From 4d45bcf503a25867b44894ba279de5928ea514a7 Mon Sep 17 00:00:00 2001 From: Benjamin Renard Date: Wed, 16 Jun 2021 13:23:16 +0200 Subject: [PATCH] Update MMS FPI FAST datasets --- NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-dismoms.xml | 2 +- NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-desmoms.xml | 381 +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-dismoms.xml | 291 +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-desmoms.xml | 381 +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-dismoms.xml | 291 +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-desmoms.xml | 381 +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-dismoms.xml | 291 +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ 7 files changed, 2017 insertions(+), 1 deletion(-) create mode 100644 NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-desmoms.xml create mode 100644 NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-dismoms.xml create mode 100644 NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-desmoms.xml create mode 100644 NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-dismoms.xml create mode 100644 NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-desmoms.xml create mode 100644 NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-dismoms.xml 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