diff --git a/Instrument/CDPP-AMDA/MMS2/FGM.xml b/Instrument/CDPP-AMDA/MMS2/FGM.xml new file mode 100644 index 0000000..3acb1c4 --- /dev/null +++ b/Instrument/CDPP-AMDA/MMS2/FGM.xml @@ -0,0 +1,37 @@ + + + 2.3.1 + + spase://CNES/Instrument/CDPP-AMDA/MMS2/FGM + + FGM + Fluxgate Magnetometer + 2017-02-04T15:37:46Z + The Fluxgate Magnetometers (FGM) on Magnetospheric Multiscale consist of a traditional Analog +Fluxgate Magnetometer (AFG), and a Digital Fluxgate magnetometer (DFG). The dual magnetometers are operated as a single + instrument providing a single intercalibrated data product. Range changes occur at different times on the two instruments + so the gains checked each periapsis can be carried out unambiguously to apoapsis. Cross correlation of calibration +parameters can separate causes of the any apparent calibration changes. Use of Electron Drift Instrument (EDI) to determine the field along the +rotation axis allows accurate monitoring of the zero levels along the rotation axis. Prior to + launch the magnetometers were calibrated at the Technical University, Braunschweig, except for the AFG magnetometers on MMS3 and MMS4, + which were calibrated at UCLA. Both sets of sensors are operated for the entire MMS orbit, with slow +survey (8 samples per second) outside of the Region of Interest (ROI), and fast survey (16 samples per second) inside the ROI. +Within the ROI burst mode data (128 samples per second) are also acquired. + + spase://CNES/Person/James.L.Burch + PrincipalInvestigator + + + spase://SMWG/Person/Christopher.T.Russell + PrincipalInvestigator + + + spase://CNES/Person/W.Magnus + PrincipalInvestigator + + + Magnetometer + + spase://CNES/Observatory/CDPP-AMDA/MMS2 + + diff --git a/Instrument/CDPP-AMDA/MMS3/FGM.xml b/Instrument/CDPP-AMDA/MMS3/FGM.xml new file mode 100644 index 0000000..c7d4dba --- /dev/null +++ b/Instrument/CDPP-AMDA/MMS3/FGM.xml @@ -0,0 +1,37 @@ + + + 2.3.1 + + spase://CNES/Instrument/CDPP-AMDA/MMS3/FGM + + FGM + Fluxgate Magnetometer + 2017-02-04T15:37:46Z + The Fluxgate Magnetometers (FGM) on Magnetospheric Multiscale consist of a traditional Analog +Fluxgate Magnetometer (AFG), and a Digital Fluxgate magnetometer (DFG). The dual magnetometers are operated as a single + instrument providing a single intercalibrated data product. Range changes occur at different times on the two instruments + so the gains checked each periapsis can be carried out unambiguously to apoapsis. Cross correlation of calibration +parameters can separate causes of the any apparent calibration changes. Use of Electron Drift Instrument (EDI) to determine the field along the +rotation axis allows accurate monitoring of the zero levels along the rotation axis. Prior to + launch the magnetometers were calibrated at the Technical University, Braunschweig, except for the AFG magnetometers on MMS3 and MMS4, + which were calibrated at UCLA. Both sets of sensors are operated for the entire MMS orbit, with slow +survey (8 samples per second) outside of the Region of Interest (ROI), and fast survey (16 samples per second) inside the ROI. +Within the ROI burst mode data (128 samples per second) are also acquired. + + spase://CNES/Person/James.L.Burch + PrincipalInvestigator + + + spase://SMWG/Person/Christopher.T.Russell + PrincipalInvestigator + + + spase://CNES/Person/W.Magnus + PrincipalInvestigator + + + Magnetometer + + spase://CNES/Observatory/CDPP-AMDA/MMS3 + + diff --git a/Instrument/CDPP-AMDA/MMS4/FGM.xml b/Instrument/CDPP-AMDA/MMS4/FGM.xml new file mode 100644 index 0000000..7d3c99d --- /dev/null +++ b/Instrument/CDPP-AMDA/MMS4/FGM.xml @@ -0,0 +1,37 @@ + + + 2.3.1 + + spase://CNES/Instrument/CDPP-AMDA/MMS4/FGM + + FGM + Fluxgate Magnetometer + 2017-02-04T15:37:46Z + The Fluxgate Magnetometers (FGM) on Magnetospheric Multiscale consist of a traditional Analog +Fluxgate Magnetometer (AFG), and a Digital Fluxgate magnetometer (DFG). The dual magnetometers are operated as a single + instrument providing a single intercalibrated data product. Range changes occur at different times on the two instruments + so the gains checked each periapsis can be carried out unambiguously to apoapsis. Cross correlation of calibration +parameters can separate causes of the any apparent calibration changes. Use of Electron Drift Instrument (EDI) to determine the field along the +rotation axis allows accurate monitoring of the zero levels along the rotation axis. Prior to + launch the magnetometers were calibrated at the Technical University, Braunschweig, except for the AFG magnetometers on MMS3 and MMS4, + which were calibrated at UCLA. Both sets of sensors are operated for the entire MMS orbit, with slow +survey (8 samples per second) outside of the Region of Interest (ROI), and fast survey (16 samples per second) inside the ROI. +Within the ROI burst mode data (128 samples per second) are also acquired. + + spase://CNES/Person/James.L.Burch + PrincipalInvestigator + + + spase://SMWG/Person/Christopher.T.Russell + PrincipalInvestigator + + + spase://CNES/Person/W.Magnus + PrincipalInvestigator + + + Magnetometer + + spase://CNES/Observatory/CDPP-AMDA/MMS4 + + diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1/FGM/mms1-fgm-brst.xml b/NumericalData/CDPP-AMDA/MMS/MMS1/FGM/mms1-fgm-brst.xml new file mode 100644 index 0000000..19f3ed7 --- /dev/null +++ b/NumericalData/CDPP-AMDA/MMS/MMS1/FGM/mms1-fgm-brst.xml @@ -0,0 +1,154 @@ + + + 2.3.1 + + spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS1/FGM/mms1-fgm-brst + + burst + burst + 2017-01-16T11:50:00 + For the purpose of creating a unified FGM Level 2 data product, burst mode data is taken from DFG and survey mode data is taken + from AFG. Because AFG and DFG are cross-calibrated on an orbit-averaged basis, + small differences in offset may be observed between Level2 burst and survey mode + data. Consequently, any differences are within the error of the measurement. Based on preliminary analysis of the data, + the absolute error within the Region of Interest (ROI) is estimated to be no more than 0.1 nT in the spin-plane, + 0.15 nT along the spin-axis and 0.2 nT in total magnitude + + + spase://CNES/Person/James.L.Burch + PrincipalInvestigator + + + spase://SMWG/Person/Christopher.T.Russell + PrincipalInvestigator + + + spase://CNES/Person/W.Magnus + PrincipalInvestigator + + + MMS home page at GSFC + http://mms.gsfc.nasa.gov/ + + + SMART package home page at SWRI + http://mms.space.swri.edu/index.html + + + Science Data Center at LASP + https://lasp.colorado.edu/mms/sdc + + + FGM team home page at UCLA + http://www-spc.igpp.ucla.edu/ssc/mms + + + FGM team at IWF + http://www.iwf.oeaw.ac.at + + + + spase://SMWG/Repository/CNES/CDPP-AMDA + Online + Open + + AMDA at CDPP + amda.cdpp.eu + + NetCDF + + IRAP + spase://CNES/Instrument/CDPP-AMDA/MMS1/FGM + MagneticField + + + 2015-09-01T00:00:00Z + 2019-01-14T15:58:00Z + + PT0.01S + + + b_gse + mms1_brst_bgse + + + nT + + + Cartesian + GSE + + + TimeSeries + + + 3 + + bx + Component.I + 1 + mms1_brst_bgse(0) + + + by + Component.J + 2 + mms1_brst_bgse(1) + + + bz + Component.K + 3 + mms1_brst_bgse(2) + + + + + b_gsm + mms1_brst_bgsm + + + nT + + + Cartesian + GSM + + + TimeSeries + + + 3 + + bx + Component.I + 1 + mms1_brst_bgsm(0) + + + by + Component.J + 2 + mms1_brst_bgsm(1) + + + bz + Component.K + 3 + mms1_brst_bgsm(2) + + + + + |b| + mms1_brst_btot + + + nT + + + TimeSeries + + + + diff --git a/NumericalData/CDPP-AMDA/MMS/MMS2/FGM/mms2-fgm-brst.xml b/NumericalData/CDPP-AMDA/MMS/MMS2/FGM/mms2-fgm-brst.xml new file mode 100644 index 0000000..24987b1 --- /dev/null +++ b/NumericalData/CDPP-AMDA/MMS/MMS2/FGM/mms2-fgm-brst.xml @@ -0,0 +1,154 @@ + + + 2.3.1 + + spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS2/FGM/mms2-fgm-brst + + burst + burst + 2017-01-16T11:50:00 + For the purpose of creating a unified FGM Level 2 data product, burst mode data is taken from DFG and survey mode data is taken + from AFG. Because AFG and DFG are cross-calibrated on an orbit-averaged basis, + small differences in offset may be observed between Level2 burst and survey mode + data. Consequently, any differences are within the error of the measurement. Based on preliminary analysis of the data, + the absolute error within the Region of Interest (ROI) is estimated to be no more than 0.1 nT in the spin-plane, + 0.15 nT along the spin-axis and 0.2 nT in total magnitude + + + spase://CNES/Person/James.L.Burch + PrincipalInvestigator + + + spase://SMWG/Person/Christopher.T.Russell + PrincipalInvestigator + + + spase://CNES/Person/W.Magnus + PrincipalInvestigator + + + MMS home page at GSFC + http://mms.gsfc.nasa.gov/ + + + SMART package home page at SWRI + http://mms.space.swri.edu/index.html + + + Science Data Center at LASP + https://lasp.colorado.edu/mms/sdc + + + FGM team home page at UCLA + http://www-spc.igpp.ucla.edu/ssc/mms + + + FGM team at IWF + http://www.iwf.oeaw.ac.at + + + + spase://SMWG/Repository/CNES/CDPP-AMDA + Online + Open + + AMDA at CDPP + amda.cdpp.eu + + NetCDF + + IRAP + spase://CNES/Instrument/CDPP-AMDA/MMS2/FGM + MagneticField + + + 2015-09-01T00:00:00Z + 2019-01-14T15:58:00Z + + PT0.01S + + + b_gse + mms2_brst_bgse + + + nT + + + Cartesian + GSE + + + TimeSeries + + + 3 + + bx + Component.I + 1 + mms2_brst_bgse(0) + + + by + Component.J + 2 + mms2_brst_bgse(1) + + + bz + Component.K + 3 + mms2_brst_bgse(2) + + + + + b_gsm + mms2_brst_bgsm + + + nT + + + Cartesian + GSM + + + TimeSeries + + + 3 + + bx + Component.I + 1 + mms2_brst_bgsm(0) + + + by + Component.J + 2 + mms2_brst_bgsm(1) + + + bz + Component.K + 3 + mms2_brst_bgsm(2) + + + + + |b| + mms2_brst_btot + + + nT + + + TimeSeries + + + + diff --git a/NumericalData/CDPP-AMDA/MMS/MMS3/FGM/mms3-fgm-brst.xml b/NumericalData/CDPP-AMDA/MMS/MMS3/FGM/mms3-fgm-brst.xml new file mode 100644 index 0000000..0cb7cb4 --- /dev/null +++ b/NumericalData/CDPP-AMDA/MMS/MMS3/FGM/mms3-fgm-brst.xml @@ -0,0 +1,154 @@ + + + 2.3.1 + + spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS3/FGM/mms3-fgm-brst + + burst + burst + 2017-01-16T11:50:00 + For the purpose of creating a unified FGM Level 2 data product, burst mode data is taken from DFG and survey mode data is taken + from AFG. Because AFG and DFG are cross-calibrated on an orbit-averaged basis, + small differences in offset may be observed between Level2 burst and survey mode + data. Consequently, any differences are within the error of the measurement. Based on preliminary analysis of the data, + the absolute error within the Region of Interest (ROI) is estimated to be no more than 0.1 nT in the spin-plane, + 0.15 nT along the spin-axis and 0.2 nT in total magnitude + + + spase://CNES/Person/James.L.Burch + PrincipalInvestigator + + + spase://SMWG/Person/Christopher.T.Russell + PrincipalInvestigator + + + spase://CNES/Person/W.Magnus + PrincipalInvestigator + + + MMS home page at GSFC + http://mms.gsfc.nasa.gov/ + + + SMART package home page at SWRI + http://mms.space.swri.edu/index.html + + + Science Data Center at LASP + https://lasp.colorado.edu/mms/sdc + + + FGM team home page at UCLA + http://www-spc.igpp.ucla.edu/ssc/mms + + + FGM team at IWF + http://www.iwf.oeaw.ac.at + + + + spase://SMWG/Repository/CNES/CDPP-AMDA + Online + Open + + AMDA at CDPP + amda.cdpp.eu + + NetCDF + + IRAP + spase://CNES/Instrument/CDPP-AMDA/MMS3/FGM + MagneticField + + + 2015-09-01T00:00:00Z + 2019-01-14T15:58:00Z + + PT0.01S + + + b_gse + mms3_brst_bgse + + + nT + + + Cartesian + GSE + + + TimeSeries + + + 3 + + bx + Component.I + 1 + mms3_brst_bgse(0) + + + by + Component.J + 2 + mms3_brst_bgse(1) + + + bz + Component.K + 3 + mms3_brst_bgse(2) + + + + + b_gsm + mms3_brst_bgsm + + + nT + + + Cartesian + GSM + + + TimeSeries + + + 3 + + bx + Component.I + 1 + mms3_brst_bgsm(0) + + + by + Component.J + 2 + mms3_brst_bgsm(1) + + + bz + Component.K + 3 + mms3_brst_bgsm(2) + + + + + |b| + mms3_brst_btot + + + nT + + + TimeSeries + + + + diff --git a/NumericalData/CDPP-AMDA/MMS/MMS4/FGM/mms4-fgm-brst.xml b/NumericalData/CDPP-AMDA/MMS/MMS4/FGM/mms4-fgm-brst.xml new file mode 100644 index 0000000..e09fb7d --- /dev/null +++ b/NumericalData/CDPP-AMDA/MMS/MMS4/FGM/mms4-fgm-brst.xml @@ -0,0 +1,154 @@ + + + 2.3.1 + + spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS4/FGM/mms4-fgm-brst + + burst + burst + 2017-01-16T11:50:00 + For the purpose of creating a unified FGM Level 2 data product, burst mode data is taken from DFG and survey mode data is taken + from AFG. Because AFG and DFG are cross-calibrated on an orbit-averaged basis, + small differences in offset may be observed between Level2 burst and survey mode + data. Consequently, any differences are within the error of the measurement. Based on preliminary analysis of the data, + the absolute error within the Region of Interest (ROI) is estimated to be no more than 0.1 nT in the spin-plane, + 0.15 nT along the spin-axis and 0.2 nT in total magnitude + + + spase://CNES/Person/James.L.Burch + PrincipalInvestigator + + + spase://SMWG/Person/Christopher.T.Russell + PrincipalInvestigator + + + spase://CNES/Person/W.Magnus + PrincipalInvestigator + + + MMS home page at GSFC + http://mms.gsfc.nasa.gov/ + + + SMART package home page at SWRI + http://mms.space.swri.edu/index.html + + + Science Data Center at LASP + https://lasp.colorado.edu/mms/sdc + + + FGM team home page at UCLA + http://www-spc.igpp.ucla.edu/ssc/mms + + + FGM team at IWF + http://www.iwf.oeaw.ac.at + + + + spase://SMWG/Repository/CNES/CDPP-AMDA + Online + Open + + AMDA at CDPP + amda.cdpp.eu + + NetCDF + + IRAP + spase://CNES/Instrument/CDPP-AMDA/MMS4/FGM + MagneticField + + + 2015-09-01T00:00:00Z + 2019-01-14T15:58:00Z + + PT0.01S + + + b_gse + mms4_brst_bgse + + + nT + + + Cartesian + GSE + + + TimeSeries + + + 3 + + bx + Component.I + 1 + mms4_brst_bgse(0) + + + by + Component.J + 2 + mms4_brst_bgse(1) + + + bz + Component.K + 3 + mms4_brst_bgse(2) + + + + + b_gsm + mms4_brst_bgsm + + + nT + + + Cartesian + GSM + + + TimeSeries + + + 3 + + bx + Component.I + 1 + mms4_brst_bgsm(0) + + + by + Component.J + 2 + mms4_brst_bgsm(1) + + + bz + Component.K + 3 + mms4_brst_bgsm(2) + + + + + |b| + mms4_brst_btot + + + nT + + + TimeSeries + + + + -- libgit2 0.21.2