2.3.2 spase://NASA/NumericalData/RBSP/B/RPS/L2/PT1M Van Allen Probe B Proton Spectrometer Belt Research - Relativistic Proton Spectrometer (PSBR-RPS) Energies from ~60 MeV to ~2 GeV, Level 2 (L2), 1 min Data 2021-04-27T15:38:11Z Van Allen Probe B, Relativistic Proton Spectrometer, RPS, Proton Spectrometer Belt Research, PSBR, Data. The RPS Instrument is a Solid State Detector Telescope combined with a Cherenkov Radiator. It measures Protons with Energies from about 60 MeV to about 2 GeV. For more Information, see http://rbsp.aerospace.org/. For a complete Description of the Instrument, see Mazur et al., 2012, The Relativistic Proton Spectrometer (RPS) for the Van Allen Probes Mission (formerly known as Radiation Belt Storm Probes, RBSP), Space Science Reviews. DOI 10.1007/s11214-012-9926-9, http://www.springerlink.com/content/p84680786570g7qp/. The instrument PI, Joseph Mazur, can be reached at Joseph.E.Mazur@aero.org. J. Mazur. The Aerospace Corporation designed and built the RPS Instrument with Funding from The National Reconnaissance Office. The RPS Principal Investigator is Joseph Mazur. Those wishing to use RPS Data are strongly urged to notify the Principal Investigator concerning the Topic of their Work. This will enable the RPS Team to assist in Use of the Data and to track the Utility of the Instrument to the broader Community. spase://SMWG/Person/Joseph.Mazur PrincipalInvestigator spase://SMWG/Person/Robert.E.McGuire MetadataContact spase://SMWG/Person/Lee.Frost.Bargatze MetadataContact Van Allen Probes Home Page, JHU/APL http://vanallenprobes.jhuapl.edu Van Allen Probes Home Page, Exploring Earth's Radiation Belts and the Extremes of Space Weather, Applied Physics Laboratory, Johns Hopkins University Van Allen Probes Science Gateway for access to Data, Models, Software and Tools for Researchers, Students and the General Public, JHU/APL http://rbspgway.jhuapl.edu/ Van Allen Probes Science Gateway for access to Data, Models, Software and Tools for Researchers, Students and the General Public at the Applied Physics Laboratory, Johns Hopkins University Van Allen Probes Science Gateway, Mission Rules of the Road for Data Usage, JHU/APL http://rbspgway.jhuapl.edu/data_policy Van Allen Probes Science Gateway, Mission Rules of the Road for Data Usage, Applied Physics Laboratory at the Applied Physics Laboratory, Johns Hopkins University Van Allen Probes RPS, Web Page for Instrument Summary and Data Access, ViRBO http://virbo.org/RBSP/RPS Van Allen Probes Relativistic Proton Spectrometer, RPS, Web Page for Instrument Description Summary and Data Access Links, at the Virtual Radiation Belt Observatory spase://VSPO/NumericalData/RBSP/B/PSBR/RPS/L2/PT1M spase://VSPO/NumericalData/RBSP/B/PSBR/RelativisticProtonSpectrometer/Level2/PT1M spase://VSPO/NumericalData/RBSP/B/RPS/L2/PT1M spase://SMWG/Repository/NASA/GSFC/SPDF Online Open FTPS from SPDF (not with most browsers) ftps://spdf.gsfc.nasa.gov/pub/data/rbsp/rbspb/l2/psbr/rps-1min/ Access to Data in CDF Format via ftp from SPDF HTTPS from SPDF https://spdf.gsfc.nasa.gov/pub/data/rbsp/rbspb/l2/psbr/rps-1min/ Access to Data in CDF Format via http from SPDF CDAWeb