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CDAWeb Served Heliophysics Datasets Beginning with 'S'

SAKIGAKE_HELIO1DAY_POSITION: Position in heliocentric coordinates from SPDF Helioweb - Natalia Papitashvili (NASA/GSFC/SPDF)
SATURN_HELIO1DAY_POSITION: Position in heliocentric coordinates from SPDF Helioweb - Natalia Papitashvili (NASA/GSFC/SPDF)
SE_K0_AIS: SESAME Advanced Ionospheric Sounder, Key Parameters - J. Dudeney (British Antarctic Survey)
SE_K0_FPI: SESAME Fabry-Perot Interferometer, Key Parameters - J.R. Dudeney (British Antarctic Survey)
SE_K0_MAG: SESAME Fluxgate Magnetometer Key Parameters - J. Dudeney (British Antarctic Survey)
SE_K0_RIO: SESAME 30MHz Riometer Array, Key Parameters - J. Dudeney (British Antarctic Survey)
SE_K0_VLF: SESAME VLF/ELF Logger Experiment (VELOX)Key Parameters - J. Dudeney (British Antarctic Survey)
SNOE_L3_GEO: NO density, 100 - 150 km, geographic coordinates - Charles A. Barth (LASP/CU)
SNOE_L3_MAG: NO density, 100 - 150 km, geomagnetic coordinates - Charles A. Barth (LASP/CU)
SOHO_HELIO1DAY_POSITION: Position in heliocentric coordinates from SPDF Helioweb - Natalia Papitashvili (NASA/GSFC/SPDF)
SOLO_HELIO1DAY_POSITION: Position in heliocentric coordinates from SPDF Helioweb - Natalia Papitashvili (NASA/GSFC/SPDF)
SOLO_L2_EPD-EPT-ASUN-BURST-ELE-CLOSE: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, Anti-Sun direction, Burst, Electrons, Close mode - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-EPT-ASUN-BURST-ION: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, Anti-Sun direction, Burst, Ions - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-EPT-ASUN-HCAD: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, Anti-Sun direction, High Cadence - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-EPT-ASUN-RATES: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, Anti-Sun direction, Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-EPT-NORTH-BURST-ELE-CLOSE: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, North direction, Burst, Electrons, Close mode - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-EPT-NORTH-BURST-ION: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, North direction, Burst, Ions - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-EPT-NORTH-HCAD: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, North direction, High Cadence - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-EPT-NORTH-RATES: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, North direction, Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-EPT-SOUTH-BURST-ELE-CLOSE: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, South direction, Burst, Electrons, Close mode - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-EPT-SOUTH-BURST-ION: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, South direction, Burst, Ions - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-EPT-SOUTH-HCAD: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, South direction, High Cadence - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-EPT-SOUTH-RATES: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, South direction, Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-EPT-SUN-BURST-ELE-CLOSE: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, Sun direction, Burst, Electrons, Close mode - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-EPT-SUN-BURST-ION: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, Sun direction, Burst, Ions - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-EPT-SUN-HCAD: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, Sun direction, High Cadence - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-EPT-SUN-RATES: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron Proton Telescope, Sun direction, Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-HET-ASUN-BURST: Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Anti-Sun direction, Burst - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-HET-ASUN-RATES: Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Anti-Sun direction, Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-HET-NORTH-BURST: Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, North direction, Burst - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-HET-NORTH-RATES: Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, North direction, Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-HET-SOUTH-BURST: Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, South direction, Burst - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-HET-SOUTH-RATES: Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, South direction, Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-HET-SUN-BURST: Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Sun direction, Burst - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-HET-SUN-RATES: Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Sun direction, Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-SIS-A-HEHIST: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Suprathermal Ion Spectrograph, A Telescope, Helium histogram - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-SIS-A-RATES-FAST: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Suprathermal Ion Spectrograph, A Telescope, Particle rates, fast cadence - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-SIS-A-RATES-MEDIUM: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Suprathermal Ion Spectrograph, A Telescope, Particle rates, medium cadence - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-SIS-A-RATES-SLOW: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Suprathermal Ion Spectrograph, A Telescope, Particle rates, slow cadence - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-SIS-B-HEHIST: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Suprathermal Ion Spectrograph, B Telescope, Helium histogram - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-SIS-B-RATES-FAST: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Suprathermal Ion Spectrograph, B Telescope, Particle rates, fast cadence - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-SIS-B-RATES-MEDIUM: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Suprathermal Ion Spectrograph, B Telescope, Particle rates, medium cadence - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-SIS-B-RATES-SLOW: Solar Orbiter, Level 2 Data, Energetic Particle Detector, Suprathermal Ion Spectrograph, B Telescope, Particle rates, slow cadence - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-STEP-BURST: Solar Orbiter, Level 2 Data, Energetic Particle Detector, SupraThermal Electrons and Protons, Burst - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-STEP-HCAD: Solar Orbiter, Level 2 Data, Energetic Particle Detector, SupraThermal Electrons and Protons, High Cadence - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_EPD-STEP-RATES: Solar Orbiter, Level 2 Data, Energetic Particle Detector, SupraThermal Electrons and Protons, Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_L2_MAG-RTN-BURST: Solar Orbiter Magnetometer L2 Data - T. Horbury (The Blackett Laboratory, Imperial College London)
