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CDAWeb Served Heliophysics Datasets Beginning with 'R'

RBSP-A-RBSPICE_LEV-2_ESRHELT: High-energy low-time resolution electron fluxes ~0.02-1.0 MeV (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-2_ESRLEHT: Low-energy high-time resolution electron fluxes ~0.02-1.0 MeV (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-2_ISRHELT: Diagnostic Data Use only - DO NOT USE FOR SCIENTIFIC PURPOSES. High-energy low-time resolution RBSPICE Ion Energy mode measurement of all particle fluxes (electron/ion) ~0.05-1.0 MeV (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-2_TOFXEH: TOF x Energy Hydrogen Rates (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-2_TOFXEION: TOF x Energy Ion Fluxes 0.02-1 MeV measured at high energy resolution and low time resolution (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-2_TOFXENONH: TOF x E non Hydrogen (Helium and Oxygen) Rates ~0.02-1.0 MeV measured at high energy and low time resolution (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-2_TOFXPHHHELT: High-energy low-time resolution proton and oxygen fluxes from TOF x PH Hydrogen Rates (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-2_TOFXPHHLEHT: TOF x Pulse Height Hydrogen and Oxygen Fluxes ~0.01-0.2 MeV measured at low energy resolution and high time resolution (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_ESRHELT: High Energy Low Time resolution electron intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_ESRLEHT: Low Energy High Time resolution electron intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXEH: TOF x Energy High Energy Low Time resolution proton intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXEHE: TOF x Energy High Energy Low Time resolution Helium intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXEHE-0: TOF x Energy High Energy Low Time resolution Helium intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXEION: TOF x Energy High Energy Low Time resolution ion intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXEO: TOF x Energy High Energy Low Time resolution Oxygen intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXEO-0: TOF x Energy High Energy Low Time resolution Oxygen intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXPHHHELT: TOF x Pulse Height Energies High Energy Low Time resolution proton intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXPHHLEHT: TOF x Pulse Height Energies High Energy Low Time resolution proton intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXPHOHELT: TOF x Pulse Height Energies High Energy Low Time resolution Oxygen intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3-PAP_TOFXPHOLEHT: TOF x Pulse Height Energies Low Energy High Time resolution Oxygen intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_ESRHELT: High-energy low-time resolution electron fluxes ~0.02-1.0 MeV (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_ESRLEHT: Low-energy high-time resolution electron fluxes ~0.02-1.0 MeV (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_ISRHELT: Diagnostic Data Use only - DO NOT USE FOR SCIENTIFIC PURPOSES. High-energy low-time resolution RBSPICE Ion Energy mode measurement with pitch angles of all particle fluxes (electron/ion) ~0.05-1.0 MeV (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_TOFXEH: TOF x Energy Hydrogen Rates (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_TOFXEION: TOF x Energy Ion Fluxes 0.02-1 MeV measured at high energy resolution and low time resolution (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_TOFXENONH: TOF x E non Hydrogen (Helium and Oxygen) Rates ~0.02-1.0 MeV measured at high energy and low time resolution (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_TOFXPHHHELT: High-energy low-time resolution proton and oxygen fluxes from TOF x PH Hydrogen Rates (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A-RBSPICE_LEV-3_TOFXPHHLEHT: TOF x Pulse Height Hydrogen and Oxygen Fluxes ~0.01-0.2 MeV measured at low energy resolution and high time resolution (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-A_DENSITY_EMFISIS-L4: 1-second 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 ~5-10,000 Hz - Craig Kletzing (University of Iowa)
RBSP-A_HFR-SPECTRA-MERGED_EMFISIS-L2: Single Axis AC Electric Field Spectra ~5-10,000 Hz - Craig Kletzing (University of Iowa)
RBSP-A_HFR-SPECTRA_EMFISIS-L2: Single Axis AC Electric Field Spectra ~5-10,000 Hz - Craig Kletzing (University of Iowa)
RBSP-A_HFR-WAVEFORM_EMFISIS-L2: High Frequency Receiver (HFR) Field Waveform Samples in V/m (Selectable between the U, V and W Axes) - 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_MAGNETOMETER_UVW_EMFISIS-L2: Fluxgate magnetometer data - Craig Kletzing (University of Iowa)
RBSP-A_WFR-SPECTRAL-MATRIX-DIAGONAL-MERGED_EMFISIS-L2: WaveForm Receiver (WFR) Spectral Matrix ~5-10,000 Hz (Merged, Diagonal Elements Only) - Craig Kletzing (University of Iowa)
RBSP-A_WFR-SPECTRAL-MATRIX-DIAGONAL_EMFISIS-L2: WaveForm Receiver (WFR) Spectral Matrix ~5-10000 Hz (Diagonal Elements Only) - 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: WaveForm Receiver (WFR) Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV, BW) continuous burst waveforms @ 35 kS/sec - Craig Kletzing (University of Iowa)