https://cdaweb.gsfc.nasa.gov/cgi-bin/eval2.cgi?dataset=RBSPB_L2-1MIN_PSBR-RPS&index=sp_phys RBSPB_L2-1MIN_PSBR-RPS Access to ASCII, CDF, and Plots via NASA/GSFC CDAWeb CDF None J. Mazur. The Aerospace Corporation designed and built the RPS Instrument with Funding from The National Reconnaissance Office. The RPS Principal Investigator is Joseph Mazur. Those wishing to use RPS Data are strongly urged to notify the Principal Investigator concerning the Topic of their Work. This will enable the RPS Team to assist in Use of the Data and to track the Utility of the Instrument to the broader Community. Please acknowledge the Data Providers and CDAWeb when using these Data. spase://SMWG/Repository/NASA/GSFC/SPDF Online Open CDAWeb HAPI Server https://cdaweb.gsfc.nasa.gov/hapi RBSPB_L2-1MIN_PSBR-RPS Web Service to this product using the HAPI interface. CSV J. Mazur. The Aerospace Corporation designed and built the RPS Instrument with Funding from The National Reconnaissance Office. The RPS Principal Investigator is Joseph Mazur. Those wishing to use RPS Data are strongly urged to notify the Principal Investigator concerning the Topic of their Work. This will enable the RPS Team to assist in Use of the Data and to track the Utility of the Instrument to the broader Community. Please acknowledge the Data Providers and CDAWeb when using these Data. Calibrated spase://SMWG/Instrument/RBSP/B/Ephemeris spase://SMWG/Instrument/RBSP/B/RPS EnergeticParticles InstrumentStatus MagneticField 2012-09-01T00:00:30.000 2019-10-18T16:30:00Z PT1M Earth.Magnetosphere Earth.Magnetosphere.Main Earth.Magnetosphere.RadiationBelt Earth.NearSurface.EquatorialRegion Epoch Time, UTC, Midpoint Time Series defined by using: EPOCH Epoch Epoch Time, Coordinated Universal Time, UTC, Midpoint of 1 s Data PT1M ms 1.0e-3>s TimeSeries Epoch LinearScale 01-Jan-0000 00:00:00.000 31-Dec-9999 23:59:59.998 31-Dec-9999 23:59:59.999 Scalar Temporal Seconds of Livetime Time Series defined by using: EPOCH Seconds Seconds of Livetime in the Minute PT1M s TimeSeries Seconds E15.8 LinearScale 0.0 61.0 -1.0e+31 Scalar Temporal Mission Elapsed Time, Midpoint Time Series defined by using: EPOCH MET_SEC Mission Elapsed Time, MET, Midpoint of the Minute in Seconds PT1M s TimeSeries MET SEC E15.8 LinearScale 0.0 1.0e+10 -1.0e+31 Scalar Temporal Mission Day, Level 0 Data Point Time Series defined by using: EPOCH Mission_Day Mission Day of Level 0 Files for this Data Point PT1M TimeSeries Mission Day I10 LinearScale 0 10000 65535 Scalar Other Spacecraft Position Vector, Geographic Cartesian Coordinates Time Series defined by using: EPOCH Position Spacecraft Position Vector, Geographic, GEO, Cartesian Coordinates PT1M km 1.0e3>m Cartesian GEO TimeSeries Position E12.2 LinearScale 3 Xgeo 1 Xgeo Ygeo 2 Ygeo Zgeo 3 Zgeo -50000.0 50000.0 -1.0e+31 Vector Array Positional Data Quality Flag, Spacecraft Position Vector, Geographic Cartesian Coordinates Time Series defined by using: EPOCH Position_Quality Data Quality Flag, Spacecraft Position Vector, Geographic, GEO, Cartesian Coordinates, 0=Definitive, 1=Predicted PT1M (0=def) TimeSeries Position Quality I10 LinearScale 0 1 65535 Scalar Other Orbit Number