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CDAWeb Served Heliophysics Datasets Beginning with 'R'

RBSP-A-RBSPICE_LEV-2_ESRHELT: RBSP_H0_RBSPICE_ESR_HELT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-2_ESRLEHT: RBSP_H0_RBSPICE_ESR_LEHT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-2_ISRHELT: RBSP_H0_RBSPICE_ISR_HELT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-2_TOFXEH: RBSP_H0_RBSPICE_TOFxE_H - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-2_TOFXEION: RBSP_H0_RBSPICE_TOFxE_Ion - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-2_TOFXENONH: RBSP_H0_RBSPICE_TOFxE_nonH - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-2_TOFXPHHHELT: RBSP_H0_RBSPICE_TOFxPH_H_HELT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-2_TOFXPHHLEHT: RBSP_H0_RBSPICE_TOFxPH_H_HELT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_ESRHELT: rbsp-a-rbspice_level_3_esrhelt - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_ESRLEHT: rbsp-a-rbspice_level_3_esrleht - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXEH: rbsp-a-rbspice_level_3_tofxeh - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXEHE: rbsp-a-rbspice_level_3_tofxenonh - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXEHE-0: rbsp-a-rbspice_level_3_tofxenonh - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXEION: rbsp-a-rbspice_level_3_tofxeion - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXEO: rbsp-a-rbspice_level_3_tofxenonh - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXEO-0: rbsp-a-rbspice_level_3_tofxenonh - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXPHHHELT: rbsp-a-rbspice_level_3_tofxphhhelt - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXPHHLEHT: rbsp-a-rbspice_level_3_tofxphhleht - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXPHOHELT: rbsp-a-rbspice_level_3_tofxphhhelt - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXPHOLEHT: rbsp-a-rbspice_level_3_tofxphhleht - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_ESRHELT: rbsp-a-rbspice_level_3_ESRHELT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_ESRLEHT: rbsp-a-rbspice_level_3_ESRLEHT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_ISRHELT: rbsp-a-rbspice_level_3_ISRHELT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_TOFXEH: rbsp-a-rbspice_level_3_TOFXEH - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_TOFXEION: rbsp-a-rbspice_level_3_TOFXEION - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_TOFXENONH: rbsp-a-rbspice_level_3_TOFXENONH - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_TOFXPHHHELT: rbsp-a-rbspice_level_3_TOFXPHHHELT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_TOFXPHHLEHT: rbsp-a-rbspice_level_3_TOFXPHHLEHT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A_DENSITY_EMFISIS-L4: Density and other parameters inferred by digitizing the trace on the spectrograms. - Craig Kletzing (University of Iowa)
RBSP-A_HFR-SPECTRA-BURST_EMFISIS-L2: Single Axis AC Electric Field Spectra - Craig Kletzing (University of Iowa)
RBSP-A_HFR-SPECTRA-MERGED_EMFISIS-L2: Single Axis AC Electric Field Spectra - Craig Kletzing (University of Iowa)
RBSP-A_HFR-SPECTRA_EMFISIS-L2: Single Axis AC Electric Field Spectra - Craig Kletzing (University of Iowa)
RBSP-A_HFR-WAVEFORM_EMFISIS-L2: High Frequency Receiver Waveform - Craig Kletzing (University of Iowa)
RBSP-A_MAGNETOMETER_1SEC-GEI_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_MAGNETOMETER_1SEC-GEO_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_MAGNETOMETER_1SEC-GSE_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_MAGNETOMETER_1SEC-GSM_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_MAGNETOMETER_1SEC-SM_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_MAGNETOMETER_4SEC-GEI_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_MAGNETOMETER_4SEC-GEO_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_MAGNETOMETER_4SEC-GSE_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_MAGNETOMETER_4SEC-GSM_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_MAGNETOMETER_4SEC-SM_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_MAGNETOMETER_HIRES-GEI_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_MAGNETOMETER_HIRES-GEO_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_MAGNETOMETER_HIRES-GSE_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_MAGNETOMETER_HIRES-GSM_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_MAGNETOMETER_HIRES-SM_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_WFR-SPECTRAL-MATRIX-DIAGONAL-MERGED_EMFISIS-L2: WFR Spectral Matrix - Craig Kletzing (University of Iowa)
RBSP-A_WFR-SPECTRAL-MATRIX-DIAGONAL_EMFISIS-L2: WFR Spectral Matrix - Craig Kletzing (University of Iowa)
RBSP-A_WFR-SPECTRAL-MATRIX_EMFISIS-L2: WFR Spectral Matrix - Craig Kletzing (University of Iowa)
RBSP-A_WFR-WAVEFORM-CONTINUOUS-BURST_EMFISIS-L2: WFR Spectral Matrix - Craig Kletzing (University of Iowa)
RBSP-A_WFR-WAVEFORM_EMFISIS-L2: WFR Spectral Matrix - Craig Kletzing (University of Iowa)
RBSP-B-RBSPICE_LEV-2_ESRHELT: RBSP_H0_RBSPICE_ESR_HELT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-2_ESRLEHT: RBSP_H0_RBSPICE_ESR_LEHT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-2_ISRHELT: RBSP_H0_RBSPICE_ISR_HELT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-2_TOFXEH: RBSP_H0_RBSPICE_TOFxE_H - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-2_TOFXEION: RBSP_H0_RBSPICE_TOFxE_Ion - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-2_TOFXENONH: RBSP_H0_RBSPICE_TOFxE_nonH - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-2_TOFXPHHHELT: RBSP_H0_RBSPICE_TOFxPH_H_HELT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-2_TOFXPHHLEHT: RBSP_H0_RBSPICE_TOFxPH_H_HELT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_ESRHELT: rbsp-b-rbspice_level_3_esrhelt - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_ESRLEHT: rbsp-b-rbspice_level_3_esrleht - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXEH: rbsp-b-rbspice_level_3_tofxeh - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXEHE: rbsp-b-rbspice_level_3_tofxenonh - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXEHE-0: rbsp-b-rbspice_level_3_tofxenonh - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXEION: rbsp-b-rbspice_level_3_tofxeion - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXEO: rbsp-b-rbspice_level_3_tofxenonh - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXEO-0: rbsp-b-rbspice_level_3_tofxenonh - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXPHHHELT: rbsp-b-rbspice_level_3_tofxphhhelt - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXPHHLEHT: rbsp-b-rbspice_level_3_tofxphhleht - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXPHOHELT: rbsp-b-rbspice_level_3_tofxphhhelt - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXPHOLEHT: rbsp-b-rbspice_level_3_tofxphhleht - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_ESRHELT: rbsp-b-rbspice_level_3_ESRHELT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_ESRLEHT: rbsp-b-rbspice_level_3_ESRLEHT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_ISRHELT: rbsp-b-rbspice_level_3_ISRHELT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_TOFXEH: rbsp-b-rbspice_level_3_TOFXEH - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_TOFXEION: rbsp-b-rbspice_level_3_TOFXEION - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_TOFXENONH: rbsp-b-rbspice_level_3_TOFXENONH - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_TOFXPHHHELT: rbsp-b-rbspice_level_3_TOFXPHHHELT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_TOFXPHHLEHT: rbsp-b-rbspice_level_3_TOFXPHHLEHT - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B_DENSITY_EMFISIS-L4: Density and other parameters inferred by digitizing the trace on the spectrograms. - Craig Kletzing (University of Iowa)
RBSP-B_HFR-SPECTRA-BURST_EMFISIS-L2: Single Axis AC Electric Field Spectra - Craig Kletzing (University of Iowa)
RBSP-B_HFR-SPECTRA-MERGED_EMFISIS-L2: Single Axis AC Electric Field Spectra - Craig Kletzing (University of Iowa)
RBSP-B_HFR-SPECTRA_EMFISIS-L2: Single Axis AC Electric Field Spectra - Craig Kletzing (University of Iowa)
RBSP-B_HFR-WAVEFORM_EMFISIS-L2: High Frequency Receiver Waveform - Craig Kletzing (University of Iowa)
RBSP-B_MAGNETOMETER_1SEC-GEI_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_MAGNETOMETER_1SEC-GEO_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_MAGNETOMETER_1SEC-GSE_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_MAGNETOMETER_1SEC-GSM_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_MAGNETOMETER_1SEC-SM_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_MAGNETOMETER_4SEC-GEI_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_MAGNETOMETER_4SEC-GEO_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_MAGNETOMETER_4SEC-GSE_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_MAGNETOMETER_4SEC-GSM_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_MAGNETOMETER_4SEC-SM_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_MAGNETOMETER_HIRES-GEI_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_MAGNETOMETER_HIRES-GEO_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_MAGNETOMETER_HIRES-GSE_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_MAGNETOMETER_HIRES-GSM_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_MAGNETOMETER_HIRES-SM_EMFISIS-L3: Fluxgate Magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_WFR-SPECTRAL-MATRIX-DIAGONAL-MERGED_EMFISIS-L2: WFR Spectral Matrix - Craig Kletzing (University of Iowa)
RBSP-B_WFR-SPECTRAL-MATRIX-DIAGONAL_EMFISIS-L2: WFR Spectral Matrix - Craig Kletzing (University of Iowa)
RBSP-B_WFR-SPECTRAL-MATRIX_EMFISIS-L2: WFR Spectral Matrix - Craig Kletzing (University of Iowa)
RBSP-B_WFR-WAVEFORM-CONTINUOUS-BURST_EMFISIS-L2: WFR Spectral Matrix - Craig Kletzing (University of Iowa)
RBSP-B_WFR-WAVEFORM_EMFISIS-L2: WFR Spectral Matrix - Craig Kletzing (University of Iowa)
RBSPA_EFW-L2_E-HIRES-UVW: DERIVED FROM: Reference for Spin Axis Vector in GSE - J. R. Wygant (University of Minnesota)
RBSPA_EFW-L2_E-SPINFIT-MGSE: DERIVED FROM: Spinfit DC Electric Field estimates in M-GSE coordinates - J. R. Wygant (University of Minnesota)
RBSPA_EFW-L2_ESVY_DESPUN: DERIVED FROM: Spinfit DC Electric Field estimates in M-GSE coordinates - J. R. Wygant (University of Minnesota)
RBSPA_EFW-L2_FBK: Filterbank data product from RBSP-EFW - J. R. Wygant (University of Minnesota)
RBSPA_EFW-L2_SPEC: Spectral data product from RBSP-EFW - J. R. Wygant (University of Minnesota)
RBSPA_EFW-L2_VSVY-HIRES: DERIVED FROM: Spinfit DC Electric Field estimates in M-GSE coordinates - J. R. Wygant (University of Minnesota)
RBSPA_EFW-L3: L3 CDF files for individual distribution by EFW team - J. R. Wygant (University of Minnesota)
RBSPA_EFW_BURST-WAVEFORM-UVW-L1: Burst Mode 1 (512 samples/sec) Electric and Magnetic Fields - J. R. Wygant
RBSPA_L1_EB1: Electric field, Burst-1 mode in UVW coordinates - J. R. Wygant (U. of Minnesota)
RBSPA_L1_EB2: Electric field, Burst-2 mode in UVW coordinates - J. R. Wygant (U. of Minnesota)
RBSPA_L1_MSCB1: Searchcoil magnetic field, Burst-1 mode in UVW coordinates - J. R. Wygant (U. of Minnesota)
RBSPA_L1_MSCB2: Searchcoil magnetic field, Burst-2 mode in UVW coordinates - J. R. Wygant (U. of Minnesota)
RBSPA_L1_VB1: Sensor Voltages, Burst-1 mode V1-V6 - J. R. Wygant (U. of Minnesota)
RBSPA_L1_VB2: Sensor Voltages, Burst-2 mode V1-V6 - J. R. Wygant (U. of Minnesota)
RBSPA_L2-1MIN_PSBR-RPS: Van Allen Probes/RPS Level 2 1-Minute Data - J. Mazur (The Aerospace Corporation)
RBSPA_L2_PSBR-RPS: Van Allen Probes/RPS Level 2 Data - J. Mazur (The Aerospace Corporation)
RBSPA_REL03_ECT-MAGEIS-L2: rbsp-a_ect-mageis-l2_pre - J. Bernard Blake (JBernard.Blake@aero.org) (The Aerospace Corporation)
RBSPA_REL03_ECT-REPT-SCI-L2: rbspa>Level 2 data for the REPT instrument - D. Baker (University of Colorado at Boulder)
RBSPA_REL03_ECT-REPT-SCI-L3: RBSP/ECT REPT Pitch Angle Resolved Electron and Proton Fluxes. Electron energies: 1.8 - 20 MeV. Proton energies: 21.25 - 4.94066e-324 MeV - D. Baker (University of Colorado at Boulder)
RBSPA_REL04_ECT-HOPE-MOM-L3: Spin resolved HOPE science data. Electrons and protons measured in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPA_REL04_ECT-HOPE-PA-L3: Pitch angle resolved HOPE science data. Electrons and protons measured in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPA_REL04_ECT-HOPE-SCI-L2: Spin resolved HOPE science data. Electrons and protons measured in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPA_REL04_ECT-HOPE-SCI-L2SA: Spin averaged HOPE science data. Electrons and protons measured in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPA_REL04_ECT-MAGEIS-L3: 13 - J. Bernard Blake (JBernard.Blake@aero.org) (The Aerospace Corporation)
RBSPB_EFW-L2_E-HIRES-UVW: DERIVED FROM: Reference for Spin Axis Vector in GSE - J. R. Wygant (University of Minnesota)
RBSPB_EFW-L2_E-SPINFIT-MGSE: DERIVED FROM: Spinfit DC Electric Field estimates in M-GSE coordinates - J. R. Wygant (University of Minnesota)
RBSPB_EFW-L2_ESVY_DESPUN: DERIVED FROM: Spinfit DC Electric Field estimates in M-GSE coordinates - J. R. Wygant (University of Minnesota)
RBSPB_EFW-L2_FBK: Filterbank data product from RBSP-EFW - J. R. Wygant (University of Minnesota)
RBSPB_EFW-L2_SPEC: Spectral data product from RBSP-EFW - J. R. Wygant (University of Minnesota)
RBSPB_EFW-L2_VSVY-HIRES: DERIVED FROM: Spinfit DC Electric Field estimates in M-GSE coordinates - J. R. Wygant (University of Minnesota)
RBSPB_EFW-L3: L3 CDF files for individual distribution by EFW team - J. R. Wygant (University of Minnesota)
RBSPB_EFW_BURST-WAVEFORM-UVW-L1: Burst Mode 1 (512 samples/sec) Electric and Magnetic Fields - J. R. Wygant
RBSPB_L1_EB1: Electric field, Burst-1 mode in UVW coordinates - J. R. Wygant (U. of Minnesota)
RBSPB_L1_EB2: Electric field, Burst-2 mode in UVW coordinates - J. R. Wygant (U. of Minnesota)
RBSPB_L1_MSCB1: Searchcoil magnetic field, Burst-1 mode in UVW coordinates - J. R. Wygant (U. of Minnesota)
RBSPB_L1_MSCB2: Searchcoil magnetic field, Burst-2 mode in UVW coordinates - J. R. Wygant (U. of Minnesota)
RBSPB_L1_VB1: Sensor Voltages, Burst-1 mode V1-V6 - J. R. Wygant (U. of Minnesota)
RBSPB_L1_VB2: Sensor Voltages, Burst-2 mode V1-V6 - J. R. Wygant (U. of Minnesota)
RBSPB_L2-1MIN_PSBR-RPS: Van Allen Probes/RPS Level 2 1-Minute Data - J. Mazur (The Aerospace Corporation)
RBSPB_L2_PSBR-RPS: Van Allen Probes/RPS Level 2 Data - J. Mazur (The Aerospace Corporation)
RBSPB_REL03_ECT-MAGEIS-L2: rbsp-a_ect-mageis-l2_pre - J. Bernard Blake (JBernard.Blake@aero.org) (The Aerospace Corporation)
RBSPB_REL03_ECT-REPT-SCI-L2: rbspb>Level 2 data for the REPT instrument - D. Baker (University of Colorado at Boulder)
RBSPB_REL03_ECT-REPT-SCI-L3: RBSP/ECT REPT Pitch Angle Resolved Electron and Proton Fluxes. Electron energies: 1.8 - 20 MeV. Proton energies: 21.25 - 4.94066e-324 MeV - D. Baker (University of Colorado at Boulder)
RBSPB_REL04_ECT-HOPE-MOM-L3: Spin resolved HOPE science data. Electrons and protons measured in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPB_REL04_ECT-HOPE-PA-L3: Pitch angle resolved HOPE science data. Electrons and protons measured in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPB_REL04_ECT-HOPE-SCI-L2: Spin resolved HOPE science data. Electrons and protons measured in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPB_REL04_ECT-HOPE-SCI-L2SA: Spin averaged HOPE science data. Electrons and protons measured in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPB_REL04_ECT-MAGEIS-L3: 16 - J. Bernard Blake (JBernard.Blake@aero.org) (The Aerospace Corporation)
RBSP_ECT-REPT-SCI-L3-SELESNICK-MODEL: RBSP/ECT REPT Monthly Intensities as a function of Energy, Pitch Angle and L-shell from the Selesnick model - D. Baker (University of Colorado at Boulder)
RENU2_H0_EFIELD: H0 - RENU2 COWBOY Electric Field. - Marc Lessard, David Hysell (University of New Hampshire, Cornell University)
RENU2_H0_EPLAS: H0 - RENU2 EPLAS Electron Flux. - Marc Lessard (University of New Hampshire)
RENU2_H0_ERPAMAIN: H0 - RENU2 ERPA Thermal Electrons. - Marc Lessard (University of New Hampshire)
RENU2_H0_ERPASUB: H0 - RENU2 ERPA Thermal Electrons. - Marc Lessard (University of New Hampshire)
RENU2_H0_FGM: H0 - RENU2 Magnetic Field. - Marc Lessard (University of New Hampshire, Cornell University)
RENU2_H0_IG2: H0 - RENU2 ionization gauge - James Clemmons (University of New Hampshire)
RENU2_H0_PMT: H0 - RENU2 PMT Rayleighs. - Jim Hecht (University of New HampshireAerospace Corporation)
RENU2_H0_UVPMT: H0 - RENU2 UV PMT Counts. - Marc Lessard (University of New Hampshire)
RENU2_H0_VLF: H0 - RENU2 COWBOY Electric Field. - Marc Lessard, David Hysell (University of New Hampshire, Cornell University)
ROSETTA_HELIO1DAY_POSITION: Position in heliocentric coordinates from SPDF Helioweb - Natalia Papitashvili (NASA/GSFC/SPDF)
RS_K0_IPEI: ROCSAT-1(FORMOSAT-1)/IPEI, Key Parameters - Shin-Yi Su (Institution of Space Science, National Central University, Taiwan, R.O.C.)