RBSP-A_WFR-WAVEFORM_EMFISIS-L2: WFR Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV, BW) waveforms as 16384 samples @ 35 kS/sec - Craig Kletzing (University of Iowa)
RBSP-B-RBSPICE_LEV-2_ESRHELT: High-energy low-time resolution electron fluxes ~0.02-1.0 MeV (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-2_ESRLEHT: Low-energy high-time resolution electron fluxes ~0.02-1.0 MeV (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-2_ISRHELT: Diagnostic Data Use only - DO NOT USE FOR SCIENTIFIC PURPOSES. High-energy low-time resolution RBSPICE Ion Energy mode measurement of all particle fluxes (electron/ion) ~0.05-1.0 MeV (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-2_TOFXEH: TOF x Energy Hydrogen Rates (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-2_TOFXEION: TOF x Energy Ion Fluxes 0.02-1 MeV measured at high energy resolution and low time resolution (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-2_TOFXENONH: TOF x E non Hydrogen (Helium and Oxygen) Rates ~0.02-1.0 MeV measured at high energy and low time resolution (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-2_TOFXPHHHELT: High-energy low-time resolution proton and oxygen fluxes from TOF x PH Hydrogen Rates (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-2_TOFXPHHLEHT: TOF x Pulse Height Hydrogen and Oxygen Fluxes ~0.01-0.2 MeV measured at low energy resolution and high time resolution (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_ESRHELT: High Energy Low Time resolution electron intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_ESRLEHT: Low Energy High Time resolution electron intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXEH: TOF x Energy High Energy Low Time resolution proton intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXEHE: TOF x Energy High Energy Low Time resolution Helium intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXEHE-0: TOF x Energy High Energy Low Time resolution Helium intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXEION: TOF x Energy High Energy Low Time resolution ion intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXEO: TOF x Energy High Energy Low Time resolution Oxygen intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXEO-0: TOF x Energy High Energy Low Time resolution Oxygen intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXPHHHELT: TOF x Pulse Height Energies High Energy Low Time resolution proton intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXPHHLEHT: TOF x Pulse Height Energies High Energy Low Time resolution proton intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXPHOHELT: TOF x Pulse Height Energies High Energy Low Time resolution Oxygen intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3-PAP_TOFXPHOLEHT: TOF x Pulse Height Energies Low Energy High Time resolution Oxygen intensities and pressures sorted by pitch angles - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_ESRHELT: High-energy low-time resolution electron fluxes ~0.02-1.0 MeV (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_ESRLEHT: Low-energy high-time resolution electron fluxes ~0.02-1.0 MeV (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_ISRHELT: Diagnostic Data Use only - DO NOT USE FOR SCIENTIFIC PURPOSES. High-energy low-time resolution RBSPICE Ion Energy mode measurement with pitch angles of all particle fluxes (electron/ion) ~0.05-1.0 MeV (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_TOFXEH: TOF x Energy Hydrogen Rates (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_TOFXEION: TOF x Energy Ion Fluxes 0.02-1 MeV measured at high energy resolution and low time resolution (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_TOFXENONH: TOF x E non Hydrogen (Helium and Oxygen) Rates ~0.02-1.0 MeV measured at high energy and low time resolution (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_TOFXPHHHELT: High-energy low-time resolution proton and oxygen fluxes from TOF x PH Hydrogen Rates (with multi-spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B-RBSPICE_LEV-3_TOFXPHHLEHT: TOF x Pulse Height Hydrogen and Oxygen Fluxes ~0.01-0.2 MeV measured at low energy resolution and high time resolution (with spin accumulations plotted at end of accumulation in sector order) - Lou Lanzerotti (New Jersey Institute of Technology)
RBSP-B_DENSITY_EMFISIS-L4: 1-second 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 ~5-10,000 Hz - Craig Kletzing (University of Iowa)
RBSP-B_HFR-SPECTRA-MERGED_EMFISIS-L2: Single Axis AC Electric Field Spectra ~5-10,000 Hz - Craig Kletzing (University of Iowa)
RBSP-B_HFR-SPECTRA_EMFISIS-L2: Single Axis AC Electric Field Spectra ~5-10,000 Hz - Craig Kletzing (University of Iowa)
RBSP-B_HFR-WAVEFORM_EMFISIS-L2: High Frequency Receiver (HFR) Field Waveform Samples in V/m (Selectable between the U, V and W Axes) - 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_MAGNETOMETER_UVW_EMFISIS-L2: Fluxgate magnetometer data - Craig Kletzing (University of Iowa)
RBSP-B_WFR-SPECTRAL-MATRIX-DIAGONAL-MERGED_EMFISIS-L2: WaveForm Receiver (WFR) Spectral Matrix ~5-10,000 Hz (Merged, Diagonal Elements Only) - Craig Kletzing (University of Iowa)
RBSP-B_WFR-SPECTRAL-MATRIX-DIAGONAL_EMFISIS-L2: WaveForm Receiver (WFR) Spectral Matrix ~5-10000 Hz (Diagonal Elements Only) - 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: WaveForm Receiver (WFR) Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV, BW) continuous burst waveforms @ 35 kS/sec - Craig Kletzing (University of Iowa)
