diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-dismoms.xml b/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-dismoms.xml
index be8edfc..749be11 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-dismoms.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-dismoms.xml
@@ -47,7 +47,7 @@ dicated time.
NetCDF
- IRAP
+ LASP
spase://CNES/Instrument/CDPP-AMDA/MMS1/FPI
MagneticField
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-desmoms.xml b/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-desmoms.xml
new file mode 100644
index 0000000..2d0d991
--- /dev/null
+++ b/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-desmoms.xml
@@ -0,0 +1,381 @@
+
+
+ 2.3.1
+
+ spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-desmoms
+
+ des-moms : electrons
+ electron moments : fast mode
+ 2017-01-16T11:50:00
+ FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for
+the current Mission Phase. Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made
+ available at survey (4.5 s) resolution. Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
+, FPI usually operates in Slow Survey (SS) Mode (60 s resolution) outside of ROI. This moments product contains results
+ from integrating the standard moments of phase-space distributions formed from the indicated data type (DES/DIS burst,
+ FS or SS). For convenience, some additional parameters are included to augment those most commonly found in a moments
+product of this sort, plus time-stamps and other annotation characterizing the state of the instrument system at the in
+dicated time.
+
+ spase://CNES/Person/James.L.Burch
+ PrincipalInvestigator
+
+
+ spase://CNES/Person/B.Giles
+ PrincipalInvestigator
+
+
+ MMS home page at GSFC
+ http://mms.gsfc.nasa.gov
+
+
+ FPI overview
+ http://www.nasa.gov/mission_pages/mms/spacecraft/instruments.html#fpi
+
+
+ mms2-fpi-fast
+ PartOf
+ fast mode
+
+
+
+ spase://SMWG/Repository/CNES/CDPP-AMDA
+ Online
+ Open
+
+ AMDA at CDPP
+ amda.cdpp.eu
+
+ NetCDF
+
+ LASP
+ spase://CNES/Instrument/CDPP-AMDA/MMS2/FPI
+ MagneticField
+
+
+ 2000-08-22T00:00:00Z
+ 2019-01-14T15:58:00Z
+
+ PT4.5S
+
+
+ density
+ mms2_des_ne
+
+
+ cm^-3
+
+
+ TimeSeries
+
+
+
+ density : err
+ mms2_des_ne_err
+
+
+ cm^-3
+
+
+ TimeSeries
+
+
+
+ v_gse
+ mms2_des_vgse
+
+
+ km/s
+
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 3
+
+ vx
+ Component.I
+ 1
+ mms2_des_vgse(0)
+
+
+ vy
+ Component.J
+ 2
+ mms2_des_vgse(1)
+
+
+ vz
+ Component.K
+ 3
+ mms2_des_vgse(2)
+
+
+
+
+ v_gse : err
+ mms2_des_v_err
+
+
+ km/s
+
+
+ TimeSeries
+
+
+ 3
+
+ vx
+ Component.I
+ 1
+ mms2_des_v_err(0)
+
+
+ vy
+ Component.J
+ 2
+ mms2_des_v_err(1)
+
+
+ vz
+ Component.K
+ 3
+ mms2_des_v_err(2)
+
+
+
+
+ t_para
+ mms2_des_tpara
+
+
+ eV
+
+
+ TimeSeries
+
+
+
+ t_perp
+ mms2_des_tperp
+
+
+ eV
+
+
+ TimeSeries
+
+
+
+ heatq_gse
+ mms2_des_heatq
+
+ phys.pressure
+ nPa
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 3
+
+ x
+ 1
+ mms2_des_heatq(0)
+
+
+ y
+ 2
+ mms2_des_heatq(1)
+
+
+ z
+ 3
+ mms2_des_heatq(2)
+
+
+
+ Electron
+ Vector
+ HeatFlux
+
+
+
+ pressure_gse
+ mms2_des_press
+
+ phys.pressure
+ nPa
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 9
+
+ xx
+ 1
+ mms2_des_press(0)
+
+
+ xy
+ 2
+ mms2_des_press(1)
+
+
+ xz
+ 3
+ mms2_des_press(2)
+
+
+ yx
+ 4
+ mms2_des_press(3)
+
+
+ yy
+ 5
+ mms2_des_press(4)
+
+
+ yz
+ 6
+ mms2_des_press(5)
+
+
+ zx
+ 7
+ mms2_des_press(6)
+
+
+ zy
+ 8
+ mms2_des_press(7)
+
+
+ zz
+ 9
+ mms2_des_press(8)
+
+
+
+ Electron
+ Tensor
+ Pressure
+
+
+
+ elec eflux : omni
+ mms2_des_omni
+
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ elec eflux : para
+ mms2_des_para
+
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ elec eflux : anti
+ mms2_des_anti
+
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ elec eflux : perp
+ mms2_des_perp
+
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ pa dist : lowen
+ mms2_des_palow
+ Low energy bin: 0 eV - 200 eV.