RBSP-A-RBSPICE_LEV-2_ESRHELT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L2/ESRHELT)
Description
RBSP RBSPICE High Energy Resolution Electron Rates converted into units of
physical intensity (counts/(s*sr*cm^2*MeV) measured at high energy resolution
and low time resolution.
For more information regarding this data and the
RBSPICE science goals and mission statement see the RBSPICE team web site at:
http:// rbspice.ftecs.com.
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-2_ESRLEHT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L2/ESRLEHT)
Description
RBSP RBSPICE Low Energy Resolution Electron Rates converted into units of
physical intensity (counts/(s*sr*cm^2*MeV) measured at high energy resolution
and low time resolution.
For more information regarding this data and the
RBSPICE science goals and mission statement see the RBSPICE team web site at:
http:// rbspice.ftecs.com.
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-2_ISRHELT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L2/ISRHELT)
Description
RBSP RBSPICE High Energy Resolution Ion Species Rates converted into units of
physical intensity (counts/(s*sr*cm^2*MeV) measured at high energy resolution
and low time resolution.
For more information regarding this data and the
RBSPICE science goals and mission statement see the RBSPICE team web site at:
http:// rbspice.ftecs.com.
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-2_TOFXEH (spase://NASA/NumericalData/RBSP/A/RBSPICE/L2/TOFXEH)
Description
RBSP RBSPICE TOF x Energy Hydrogen Rates converted into units of physical
intensity (counts/(s*sr*cm^2*MeV) measured at high energy resolution and low
time resolution.
For more information regarding this data and the RBSPICE
science goals and mission statement see the RBSPICE team web site at: http:// 
rbspice.ftecs.com.
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-2_TOFXEION (spase://NASA/NumericalData/RBSP/A/RBSPICE/L2/TOFXEION)
Description
RBSP RBSPICE TOF x Energy Ion Rates converted into units of physical intensity
(counts/(s*sr*cm^2*MeV) measured at high energy resolution and low time
resolution.
For more information regarding this data and the RBSPICE science
goals and mission statement see the RBSPICE team web site at: http:// 
rbspice.ftecs.com.
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-2_TOFXENONH (spase://NASA/NumericalData/RBSP/A/RBSPICE/L2/TOFXENONH)
Description
RBSP RBSPICE TOF x E non Hydrogen (Helium and Oxygen) Rates converted into units
of physical intensity (counts/(s*sr*cm^2*MeV) measured at high energy resolution
and low time resolution.
For more information regarding this data and the
RBSPICE science goals and mission statement see the RBSPICE team web site at:
http:// rbspice.ftecs.com.
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-2_TOFXPHHHELT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L2/TOFXPHHHELT)
Description
RBSP RBSPICE TOF x PH Hydrogen Rates converted into units of physical intensity
(counts/(s*sr*cm^2*MeV) measured at high energy resolution and low time
resolution.
For more information regarding this data and the RBSPICE science
goals and mission statement see the RBSPICE team web site at: http:// 
rbspice.ftecs.com.
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-2_TOFXPHHLEHT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L2/TOFXPHHLEHT)
Description
RBSP RBSPICE TOF x PH Hydrogen Rates converted into units of physical intensity
(counts/(s*sr*cm^2*MeV) measured at low energy resolution and high time
resolution.
For more information regarding this data and the RBSPICE science
goals and mission statement see the RBSPICE team web site at: http:// 
rbspice.ftecs.com.
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3-PAP_ESRHELT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/PAP/ESRHELT/PT10.9S)
Description
rbspa rbspice high energy res low time res electron energy intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3-PAP_ESRLEHT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/PAP/ESRLEHT/PT10.9S)
Description
rbspa rbspice low energy res high time res electron energy intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3-PAP_TOFXEH (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/PAP/TOFXEH/PT10.9S)
Description
rbspice high energy res low time res tofxe proton intensities/pressures sorted
by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
Version 2.0 Skeleton Produced October 1, 2015
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3-PAP_TOFXEHE (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/PAP/TOFXEHE/PT10.9S)
Description
rbspa rbspice high energy res low time res tofxe helium intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3-PAP_TOFXEHE-0 (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/PAP/TOFXEHE-0/PT10.9S)
Description
rbspa rbspice high energy res low time res tofxe helium intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3-PAP_TOFXEION (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/PAP/TOFXEION/PT10.9S)
Description
rbspa rbspice high energy res low time res tofxe ion(proton)
intensities/pressures sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced August 5, 2015
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3-PAP_TOFXEO (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/PAP/TOFXEO/PT10.9S)
Description
rbspa rbspice high energy res low time res tofxe oxygen intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3-PAP_TOFXEO-0 (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/PAP/TOFXEO-0/PT10.9S)
Description
rbspa rbspice high energy res low time res tofxe oxygen intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3-PAP_TOFXPHHHELT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/PAP/TOFXPHHHELT/PT10.9S)
Description
rbspa rbspice high energy res low time res tofxph proton intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3-PAP_TOFXPHHLEHT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/PAP/TOFXPHHLEHT/PT10.9S)
Description
rbspa rbspice low energy res high time res tofxph proton intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3-PAP_TOFXPHOHELT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/PAP/TOFXPHOHELT/PT10.9S)
Description
rbspa rbspice high energy res low time res tofxph oxygen intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3-PAP_TOFXPHOLEHT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/PAP/TOFXPHOLEHT/PT10.9S)
Description
rbspa rbspice low energy res high time res tofxph oxygen intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3_ESRHELT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/ESRHELT)
Description
RBSPA RBSPICE High Energy Res Low Time Res Electron Intensities with Pitch
Angles converted into units of physical intensity (counts/(s*sr*cm^2*MeV)
measured at high energy resolution and low time resolution which includes
RBSPICE Pitch angle and Magnetic Field derived values. \n For more information
regarding this data and the RBSPICE science goals and mission statement see the
RBSPICE team web site at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3_ESRLEHT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/ESRLEHT)
Description
RBSPA RBSPICE Low Energy Res High Time Res Electron Intensities with Pitch
Angles converted into units of physical intensity (counts/(s*sr*cm^2*MeV)
measured at high energy resolution and low time resolution which includes
RBSPICE Pitch angle and Magnetic Field derived values. \n For more information
regarding this data and the RBSPICE science goals and mission statement see the
RBSPICE team web site at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3_ISRHELT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/ISRHELT)
Description
RBSPA RBSPICE High Energy Res Low Time Res Ion Energy Intensities with Pitch
Angles converted into units of physical intensity (counts/(s*sr*cm^2*MeV)
measured at high energy resolution and low time resolution which includes
RBSPICE Pitch angle and Magnetic Field derived values. \n For more information
regarding this data and the RBSPICE science goals and mission statement see the
RBSPICE team web site at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3_TOFXEH (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/TOFXEH)
Description
RBSPA RBSPICE High Energy Res Low Time Res TOFxE Proton Intensities with Pitch
Angles converted into units of physical intensity (counts/(s*sr*cm^2*MeV)
measured at high energy resolution and low time resolution which includes
RBSPICE Pitch angle and Magnetic Field derived values. \n For more information
regarding this data and the RBSPICE science goals and mission statement see the
RBSPICE team web site at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3_TOFXEION (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/TOFXEION)
Description
RBSPA RBSPICE High Energy Res Low Time Res TOFxE Ion Intensities with Pitch
Angles converted into units of physical intensity (counts/(s*sr*cm^2*MeV)
measured at high energy resolution and low time resolution which includes
RBSPICE Pitch angle and Magnetic Field derived values. \n For more information
regarding this data and the RBSPICE science goals and mission statement see the
RBSPICE team web site at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3_TOFXENONH (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/TOFXENONH)
Description
RBSPA RBSPICE High Energy Res Low Time Res TOFxE non Proton Intensities with
Pitch Angles converted into units of physical intensity (counts/(s*sr*cm^2*MeV)
measured at high energy resolution and low time resolution which includes
RBSPICE Pitch angle and Magnetic Field derived values. \n For more information
regarding this data and the RBSPICE science goals and mission statement see the
RBSPICE team web site at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3_TOFXPHHHELT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/TOFXPHHHELT)
Description
RBSPA RBSPICE High Energy Res Low Time Res TOFxPH Proton Intensities with Pitch
Angles converted into units of physical intensity (counts/(s*sr*cm^2*MeV)
measured at high energy resolution and low time resolution which includes
RBSPICE Pitch angle and Magnetic Field derived values. \n For more information
regarding this data and the RBSPICE science goals and mission statement see the
RBSPICE team web site at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3_TOFXPHHLEHT (spase://NASA/NumericalData/RBSP/A/RBSPICE/L3/TOFXPHHLEHT)
Description
RBSPA RBSPICE Low Energy Res High Time Res TOFxPH Proton Rates converted into
units of physical intensity (counts/(s*sr*cm^2*MeV) measured at high energy
resolution and low time resolution which includes RBSPICE Pitch angle and
Magnetic Field derived values. \n For more information regarding this data and
the RBSPICE science goals and mission statement see the RBSPICE team web site
at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-A_DENSITY_EMFISIS-L4 (spase://NASA/NumericalData/RBSP/A/EMFISIS/WFR/L4/ElectronDensity/PT0.5S)
Description
Density and other parameters inferred by digitizing the trace on the
spectrograms.
 