RBSP-B_WFR-WAVEFORM_EMFISIS-L2: WFR Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV, BW) waveforms as 16384 samples @ 35 kS/sec - Craig Kletzing (University of Iowa)
RBSPA_EFW-L2_E-HIRES-UVW: Reference for Spin Axis Vector in GSE - J. R. Wygant (University of Minnesota)
RBSPA_EFW-L2_E-SPINFIT-MGSE: Spinfit (10.9 sec resolution) DC Electric Field estimates in M-GSE coordinates. - J. R. Wygant (University of Minnesota)
RBSPA_EFW-L2_ESVY_DESPUN: Despun (32 Samples/sec) E-Field estimates in M-GSE coords - J. R. Wygant (University of Minnesota)
RBSPA_EFW-L2_FBK: Filterbank peak and average values 1-7000 Hz from RBSP-EFW (with peak and average values returned for 2 of 20 possible sources at any one time) - J. R. Wygant (University of Minnesota)
RBSPA_EFW-L2_SPEC: On-Board Spin-Fit 4-8000 Hz electric and magnetic field spectral data from RBSP-EFW (with 7 of 75 possible sources returned at any one time) - 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 Spin-fit Electric field in modified-GSE (MGSE) coordinates, density from EFW S/C Potential, and other products - 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_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-HOPE-MOM-L3: Spin resolved HOPE science data. Plasma moments from electrons >200 eV and ions >30 eV measured at apogee in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPA_REL03_ECT-HOPE-PA-L3: Pitch angle resolved ECT-HOPE science data. Electron fluxes ~15-50,000 eV, ion fluxes ~1-50,000 eV. Electrons and ions measured in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPA_REL03_ECT-HOPE-SCI-L2: Spin resolved ECT-HOPE science data. Electron fluxes ~15-50,000 eV, ion fluxes ~1-50,000 eV. Electrons and ions measured in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPA_REL03_ECT-HOPE-SCI-L2SA: Spin averaged ECT-HOPE science data. Electron fluxes ~15-50,000 eV, ion fluxes ~1-50,000 eV. Electrons and ions measured in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPA_REL03_ECT-MAGEIS-L2: Electron fluxes ~20-4000 keV and proton fluxes ~50-1500 keV from ECT/MAGEIS - J. Bernard Blake / JBernard.Blake@aero.org (The Aerospace Corporation)
RBSPA_REL03_ECT-MAGEIS-L3: Electron fluxes ~20-4000 keV and proton fluxes ~60-1500 keV from ECT/MagEIS - J. Bernard Blake (JBernard.Blake@aero.org) (The Aerospace Corporation)
RBSPA_REL03_ECT-REPT-SCI-L2: Electron fluxes 2-20 MeV and proton fluxes 20-120 MeV from ECT/REPT - 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: 2 - 59.45 MeV. Proton energies: 21.25 - 0 MeV - D. Baker (University of Colorado at Boulder)
RBSPB_EFW-L2_E-HIRES-UVW: Reference for Spin Axis Vector in GSE - J. R. Wygant (University of Minnesota)
RBSPB_EFW-L2_E-SPINFIT-MGSE: Spinfit (10.9 sec resolution) DC Electric Field estimates in M-GSE coordinates. - J. R. Wygant (University of Minnesota)
RBSPB_EFW-L2_ESVY_DESPUN: Despun (32 Samples/sec) E-Field estimates in M-GSE coords - J. R. Wygant (University of Minnesota)
RBSPB_EFW-L2_FBK: Filterbank peak and average values 1-7000 Hz from RBSP-EFW (with peak and average values returned for 2 of 20 possible sources at any one time) - J. R. Wygant (University of Minnesota)
RBSPB_EFW-L2_SPEC: On-Board Spin-Fit 4-8000 Hz electric and magnetic field spectral data from RBSP-EFW (with 7 of 75 possible sources returned at any one time) - 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 Spin-fit Electric field in modified-GSE (MGSE) coordinates, density from EFW S/C Potential, and other products - 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_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-HOPE-MOM-L3: Spin resolved HOPE science data. Plasma moments from electrons >200 eV and ions >30 eV measured at apogee in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPB_REL03_ECT-HOPE-PA-L3: Pitch angle resolved ECT-HOPE science data. Electron fluxes ~15-50,000 eV, ion fluxes ~1-50,000 eV. Electrons and ions measured in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPB_REL03_ECT-HOPE-SCI-L2: Spin resolved ECT-HOPE science data. Electron fluxes ~15-50,000 eV, ion fluxes ~1-50,000 eV. Electrons and ions measured in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPB_REL03_ECT-HOPE-SCI-L2SA: Spin averaged ECT-HOPE science data. Electron fluxes ~15-50,000 eV, ion fluxes ~1-50,000 eV. Electrons and ions measured in alternate spin cadence. - Herbert Funsten (Los Alamos National Laboratory)
RBSPB_REL03_ECT-MAGEIS-L2: Electron fluxes ~20-4000 keV and proton fluxes ~50-1500 keV from ECT/MAGEIS - J. Bernard Blake / JBernard.Blake@aero.org (The Aerospace Corporation)
RBSPB_REL03_ECT-MAGEIS-L3: Electron fluxes ~20-4000 keV and proton fluxes ~60-1500 keV from ECT/MagEIS - J. Bernard Blake (JBernard.Blake@aero.org) (The Aerospace Corporation)
RBSPB_REL03_ECT-REPT-SCI-L2: Electron fluxes 2-20 MeV and proton fluxes 20-120 MeV from ECT/REPT - 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: 2 - 59.45 MeV. Proton energies: 21.25 - 0 MeV - D. Baker (University of Colorado at Boulder)
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_PMT: H0 - RENU2 PMT Counts. - Marc Lessard (University of New Hampshire)
RS_K0_IPEI: ROCSAT-1(FORMOSAT-1)/IPEI, Key Parameters - Shin-Yi Su (Institute of Space Science, National Central University, Taiwan, R.O.C.)