+ Pitch-angle bin size: 6 deg. Note that pitch angles are calculated in the spacecraft frame;
+ i.e., not shifted by the bulk velocity
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ pa dist : miden
+ mms2_des_pamid
+ Mid energy bin: 200 eV - 2 keV.
+ Pitch-angle bin size: 6 deg. Note that pitch angles are calculated in the spacecraft frame;
+ i.e., not shifted by the bulk velocity
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ pa dist : highen
+ mms2_des_pahigh
+ High energy bin: 2 keV - 30 keV.
+ Pitch-angle bin size: 6 deg. Note that pitch angles are calculated in the spacecraft frame;
+ i.e., not shifted by the bulk velocity
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-dismoms.xml b/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-dismoms.xml
new file mode 100644
index 0000000..0b2ec9b
--- /dev/null
+++ b/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-dismoms.xml
@@ -0,0 +1,291 @@
+
+
+ 2.3.1
+
+ spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-dismoms
+
+ dis-moms : ions
+ ion moments : fast mode
+ 2017-01-16T11:50:00
+ FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for
+the current Mission Phase. Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made
+ available at survey (4.5 s) resolution. Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
+, FPI usually operates in Slow Survey (SS) Mode (60 s resolution) outside of ROI. This moments product contains results
+ from integrating the standard moments of phase-space distributions formed from the indicated data type (DES/DIS burst,
+ FS or SS). For convenience, some additional parameters are included to augment those most commonly found in a moments
+product of this sort, plus time-stamps and other annotation characterizing the state of the instrument system at the in
+dicated time.
+
+ spase://CNES/Person/James.L.Burch
+ PrincipalInvestigator
+
+
+ spase://CNES/Person/B.Giles
+ PrincipalInvestigator
+
+
+ MMS home page at GSFC
+ http://mms.gsfc.nasa.gov
+
+
+ FPI overview
+ http://www.nasa.gov/mission_pages/mms/spacecraft/instruments.html#fpi
+
+
+ mms2-fpi-fast
+ PartOf
+ fast mode
+
+
+
+ spase://SMWG/Repository/CNES/CDPP-AMDA
+ Online
+ Open
+
+ AMDA at CDPP
+ amda.cdpp.eu
+
+ NetCDF
+
+ LASP
+ spase://CNES/Instrument/CDPP-AMDA/MMS2/FPI
+ MagneticField
+
+
+ 2000-08-22T00:00:00Z
+ 2019-01-14T15:58:00Z
+
+ PT4.5S
+
+
+ density
+ mms2_dis_ni
+
+
+ cm^-3
+
+
+ TimeSeries
+
+
+
+ density : err
+ mms2_dis_ni_err
+
+
+ cm^-3
+
+
+ TimeSeries
+
+
+
+ v_gse
+ mms2_dis_vgse
+
+
+ km/s
+
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 3
+
+ vx
+ Component.I
+ 1
+ mms2_dis_vgse(0)
+
+
+ vy
+ Component.J
+ 2
+ mms2_dis_vgse(1)
+
+
+ vz
+ Component.K
+ 3
+ mms2_dis_vgse(2)
+
+
+
+
+ v_gse : err
+ mms2_dis_v_err
+
+
+ km/s
+
+
+ TimeSeries
+
+
+ 3
+
+ vx
+ Component.I
+ 1
+ mms2_dis_v_err(0)
+
+
+ vy
+ Component.J
+ 2
+ mms2_dis_v_err(1)
+
+
+ vz
+ Component.K
+ 3
+ mms2_dis_v_err(2)
+
+
+
+
+ t_para
+ mms2_dis_tpara
+
+
+ eV
+
+
+ TimeSeries
+
+
+
+ t_perp
+ mms2_dis_tperp
+
+
+ eV
+
+
+ TimeSeries
+
+
+
+ heatq_gse
