibrated</ProcessingLevel>
- <ProviderResourceName>Cluster Samba Spin Resolution Fluxgate Magnetometer (FGM) Data</ProviderResourceName>
+ <ProviderResourceName>C3_CP_FGM_SPIN</ProviderResourceName>
<ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
<InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Samba/FGM</InstrumentID>
<MeasurementType>MagneticField</MeasurementType>
@@ -58,7 +62,7 @@
<Parameter>
<Name>b_gse</Name>
<ParameterKey>c3_b_gse</ParameterKey>
- <Description>Cluster Samba Fluxgate Magnetometer magnetic field vector at spin time resolution</Description>
+ <Description>FGM: magnetic field vector (3 GSE components), 4s resolution</Description>
<Ucd>phys.magField</Ucd>
<Cadence>PT4S</Cadence>
<Units>nT</Units>
@@ -100,7 +104,7 @@
<Parameter>
<Name>b_gsm</Name>
<ParameterKey>c3_b_gsm</ParameterKey>
- <Description>Cluster Samba Fluxgate Magnetometer magnetic field vector at spin time resolution</Description>
+ <Description>FGM: magnetic field vector (3 GSM components), 4s resolution</Description>
<Ucd>phys.magField</Ucd>
<Cadence>PT4S</Cadence>
<Units>nT</Units>
@@ -142,7 +146,7 @@
<Parameter>
<Name>|b|</Name>
<ParameterKey>c3_btot</ParameterKey>
- <Description>Cluster Samba Fluxgate Magnetometer magnetic field magnitude at spin time resolution</Description>
+ <Description>FGM: magnetic field vector magnitude</Description>
<Ucd>phys.magField</Ucd>
<Cadence>PT4S</Cadence>
<Units>nT</Units>
diff --git a/NumericalData/AMDA/Cluster/Cluster4/FGM/clust4-fgm-prp.xml b/NumericalData/AMDA/Cluster/Cluster4/FGM/clust4-fgm-prp.xml
index b090ab3..1131f3d 100644
--- a/NumericalData/AMDA/Cluster/Cluster4/FGM/clust4-fgm-prp.xml
+++ b/NumericalData/AMDA/Cluster/Cluster4/FGM/clust4-fgm-prp.xml
@@ -6,14 +6,19 @@
<ResourceHeader>
<ResourceName>4 sec (spin)</ResourceName>
<AlternateName>Cluster 4 Spin Resolution FGM Data</AlternateName>
- <ReleaseDate>2015-10-16T16:00:00Z</ReleaseDate>
- <Description>This dataset contains spin resolution measurements of the magnetic field vector from the fluxgate magnetometer (FGM) instrument
- on the Cluster Tango spacecraft.</Description>
- <Acknowledgement>NASA, Andre Balogh, Elizabeth E. Lucek</Acknowledgement>
+ <ReleaseDate>2016-10-16T16:14:00Z</ReleaseDate>
+ <Description>This dataset contains spin resolution (~4s) measurements of the magnetic field vector from the fluxgate magnetometer (FGM) instrument
+ on the Cluster4 spacecraft.</Description>
+ <Acknowledgement>Principal Investigator: Chris Carr</Acknowledgement>
<Contact>
- <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
- <Role>TechnicalContact</Role>
- </Contact>
+ <PersonID>spase://SMWG/Person/Chris.Carr</PersonID>
+ <Role>PrincipalInvestigator</Role>
+ </Contact>
+ <InformationURL>
+ <Name>ESA web page</Name>
+ <URL>http://www.cosmos.esa.int/web/csa/documentation</URL>
+ <Description>This site contains FGM data documentation</Description>
+ </InformationURL>
<InformationURL>
<Name>NSSDC Master Catalog listing for Cluster Tango Fluxgate Magnetometer (FGM)</Name>
<URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-04</URL>
@@ -28,12 +33,11 @@
<Name>AMDA at CDPP</Name>
<URL>http://amda.cdpp.eu</URL>
</AccessURL>
- <Format>NetCDF</Format>
- <Acknowledgement>NASA, Andre Balogh, Elizabeth E. Lucek</Acknowledgement>
+ <Format>NetCDF</Format>
</AccessInformation>
<ProviderName>CSA</ProviderName>
<ProcessingLevel>Calibrated</ProcessingLevel>
- <ProviderResourceName>Cluster Tango Spin Resolution Fluxgate Magnetometer (FGM) Data</ProviderResourceName>
+ <ProviderResourceName>C4_CP_FGM_SPIN</ProviderResourceName>
<ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
<InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Tango/FGM</InstrumentID>
<MeasurementType>MagneticField</MeasurementType>
@@ -58,7 +62,7 @@
<Parameter>
<Name>b_gse</Name>
<ParameterKey>c4_b_gse</ParameterKey>
- <Description>Cluster Tango Fluxgate Magnetometer magnetic field vector at spin time resolution</Description>
+ <Description>FGM: magnetic field vector (3 GSE components), 4s resolution</Description>
<Ucd>phys.magField</Ucd>
<Cadence>PT4S</Cadence>
<Units>nT</Units>
@@ -76,19 +80,19 @@
<Name>bx</Name>
<Qualifier>Component.I</Qualifier>
<Index>1</Index>
- <ParameterKey>c4_b(0)</ParameterKey>
+ <ParameterKey>c4_b_gse(0)</ParameterKey>
</Element>
<Element>
<Name>by</Name>
<Qualifier>Component.J</Qualifier>
<Index>2</Index>
- <ParameterKey>c4_b(1)</ParameterKey>
+ <ParameterKey>c4_b_gse(1)</ParameterKey>
</Element>
<Element>
<Name>bz</Name>
<Qualifier>Component.K</Qualifier>
<Index>3</Index>
- <ParameterKey>c4_b(2)</ParameterKey>
+ <ParameterKey>c4_b_gse(2)</ParameterKey>
</Element>
</Structure>
<FillValue>-1.0000e+31</FillValue>
@@ -100,7 +104,7 @@
<Parameter>
<Name>b_gsm</Name>
<ParameterKey>c4_b_gsm</ParameterKey>
- <Description>Cluster Tango Fluxgate Magnetometer magnetic field vector at spin time resolution</Description>
+ <Description>FGM: magnetic field vector (3 GSM components), 4s resolution</Description>
<Ucd>phys.magField</Ucd>
<Cadence>PT4S</Cadence>
<Units>nT</Units>
@@ -142,7 +146,7 @@
<Parameter>
<Name>|b|</Name>
<ParameterKey>c4_btot</ParameterKey>
- <Description>Cluster Tango Fluxgate Magnetometer magnetic field magnitude at spin time resolution</Description>
+ <Description>FGM: magnetic field vector magnitude</Description>
<Ucd>phys.magField</Ucd>
<Cadence>PT4S</Cadence>
<Units>nT</Units>
--
libgit2 0.21.2