Time Series defined by using: EPOCH Orbit_Number Orbit Number PT1M TimeSeries Orbit Number I10 LinearScale 0 10000 65535 Scalar Other Orbit Status Time Series defined by using: EPOCH Orbit_Status Orbit Status: 0=Outbound, 1=Inbound PT1M (0=out,1=in) TimeSeries Orbit Status I10 LinearScale 0 1 255 Scalar InstrumentMode Orbit Epoch Time Series defined by using: EPOCH Orbit_Epoch Orbit Epoch, Decimal Hours since Perigee PT1M h 3600>s TimeSeries Orbit Epoch F15.10 LinearScale 0.0 10.0 -1.0e+31 Scalar Temporal Earth Cone Angle Time Series defined by using: EPOCH EarthConeAngle Earth Cone Angle, Half-Angle of Earth as seen from the Spacecraft PT1M ° 0.0174532925>rad TimeSeries EarthConeAngle E12.2 LinearScale 0.0 90.0 -1.0e+31 Scalar Other Measured Magnetic Field Vector, Geographic Cartesian Coordinates Time Series defined by using: EPOCH B_Meas Measured Magnetic Field Vector, Geographic, GEO, Cartesian Coordinates PT1M nT 1.0e-9>T TimeSeries B Meas E12.2 LinearScale 3 Meas. BXgeo 1 Meas. BXgeo Meas. BYgeo 2 Meas. BYgeo Meas. BZgeo 3 Meas. BZgeo -200000.0 200000.0 -1.0e+31 Vector Array Magnetic Measured Magnetic Field Flag Time Series defined by using: EPOCH B_Meas_Flag Measured Magnetic Field Flag: 0=MAG L0 File, 1=MAG L1 File, etc. If this Flag equals 255, then the Olson-Pfitzer 1977 Quiet, OP77Q, Magnetic Field Model is used for computing Alpha and Beta PT1M (source level) TimeSeries B Meas Flag I10 LinearScale 0 5 255 Scalar InstrumentMode Spin Rate, Omega Time Series defined by using: EPOCH SPIN_OMEGA Spin Rate, Omega, the Relativistic Proton Spectrometer, RPS, Spin Axis Vector in Geographic, GEO, Cartesian Coordinates, the Vector Norm is the Spin Rate PT1M rad/s TimeSeries SPIN OMEGA E12.2 LinearScale 3 Spin Xgeo 1 Spin Xgeo Spin Ygeo 2 Spin Ygeo Spin Zgeo 3 Spin Zgeo -10.0 10.0 -1.0e+31 Array Positional Data Channel Count Rate, Spectrograms Time Series defined by using: EPOCH DATA_CHANNEL_COUNTS Data Channel Count Rate, Spectrograms based on EVENT_ENERGY_MIN2SSD, the Estimated Event Energy calculated by using the Average of Minimum 2 Solid State Detector, SSD, Deposits Algorithm PT1M s^-1 Spectrogram DATA CHANNEL COUNTS E12.2 LogScale 20 0 1 0 1 2 1 2 3 2 3 4 3 4 5 4 5 6 5 6 7 6 7 8 7 8 9 8 9 10 9 10 11 10 11 12 11 12 13 12 13 14 13 14 15 14 15 16 15 16 17 16 17 18 17 18 19 18 19 20 19 0.0 100000.0 -1.0e+31 Ion Array CountRate Proton Differential Flux Intensity, Isotropic Assumption Time Series defined by using: EPOCH FPDI Proton Differential Flux Intensity, Unidirectional, Spectrograms versus Energy, Isotropic Assumption FPDI stands for Flux, Proton, Differential, Isotropic PT1M (cm^2 s sr MeV)^-1 6.24161e-19>(m^2 s sr J)^-1 Spectrogram FPDI E12.2 LogScale 20 58 MeV 1 58.1000 75 MeV 2 74.9000 90 MeV 3 89.9000 106 MeV 4 106.000 123 MeV 5 123.000 143 MeV 6 143.000 165 MeV 7 165.000 192 MeV 8 192.000 224 MeV 9 224.000 261 MeV 10 261.000 305 MeV 11 305.000 356 MeV 12 356.000 414 MeV 13 414.000 469 MeV 14 469.000 529 MeV 15 529.000 600 MeV 16 600.000 683 MeV 17 683.000 787 MeV 18 787.000 907 MeV 19 907.000 1325 MeV 20 1320.00 0.0 1.0e+10 -1.0e+31 Proton Array NumberFlux 1 RMS Error, Natural Logarithm, Proton Differential