2.4.1 spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-dismoms DIS : ions Dual Ion Spectrometers : fast mode 2024-05-23T02:41:21Z 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://SMWG/Person/James.L.Burch PrincipalInvestigator spase://CNES/Person/CDPP-AMDA/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 mms1-fpi-fast PartOf fast mode spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi mms1-fpi-dismoms Web Service to this product using the HAPI interface. CSV Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA Web application https://amda.cdpp.eu Access to Data via CDPP/AMDA Web application. CSV VOTable CDF PNG Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. LASP spase://CNES/Instrument/CDPP-AMDA/MMS1/FPI MagneticField 2015-07-15T15:11:27Z 2024-03-30T23:59:59Z PT4.5S density mms1_dis_ni cm^-3 TimeSeries Electron Scalar NumberDensity density : err mms1_dis_ni_err cm^-3 TimeSeries Electron Scalar NumberDensity v_gse mms1_dis_vgse km/s Cartesian GSE TimeSeries 3 vx Component.I 1 mms1_dis_vgse(0) vy Component.J 2 mms1_dis_vgse(1) vz Component.K 3 mms1_dis_vgse(2) Electron Vector Velocity v_gse : err mms1_dis_v_err km/s TimeSeries 3 vx Component.I 1 mms1_dis_v_err(0) vy Component.J 2 mms1_dis_v_err(1) vz Component.K 3 mms1_dis_v_err(2) Electron Vector Velocity t_para mms1_dis_tpara eV TimeSeries Electron Scalar Temperature t_perp mms1_dis_tperp eV TimeSeries Electron Scalar Temperature heatq_gse mms1_dis_heatq phys.pressure mW/m^2 Cartesian GSE TimeSeries 3 x 1 mms1_dis_heatq(0) y 2 mms1_dis_heatq(1) z 3 mms1_dis_heatq(2) Ion Vector HeatFlux pressure_gse mms1_dis_press phys.pressure nPa Cartesian GSE TimeSeries 9 xx 1 mms1_dis_press(0) xy 2 mms1_dis_press(1) xz 3 mms1_dis_press(2) yx 4 mms1_dis_press(3) yy 5 mms1_dis_press(4) yz 6 mms1_dis_press(5) zx 7 mms1_dis_press(6) zy 8 mms1_dis_press(7) zz 9 mms1_dis_press(8) Ion Tensor Pressure ion eflux : omni mms1_dis_omni keV/(cm^2-s-sr-keV) Spectrogram Ion EnergyFlux