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RBSP-A_HFR-SPECTRA-BURST_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/A/EMFISIS/HFR/L2/SPECTRA-BURST/PT6S)
Description
Single Axis AC Electric Field Spectra (Selectable between the U, V and W Axis).
Frequency range: 10 kHz to 486.97kHz    (Band width:480 Hz to 23.231kHz). 82
logarithmically spaced frequency bins. Cadence: 1 spectral matrix per 6 seconds.
 
Dataset in CDAWeb
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RBSP-A_HFR-SPECTRA-MERGED_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/A/EMFISIS/HFR/L2/SPECTRA-MERGED/PT6S)
Description
Single Axis AC Electric Field Spectra (Selectable between the U, V and W Axis).
Frequency range: 10 kHz to 486.97kHz    (Band width:480 Hz to 23.231kHz). 82
logarithmically spaced frequency bins. Cadence: 1 spectral matrix per 6 seconds.
 
Dataset in CDAWeb
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RBSP-A_HFR-SPECTRA_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/A/EMFISIS/HFR/L2/SPECTRA/PT6S)
Description
Single Axis AC Electric Field Spectra (Selectable between the U, V and W Axis).
Frequency range: 10 kHz to 486.97kHz    (Band width:480 Hz to 23.231kHz). 82
logarithmically spaced frequency bins. Cadence: 1 spectral matrix per 6 seconds.
 
Dataset in CDAWeb
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RBSP-A_HFR-WAVEFORM_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/A/EMFISIS/HFR/L2/WAVEFORM)
Description
Single Axis AC Electric Field Waveform (Selectable between the U, V and W Axis).
Units: V/m. Sample Rate: 1 Msample/sec. Sample Size: 4096 samples. Cadence:
variable.
 
Dataset in CDAWeb
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RBSP-A_MAGNETOMETER_1SEC-GEI_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/A/EMFISIS/MAGNETOMETER/L3/GEI/PT1S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-A_MAGNETOMETER_1SEC-GEO_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/A/EMFISIS/MAGNETOMETER/L3/GEO/PT1S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-A_MAGNETOMETER_1SEC-GSE_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/A/EMFISIS/MAGNETOMETER/L3/GSE/PT1S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-A_MAGNETOMETER_1SEC-GSM_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/A/EMFISIS/MAGNETOMETER/L3/GSM/PT1S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-A_MAGNETOMETER_1SEC-SM_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/A/EMFISIS/MAGNETOMETER/L3/SM/PT1S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-A_MAGNETOMETER_4SEC-GEI_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/A/EMFISIS/MAGNETOMETER/L3/GEI/PT4S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-A_MAGNETOMETER_4SEC-GEO_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/A/EMFISIS/MAGNETOMETER/L3/GEO/PT4S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-A_MAGNETOMETER_4SEC-GSE_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/A/EMFISIS/MAGNETOMETER/L3/GSE/PT4S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-A_MAGNETOMETER_4SEC-GSM_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/A/EMFISIS/MAGNETOMETER/L3/GSM/PT4S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-A_MAGNETOMETER_4SEC-SM_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/A/EMFISIS/MAGNETOMETER/L3/SM/PT4S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-A_MAGNETOMETER_HIRES-GEI_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/A/EMFISIS/MAGNETOMETER/L3/GEI/PT0.015625S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-A_MAGNETOMETER_HIRES-GEO_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/A/EMFISIS/MAGNETOMETER/L3/GEO/PT0.015625S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-A_MAGNETOMETER_HIRES-GSE_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/A/EMFISIS/MAGNETOMETER/L3/GSE/PT0.015625S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-A_MAGNETOMETER_HIRES-GSM_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/A/EMFISIS/MAGNETOMETER/L3/GSM/PT0.015625S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-A_MAGNETOMETER_HIRES-SM_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/A/EMFISIS/MAGNETOMETER/L3/SM/PT0.015625S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-A_WFR-SPECTRAL-MATRIX-DIAGONAL-MERGED_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/A/EMFISIS/WFR/L2/SPECTRAL-MATRIX-DIAGONAL-MERGED/PT6S)
Description
Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV,
BW)  cross spectral matrix,  6 diagonal components and 15 off-diagonal
components.Frequency range: 10 kHz to 487kHz..82 Frequency Bins.Cadence: 1
spectra per 6 seconds (survey).
 
Dataset in CDAWeb
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RBSP-A_WFR-SPECTRAL-MATRIX-DIAGONAL_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/A/EMFISIS/WFR/L2/SPECTRAL-MATRIX-DIAGONAL/PT6S)
Description
Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV,
BW)  cross spectral matrix,  6 diagonal components and 15 off-diagonal
components.Frequency range: 10 kHz to 487kHz..82 Frequency Bins.Cadence: 1
spectra per 6 seconds (survey).
 
Dataset in CDAWeb
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RBSP-A_WFR-SPECTRAL-MATRIX_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/A/EMFISIS/WFR/L2/SPECTRAL-MATRIX/PT6S)
Description
Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV,
BW)  cross spectral matrix,  6 diagonal components and 15 off-diagonal
components.Frequency range: 10 kHz to 487kHz..82 Frequency Bins.Cadence: 1
spectra per 6 seconds (survey).
 