Flux Intensity, Isotropic Assumption Time Series defined by using: EPOCH FPDI_RMSE RMS Error, Natural Logarithm of the Proton Differential Flux Intensity, ln(FPDI), Spectrograms versus Energy, Isotropic Assumption, including Poisson and Cross-Calibration Errors FPDI stands for Flux, Proton, Differential, Isotropic PT1M Spectrogram FPDI RMSE E12.2 LinearScale 20 58 MeV 1 58.1000 75 MeV 2 74.9000 90 MeV 3 89.9000 106 MeV 4 106.000 123 MeV 5 123.000 143 MeV 6 143.000 165 MeV 7 165.000 192 MeV 8 192.000 224 MeV 9 224.000 261 MeV 10 261.000 305 MeV 11 305.000 356 MeV 12 356.000 414 MeV 13 414.000 469 MeV 14 469.000 529 MeV 15 529.000 600 MeV 16 600.000 683 MeV 17 683.000 787 MeV 18 787.000 907 MeV 19 907.000 1325 MeV 20 1320.00 0.0 1000.0 -1.0e+31 Proton Array NumberFlux 1 Data Quality Flag, Proton Differential Flux Intensity, Unidirectional Time Series defined by using: EPOCH FPDI_Quality Data Quality Flag, Proton Differential Flux Intensity, Unidirectional, Spectrograms versus Energy: 0=Highest Quality, 1=Problem with Time Resolution, 2=Contamination, 3=Saturation, 4=Other Problem, 5=Background, 10=Not yet quality checked FPDI stands for Flux, Proton, Differential, Isotropic PT1M Spectrogram FPDI Quality I10 LinearScale 20 58 MeV 1 58.1000 75 MeV 2 74.9000 90 MeV 3 89.9000 106 MeV 4 106.000 123 MeV 5 123.000 143 MeV 6 143.000 165 MeV 7 165.000 192 MeV 8 192.000 224 MeV 9 224.000 261 MeV 10 261.000 305 MeV 11 305.000 356 MeV 12 356.000 414 MeV 13 414.000 469 MeV 14 469.000 529 MeV 15 529.000 600 MeV 16 600.000 683 MeV 17 683.000 787 MeV 18 787.000 907 MeV 19 907.000 1325 MeV 20 1320.00 0 100 65535 Array Other Mission accumulated Dose, Dosimeter 1 Time Series defined by using: EPOCH DOSE1 Mission accumulated Dose, Dosimeter 1, Front PT1M rad 0.01>Gy TimeSeries DOSE1 E12.2 LinearScale 0.0 1.0e+07 -1.0e+31 Other Scalar Dose Rate, Dosimeter 1 Time Series defined by using: EPOCH DOSE1_RATE Dose Rate, Dosimeter 1, Front PT1M rad/s 0.01>Gy/s TimeSeries DOSE1 RATE E12.2 LinearScale 0.0 1.0 -1.0e+31 Other Scalar Mission accumulated Dose, Dosimeter 2 Time Series defined by using: EPOCH DOSE2 Mission accumulated Dose, Dosimeter 2, Side PT1M rad 0.01>Gy TimeSeries DOSE2 E12.2 LinearScale 0.0 1.0e+07 -1.0e+31 Other Scalar Dose Rate, Dosimeter 2 Time Series defined by using: EPOCH DOSE2_RATE Dose Rate, Dosimeter 2, Side PT1M rad/s 0.01>Gy/s TimeSeries DOSE2 RATE E12.2 LinearScale 0.0 1.0 -1.0e+31 Other Scalar McIlwain L Shell Parameter, locally mirroring Particle, OP77Q Magnetic Field Model Time Series defined by using: EPOCH L McIlwain L Shell Parameter for a locally mirroring Particle, computed by using the Olson-Pfitzer 1977 Quiet, OP77Q, Magnetic Field Model PT1M Re 6.3712e6>m TimeSeries L E12.2 LinearScale 0.0 20.0 -1.0e+31 Scalar Other Roederer L* generalized L Shell Parameter, 90° Particle, OP77Q Magnetic Field Model Time Series defined by using: EPOCH L_star Roederer L* generalized L Shell Parameter for a 90° Pitch Angle Particle, computed by using the Olson-Pfitzer 1977 Quiet, OP77Q, Magnetic Field Model PT1M Re 6.3712e6>m TimeSeries L star E12.2 LinearScale 0.0 20.0 -1.0e+31 Scalar Other Third Drift Invariant, Phi, 90° Particle, OP77Q