+ mms2_dis_heatq
+
+ phys.pressure
+ nPa
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 3
+
+ x
+ 1
+ mms2_dis_heatq(0)
+
+
+ y
+ 2
+ mms2_dis_heatq(1)
+
+
+ z
+ 3
+ mms2_dis_heatq(2)
+
+
+
+ Ion
+ Vector
+ HeatFlux
+
+
+
+ pressure_gse
+ mms2_dis_press
+
+ phys.pressure
+ nPa
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 9
+
+ xx
+ 1
+ mms2_dis_press(0)
+
+
+ xy
+ 2
+ mms2_dis_press(1)
+
+
+ xz
+ 3
+ mms2_dis_press(2)
+
+
+ yx
+ 4
+ mms2_dis_press(3)
+
+
+ yy
+ 5
+ mms2_dis_press(4)
+
+
+ yz
+ 6
+ mms2_dis_press(5)
+
+
+ zx
+ 7
+ mms2_dis_press(6)
+
+
+ zy
+ 8
+ mms2_dis_press(7)
+
+
+ zz
+ 9
+ mms2_dis_press(8)
+
+
+
+ Ion
+ Tensor
+ Pressure
+
+
+
+ ion eflux : omni
+ mms2_dis_omni
+
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Ion
+ EnergyFlux
+
+
+
+
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-desmoms.xml b/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-desmoms.xml
new file mode 100644
index 0000000..b152ee8
--- /dev/null
+++ b/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-desmoms.xml
@@ -0,0 +1,381 @@
+
+
+ 2.3.1
+
+ spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-desmoms
+
+ des-moms : electrons
+ electron moments : fast mode
+ 2017-01-16T11:50:00
+ FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for
+the current Mission Phase. Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made
+ available at survey (4.5 s) resolution. Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
+, FPI usually operates in Slow Survey (SS) Mode (60 s resolution) outside of ROI. This moments product contains results
+ from integrating the standard moments of phase-space distributions formed from the indicated data type (DES/DIS burst,
+ FS or SS). For convenience, some additional parameters are included to augment those most commonly found in a moments
+product of this sort, plus time-stamps and other annotation characterizing the state of the instrument system at the in
+dicated time.
+
+ spase://CNES/Person/James.L.Burch
+ PrincipalInvestigator
+
+
+ spase://CNES/Person/B.Giles
+ PrincipalInvestigator
+
+
+ MMS home page at GSFC
+ http://mms.gsfc.nasa.gov
+
+
+ FPI overview
+ http://www.nasa.gov/mission_pages/mms/spacecraft/instruments.html#fpi
+
+
+ mms3-fpi-fast
+ PartOf
+ fast mode
+
+
+
+ spase://SMWG/Repository/CNES/CDPP-AMDA
+ Online
+ Open
+
+ AMDA at CDPP
+ amda.cdpp.eu
+
+ NetCDF
+
+ LASP
+ spase://CNES/Instrument/CDPP-AMDA/MMS3/FPI
+ MagneticField
+
+
+ 2000-08-22T00:00:00Z
+ 2019-01-14T15:58:00Z
+
+ PT4.5S
+
+
+ density
+ mms3_des_ne
+
+
+ cm^-3
+
+
+ TimeSeries
+
+
+
+ density : err
+ mms3_des_ne_err
+
+
+ cm^-3
+
+
+ TimeSeries
+
+
+
+ v_gse
+ mms3_des_vgse
+
+
+ km/s
+
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 3
+
+ vx
+ Component.I
+ 1
+ mms3_des_vgse(0)
+
+
+ vy
+ Component.J
+ 2
+ mms3_des_vgse(1)
+
+
+ vz
+ Component.K
+ 3
+ mms3_des_vgse(2)
+
+
+
+
+ v_gse : err
+ mms3_des_v_err
+
+
+ km/s
+
+
+ TimeSeries
+
+
+ 3
+
+ vx
+ Component.I
+ 1
+ mms3_des_v_err(0)
+
+
+ vy
+ Component.J
+ 2
+ mms3_des_v_err(1)
+
+
+ vz
+ Component.K
+ 3
+ mms3_des_v_err(2)
