2.3.1 spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-desmoms DES : electrons Dual Electron Spectrometers : 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