Magnetic Field Model Time Series defined by using: EPOCH Phi Third Drift Invariant, Phi, for a 90° Pitch Angle Particle, computed by using the Olson-Pfitzer 1977 Quiet, OP77Q, Magnetic Field Model PT1M nT Re^2 4.05922e+4>T m^2 TimeSeries Phi E12.2 LinearScale 1000.0 1.0e+06 -1.0e+31 Scalar Magnetic Equatorial Pitch Angle, Alpha, 90° Particle, OP77Q Magnetic Field Model Time Series defined by using: EPOCH Alpha_Eq Equatorial Pitch Angle, Alpha, for a 90° Pitch Angle Particle, computed by using the Olson-Pfitzer 1977 Quiet, OP77Q, Magnetic Field Model PT1M ° 0.0174532925>rad TimeSeries Alpha Eq E12.2 LinearScale 0.0 90.0 -1.0e+31 Scalar Other Model Spacecraft Magnetic Field Vector, Geographic Cartesian Coordinates, OP77Q Magnetic Field Model Time Series defined by using: EPOCH B_Calc Model Spacecraft Magnetic Field Vector, Geographic, GEO, Cartesian Coordinates, computed by using the Olson-Pfitzer 1977 Quiet, OP77Q, Magnetic Field Model PT1M nT 1.0e-9>T TimeSeries B Calc E12.2 LinearScale 3 OPQ BXgeo 1 OPQ BXgeo OPQ BYgeo 2 OPQ BYgeo OPQ BZgeo 3 OPQ BZgeo -200000.0 200000.0 -1.0e+31 Vector Array Magnetic Model Magnetic Field Magnitude, Field Line Local Minimum, OP77Q Magnetic Field Model Time Series defined by using: EPOCH B_Eq Model Magnetic Field Magnitude, Field Line Local Minimum, computed by using the Olson-Pfitzer 1977 Quiet, OP77Q, Magnetic Field Model PT1M nT 1.0e-9>T TimeSeries B Eq E12.2 LinearScale 0.0 200000.0 -1.0e+31 Magnitude Scalar Magnetic Spacecraft Position, Magnetic Local Time, OP77Q Magnetic Field Model Time Series defined by using: EPOCH MLT Spacecraft Position, Magnetic Local Time, MLT, in Hours, computed by using the Olson-Pfitzer 1977 Quiet, OP77Q, Magnetic Field Model PT1M h 3600>s Spherical MAG TimeSeries MLT E12.2 LinearScale 0.0 24.0 -1.0e+31 DirectionAngle.ElevationAngle Scalar Positional Cross-Calibration Factors, Proton Differential Flux Intensity FPDI_Crosscalib Cross-Calibration Factors, Proton Differential Flux Intensity, relative to Reference Instrument PT1M FPDI Crosscalib E12.2 LinearScale 20 0.0 1.0e+10 -1.0e+31 Proton Array NumberFlux 1 RMS Error, Natural Logarithm, Proton Differential Flux Intensity FPDI_Crosscalib_RMSE RMS Error, Natural Logarithm of the Proton Differential Flux Intensity, ln(FPDI), relative to Reference Instrument Currently derived by using Bowtie Analysis PT1M FPDI Crosscalib RMSE E12.2 LinearScale 20 0.0 1000.0 -1.0e+31 Proton Array NumberFlux 1 Proton Channel, Energy FPDI_Energy Proton Energy Channel Currently derived by using Bowtie Analysis PT1M MeV 1.602176565e-13>J FPDI Energy E12.2 LogScale 20 0.0 10000.0 -1.0e+31 Proton Array Energy 1 Proton Channel, Energy Range FPDI_EnergyRange Proton Channel, Nominal Energy Range for each Channel Selection Limits for Events assigned to each Channel PT1M MeV 1.602176565e-13>J FPDI EnergyRange E12.2 LogScale 20 2 -1.0e+31 Proton Array Energy 1 Proton Flux Intensity, Differential, Geometric-Energy Factors FPDI_GdE Proton Flux Intensity, Differential, Geometric-Energy Factors, calculated from Bowtie Analysis PT1M cm^2 sr MeV 1.602176565e-17>J m^2 sr FPDI GdE E12.2 LinearScale 20 0.0 10000.0 -1.0e+31 Array InstrumentMode