+
+
+
+
+ t_para
+ mms3_des_tpara
+
+
+ eV
+
+
+ TimeSeries
+
+
+
+ t_perp
+ mms3_des_tperp
+
+
+ eV
+
+
+ TimeSeries
+
+
+
+ heatq_gse
+ mms3_des_heatq
+
+ phys.pressure
+ nPa
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 3
+
+ x
+ 1
+ mms3_des_heatq(0)
+
+
+ y
+ 2
+ mms3_des_heatq(1)
+
+
+ z
+ 3
+ mms3_des_heatq(2)
+
+
+
+ Electron
+ Vector
+ HeatFlux
+
+
+
+ pressure_gse
+ mms3_des_press
+
+ phys.pressure
+ nPa
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 9
+
+ xx
+ 1
+ mms3_des_press(0)
+
+
+ xy
+ 2
+ mms3_des_press(1)
+
+
+ xz
+ 3
+ mms3_des_press(2)
+
+
+ yx
+ 4
+ mms3_des_press(3)
+
+
+ yy
+ 5
+ mms3_des_press(4)
+
+
+ yz
+ 6
+ mms3_des_press(5)
+
+
+ zx
+ 7
+ mms3_des_press(6)
+
+
+ zy
+ 8
+ mms3_des_press(7)
+
+
+ zz
+ 9
+ mms3_des_press(8)
+
+
+
+ Electron
+ Tensor
+ Pressure
+
+
+
+ elec eflux : omni
+ mms3_des_omni
+
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ elec eflux : para
+ mms3_des_para
+
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ elec eflux : anti
+ mms3_des_anti
+
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ elec eflux : perp
+ mms3_des_perp
+
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ pa dist : lowen
+ mms3_des_palow
+ Low energy bin: 0 eV - 200 eV.
+ Pitch-angle bin size: 6 deg. Note that pitch angles are calculated in the spacecraft frame;
+ i.e., not shifted by the bulk velocity
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ pa dist : miden
+ mms3_des_pamid
+ Mid energy bin: 200 eV - 2 keV.
+ Pitch-angle bin size: 6 deg. Note that pitch angles are calculated in the spacecraft frame;
+ i.e., not shifted by the bulk velocity
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ pa dist : highen
+ mms3_des_pahigh
+ High energy bin: 2 keV - 30 keV.
+ Pitch-angle bin size: 6 deg. Note that pitch angles are calculated in the spacecraft frame;
+ i.e., not shifted by the bulk velocity
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-dismoms.xml b/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-dismoms.xml
new file mode 100644
index 0000000..3c901de
--- /dev/null
+++ b/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-dismoms.xml
@@ -0,0 +1,291 @@
+
+
+ 2.3.1
+
+ spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-dismoms
+
+ dis-moms : ions
+ ion moments : fast mode
+ 2017-01-16T11:50:00
+ FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for
+the current Mission Phase. Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made
+ available at survey (4.5 s) resolution. Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
+, FPI usually operates in Slow Survey (SS) Mode (60 s resolution) outside of ROI. This moments product contains results
+ from integrating the standard moments of phase-space distributions formed from the indicated data type (DES/DIS burst,
+ FS or SS). For convenience, some additional parameters are included to augment those most commonly found in a moments
+product of this sort, plus time-stamps and other annotation characterizing the state of the instrument system at the in
+dicated time.