Dataset in CDAWeb
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RBSP-A_WFR-WAVEFORM-CONTINUOUS-BURST_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/A/EMFISIS/WFR/L2/WaveformContinuousBurst/PT6S)
Description
Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV,
BW)  continuous burst waveforms208896 samples @ 35 kS/sec...Calibration
Notes:.Warning: All L2 Waveform products are calibrated in amplitude at 1kHz
only.  There is no phase calibration applied at this stage...Before using these
waveforms to process wave parameters, please follow the calibration process
described below or the results will be wrong...Level-2 (L2) Waveform data is
amplitude-calibrated at 1 kHz.  But there are amplitude deviations at other
frequencies, and there are phase shifts which are not reflected in the L2 data
at all. The phase shift is a frequency-dependent shift in the phase of the
observed wave relative to the input wave, tantamount to a time delay at that
frequency. . .The L2 data can be adjusted over frequency by applying
dimensionless complex factors over frequency immediately after Fourier
transforming the L2 data. The Variables BCalibrationCoef and ECalibration Coef
in the cdf consists of a table for the B sensors and a table for the E sensors.
Each table has 5600 X 2 entries. The  first column is the real component and the
second is the imaginary component of the calibration, extending from 2.13623 to
11962.89 Hz, in steps of 2.13623 Hz  (Variable: CalFrequencies contains the
associated frequencies of the calibration coeficients). Above the highest
frequency the WFR filters roll off; no calibration measurements exist, but one
could apply the last value to any frequencies above that.. .The table is
constructed assuming 16384 data points are to be FFT'ed. If fewer than that are
to be transformed, then the table can be decimated to accommodate a shorter data
set. The procedure is;  FFT the L2 data at the desired resolution and then
perform a complex multiplication of the FFT'ed dataset  and the E or B
adjustment table.. .If comparing results of the frequency-adjusted L2 data with
the onboard survey spectra, note that the L2 data has units of volts/meter and
nanoTesla for E and B respectively, whereas the onboard survey spectra have
units of RMS volts/meter and RMS nanoTesla.. 
 
Dataset in CDAWeb
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RBSP-A_WFR-WAVEFORM_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/A/EMFISIS/WFR/L2/WAVEFORM/PT6S)
Description
Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV,
BW)  waveforms16384 samples @ 35 kS/sec...Calibration Notes:.Warning: All L2
Waveform products are calibrated in amplitude at 1kHz only.  There is no phase
calibration applied at this stage...Before using these waveforms to process wave
parameters, please follow the calibration process described below or the results
will be wrong...Level-2 (L2) Waveform data is amplitude-calibrated at 1 kHz. 
But there are amplitude deviations at other frequencies, and there are phase
shifts which are not reflected in the L2 data at all. The phase shift is a
frequency-dependent shift in the phase of the observed wave relative to the
input wave, tantamount to a time delay at that frequency. . .The L2 data can be
adjusted over frequency by applying dimensionless complex factors over frequency
immediately after Fourier transforming the L2 data. The Variables
BCalibrationCoef and ECalibration Coef in the cdf consists of a table for the B
sensors and a table for the E sensors. Each table has 5600 X 2 entries. The 
first column is the real component and the second is the imaginary component of
the calibration, extending from 2.13623 to 11962.89 Hz, in steps of 2.13623 Hz 
(Variable: CalFrequencies contains the associated frequencies of the calibration
coeficients). Above the highest frequency the WFR filters roll off; no
calibration measurements exist, but one could apply the last value to any
frequencies above that.. .The table is constructed assuming 16384 data points
are to be FFT'ed. If fewer than that are to be transformed, then the table can
be decimated to accommodate a shorter data set. The procedure is;  FFT the L2
data at the desired resolution and then perform a complex multiplication of the
FFT'ed dataset  and the E or B adjustment table.. .If comparing results of the
frequency-adjusted L2 data with the onboard survey spectra, note that the L2
data has units of volts/meter and nanoTesla for E and B respectively, whereas
the onboard survey spectra have units of RMS volts/meter and RMS nanoTesla.. 
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-2_ESRHELT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L2/ESRHELT)
Description
RBSP RBSPICE High Energy Resolution Electron Rates converted into units of
physical intensity (counts/(s*sr*cm^2*MeV) measured at high energy resolution
and low time resolution.
For more information regarding this data and the
RBSPICE science goals and mission statement see the RBSPICE team web site at:
http:// rbspice.ftecs.com.
Modification History
Skeleton Produced June 6, 2012
Level 1.3 version produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-2_ESRLEHT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L2/ESRLEHT)
Description
RBSP RBSPICE Low Energy Resolution Electron Rates converted into units of
physical intensity (counts/(s*sr*cm^2*MeV) measured at high energy resolution
and low time resolution.
For more information regarding this data and the
RBSPICE science goals and mission statement see the RBSPICE team web site at:
http:// rbspice.ftecs.com.
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-2_ISRHELT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L2/ISRHELT)
Description
RBSP RBSPICE high energy resolution Ion Species Rates (ISRHELT) converted into
units of physical intensity (counts/(s*sr*cm^2*MeV) measured at high energy
resolution and low time resolution.
For more information regarding this data and
the RBSPICE science goals and mission statement see the RBSPICE team web site
at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-2_TOFXEH (spase://NASA/NumericalData/RBSP/B/RBSPICE/L2/TOFXEH)
Description
RBSP RBSPICE TOF x Energy Hydrogen Rates converted into units of physical
intensity (counts/(s*sr*cm^2*MeV) measured at high energy resolution and low
time resolution.
For more information regarding this data and the RBSPICE
science goals and mission statement see the RBSPICE team web site at: http:// 
rbspice.ftecs.com.
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-2_TOFXEION (spase://NASA/NumericalData/RBSP/B/RBSPICE/L2/TOFXEION)
Description
RBSP RBSPICE TOF x Energy Ion Rates converted into units of physical intensity
(counts/(s*sr*cm^2*MeV) measured at high energy resolution and low time
resolution.
For more information regarding this data and the RBSPICE science
goals and mission statement see the RBSPICE team web site at: http:// 
rbspice.ftecs.com.
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-2_TOFXENONH (spase://NASA/NumericalData/RBSP/B/RBSPICE/L2/TOFXENONH)
Description
RBSP RBSPICE TOF x E non Hydrogen (Helium and Oxygen) Rates converted into units
of physical intensity (counts/(s*sr*cm^2*MeV) measured at high energy resolution
and low time resolution.
For more information regarding this data and the
RBSPICE science goals and mission statement see the RBSPICE team web site at:
http:// rbspice.ftecs.com.
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-2_TOFXPHHHELT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L2/TOFXPHHHELT)
Description
RBSP RBSPICE TOF x PH Hydrogen Rates converted into units of physical intensity
(counts/(s*sr*cm^2*MeV) measured at high energy resolution and low time
resolution.
For more information regarding this data and the RBSPICE science
goals and mission statement see the RBSPICE team web site at: http:// 
rbspice.ftecs.com.
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-2_TOFXPHHLEHT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L2/TOFXPHHLEHT)
Description
RBSP RBSPICE TOF x PH Hydrogen Rates converted into units of physical intensity
(counts/(s*sr*cm^2*MeV) measured at low energy resolution and high time
resolution.
For more information regarding this data and the RBSPICE science
goals and mission statement see the RBSPICE team web site at: http:// 
rbspice.ftecs.com.
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3-PAP_ESRHELT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/PAP/ESRHELT/PT10.9S)
Description
rbspb rbspice high energy res low time res electron energy intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3-PAP_ESRLEHT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/PAP/ESRLEHT/PT10.9S)
Description
rbspb rbspice low energy res high time res electron energy intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3-PAP_TOFXEH (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/PAP/TOFXEH/PT10.9S)
Description
rbspice high energy res low time res tofxe proton intensities/pressures sorted
by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
Version 2.0 Skeleton Produced October 1, 2015
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3-PAP_TOFXEHE (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/PAP/TOFXEHE/PT10.9S)
Description
rbspb rbspice high energy res low time res tofxe helium intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3-PAP_TOFXEHE-0 (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/PAP/TOFXEHE-0/PT10.9S)
Description
rbspb rbspice high energy res low time res tofxe helium intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3-PAP_TOFXEION (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/PAP/TOFXEION/PT10.9S)
Description
rbspb rbspice high energy res low time res tofxe ion(proton)
intensities/pressures sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced August 5, 2015
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3-PAP_TOFXEO (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/PAP/TOFXEO/PT10.9S)
Description
rbspb rbspice high energy res low time res tofxe oxygen intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3-PAP_TOFXEO-0 (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/PAP/TOFXEO-0/PT10.9S)
Description
rbspb rbspice high energy res low time res tofxe oxygen intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3-PAP_TOFXPHHHELT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/PAP/TOFXPHHHELT/PT10.9S)
Description
rbspb rbspice high energy res low time res tofxph proton intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3-PAP_TOFXPHHLEHT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/PAP/TOFXPHHLEHT/PT10.9S)
Description
rbspb rbspice low energy res high time res tofxph proton intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3-PAP_TOFXPHOHELT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/PAP/TOFXPHOHELT/PT10.9S)
Description
rbspb rbspice high energy res low time res tofxph oxygen intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3-PAP_TOFXPHOLEHT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/PAP/TOFXPHOLEHT/PT10.9S)
Description
rbspb rbspice low energy res high time res tofxph oxygen intensities/pressures
sorted by pitch angles.
Modification History
Version 1.0 Skeleton Produced July 29, 2014
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3_ESRHELT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/ESRHELT)
Description
RBSPB RBSPICE High Energy Res Low Time Res Electron Intensities with Pitch
Angles converted into units of physical intensity (counts/(s*sr*cm^2*MeV)
measured at high energy resolution and low time resolution which includes
RBSPICE Pitch angle and Magnetic Field derived values. \n For more information
regarding this data and the RBSPICE science goals and mission statement see the
RBSPICE team web site at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Level 1.3 version produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3_ESRLEHT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/ESRLEHT)
Description
RBSPB RBSPICE Low Energy Res High Time Res Electron Intensities with Pitch
Angles converted into units of physical intensity (counts/(s*sr*cm^2*MeV)
measured at high energy resolution and low time resolution which includes
RBSPICE Pitch angle and Magnetic Field derived values. \n For more information
regarding this data and the RBSPICE science goals and mission statement see the
RBSPICE team web site at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3_ISRHELT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/ISRHELT)
Description
RBSPB RBSPICE High Energy Res Low Time Res Ion Energy Intensities with Pitch
Angles converted into units of physical intensity (counts/(s*sr*cm^2*MeV)
measured at high energy resolution and low time resolution which includes
RBSPICE Pitch angle and Magnetic Field derived values. \n For more information
regarding this data and the RBSPICE science goals and mission statement see the
RBSPICE team web site at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3_TOFXEH (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/TOFXEH)
Description
RBSPB RBSPICE High Energy Res Low Time Res TOFxE Proton Intensities with Pitch
Angles converted into units of physical intensity (counts/(s*sr*cm^2*MeV)
measured at high energy resolution and low time resolution which includes
RBSPICE Pitch angle and Magnetic Field derived values. \n For more information
regarding this data and the RBSPICE science goals and mission statement see the
RBSPICE team web site at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3_TOFXEION (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/TOFXEION)
Description
RBSPB RBSPICE High Energy Res Low Time Res TOFxE Ion Intensities with Pitch
Angles converted into units of physical intensity (counts/(s*sr*cm^2*MeV)
measured at high energy resolution and low time resolution which includes
RBSPICE Pitch angle and Magnetic Field derived values. \n For more information
regarding this data and the RBSPICE science goals and mission statement see the
RBSPICE team web site at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3_TOFXENONH (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/TOFXENONH)
Description
RBSPB RBSPICE High Energy Res Low Time Res TOFxE non Proton Intensities with
Pitch Angles converted into units of physical intensity (counts/(s*sr*cm^2*MeV)
measured at high energy resolution and low time resolution which includes
RBSPICE Pitch angle and Magnetic Field derived values. \n For more information
regarding this data and the RBSPICE science goals and mission statement see the
RBSPICE team web site at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3_TOFXPHHHELT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/TOFXPHHHELT)
Description
RBSPB RBSPICE High Energy Res Low Time Res TOFxPH Proton Intensities with Pitch
Angles converted into units of physical intensity (counts/(s*sr*cm^2*MeV)
measured at high energy resolution and low time resolution which includes
RBSPICE Pitch angle and Magnetic Field derived values. \n For more information
regarding this data and the RBSPICE science goals and mission statement see the
RBSPICE team web site at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3_TOFXPHHLEHT (spase://NASA/NumericalData/RBSP/B/RBSPICE/L3/TOFXPHHLEHT)
Description
RBSPB RBSPICE Low Energy Res High Time Res TOFxPH Proton Rates converted into
units of physical intensity (counts/(s*sr*cm^2*MeV) measured at high energy
resolution and low time resolution which includes RBSPICE Pitch angle and
Magnetic Field derived values. \n For more information regarding this data and
the RBSPICE science goals and mission statement see the RBSPICE team web site
at: http:// rbspice.ftecs.com. 
Modification History
Skeleton Produced June 6, 2012
Version 1.3 produced December 20, 2012
L
 
Dataset in CDAWeb
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RBSP-B_DENSITY_EMFISIS-L4 (spase://NASA/NumericalData/RBSP/B/EMFISIS/WFR/L4/ElectronDensity/PT0.5S)
Description
Density and other parameters inferred by digitizing the trace on the
spectrograms.
 
