2.3.1 spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-brst.desm des-moms : electrons electron moments : burst 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. Error Flags : Value of zero signifies no quality errors. For non-zero values: * Bit-0 = manually flagged interval * Bit-1 = overcounting/saturation effects likely present in skymap * Bit-2 = reported spacecraft potential above 20V * Bit-3 = invalid/unavailable spacecraft potential * Bit-4 = significant (greater than 10%) cold plasma (lower than 10eV) component * Bit-5 = significant (greater than 25%) hot plasma (greater than 30keV) component * Bit-6 = high sonic Mach number (v/vth greater than 2.5) * Bit-7 = low calculated density (0.05 cm^-3) * Bit-8 = bentPipe magnetic field used instead of brst l2pre magnetic field * Bit-9 = srvy l2pre magnetic field used instead of brst l2pre magnetic field * Bit-10 = no internally generated photoelectron correction applied * Bit-11 = compression pipeline error * Bit-12 = spintone calculation error (DBCS only) 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-brst PartOf burst spase://SMWG/Repository/CNES/CDPP-AMDA Online Open AMDA at CDPP amda.cdpp.eu NetCDF IRAP spase://CNES/Instrument/CDPP-AMDA/MMS2/FPI ThermalPlasma 2000-08-22T00:00:00Z 2019-01-14T15:58:00Z PT0.03S error flags mms2_brst_desm_err TimeSeries density mms2_brst_desm_n cm^-3 TimeSeries density : err mms2_brst_desm_nerr cm^-3 TimeSeries v_gse mms2_brst_desm_v -1e+31 km/s Cartesian GSE TimeSeries 3 vx Component.I 1 mms2_brst_desm_v(0) vy Component.J 2 mms2_brst_desm_v(1) vz Component.K 3 mms2_brst_desm_v(2) v_gse : err mms2_brst_desm_verr -1e+31 km/s TimeSeries 3 vx Component.I 1 mms2_brst_desm_verr(0) vy Component.J 2 mms2_brst_desm_verr(1) vz Component.K 3 mms2_brst_desm_verr(2) t_para mms2_brst_desm_tpar eV TimeSeries t_perp mms2_brst_desm_tperp eV TimeSeries heatq_gse mms2_brst_desm_hq phys.pressure nPa Cartesian GSE TimeSeries 3 x 1 mms2_brst_desm_hq(0) y 2 mms2_brst_desm_hq(1) z 3 mms2_brst_desm_hq(2) Electron Vector HeatFlux heatq_gse : err mms2_brst_desm_hqerr phys.pressure nPa Cartesian GSE TimeSeries 3 x 1 mms2_brst_desm_hqerr(0) y 2 mms2_brst_desm_hqerr(1) z 3 mms2_brst_desm_hqerr(2) Electron Vector HeatFlux press_tensor_gse_x mms2_brst_desmpres_x phys.pressure nPa Cartesian GSE TimeSeries 3 xx 1 mms2_brst_desmpres_x(0) xy 2 mms2_brst_desmpres_x(1) xz 3 mms2_brst_desmpres_x(2) press_tensor_gse_x : err mms2_brst_desmpreserr_x phys.pressure nPa Cartesian GSE TimeSeries 3 xx 1 mms2_brst_desmpreserr_x(0) xy 2 mms2_brst_desmpreserr_x(1) xz 3 mms2_brst_desmpreserr_x(2) Electron Tensor Pressure press_tensor_gse_y mms2_brst_desmpres_y phys.pressure nPa Cartesian GSE TimeSeries 3 yx 1 mms2_brst_desmpres_y(0) yy 2 mms2_brst_desmpres_y(1) yz 3 mms2_brst_desmpres_y(2) press_tensor_gse_y : err mms2_brst_desmpreserr_y phys.pressure nPa Cartesian GSE TimeSeries 3 yx 1 mms2_brst_desmpreserr_y(0) yy 2 mms2_brst_desmpreserr_y(1) yz 3 mms2_brst_desmpreserr_y(2) Electron Tensor Pressure press_tensor_gse_z mms2_brst_desmpres_z phys.pressure nPa Cartesian GSE TimeSeries 3 zx 1 mms2_brst_desmpres_z(0) zy 2 mms2_brst_desmpres_z(1) zz 3 mms2_brst_desmpres_z(2) press_tensor_gse_z : err mms2_brst_desmpreserr_z phys.pressure nPa Cartesian GSE TimeSeries 3 zx 1 mms2_brst_desmpreserr_z(0) zy 2 mms2_brst_desmpreserr_z(1) zz 3 mms2_brst_desmpreserr_z(2) Electron Tensor Pressure temp_tensor_gse_x mms2_brst_desm_tx eV Cartesian GSE TimeSeries 3 xx 1 mms2_brst_desm_tx(0) xy 2 mms2_brst_desm_tx(1) xz 3 mms2_brst_desm_tx(2) Electron Tensor Temperature temp_tensor_gse_y mms2_brst_desm_ty eV Cartesian GSE TimeSeries 3 yx 1 mms2_brst_desm_ty(0) yy 2 mms2_brst_desm_ty(1) yz 3 mms2_brst_desm_ty(2) Electron Tensor Temperature temp_tensor_gse_z mms2_brst_desm_tz eV Cartesian GSE TimeSeries 3 zx 1 mms2_brst_desm_tz(0) zy 2 mms2_brst_desm_tz(1) zz 3 mms2_brst_desm_tz(2) Electron Tensor Temperature elec eflux : omni mms2_brst_desm_spom keV/(cm^2-s-sr-keV) Spectrogram Electron EnergyFlux elec eflux : para mms2_brst_des_para keV/(cm^2-s-sr-keV) Spectrogram Electron EnergyFlux elec eflux : anti mms2_brst_des_anti keV/(cm^2-s-sr-keV) Spectrogram Electron EnergyFlux elec eflux : perp mms2_brst_des_perp keV/(cm^2-s-sr-keV) Spectrogram Electron EnergyFlux pa dist : lowen mms2_brst_des_palow Low energy bin: energy steps 0-10 (of total steps 0-31). 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_brst_des_pamid Mid energy bin: energy steps 11-20 (of total steps 0-31). 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_brst_des_pahigh High energy bin: energy steps 21-31 (of total steps 0-31). 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