SOLO_L2_MAG-RTN-NORMAL: Solar Orbiter Magnetometer L2 Data - T. Horbury (The Blackett Laboratory, Imperial College London)
SOLO_L2_MAG-RTN-NORMAL-1-MINUTE: Solar Orbiter Magnetometer L2 Data - T. Horbury (The Blackett Laboratory, Imperial College London)
SOLO_L2_MAG-SRF-BURST: Solar Orbiter Magnetometer L2 Data - T. Horbury (The Blackett Laboratory, Imperial College London)
SOLO_L2_MAG-SRF-NORMAL: Solar Orbiter Magnetometer L2 Data - T. Horbury (The Blackett Laboratory, Imperial College London)
SOLO_L2_RPW-HFR-SURV: Solar Orbiter Radio/Plasma Wave, HFR L2 parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_L2_RPW-LFR-SURV-ASM: Solar Orbiter Radio/Plasma Wave, LFR L2 parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_L2_RPW-LFR-SURV-BP1: Solar Orbiter Radio/Plasma Wave, LFR L2 parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_L2_RPW-LFR-SURV-BP2: Solar Orbiter Radio/Plasma Wave, LFR L2 parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_L2_RPW-LFR-SURV-CWF-B: Solar Orbiter Radio/Plasma Wave, LFR L2 magnetic parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_L2_RPW-LFR-SURV-CWF-E: Solar Orbiter Radio/Plasma Wave, LFR L2 electric parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_L2_RPW-LFR-SURV-SWF-B: Solar Orbiter Radio/Plasma Wave, LFR L2 magnetic parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_L2_RPW-LFR-SURV-SWF-E: Solar Orbiter Radio/Plasma Wave, LFR L2 electric parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_L2_RPW-TDS-SURV-HIST1D: Solar Orbiter Radio/Plasma Wave, TDS L2 parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_L2_RPW-TDS-SURV-HIST2D: Solar Orbiter Radio/Plasma Wave, TDS L2 parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_L2_RPW-TDS-SURV-MAMP: Solar Orbiter Radio/Plasma Wave, TDS L2 parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_L2_RPW-TDS-SURV-RSWF-B: Solar Orbiter Radio/Plasma Wave, TDS L2 magnetic parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_L2_RPW-TDS-SURV-RSWF-E: Solar Orbiter Radio/Plasma Wave, TDS L2 parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_L2_RPW-TDS-SURV-STAT: Solar Orbiter Radio/Plasma Wave, TDS L2R parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_L2_RPW-TDS-SURV-TSWF-B: Solar Orbiter Radio/Plasma Wave, TDS L2 magnetic parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_L2_RPW-TDS-SURV-TSWF-E: Solar Orbiter Radio/Plasma Wave, TDS L2S parameters - M.Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_LL02_EPD-EPT-ASUN-RATES: Solar Orbiter, Level 2 Low Latency, Energetic Particle Detector, Electron Proton Telescope, asun direction, Particle Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_LL02_EPD-EPT-NORTH-RATES: Solar Orbiter, Level 2 Low Latency, Energetic Particle Detector, Electron Proton Telescope, north direction, Particle Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_LL02_EPD-EPT-SOUTH-RATES: Solar Orbiter, Level 2 Low Latency, Energetic Particle Detector, Electron Proton Telescope, south direction, Particle Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_LL02_EPD-EPT-SUN-RATES: Solar Orbiter, Level 2 Low Latency, Energetic Particle Detector, Electron Proton Telescope, sun direction, Particle Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_LL02_EPD-HET-ASUN-RATES: Solar Orbiter, Level 2 Low Latency, Energetic Particle Detector, High Energy Telescope, asun direction, Particle Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_LL02_EPD-HET-NORTH-RATES: Solar Orbiter, Level 2 Low Latency, Energetic Particle Detector, High Energy Telescope, north direction, Particle Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_LL02_EPD-HET-SOUTH-RATES: Solar Orbiter, Level 2 Low Latency, Energetic Particle Detector, High Energy Telescope, south direction, Particle Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_LL02_EPD-HET-SUN-RATES: Solar Orbiter, Level 2 Low Latency, Energetic Particle Detector, High Energy Telescope, sun direction, Particle Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_LL02_EPD-SIS-A-RATES: Solar Orbiter, Level 2 Low Latency, Energetic Particle Detector, Suprathermal Ion Spectrograph A Telescope, Particle Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_LL02_EPD-SIS-B-RATES: Solar Orbiter, Level 2 Low Latency, Energetic Particle Detector, Suprathermal Ion Spectrograph B Telescope, Particle Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_LL02_EPD-STEP-RATES: Solar Orbiter, Level 2 Low Latency, Energetic Particle Detector, SupraThermal Electrons and Protons, Particle Rates - J. Rodriguez-Pacheco (Space Research Group, Universidad de Alcala)
SOLO_LL02_MAG: Solar Orbiter Level 2 Low Latency Magnetometer Data - T. Horbury (The Blackett Laboratory, Imperial College London)
SOLO_LL02_RPW-SBM1: Solar Orbiter Radio/Plasma Wave, LL02 parameters - M. Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_LL02_RPW-SBM2: Solar Orbiter Radio/Plasma Wave, LL02 parameters - M. Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_LL02_RPW-TNR: Solar Orbiter Radio/Plasma Wave, LL02 parameters - M. Maksimovic (LESIA, Observatoire de Paris-CNRS)
SOLO_LL02_SWA-EAS-SS: SWA-EAS Low Latency LL02 Data - C. J. Owen (MSSL-UCL, University College London, UK)
SOLO_LL02_SWA-PAS-MOM: SWA-PAS Quick Look Moments - C. J. Owen (MSSL-UCL, University College London, UK)
SO_AT_DEF: SOHO Definitive Attitude Data
SO_K0_CEL: SOHO Charge, Element and Isotope Analysis System, Key Parameters - Peter Bochsler (Physikalisches Institut, )
SO_K0_CST: SOHO ComprehensiveSuprathermal and EnergeticParticle Analyser - Horst Kunow (University of Kiel, Germany)
SO_K0_ERN: SOHO Energetic and Relativistic Nuclei and Electron experiment, Key Parameters - J Torsti (University of Turku)
SO_OR_DEF: SOHO Definitive Orbit Data
SO_OR_PRE: Soho Predicted Data Orbit
ST5-094_1SEC_MAG: Magnetometer>3 component magnetic field from miniature tri-axial magnetometer. - Delores Knipp (University of Colorado, Boulder)
ST5-155_1SEC_MAG: Magnetometer>3 component magnetic field from miniature tri-axial magnetometer. - Delores Knipp (University of Colorado, Boulder)
ST5-224_1SEC_MAG: Magnetometer>3 component magnetic field from miniature tri-axial magnetometer. - Delores Knipp (University of Colorado, Boulder)
STA_COHO1HR_MERGED_MAG_PLASMA: Merged hourly magnetic field, plasma, proton fluxes, and ephermis data - Natasha Papitashvili (NASA/GSFC)
STA_HELIO1DAY_POSITION: Position in heliocentric coordinates from SPDF Helioweb - Natalia Papitashvili (NASA/GSFC/SPDF)
STA_L1_IMPACT_BURST: STEREO Ahead IMPACT Burst Criteria - J. Luhmann (UCB/SSL)
STA_L1_IMPACT_HKP: STEREO Ahead IMPACT State of Health - J. Luhmann (UCB/SSL)
STA_L1_LET: STEREO Ahead IMPACT/LET Level 1 Data. - J. Luhmann (UCB/SSL)
STA_L1_MAGB_RTN: STEREO Ahead IMPACT/MAG Magnetic Field Vectors - J. Luhmann (UCB/SSL)