Dataset in CDAWeb
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RBSP-B_HFR-SPECTRA-BURST_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/B/EMFISIS/HFR/L2/SPECTRA-BURST/PT6S)
Description
Single Axis AC Electric Field Spectra (Selectable between the U, V and W Axis).
Frequency range: 10 kHz to 486.97kHz    (Band width:480 Hz to 23.231kHz). 82
logarithmically spaced frequency bins. Cadence: 1 spectral matrix per 6 seconds.
 
Dataset in CDAWeb
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RBSP-B_HFR-SPECTRA-MERGED_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/B/EMFISIS/HFR/L2/SPECTRA-MERGED/PT6S)
Description
Single Axis AC Electric Field Spectra (Selectable between the U, V and W Axis).
Frequency range: 10 kHz to 486.97kHz    (Band width:480 Hz to 23.231kHz). 82
logarithmically spaced frequency bins. Cadence: 1 spectral matrix per 6 seconds.
 
Dataset in CDAWeb
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RBSP-B_HFR-SPECTRA_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/B/EMFISIS/HFR/L2/SPECTRA/PT6S)
Description
Single Axis AC Electric Field Spectra (Selectable between the U, V and W Axis).
Frequency range: 10 kHz to 486.97kHz    (Band width:480 Hz to 23.231kHz). 82
logarithmically spaced frequency bins. Cadence: 1 spectral matrix per 6 seconds.
 
Dataset in CDAWeb
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RBSP-B_HFR-WAVEFORM_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/B/EMFISIS/HFR/L2/WAVEFORM)
Description
Single Axis AC Electric Field Waveform (Selectable between the U, V and W Axis).
Units: V/m. Sample Rate: 1 Msample/sec. Sample Size: 4096 samples. Cadence:
variable.
 
Dataset in CDAWeb
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RBSP-B_MAGNETOMETER_1SEC-GEI_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/B/EMFISIS/MAGNETOMETER/L3/GEI/PT1S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-B_MAGNETOMETER_1SEC-GEO_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/B/EMFISIS/MAGNETOMETER/L3/GEO/PT1S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-B_MAGNETOMETER_1SEC-GSE_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/B/EMFISIS/MAGNETOMETER/L3/GSE/PT1S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-B_MAGNETOMETER_1SEC-GSM_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/B/EMFISIS/MAGNETOMETER/L3/GSM/PT1S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-B_MAGNETOMETER_1SEC-SM_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/B/EMFISIS/MAGNETOMETER/L3/SM/PT1S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-B_MAGNETOMETER_4SEC-GEI_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/B/EMFISIS/MAGNETOMETER/L3/GEI/PT4S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-B_MAGNETOMETER_4SEC-GEO_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/B/EMFISIS/MAGNETOMETER/L3/GEO/PT4S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-B_MAGNETOMETER_4SEC-GSE_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/B/EMFISIS/MAGNETOMETER/L3/GSE/PT4S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-B_MAGNETOMETER_4SEC-GSM_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/B/EMFISIS/MAGNETOMETER/L3/GSM/PT4S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-B_MAGNETOMETER_4SEC-SM_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/B/EMFISIS/MAGNETOMETER/L3/SM/PT4S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-B_MAGNETOMETER_HIRES-GEI_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/B/EMFISIS/MAGNETOMETER/L3/GEI/PT0.015625S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-B_MAGNETOMETER_HIRES-GEO_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/B/EMFISIS/MAGNETOMETER/L3/GEO/PT0.015625S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-B_MAGNETOMETER_HIRES-GSE_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/B/EMFISIS/MAGNETOMETER/L3/GSE/PT0.015625S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-B_MAGNETOMETER_HIRES-GSM_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/B/EMFISIS/MAGNETOMETER/L3/GSM/PT0.015625S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-B_MAGNETOMETER_HIRES-SM_EMFISIS-L3 (spase://NASA/NumericalData/RBSP/B/EMFISIS/MAGNETOMETER/L3/SM/PT0.015625S)
Description
3 axis Fluxgate Magnetometer data.  Sampled onboard at 64 vectors per second.  3
range states available,  Range 0 (+/- 256 nT),  Range 1 (+/- 4096 nT), Range 3
(+/- 65536 nT).
 
Dataset in CDAWeb
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RBSP-B_WFR-SPECTRAL-MATRIX-DIAGONAL-MERGED_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/B/EMFISIS/WFR/L2/SPECTRAL-MATRIX-DIAGONAL-MERGED/PT6S)
Description
Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV,
BW)  cross spectral matrix,  6 diagonal components and 15 off-diagonal
components.Frequency range: 10 kHz to 487kHz..82 Frequency Bins.Cadence: 1
spectra per 6 seconds (survey).
 
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RBSP-B_WFR-SPECTRAL-MATRIX-DIAGONAL_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/B/EMFISIS/WFR/L2/SPECTRAL-MATRIX-DIAGONAL/PT6S)
Description
Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV,
BW)  cross spectral matrix,  6 diagonal components and 15 off-diagonal
components.Frequency range: 10 kHz to 487kHz..82 Frequency Bins.Cadence: 1
spectra per 6 seconds (survey).
 
Dataset in CDAWeb
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RBSP-B_WFR-SPECTRAL-MATRIX_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/B/EMFISIS/WFR/L2/SPECTRAL-MATRIX/PT6S)
Description
Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV,
BW)  cross spectral matrix,  6 diagonal components and 15 off-diagonal
components.Frequency range: 10 kHz to 487kHz..82 Frequency Bins.Cadence: 1
spectra per 6 seconds (survey).
 
Dataset in CDAWeb
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RBSP-B_WFR-WAVEFORM-CONTINUOUS-BURST_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/B/EMFISIS/WFR/L2/WAVEFORM-CONTINUOUS-BURST/PT6S)
Description
Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV,
BW)  continuous burst waveforms208896 samples @ 35 kS/sec...Calibration
Notes:.Warning: All L2 Waveform products are calibrated in amplitude at 1kHz
only.  There is no phase calibration applied at this stage...Before using these
waveforms to process wave parameters, please follow the calibration process
described below or the results will be wrong...Level-2 (L2) Waveform data is
amplitude-calibrated at 1 kHz.  But there are amplitude deviations at other
frequencies, and there are phase shifts which are not reflected in the L2 data
at all. The phase shift is a frequency-dependent shift in the phase of the
observed wave relative to the input wave, tantamount to a time delay at that
frequency. . .The L2 data can be adjusted over frequency by applying
dimensionless complex factors over frequency immediately after Fourier
transforming the L2 data. The Variables BCalibrationCoef and ECalibration Coef
in the cdf consists of a table for the B sensors and a table for the E sensors.
Each table has 5600 X 2 entries. The  first column is the real component and the
second is the imaginary component of the calibration, extending from 2.13623 to
11962.89 Hz, in steps of 2.13623 Hz  (Variable: CalFrequencies contains the
associated frequencies of the calibration coeficients). Above the highest
frequency the WFR filters roll off; no calibration measurements exist, but one
could apply the last value to any frequencies above that.. .The table is
constructed assuming 16384 data points are to be FFT'ed. If fewer than that are
to be transformed, then the table can be decimated to accommodate a shorter data
set. The procedure is;  FFT the L2 data at the desired resolution and then
perform a complex multiplication of the FFT'ed dataset  and the E or B
adjustment table.. .If comparing results of the frequency-adjusted L2 data with
the onboard survey spectra, note that the L2 data has units of volts/meter and
nanoTesla for E and B respectively, whereas the onboard survey spectra have
units of RMS volts/meter and RMS nanoTesla.. 
 
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RBSP-B_WFR-WAVEFORM_EMFISIS-L2 (spase://NASA/NumericalData/RBSP/B/EMFISIS/WFR/L2/WAVEFORM/PT6S)
Description
Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV,
BW)  waveforms16384 samples @ 35 kS/sec...Calibration Notes:.Warning: All L2
Waveform products are calibrated in amplitude at 1kHz only.  There is no phase
calibration applied at this stage...Before using these waveforms to process wave
parameters, please follow the calibration process described below or the results
will be wrong...Level-2 (L2) Waveform data is amplitude-calibrated at 1 kHz. 
But there are amplitude deviations at other frequencies, and there are phase
shifts which are not reflected in the L2 data at all. The phase shift is a
frequency-dependent shift in the phase of the observed wave relative to the
input wave, tantamount to a time delay at that frequency. . .The L2 data can be
adjusted over frequency by applying dimensionless complex factors over frequency
immediately after Fourier transforming the L2 data. The Variables
BCalibrationCoef and ECalibration Coef in the cdf consists of a table for the B
sensors and a table for the E sensors. Each table has 5600 X 2 entries. The 
first column is the real component and the second is the imaginary component of
the calibration, extending from 2.13623 to 11962.89 Hz, in steps of 2.13623 Hz 
(Variable: CalFrequencies contains the associated frequencies of the calibration
coeficients). Above the highest frequency the WFR filters roll off; no
calibration measurements exist, but one could apply the last value to any
frequencies above that.. .The table is constructed assuming 16384 data points
are to be FFT'ed. If fewer than that are to be transformed, then the table can
be decimated to accommodate a shorter data set. The procedure is;  FFT the L2
data at the desired resolution and then perform a complex multiplication of the
FFT'ed dataset  and the E or B adjustment table.. .If comparing results of the
frequency-adjusted L2 data with the onboard survey spectra, note that the L2
data has units of volts/meter and nanoTesla for E and B respectively, whereas
the onboard survey spectra have units of RMS volts/meter and RMS nanoTesla.. 
 