RBSP-A-RBSPICE_LEV-2_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
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
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
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
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
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
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
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
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
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
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
Description
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
Description
rbspice high energy res low time res tofxe helium intensities/pressures sorted
by pitch angles.
Modification History
July 2015, SPDF renamed these files to accommodate dimension size changes which
were a result of an expanded instrument configuration.
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3-PAP_TOFXEION
Description
rbspice high energy res low time res tofxe ion 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
Description
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
Description
rbspice high energy res low time res tofxe oxygen intensities/pressures sorted
by pitch angles.
Modification History
July 2015, SPDF renamed these files to accommodate dimension size changes which
were a result of an expanded instrument configuration.
 
Dataset in CDAWeb
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RBSP-A-RBSPICE_LEV-3-PAP_TOFXPHHHELT
Description
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
Description
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_TOFXPHOHELT
Description
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
Description
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
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
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
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
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
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
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
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
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
Description
Density and other parameters inferred by digitizing the trace on the
spectrograms.
 
Dataset in CDAWeb
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RBSP-A_HFR-SPECTRA-BURST_EMFISIS-L2
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
Description
1
 
Dataset in CDAWeb
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RBSP-A_HFR-SPECTRA_EMFISIS-L2
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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_UVW_EMFISIS-L2
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
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
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
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
Description
Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV,
BW)  continuous burst waveforms208896 samples @ 35 kS/sec.
 
Dataset in CDAWeb
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RBSP-A_WFR-WAVEFORM_EMFISIS-L2
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
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
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
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
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
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
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
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
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
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
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
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
Description
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
Description
rbspice high energy res low time res tofxe helium intensities/pressures sorted
by pitch angles.
Modification History
July 2015, SPDF renamed these files to accommodate dimension size changes which
were a result of an expanded instrument configuration.
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3-PAP_TOFXEION
Description
rbspice high energy res low time res tofxeion ion 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
Description
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
Description
rbspice high energy res low time res tofxe oxygen intensities/pressures sorted
by pitch angles.
Modification History
July 2015, SPDF renamed these files to accommodate dimension size changes which
were a result of an expanded instrument configuration.
 