STA_L1_MAGB_SC: STEREO Ahead IMPACT/MAG Magnetic Field Vectors - J. Luhmann (UCB/SSL)
STA_L1_MAG_RTN: STEREO Ahead IMPACT/MAG Magnetic Field Vectors - J. Luhmann (UCB/SSL)
STA_L1_MAG_SC: STEREO Ahead IMPACT/MAG Magnetic Field Vectors - J. Luhmann (UCB/SSL)
STA_L1_SEPT: STEREO Ahead IMPACT/SEPT Level 1 Data - J. Luhmann (UCB/SSL)
STA_L1_SIT: STEREO Ahead IMPACT/SIT Level 1 Data - J. Luhmann (UCB/SSL)
STA_L1_STE: STEREO Ahead IMPACT/STE Spectra - J. Luhmann (UCB/SSL)
STA_L1_SWEA_DISB: STEREO Ahead IMPACT/SWEA 3D Burst Mode Distributions - J. Luhmann (UCB/SSL)
STA_L1_SWEA_DIST: STEREO Ahead IMPACT/SWEA 3D Distributions - J. Luhmann (UCB/SSL)
STA_L1_SWEA_SPEC: STEREO Ahead IMPACT/SWEA Spectra - J. Luhmann (UCB/SSL)
STA_L2_MAGPLASMA_1M: STEREO Behind IMPACT/MAG Magnetic Field and PLASTIC Solar Wind Plasma Data - J. Luhmann (UCB/SSL)
STA_L2_PLA_1DMAX_10MIN: STEREO/PLASTIC Level 2 - Dr. Antoinette Galvin (University of New Hampshire)
STA_L2_PLA_1DMAX_1HR: STEREO/PLASTIC Level 2 - Dr. Antoinette Galvin (University of New Hampshire)
STA_L2_PLA_1DMAX_1MIN: STEREO/PLASTIC Level 2 - Dr. Antoinette Galvin (University of New Hampshire)
STA_L2_PLA_IRON_Q_2HR: STEREO/PLASTIC Level 2 - Dr. Antoinette Galvin (University of New Hampshire)
STA_L3_PLA_HE2PL_F_VSW_01HR: He++ Phase Space Density (PSD) Binned by V/Vsw. - Dr. Antoinette Galvin (University of New Hampshire)
STA_L3_PLA_HEPLUS_24HR: He+ Fluxes Binned by V/Vsw, STEREO/PLASTIC Level 3 - Dr. Antoinette Galvin (University of New Hampshire)
STA_L3_PLA_HEPLUS_F_VSW_01HR: He+ Phase Space Density (PSD) Binned by V/Vsw. - Dr. Antoinette Galvin (University of New Hampshire)
STA_L3_PLA_HEPLUS_F_VSW_10MIN: He+ Phase Space Density (PSD) Binned by V/Vsw. - Dr. Antoinette Galvin (University of New Hampshire)
STA_L3_PLA_HEPLUS_F_VSW_24HR: He+ Phase Space Density (PSD) Binned by V/Vsw, STEREO/PLASTIC Level 3 - Dr. Antoinette Galvin (University of New Hampshire)
STA_L3_PLA_HEPLUS_SW_VELCTDIST_5MIN: He+ SW Frame Velocity Count Distributions. - Dr. Antoinette Galvin (University of New Hampshire)
STA_LB_IMPACT: STEREO Ahead IMPACT Beacon Data - J. Luhmann (UCB/SSL)
STA_LB_MAG_RTN: STEREO Ahead IMPACT/MAG Magnetic Field Vectors - J. Luhmann (UCB/SSL)
STA_LB_PLA_BROWSE: STEREO/PLASTIC Beacon Proton Parameters [PRELIM] - Dr. Antoinette Galvin (University of New Hampshire)
STB_COHO1HR_MERGED_MAG_PLASMA: Merged hourly magnetic field, plasma, proton fluxes, and ephermis data - Natasha Papitashvili (NASA/GSFC)
STB_HELIO1DAY_POSITION: Position in heliocentric coordinates from SPDF Helioweb - Natalia Papitashvili (NASA/GSFC/SPDF)
STB_L1_IMPACT_BURST: STEREO Ahead IMPACT Burst Criteria - J. Luhmann (UCB/SSL)
STB_L1_IMPACT_HKP: STEREO Behind IMPACT State of Health - J. Luhmann (UCB/SSL)
STB_L1_LET: STEREO Behind IMPACT/LET Level 1 Data. - J. Luhmann (UCB/SSL)
STB_L1_MAGB_RTN: STEREO Behind IMPACT/MAG Magnetic Field Vectors - J. Luhmann (UCB/SSL)
STB_L1_MAGB_SC: STEREO Behind IMPACT/MAG Magnetic Field Vectors - J. Luhmann (UCB/SSL)
STB_L1_MAG_RTN: STEREO Behind IMPACT/MAG Magnetic Field Vectors - J. Luhmann (UCB/SSL)
STB_L1_MAG_SC: STEREO Behind IMPACT/MAG Magnetic Field Vectors - J. Luhmann (UCB/SSL)
STB_L1_SEPT: STEREO Ahead IMPACT/SEPT Level 1 Data - J. Luhmann (UCB/SSL)
STB_L1_SIT: STEREO Behind IMPACT/SIT Level 1 Data - J. Luhmann (UCB/SSL)
STB_L1_STE: STEREO Behind IMPACT/STE Spectra - J. Luhmann (UCB/SSL)
STB_L1_SWEA_DISB: STEREO Ahead IMPACT/SWEA 3D Burst Mode Distributions - J. Luhmann (UCB/SSL)