Dataset in CDAWeb
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RBSPA_EFW-L2_E-HIRES-UVW (spase://NASA/NumericalData/RBSP/A/EFW/L2/UVW/Hires)
Description
CDAWeb interface derived data on Fri Jun 14 15:33:16 EDT 2013. Contacts: 
Tami.J.Kovalick@nasa.gov, Rita.C.Johnson@nasa.gov. High Resolution DC Electric
Field in UVW Coordinates.
Modification History
v01:  initial version.
 
Dataset in CDAWeb
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RBSPA_EFW-L2_E-SPINFIT-MGSE (spase://NASA/NumericalData/RBSP/A/EFW/L2/MGSE/PT11S)
Description
CDAWeb interface derived data on Fri Jun 14 15:33:16 EDT 2013. Contacts: 
Tami.J.Kovalick@nasa.gov, Rita.C.Johnson@nasa.gov. Spinfit DC electric field
estimates in the M-GSE coordinate system - see the EFW-FAQ
(http://rbsp.space.umn.edu/efw_faq.html) for a description of the spin fit 
algorithm and the M-GSE coordinate system.
One 2D vector estimate of the E-field is computed at a cadence of once per spin
period (typ. 10.7 to 11.1 s) using the survey E-field data product - the
potential difference between EFW sensors V1 and V2 (E12) or V3 and V4 (E34)
sampled at a nominal rate of 32 samp/s with a resolution of 16 bits.
The X-component of the E-field estimate, corresponding to the axial component in
the spacecraft coordinate system, is set to zero in this data product.  See the
EFW-FAQ (http://rbsp.space.umn.edu/efw_faq.html) for a discussion of this 
convention for this data product.
The VxB electric field in the spacecraft frame due to orbital motion of the
spacecraft around the Earth as computed from the spacecraft orbital velocity and
measured B-field in the spacraft frame has been subtracted from the measured
electric field, and so the data product is in the quasi-inertial frame
equivalent to GSE (i.e. it is NOT in the corotation frame of the Earth!).
Each spin fit is time-tagged with the time corresponding to the middle of the
spin of data that went into the spin fit algorithm; in other words, if a given
spin covers the interval [t1, t2), then the spin fit E-field estimate associated
with that spin is given the time tag 0.5*(t1 + t2).
The root mean square residual between the data included in the fit and the
resulting best-fit model, sigma, and the final number of points included in the
spin fit, npts, are also provided at spin-period cadence.
The nominal dynamic range of the E-field estimate is +/- 1 V/m in any component.
Modification History
v01:  initial version.
 
Dataset in CDAWeb
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RBSPA_EFW-L2_ESVY_DESPUN (spase://NASA/NumericalData/RBSP/A/EFW/L2/ESVY_DESPUN/PT0.031S)
Description
CDAWeb interface derived data on Fri Jun 14 15:33:16 EDT 2013. Contacts: 
Tami.J.Kovalick@nasa.gov, Rita.C.Johnson@nasa.gov. Spinfit DC electric field
estimates in the M-GSE coordinate system - see the EFW-FAQ
(http://rbsp.space.umn.edu/efw_faq.html) for a description of the spin fit 
algorithm and the M-GSE coordinate system.
One 2D vector estimate of the E-field is computed at a cadence of once per spin
period (typ. 10.7 to 11.1 s) using the survey E-field data product - the
potential difference between EFW sensors V1 and V2 (E12) or V3 and V4 (E34)
sampled at a nominal rate of 32 samp/s with a resolution of 16 bits.
The X-component of the E-field estimate, corresponding to the axial component in
the spacecraft coordinate system, is set to zero in this data product.  See the
EFW-FAQ (http://rbsp.space.umn.edu/efw_faq.html) for a discussion of this 
convention for this data product.
The VxB electric field in the spacecraft frame due to orbital motion of the
spacecraft around the Earth as computed from the spacecraft orbital velocity and
measured B-field in the spacraft frame has been subtracted from the measured
electric field, and so the data product is in the quasi-inertial frame
equivalent to GSE (i.e. it is NOT in the corotation frame of the Earth!).
Each spin fit is time-tagged with the time corresponding to the middle of the
spin of data that went into the spin fit algorithm; in other words, if a given
spin covers the interval [t1, t2), then the spin fit E-field estimate associated
with that spin is given the time tag 0.5*(t1 + t2).
The root mean square residual between the data included in the fit and the
resulting best-fit model, sigma, and the final number of points included in the
spin fit, npts, are also provided at spin-period cadence.
The nominal dynamic range of the E-field estimate is +/- 1 V/m in any component.
Modification History
v01:  initial version.
 
Dataset in CDAWeb
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RBSPA_EFW-L2_FBK (spase://NASA/NumericalData/RBSP/A/EFW/L2/FBK/PT0.125S)
Description
Up to two sources are returned. The possible sources are:
E12DC, E34DC,E56DC,
E12AC,E34AC,E56AC,
SCMU,SCMV,SCMW
(V1DC+V2DC+V3DC+V4DC)/4
 
Dataset in CDAWeb
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RBSPA_EFW-L2_SPEC (spase://NASA/NumericalData/RBSP/A/EFW/L2/SPEC/PT4S)
Description
Six spectral products are returned. The possible sources are:
E12dc,E34dc,E56dc
E12ac,E34ac,E56ac
Edcpar,Edcprp
Eacpar,Eacprp
V1ac,V2ac,V3ac,V4ac,V5ac,V6ac
SCMU,SCMV,SCMW
SCMpar,SCMprp,
(V1dc+V2dc+V3dc+V4dc)/4,
Edcprp2, Eacprp2, SCMprp2
Caveats
See THEMIS website for caveats
 
Dataset in CDAWeb
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RBSPA_EFW-L2_VSVY-HIRES (spase://NASA/NumericalData/RBSP/A/EFW/L2/VSVY/PT1S)
Description
CDAWeb interface derived data on Fri Jun 14 15:33:16 EDT 2013. Contacts: 
Tami.J.Kovalick@nasa.gov, Rita.C.Johnson@nasa.gov. Spinfit DC electric field
estimates in the M-GSE coordinate system - see the EFW-FAQ
(http://rbsp.space.umn.edu/efw_faq.html) for a description of the spin fit 
algorithm and the M-GSE coordinate system.
One 2D vector estimate of the E-field is computed at a cadence of once per spin
period (typ. 10.7 to 11.1 s) using the survey E-field data product - the
potential difference between EFW sensors V1 and V2 (E12) or V3 and V4 (E34)
sampled at a nominal rate of 32 samp/s with a resolution of 16 bits.
The X-component of the E-field estimate, corresponding to the axial component in
the spacecraft coordinate system, is set to zero in this data product.  See the
EFW-FAQ (http://rbsp.space.umn.edu/efw_faq.html) for a discussion of this 
convention for this data product.
The VxB electric field in the spacecraft frame due to orbital motion of the
spacecraft around the Earth as computed from the spacecraft orbital velocity and
measured B-field in the spacraft frame has been subtracted from the measured
electric field, and so the data product is in the quasi-inertial frame
equivalent to GSE (i.e. it is NOT in the corotation frame of the Earth!).
Each spin fit is time-tagged with the time corresponding to the middle of the
spin of data that went into the spin fit algorithm; in other words, if a given
spin covers the interval [t1, t2), then the spin fit E-field estimate associated
with that spin is given the time tag 0.5*(t1 + t2).
The root mean square residual between the data included in the fit and the
resulting best-fit model, sigma, and the final number of points included in the
spin fit, npts, are also provided at spin-period cadence.
The nominal dynamic range of the E-field estimate is +/- 1 V/m in any component.
Modification History
v01:  initial version.
 
Dataset in CDAWeb
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RBSPA_EFW-L3 (spase://NASA/NumericalData/RBSP/A/EFW/L3/MGSE/PT11S)
Description
**********************************************************
*************PRODUCTS FOR L3 FILES*******************:
**********************************************************
Eymgse, Ez mgse, spinfit  in a co-rotational
frame (Vsc x B and Ecorotation subtracted)
Include  Vsc x B, Vcoro x B as separate variables
Include separate quality flags for charging, eclipse and biasing. 
Density from SC potential
SC potential (V1-V6)
Ex mgse (spin axis component) for "good" ratios of |Bx/Bz| and |By/Bz|,
The magnetic field ratios themselves,
L value, MLT, MLAT,  and the position of the SC in GSE.
The unit vector of the spin axis in gse coordinate system.
All quantities are at spin period resolution
Modification History
v01:  initial version; started with L1 EFW VSVY CDF, removing all L0 (e.g. CCSDS
packet header) variables, changing variable type of VSVY variable from INT to
REAL to reflect tranformation from TM to Physical units; added variables for
average of opposing sensors, VSVY_AVG; added variable for sensor potential
quality flag, VSVY_QUAL. Added EFW data quality flag array.
 
Dataset in CDAWeb
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RBSPA_EFW_BURST-WAVEFORM-UVW-L1 (spase://NASA/NumericalData/RBSP/A/EFW/L1/B1/UVW/PT0.00195S)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPA_L1_EB1 (spase://NASA/NumericalData/RBSP/A/EFW/L1/B1/UVW/ElectricField/PT0.00195S)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPA_L1_EB2 (spase://NASA/NumericalData/RBSP/A/EFW/L1/B2/UVW/ElectricField/PT0.00006S)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPA_L1_MSCB1 (spase://NASA/NumericalData/RBSP/A/EFW/L1/B1/UVW/SearchCoilMagneticField/PT0.00195S)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPA_L1_MSCB2 (spase://NASA/NumericalData/RBSP/A/EFW/L1/B2/UVW/SearchCoilMagneticField/PT0.00006S)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPA_L1_VB1 (spase://NASA/NumericalData/RBSP/A/EFW/L1/B1/UVW/ElectricPotential/PT0.00195S)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPA_L1_VB2 (spase://NASA/NumericalData/RBSP/A/EFW/L1/B2/UVW/ElectricPotential/PT0.00006S)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPA_L2-1MIN_PSBR-RPS (spase://NASA/NumericalData/RBSP/A/RPS/L2/PT1M)
Description
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, Dr.
Joe Mazur, can be reached at Joseph.E.Mazur@aero.org.
Modification History
TBD
 
Dataset in CDAWeb
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RBSPA_L2_PSBR-RPS (spase://NASA/NumericalData/RBSP/A/RPS/L2/PT0.058S)
Description
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, Dr.
Joe Mazur, can be reached at Joseph.E.Mazur@aero.org.
Modification History
TBD
 
Dataset in CDAWeb
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RBSPA_REL03_ECT-MAGEIS-L2 (spase://NASA/NumericalData/RBSP/A/ECT/MagEIS/L2/Sectors/Release03/PT10.9S)
Description
MagEIS consists of 4 energetic particle sensors per RBSP spacecraft: low unit,
medium35 unit, medium75 unit and the high unit.  The low and 2 medium units are
magnetic spectrometers that measure electrons across roughly the 20 keV - 1 MeV
energy range. The high unit contains a magnetic spectrometer that measures
electrons from roughly the 700 keV to 4 MeV range. The high unit also has a
proton telescope that measures protons from roughly 50 keV to 20 MeV, Helium
ions from roughly 300 keV - 1.5 MeV and Oxygen ions from roughly 1-5 MeV. 
MagEIS is one of three instrument packages on the ECT instrument suite (HOPE and
REPT are the others).
 