+
+ spase://CNES/Person/James.L.Burch
+ PrincipalInvestigator
+
+
+ spase://CNES/Person/B.Giles
+ PrincipalInvestigator
+
+
+ MMS home page at GSFC
+ http://mms.gsfc.nasa.gov
+
+
+ FPI overview
+ http://www.nasa.gov/mission_pages/mms/spacecraft/instruments.html#fpi
+
+
+ mms3-fpi-fast
+ PartOf
+ fast mode
+
+
+
+ spase://SMWG/Repository/CNES/CDPP-AMDA
+ Online
+ Open
+
+ AMDA at CDPP
+ amda.cdpp.eu
+
+ NetCDF
+
+ LASP
+ spase://CNES/Instrument/CDPP-AMDA/MMS3/FPI
+ MagneticField
+
+
+ 2000-08-22T00:00:00Z
+ 2019-01-14T15:58:00Z
+
+ PT4.5S
+
+
+ density
+ mms3_dis_ni
+
+
+ cm^-3
+
+
+ TimeSeries
+
+
+
+ density : err
+ mms3_dis_ni_err
+
+
+ cm^-3
+
+
+ TimeSeries
+
+
+
+ v_gse
+ mms3_dis_vgse
+
+
+ km/s
+
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 3
+
+ vx
+ Component.I
+ 1
+ mms3_dis_vgse(0)
+
+
+ vy
+ Component.J
+ 2
+ mms3_dis_vgse(1)
+
+
+ vz
+ Component.K
+ 3
+ mms3_dis_vgse(2)
+
+
+
+
+ v_gse : err
+ mms3_dis_v_err
+
+
+ km/s
+
+
+ TimeSeries
+
+
+ 3
+
+ vx
+ Component.I
+ 1
+ mms3_dis_v_err(0)
+
+
+ vy
+ Component.J
+ 2
+ mms3_dis_v_err(1)
+
+
+ vz
+ Component.K
+ 3
+ mms3_dis_v_err(2)
+
+
+
+
+ t_para
+ mms3_dis_tpara
+
+
+ eV
+
+
+ TimeSeries
+
+
+
+ t_perp
+ mms3_dis_tperp
+
+
+ eV
+
+
+ TimeSeries
+
+
+
+ heatq_gse
+ mms3_dis_heatq
+
+ phys.pressure
+ nPa
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 3
+
+ x
+ 1
+ mms3_dis_heatq(0)
+
+
+ y
+ 2
+ mms3_dis_heatq(1)
+
+
+ z
+ 3
+ mms3_dis_heatq(2)
+
+
+
+ Ion
+ Vector
+ HeatFlux
+
+
+
+ pressure_gse
+ mms3_dis_press
+
+ phys.pressure
+ nPa
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 9
+
+ xx
+ 1
+ mms3_dis_press(0)
+
+
+ xy
+ 2
+ mms3_dis_press(1)
+
+
+ xz
+ 3
+ mms3_dis_press(2)
+
+
+ yx
+ 4
+ mms3_dis_press(3)
+
+
+ yy
+ 5
+ mms3_dis_press(4)
+
+
+ yz
+ 6
+ mms3_dis_press(5)
+
+
+ zx
+ 7
+ mms3_dis_press(6)
+
+
+ zy
+ 8
+ mms3_dis_press(7)
+
+
+ zz
+ 9
+ mms3_dis_press(8)
+
+
+
+ Ion
+ Tensor
+ Pressure
+
+
+
+ ion eflux : omni
+ mms3_dis_omni
+
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Ion
+ EnergyFlux
+
+
+
+
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-desmoms.xml b/NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-desmoms.xml
new file mode 100644
index 0000000..46f2ca8
--- /dev/null
+++ b/NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-desmoms.xml
@@ -0,0 +1,381 @@
+
+
+ 2.3.1
+
+ spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-desmoms
+
+ des-moms : electrons
+ electron moments : fast mode
+ 2017-01-16T11:50:00
+ FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for
+the current Mission Phase. Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made
+ available at survey (4.5 s) resolution. Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
+, FPI usually operates in Slow Survey (SS) Mode (60 s resolution) outside of ROI. This moments product contains results
+ from integrating the standard moments of phase-space distributions formed from the indicated data type (DES/DIS burst,
+ FS or SS). For convenience, some additional parameters are included to augment those most commonly found in a moments
+product of this sort, plus time-stamps and other annotation characterizing the state of the instrument system at the in
+dicated time.