Dataset in CDAWeb
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RBSP-B-RBSPICE_LEV-3-PAP_TOFXPHHHELT
Description
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
Description
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_TOFXPHOHELT
Description
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
Description
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
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
 
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RBSP-B-RBSPICE_LEV-3_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
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
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
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
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
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
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
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
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
Description
1
 
Dataset in CDAWeb
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RBSP-B_HFR-SPECTRA_EMFISIS-L2
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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_UVW_EMFISIS-L2
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
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-DIAGONAL_EMFISIS-L2
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
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
Description
Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV,
BW)  continuous burst waveforms208896 samples @ 35 kS/sec.
 
Dataset in CDAWeb
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RBSP-B_WFR-WAVEFORM_EMFISIS-L2
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
Description
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
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
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
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
Description
Six spectral products are returned. The possible sources
are:.E12dc,E34dc,E56dc.E12ac,E34ac,E56ac.Edcpar,Edcprp.Eacpar,Eacprp.V1ac,V2ac,V
3ac,V4ac,V5ac,V6ac.SCMU,SCMV,SCMW.SCMpar,SCMprp,.(V1ac+V2ac+V3ac+V4ac)/4,.Edcprp
2, Eacprp2, SCMprp2.
Caveats
See THEMIS website for caveats
 
Dataset in CDAWeb
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RBSPA_EFW-L2_VSVY-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. 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
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
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPA_L2-1MIN_PSBR-RPS
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
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-HOPE-MOM-L3
Description
none
Modification History
CDF skeleton version of 20120705.Written by B. Larsen.20140304
 
Dataset in CDAWeb
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RBSPA_REL03_ECT-HOPE-PA-L3
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_REL03_ECT-HOPE-SCI-L2
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
 
Dataset in CDAWeb
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RBSPA_REL03_ECT-HOPE-SCI-L2SA
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
 
Dataset in CDAWeb
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RBSPA_REL03_ECT-MAGEIS-L2
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-MAGEIS-L3
Description
Van Allen Probes, RBSPECT/MagEIS/M75 (Radiation Belt Storm Probes Energetic
particle, Composition and Thermal plasma suite/Magnetic Electron Ion
Spectrometer/Medium Energy 75Deg. Energy Sensor, Level 3 Pitch Angle Sorted
Data.
 
Dataset in CDAWeb
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RBSPA_REL03_ECT-REPT-SCI-L2
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
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_EFW-L2_E-HIRES-UVW
Description
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
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
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_FBK
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
Description
Six spectral products are returned. The possible sources
are:.E12dc,E34dc,E56dc.E12ac,E34ac,E56ac.Edcpar,Edcprp.Eacpar,Eacprp.V1ac,V2ac,V
3ac,V4ac,V5ac,V6ac.SCMU,SCMV,SCMW.SCMpar,SCMprp,.(V1ac+V2ac+V3ac+V4ac)/4,.Edcprp
2, Eacprp2, SCMprp2.
Caveats
See THEMIS website for caveats
 
Dataset in CDAWeb
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RBSPB_EFW-L2_VSVY-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. 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-L3
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
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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RBSPB_L2-1MIN_PSBR-RPS
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
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-HOPE-MOM-L3
Description
none
Modification History
CDF skeleton version of 20120705.Written by B. Larsen.20140304
 
Dataset in CDAWeb
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RBSPB_REL03_ECT-HOPE-PA-L3
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_REL03_ECT-HOPE-SCI-L2
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
 
Dataset in CDAWeb
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RBSPB_REL03_ECT-HOPE-SCI-L2SA
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
 
Dataset in CDAWeb
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RBSPB_REL03_ECT-MAGEIS-L2
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-MAGEIS-L3
Description
Van Allen Probes, RBSPECT/MagEIS/M75 (Radiation Belt Storm Probes Energetic
particle, Composition and Thermal plasma suite/Magnetic Electron Ion
Spectrometer/Medium Energy 75Deg. Energy Sensor, Level 3 Pitch Angle Sorted
Data.
 
Dataset in CDAWeb
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RBSPB_REL03_ECT-REPT-SCI-L2
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
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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RENU2_H0_EPLAS
Description
RENU2 EPLAS
 
Dataset in CDAWeb
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RENU2_H0_ERPAMAIN
Description
RENU2 ERPA
 
Dataset in CDAWeb
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RENU2_H0_ERPASUB
Description
RENU2 ERPA
 
Dataset in CDAWeb
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RENU2_H0_PMT
Description
RENU2 PMT
 
Dataset in CDAWeb
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RS_K0_IPEI
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
 
Dataset in CDAWeb
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