Dataset in CDAWeb
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RBSPA_REL03_ECT-REPT-SCI-L2 (spase://NASA/NumericalData/RBSP/A/ECT/REPT/L2/Sectors/Release03/PT4.2S)
Description
RBSP Relativistic Electron Proton Telescope, Level 2 science data
Modification History
CDF skeleton version of rbsp_rept_science_l2_data.template.cdf written by R.
Reukauf
 
Dataset in CDAWeb
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RBSPA_REL03_ECT-REPT-SCI-L3 (spase://NASA/NumericalData/RBSP/A/ECT/REPT/L3/Sectors/Release03/PT4.2S)
Description
Van Allen Probes, RBSPECT/REPT (Radiation Belt Storm Probes Energetic particle,
Composition and Thermal plasma suite/Relativistic Electron Proton Telescope,
Level 3 Pitch Angle Sorted Data.
 
Dataset in CDAWeb
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RBSPA_REL04_ECT-HOPE-MOM-L3 (spase://NASA/NumericalData/RBSP/A/ECT/HOPE/L3/Moments/Release04/PT24.35S)
Description
none
Modification History
CDF skeleton version of 20120705.Written by B. Larsen.20140304
 
Dataset in CDAWeb
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RBSPA_REL04_ECT-HOPE-PA-L3 (spase://NASA/NumericalData/RBSP/A/ECT/HOPE/L3/PitchAngle/Release04/PT11.35S)
Description
Pitch angle binned data from the HOPE plasma spectrometer.  Note that there are
no correections performed on the data (e.g. background subtraction, velocity
corrections, etc.)
Modification History
CDF skeleton version of 20120705. Written by R. Friedel.
20120706 version written by R. Skoug. 
20130715 revisions by J. T. Niehof.
20130808 revisions by J. T. Niehof/BA Larsen.
20130927 revision (remove per-mode variables)by J. T. Niehof.
 
Dataset in CDAWeb
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RBSPA_REL04_ECT-HOPE-SCI-L2 (spase://NASA/NumericalData/RBSP/A/ECT/HOPE/L2/Sectors/Release04/PT24S)
Description
none
Modification History
CDF skeleton version of 20120705.Written by R. Friedel..20120706 version,
written by R. Skoug.20130715 revisions by J. T. Niehof.20120706 version, written
by R. Skoug.20130715 revisions by J. T. Niehof.20120706 version, written by R.
Skoug.20130715 revisions by J. T. Niehof
20120706 version, written by R. Skoug
20130715 revisions by J. T. Niehof
 
Dataset in CDAWeb
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RBSPA_REL04_ECT-HOPE-SCI-L2SA (spase://NASA/NumericalData/RBSP/A/ECT/HOPE/L2/SpinAverage/Release04/PT24S)
Description
none
Modification History
CDF skeleton version of 20120705.Written by R. Friedel..20120706 version,
written by R. Skoug.20130715 revisions by J. T. Niehof.20120706 version, written
by R. Skoug.20130715 revisions by J. T. Niehof.20120706 version, written by R.
Skoug.20130715 revisions by J. T. Niehof
20120706 version, written by R. Skoug
20130715 revisions by J. T. Niehof
 
Dataset in CDAWeb
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RBSPA_REL04_ECT-MAGEIS-L3 (spase://NASA/NumericalData/RBSP/A/ECT/MagEIS/L3/Sectors/Release04/PT10.9S)
Description
Van Allen Probes, RBSPECT/MagEIS (Radiation Belt Storm Probes Energetic
particle, Composition and Thermal plasma suite/Magnetic Electron Ion
Spectrometer, Level 3 Pitch Angle Sorted Data.
 
Dataset in CDAWeb
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RBSPB_EFW-L2_E-HIRES-UVW (spase://NASA/NumericalData/RBSP/B/EFW/L2/UVW/Hires)
Description
CDAWeb interface derived data on Fri Jun 14 15:33:16 EDT 2013. Contacts: 
Tami.J.Kovalick@nasa.gov, Rita.C.Johnson@nasa.gov. High Resolution DC Electric
Field in UVW Coordinates.
Modification History
v01:  initial version.
 
Dataset in CDAWeb
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RBSPB_EFW-L2_E-SPINFIT-MGSE (spase://NASA/NumericalData/RBSP/B/EFW/L2/MGSE/PT11S)
Description
CDAWeb interface derived data on Fri Jun 14 15:33:16 EDT 2013. Contacts: 
Tami.J.Kovalick@nasa.gov, Rita.C.Johnson@nasa.gov. Spinfit DC electric field
estimates in the M-GSE coordinate system - see the EFW-FAQ
(http://rbsp.space.umn.edu/efw_faq.html) for a description of the spin fit 
algorithm and the M-GSE coordinate system.
One 2D vector estimate of the E-field is computed at a cadence of once per spin
period (typ. 10.7 to 11.1 s) using the survey E-field data product - the
potential difference between EFW sensors V1 and V2 (E12) or V3 and V4 (E34)
sampled at a nominal rate of 32 samp/s with a resolution of 16 bits.
The X-component of the E-field estimate, corresponding to the axial component in
the spacecraft coordinate system, is set to zero in this data product.  See the
EFW-FAQ (http://rbsp.space.umn.edu/efw_faq.html) for a discussion of this 
convention for this data product.
The VxB electric field in the spacecraft frame due to orbital motion of the
spacecraft around the Earth as computed from the spacecraft orbital velocity and
measured B-field in the spacraft frame has been subtracted from the measured
electric field, and so the data product is in the quasi-inertial frame
equivalent to GSE (i.e. it is NOT in the corotation frame of the Earth!).
Each spin fit is time-tagged with the time corresponding to the middle of the
spin of data that went into the spin fit algorithm; in other words, if a given
spin covers the interval [t1, t2), then the spin fit E-field estimate associated
with that spin is given the time tag 0.5*(t1 + t2).
The root mean square residual between the data included in the fit and the
resulting best-fit model, sigma, and the final number of points included in the
spin fit, npts, are also provided at spin-period cadence.
The nominal dynamic range of the E-field estimate is +/- 1 V/m in any component.
Modification History
v01:  initial version.
 
Dataset in CDAWeb
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RBSPB_EFW-L2_ESVY_DESPUN (spase://NASA/NumericalData/RBSP/B/EFW/L2/ESVY_DESPUN/PT0.031S)
Description
CDAWeb interface derived data on Fri Jun 14 15:33:16 EDT 2013. Contacts: 
Tami.J.Kovalick@nasa.gov, Rita.C.Johnson@nasa.gov. Spinfit DC electric field
estimates in the M-GSE coordinate system - see the EFW-FAQ
(http://rbsp.space.umn.edu/efw_faq.html) for a description of the spin fit 
algorithm and the M-GSE coordinate system.
One 2D vector estimate of the E-field is computed at a cadence of once per spin
period (typ. 10.7 to 11.1 s) using the survey E-field data product - the
potential difference between EFW sensors V1 and V2 (E12) or V3 and V4 (E34)
sampled at a nominal rate of 32 samp/s with a resolution of 16 bits.
The X-component of the E-field estimate, corresponding to the axial component in
the spacecraft coordinate system, is set to zero in this data product.  See the
EFW-FAQ (http://rbsp.space.umn.edu/efw_faq.html) for a discussion of this 
convention for this data product.
The VxB electric field in the spacecraft frame due to orbital motion of the
spacecraft around the Earth as computed from the spacecraft orbital velocity and
measured B-field in the spacraft frame has been subtracted from the measured
electric field, and so the data product is in the quasi-inertial frame
equivalent to GSE (i.e. it is NOT in the corotation frame of the Earth!).
Each spin fit is time-tagged with the time corresponding to the middle of the
spin of data that went into the spin fit algorithm; in other words, if a given
spin covers the interval [t1, t2), then the spin fit E-field estimate associated
with that spin is given the time tag 0.5*(t1 + t2).
The root mean square residual between the data included in the fit and the
resulting best-fit model, sigma, and the final number of points included in the
spin fit, npts, are also provided at spin-period cadence.
The nominal dynamic range of the E-field estimate is +/- 1 V/m in any component.
Modification History
v01:  initial version.
 
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RBSPB_EFW-L2_FBK (spase://NASA/NumericalData/RBSP/B/EFW/L2/FBK/PT0.125S)
Description
Up to two sources are returned. The possible sources are:
E12DC, E34DC,E56DC,
E12AC,E34AC,E56AC,
SCMU,SCMV,SCMW
(V1DC+V2DC+V3DC+V4DC)/4
 
Dataset in CDAWeb
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RBSPB_EFW-L2_SPEC (spase://NASA/NumericalData/RBSP/B/EFW/L2/SPEC/PT4S)
Description
Six spectral products are returned. The possible sources are:
E12dc,E34dc,E56dc
E12ac,E34ac,E56ac
Edcpar,Edcprp
Eacpar,Eacprp
V1ac,V2ac,V3ac,V4ac,V5ac,V6ac
SCMU,SCMV,SCMW
SCMpar,SCMprp,
(V1dc+V2dc+V3dc+V4dc)/4,
Edcprp2, Eacprp2, SCMprp2
Caveats
See THEMIS website for caveats
 
Dataset in CDAWeb
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RBSPB_EFW-L2_VSVY-HIRES (spase://NASA/NumericalData/RBSP/B/EFW/L2/VSVY/PT1S)
Description
CDAWeb interface derived data on Fri Jun 14 15:33:16 EDT 2013. Contacts: 
Tami.J.Kovalick@nasa.gov, Rita.C.Johnson@nasa.gov. Spinfit DC electric field
estimates in the M-GSE coordinate system - see the EFW-FAQ
(http://rbsp.space.umn.edu/efw_faq.html) for a description of the spin fit 
algorithm and the M-GSE coordinate system.
One 2D vector estimate of the E-field is computed at a cadence of once per spin
period (typ. 10.7 to 11.1 s) using the survey E-field data product - the
potential difference between EFW sensors V1 and V2 (E12) or V3 and V4 (E34)
sampled at a nominal rate of 32 samp/s with a resolution of 16 bits.
The X-component of the E-field estimate, corresponding to the axial component in
the spacecraft coordinate system, is set to zero in this data product.  See the
EFW-FAQ (http://rbsp.space.umn.edu/efw_faq.html) for a discussion of this 
convention for this data product.
The VxB electric field in the spacecraft frame due to orbital motion of the
spacecraft around the Earth as computed from the spacecraft orbital velocity and
measured B-field in the spacraft frame has been subtracted from the measured
electric field, and so the data product is in the quasi-inertial frame
equivalent to GSE (i.e. it is NOT in the corotation frame of the Earth!).
Each spin fit is time-tagged with the time corresponding to the middle of the
spin of data that went into the spin fit algorithm; in other words, if a given
spin covers the interval [t1, t2), then the spin fit E-field estimate associated
with that spin is given the time tag 0.5*(t1 + t2).
The root mean square residual between the data included in the fit and the
resulting best-fit model, sigma, and the final number of points included in the
spin fit, npts, are also provided at spin-period cadence.
The nominal dynamic range of the E-field estimate is +/- 1 V/m in any component.
Modification History
v01:  initial version.
 