+
+ spase://CNES/Person/James.L.Burch
+ PrincipalInvestigator
+
+
+ spase://CNES/Person/B.Giles
+ PrincipalInvestigator
+
+
+ MMS home page at GSFC
+ http://mms.gsfc.nasa.gov
+
+
+ FPI overview
+ http://www.nasa.gov/mission_pages/mms/spacecraft/instruments.html#fpi
+
+
+ mms4-fpi-fast
+ PartOf
+ fast mode
+
+
+
+ spase://SMWG/Repository/CNES/CDPP-AMDA
+ Online
+ Open
+
+ AMDA at CDPP
+ amda.cdpp.eu
+
+ NetCDF
+
+ LASP
+ spase://CNES/Instrument/CDPP-AMDA/MMS4/FPI
+ MagneticField
+
+
+ 2000-08-22T00:00:00Z
+ 2019-01-14T15:58:00Z
+
+ PT4.5S
+
+
+ density
+ mms4_des_ne
+
+
+ cm^-3
+
+
+ TimeSeries
+
+
+
+ density : err
+ mms4_des_ne_err
+
+
+ cm^-3
+
+
+ TimeSeries
+
+
+
+ v_gse
+ mms4_des_vgse
+
+
+ km/s
+
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 3
+
+ vx
+ Component.I
+ 1
+ mms4_des_vgse(0)
+
+
+ vy
+ Component.J
+ 2
+ mms4_des_vgse(1)
+
+
+ vz
+ Component.K
+ 3
+ mms4_des_vgse(2)
+
+
+
+
+ v_gse : err
+ mms4_des_v_err
+
+
+ km/s
+
+
+ TimeSeries
+
+
+ 3
+
+ vx
+ Component.I
+ 1
+ mms4_des_v_err(0)
+
+
+ vy
+ Component.J
+ 2
+ mms4_des_v_err(1)
+
+
+ vz
+ Component.K
+ 3
+ mms4_des_v_err(2)
+
+
+
+
+ t_para
+ mms4_des_tpara
+
+
+ eV
+
+
+ TimeSeries
+
+
+
+ t_perp
+ mms4_des_tperp
+
+
+ eV
+
+
+ TimeSeries
+
+
+
+ heatq_gse
+ mms4_des_heatq
+
+ phys.pressure
+ nPa
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 3
+
+ x
+ 1
+ mms4_des_heatq(0)
+
+
+ y
+ 2
+ mms4_des_heatq(1)
+
+
+ z
+ 3
+ mms4_des_heatq(2)
+
+
+
+ Electron
+ Vector
+ HeatFlux
+
+
+
+ pressure_gse
+ mms4_des_press
+
+ phys.pressure
+ nPa
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 9
+
+ xx
+ 1
+ mms4_des_press(0)
+
+
+ xy
+ 2
+ mms4_des_press(1)
+
+
+ xz
+ 3
+ mms4_des_press(2)
+
+
+ yx
+ 4
+ mms4_des_press(3)
+
+
+ yy
+ 5
+ mms4_des_press(4)
+
+
+ yz
+ 6
+ mms4_des_press(5)
+
+
+ zx
+ 7
+ mms4_des_press(6)
+
+
+ zy
+ 8
+ mms4_des_press(7)
+
+
+ zz
+ 9
+ mms4_des_press(8)
+
+
+
+ Electron
+ Tensor
+ Pressure
+
+
+
+ elec eflux : omni
+ mms4_des_omni
+
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ elec eflux : para
+ mms4_des_para
+
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ elec eflux : anti
+ mms4_des_anti
+
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ elec eflux : perp
+ mms4_des_perp
+
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ pa dist : lowen
+ mms4_des_palow
+ Low energy bin: 0 eV - 200 eV.
+ Pitch-angle bin size: 6 deg. Note that pitch angles are calculated in the spacecraft frame;
+ i.e., not shifted by the bulk velocity
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ pa dist : miden
+ mms4_des_pamid
+ Mid energy bin: 200 eV - 2 keV.
+ Pitch-angle bin size: 6 deg. Note that pitch angles are calculated in the spacecraft frame;
+ i.e., not shifted by the bulk velocity
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+ pa dist : highen
+ mms4_des_pahigh
+ High energy bin: 2 keV - 30 keV.
+ Pitch-angle bin size: 6 deg. Note that pitch angles are calculated in the spacecraft frame;
+ i.e., not shifted by the bulk velocity
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Electron
+ EnergyFlux
+
+
+
+
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-dismoms.xml b/NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-dismoms.xml
new file mode 100644
index 0000000..468af93
--- /dev/null
+++ b/NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-dismoms.xml
@@ -0,0 +1,291 @@
+
+
+ 2.3.1
+
+ spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-dismoms
+
+ dis-moms : ions
+ ion moments : fast mode
+ 2017-01-16T11:50:00
+ FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for
+the current Mission Phase. Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made
+ available at survey (4.5 s) resolution. Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
+, FPI usually operates in Slow Survey (SS) Mode (60 s resolution) outside of ROI. This moments product contains results
+ from integrating the standard moments of phase-space distributions formed from the indicated data type (DES/DIS burst,
+ FS or SS). For convenience, some additional parameters are included to augment those most commonly found in a moments
+product of this sort, plus time-stamps and other annotation characterizing the state of the instrument system at the in
+dicated time.