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RBSPB_EFW-L3 (spase://NASA/NumericalData/RBSP/B/EFW/L3/PT11S)
Description
**********************************************************
*************PRODUCTS FOR L3 FILES*******************:
**********************************************************
Eymgse, Ez mgse, spinfit  in a co-rotational
frame (Vsc x B and Ecorotation subtracted)
Include  Vsc x B, Vcoro x B as separate variables
Include separate quality flags for charging, eclipse and biasing. 
Density from SC potential
SC potential (V1-V6)
Ex mgse (spin axis component) for "good" ratios of |Bx/Bz| and |By/Bz|,
The magnetic field ratios themselves,
L value, MLT, MLAT,  and the position of the SC in GSE.
The unit vector of the spin axis in gse coordinate system.
All quantities are at spin period resolution
Modification History
v01:  initial version; started with L1 EFW VSVY CDF, removing all L0 (e.g. CCSDS
packet header) variables, changing variable type of VSVY variable from INT to
REAL to reflect tranformation from TM to Physical units; added variables for
average of opposing sensors, VSVY_AVG; added variable for sensor potential
quality flag, VSVY_QUAL. Added EFW data quality flag array.
 
Dataset in CDAWeb
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RBSPB_EFW_BURST-WAVEFORM-UVW-L1 (spase://NASA/NumericalData/RBSP/B/EFW/L1/B1/UVW/PT0.00195S)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPB_L1_EB1 (spase://NASA/NumericalData/RBSP/B/EFW/L1/B1/UVW/ElectricField/PT0.00195S)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPB_L1_EB2 (spase://NASA/NumericalData/RBSP/B/EFW/L1/B2/UVW/ElectricField/PT0.00006S)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPB_L1_MSCB1 (spase://NASA/NumericalData/RBSP/B/EFW/L1/B1/UVW/SearchCoilMagneticField/PT0.00195S)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPB_L1_MSCB2 (spase://NASA/NumericalData/RBSP/B/EFW/L1/B2/UVW/SearchCoilMagneticField/PT0.00006S)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPB_L1_VB1 (spase://NASA/NumericalData/RBSP/B/EFW/L1/B1/UVW/ElectricPotential/PT0.00195S)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPB_L1_VB2 (spase://NASA/NumericalData/RBSP/B/EFW/L1/B2/UVW/ElectricPotential/PT0.00006S)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPB_L2-1MIN_PSBR-RPS (spase://NASA/NumericalData/RBSP/B/RPS/L2/PT1M)
Description
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, Dr.
Joe Mazur, can be reached at Joseph.E.Mazur@aero.org.
Modification History
TBD
 
Dataset in CDAWeb
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RBSPB_L2_PSBR-RPS (spase://NASA/NumericalData/RBSP/B/RPS/L2/PT0.058S)
Description
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, Dr.
Joe Mazur, can be reached at Joseph.E.Mazur@aero.org.
Modification History
TBD
 
Dataset in CDAWeb
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RBSPB_REL03_ECT-MAGEIS-L2 (spase://NASA/NumericalData/RBSP/B/ECT/MagEIS/L2/Sectors/Release03/PT10.9S)
Description
MagEIS consists of 4 energetic particle sensors per RBSP spacecraft: low unit,
medium35 unit, medium75 unit and the high unit.  The low and 2 medium units are
magnetic spectrometers that measure electrons across roughly the 20 keV - 1 MeV
energy range. The high unit contains a magnetic spectrometer that measures
electrons from roughly the 700 keV to 4 MeV range. The high unit also has a
proton telescope that measures protons from roughly 50 keV to 20 MeV, Helium
ions from roughly 300 keV - 1.5 MeV and Oxygen ions from roughly 1-5 MeV. 
MagEIS is one of three instrument packages on the ECT instrument suite (HOPE and
REPT are the others).
 
Dataset in CDAWeb
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RBSPB_REL03_ECT-REPT-SCI-L2 (spase://NASA/NumericalData/RBSP/B/ECT/REPT/L2/Sectors/Release03/PT4.2S)
Description
RBSP Relativistic Electron Proton Telescope, Level 2 science data
Modification History
CDF skeleton version of rbsp_rept_science_l2_data.template.cdf written by R.
Reukauf
 
Dataset in CDAWeb
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RBSPB_REL03_ECT-REPT-SCI-L3 (spase://NASA/NumericalData/RBSP/B/ECT/REPT/L3/Sectors/Release03/PT4.2S)
Description
Van Allen Probes, RBSPECT/REPT (Radiation Belt Storm Probes Energetic particle,
Composition and Thermal plasma suite/Relativistic Electron Proton Telescope,
Level 3 Pitch Angle Sorted Data.
 
Dataset in CDAWeb
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RBSPB_REL04_ECT-HOPE-MOM-L3 (spase://NASA/NumericalData/RBSP/B/ECT/HOPE/L3/Moments/Release04/PT24.35S)
Description
none
Modification History
CDF skeleton version of 20120705.Written by B. Larsen.20140304
 
Dataset in CDAWeb
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RBSPB_REL04_ECT-HOPE-PA-L3 (spase://NASA/NumericalData/RBSP/B/ECT/HOPE/L3/PitchAngle/Release04/PT11.35S)
Description
Pitch angle binned data from the HOPE plasma spectrometer.  Note that there are
no correections performed on the data (e.g. background subtraction, velocity
corrections, etc.)
Modification History
CDF skeleton version of 20120705. Written by R. Friedel.
20120706 version written by R. Skoug. 
20130715 revisions by J. T. Niehof.
20130808 revisions by J. T. Niehof/BA Larsen.
20130927 revision (remove per-mode variables)by J. T. Niehof.
 
Dataset in CDAWeb
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RBSPB_REL04_ECT-HOPE-SCI-L2 (spase://NASA/NumericalData/RBSP/B/ECT/HOPE/L2/Sectors/Release04/PT24S)
Description
none
Modification History
CDF skeleton version of 20120705.Written by R. Friedel..20120706 version,
written by R. Skoug.20130715 revisions by J. T. Niehof.20120706 version, written
by R. Skoug.20130715 revisions by J. T. Niehof.20120706 version, written by R.
Skoug.20130715 revisions by J. T. Niehof
20120706 version, written by R. Skoug
20130715 revisions by J. T. Niehof
 
Dataset in CDAWeb
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RBSPB_REL04_ECT-HOPE-SCI-L2SA (spase://NASA/NumericalData/RBSP/B/ECT/HOPE/L2/SpinAverage/Release04/PT24S)
Description
none
Modification History
CDF skeleton version of 20120705.Written by R. Friedel..20120706 version,
written by R. Skoug.20130715 revisions by J. T. Niehof.20120706 version, written
by R. Skoug.20130715 revisions by J. T. Niehof.20120706 version, written by R.
Skoug.20130715 revisions by J. T. Niehof
20120706 version, written by R. Skoug
20130715 revisions by J. T. Niehof
 
Dataset in CDAWeb
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RBSPB_REL04_ECT-MAGEIS-L3 (spase://NASA/NumericalData/RBSP/B/ECT/MagEIS/L3/Sectors/Release04/PT10.9S)
Description
Van Allen Probes, RBSPECT/MagEIS (Radiation Belt Storm Probes Energetic
particle, Composition and Thermal plasma suite/Magnetic Electron Ion
Spectrometer, Level 3 Pitch Angle Sorted Data.
 
Dataset in CDAWeb
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RBSP_ECT-REPT-SCI-L3-SELESNICK-MODEL (spase://NASA/NumericalData/RBSP/ECT/REPT/SelesnickModel/L3/P1M)
Description
The files contain model radiation belt proton intensity derived from data taken
by the Van Allen Probes REPT instruments using the method described by:
Selesnick, R. S., Baker, D. N., Kanekal, S. G., Hoxie, V. C., & Li, X. (2018). 
Modeling the proton radiation belt with Van Allen Probes Relativistic
Electron-Proton Telescope data. Journal of Geophysical Research: Space Physics,
123. https://doi.org/10.1002/2017JA024661 Each file contains average intensity, 
as a function of kinetic energy, equatorial pitch angle, and L-shell, derived
from 1 month of data. 
 
Dataset in CDAWeb
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RENU2_H0_EFIELD (spase://NASA/NumericalData/RENU2/COWBOY/ElectricField/PT0.001S)
Description
RENU2 COWBOY
 
Dataset in CDAWeb
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RENU2_H0_EPLAS (spase://NASA/NumericalData/RENU2/EPLAS/PT0.042S)
Description
RENU2 EPLAS
 
Dataset in CDAWeb
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RENU2_H0_ERPAMAIN (spase://NASA/NumericalData/RENU2/ERPA/MAIN/PT0.0005S)
Description
RENU2 ERPA
 
Dataset in CDAWeb
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RENU2_H0_ERPASUB (spase://NASA/NumericalData/RENU2/ERPA/SUB/PT0.0005S)
Description
RENU2 ERPA
 
Dataset in CDAWeb
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RENU2_H0_FGM (spase://NASA/NumericalData/RENU2/FGM/PT0.001S)
Description
RENU2 magnetometer
 
Dataset in CDAWeb
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RENU2_H0_IG2 (spase://NASA/NumericalData/RENU2/IG2/PT0.001S)
Description
RENU2 ionization gauge
 
Dataset in CDAWeb
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RENU2_H0_PMT (spase://NASA/NumericalData/RENU2/PMT/PT0.004S)
Description
RENU2 PMT counts converted to Rayleighs and background subtracted
 
Dataset in CDAWeb
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RENU2_H0_UVPMT (spase://NASA/NumericalData/RENU2/UVPMT/PT0.042S)
Description
RENU2 UV PMT
 
Dataset in CDAWeb
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RENU2_H0_VLF (spase://NASA/NumericalData/RENU2/COWBOY/VLF/PT0.001S)
Description
RENU2 COWBOY
 
Dataset in CDAWeb
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ROSETTA_HELIO1DAY_POSITION (spase://NASA/NumericalData/Rosetta/HelioWeb/Ephemeris/P1D)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RS_K0_IPEI (spase://NASA/NumericalData/ROCSAT-1/IPEI/PT1s)
Description
1-second averaged data
***Important Notes*** on Accuracy of VperpM_MF (meridional),VperpZ_MF (zonal),
and VparaMF (parallel) components.
Geophysical flow components VperpM_MF, VperpZ_MF, and VparaMF are converted from
flow velocities, Vx, Vy, and Vz 
measured in the S/C coordinate system. Vx points along the S/C trajectory
vector, Vz is in the nadir direction, 
and Vy points to the right of the S/C trajectory vector (in the anti-angular
momentum direction).
1) Vx, Vy, and Vz are measured flow velocities at S/C coordinate in the
Earth-centered Inertia Coordinate System (non-rotating) (ECI coordinate).
2) VperZ_MF, VperM_MF, and VparaMF are geophysical flows in the Earth-centered
Fixed Coordinated System (rotate with the Earth) (ECF coordinate).
3) Uncertainty of +-(37.8-75.45) m/s in Vx based on 0.5% - 1% error in fitting
could be introduced to all geophysical flow components.
4) VperpM_MF at low latitude is almost identical to (-Vz). No Vx is included so
that it is very reliable.
5) Uncertainties from Vx could exist in VperpZ_MF and VparaMF.
6) VperpZ_MF and VparaMF can be used to study the relative changes in flow
velocity due to  geophysical effects.
But can not be used to study the long-term variations because the result could
be biased by the uncertainty in Vx.
Modification History
Version 1.0 Jan. 28, 2008
 
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