+
+ spase://CNES/Person/James.L.Burch
+ PrincipalInvestigator
+
+
+ spase://CNES/Person/B.Giles
+ PrincipalInvestigator
+
+
+ MMS home page at GSFC
+ http://mms.gsfc.nasa.gov
+
+
+ FPI overview
+ http://www.nasa.gov/mission_pages/mms/spacecraft/instruments.html#fpi
+
+
+ mms4-fpi-fast
+ PartOf
+ fast mode
+
+
+
+ spase://SMWG/Repository/CNES/CDPP-AMDA
+ Online
+ Open
+
+ AMDA at CDPP
+ amda.cdpp.eu
+
+ NetCDF
+
+ LASP
+ spase://CNES/Instrument/CDPP-AMDA/MMS4/FPI
+ MagneticField
+
+
+ 2000-08-22T00:00:00Z
+ 2019-01-14T15:58:00Z
+
+ PT4.5S
+
+
+ density
+ mms4_dis_ni
+
+
+ cm^-3
+
+
+ TimeSeries
+
+
+
+ density : err
+ mms4_dis_ni_err
+
+
+ cm^-3
+
+
+ TimeSeries
+
+
+
+ v_gse
+ mms4_dis_vgse
+
+
+ km/s
+
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 3
+
+ vx
+ Component.I
+ 1
+ mms4_dis_vgse(0)
+
+
+ vy
+ Component.J
+ 2
+ mms4_dis_vgse(1)
+
+
+ vz
+ Component.K
+ 3
+ mms4_dis_vgse(2)
+
+
+
+
+ v_gse : err
+ mms4_dis_v_err
+
+
+ km/s
+
+
+ TimeSeries
+
+
+ 3
+
+ vx
+ Component.I
+ 1
+ mms4_dis_v_err(0)
+
+
+ vy
+ Component.J
+ 2
+ mms4_dis_v_err(1)
+
+
+ vz
+ Component.K
+ 3
+ mms4_dis_v_err(2)
+
+
+
+
+ t_para
+ mms4_dis_tpara
+
+
+ eV
+
+
+ TimeSeries
+
+
+
+ t_perp
+ mms4_dis_tperp
+
+
+ eV
+
+
+ TimeSeries
+
+
+
+ heatq_gse
+ mms4_dis_heatq
+
+ phys.pressure
+ nPa
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 3
+
+ x
+ 1
+ mms4_dis_heatq(0)
+
+
+ y
+ 2
+ mms4_dis_heatq(1)
+
+
+ z
+ 3
+ mms4_dis_heatq(2)
+
+
+
+ Ion
+ Vector
+ HeatFlux
+
+
+
+ pressure_gse
+ mms4_dis_press
+
+ phys.pressure
+ nPa
+
+ Cartesian
+ GSE
+
+
+ TimeSeries
+
+
+ 9
+
+ xx
+ 1
+ mms4_dis_press(0)
+
+
+ xy
+ 2
+ mms4_dis_press(1)
+
+
+ xz
+ 3
+ mms4_dis_press(2)
+
+
+ yx
+ 4
+ mms4_dis_press(3)
+
+
+ yy
+ 5
+ mms4_dis_press(4)
+
+
+ yz
+ 6
+ mms4_dis_press(5)
+
+
+ zx
+ 7
+ mms4_dis_press(6)
+
+
+ zy
+ 8
+ mms4_dis_press(7)
+
+
+ zz
+ 9
+ mms4_dis_press(8)
+
+
+
+ Ion
+ Tensor
+ Pressure
+
+
+
+ ion eflux : omni
+ mms4_dis_omni
+
+
+ keV/(cm^2-s-sr-keV)
+
+ Spectrogram
+
+
+ Ion
+ EnergyFlux
+
+
+
+
--
libgit2 0.21.2