STB_L1_SWEA_DIST: STEREO Ahead IMPACT/SWEA 3D Distributions - J. Luhmann (UCB/SSL)
STB_L1_SWEA_SPEC: STEREO Ahead IMPACT/SWEA Spectra - J. Luhmann (UCB/SSL)
STB_L2_MAGPLASMA_1M: STEREO Behind IMPACT/MAG Magnetic Field and PLASTIC Solar Wind Plasma Data - J. Luhmann (UCB/SSL)
STB_L2_PLA_1DMAX_10MIN: STEREO/PLASTIC Level 2 - Dr. Antoinette Galvin (University of New Hampshire)
STB_L2_PLA_1DMAX_1HR: STEREO/PLASTIC Level 2 - Dr. Antoinette Galvin (University of New Hampshire)
STB_L2_PLA_1DMAX_1MIN: STEREO/PLASTIC Level 2 - Dr. Antoinette Galvin (University of New Hampshire)
STB_L2_PLA_IRON_Q_2HR: STEREO/PLASTIC Level 2 - Dr. Antoinette Galvin (University of New Hampshire)
STB_LB_IMPACT: STEREO Ahead IMPACT Beacon Data - J. Luhmann (UCB/SSL)
STB_LB_PLA_BROWSE: STEREO/PLASTIC Beacon Proton Parameters [PRELIM] - Dr. Antoinette Galvin (University of New Hampshire)
STEREO_LEVEL2_SWAVES: STEREO WAVES (SWAVES) Radio Intensity Spectra, both Ahead and Behind s/c - M. Kaiser (NASA/GSFC)
SUISEI_HELIO1DAY_POSITION: Position in heliocentric coordinates from SPDF Helioweb - Natalia Papitashvili (NASA/GSFC/SPDF)
SX_K0_30F: 30-s averaged fluxes: 4 Instruments - Glenn Mason (U. Maryland )
SX_K0_POF: SAMPEX POLARCAP Averages: 4 Instruments - G.MASON (U.MD )

SAKIGAKE_HELIO1DAY_POSITION (spase://NASA/NumericalData/Sakigake/HelioWeb/Ephemeris/P1D)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SATURN_HELIO1DAY_POSITION (spase://NASA/NumericalData/Planet/Saturn/HelioWeb/Ephemeris/P1D)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SE_K0_AIS (spase://NASA/NumericalData/SESAME/KeyParameters/AIS/PT900S)
Description
Ionospheric parameters derived from quarter-hourly ionograms
Ref: Grubb,RN The NOAA SEL HF Radar system (ionospheric sounder) NOAA Tech Memo 
ERL SEL-55, Space Environ Lab, Boulder, CO, 1979
Ref: Jarvis,MJ & Dudeney ,JR Reduction of ambiguities in HF radar results
through a revised receiving array & sounding pattern. Radio Sci 21, 151-158,
1986
Ref: Satellite Experiments Simultaneous with Antarctic Measurements (SESAME), 
in GGS Instrument Papers, submitted to Space Science Reviews
Info:Rob Hibbins,Data manager,British Antarctic Survey,Cambridge,CB3 0ET,UK
E-mail: ggs@nbs.ac.uk
QUALITY_FLAG Comprised of several additive values each with a specific meaning:-
0 okay,+1 <6 echoes used for fmin,+2 <6 echoes for fEmax,+4 <6 echoes for fFmax,
+8 fmin approx= min tx frequency,+16 fEmax approx= max tx frequency,
+32 fFmax approx= max tx  frequency (tx=transmitter)
+64 High power tx off
+128 Echoes between 70-90Km
eg 37 indicates <6 echoes used for fmin & fFmax, & fFmax approx= max tx freq
Modification History
This is first  operational version
 
Dataset in CDAWeb
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SE_K0_FPI (spase://NASA/NumericalData/SESAME/KeyParameters/FPI/PT1800S)
Description
Measurements made looking in South and East directions (positive) 
Ref1: Satellite Experiments Simultaneous with Antarctic Measurements (SESAME),
in GGS Instrument Papers, submitted to Space Science Reviews.
Ref2: Nature,317,p45 1985. Ref3: R.D.Stewart, PhD Thesis, Univ of Ulster, 1986
Info:Keith Morrison,GGS Scientist,British Antarctic Survey,Cambridge,CB3 0ET,UK
E-mail: 19989::MORRISON
Modification History
29-Oct-92 Changes in accordance with new Standards & Conventions document
 
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SE_K0_MAG (spase://NASA/NumericalData/SESAME/KeyParameters/MAG/PT60S)
Description
H, D and Z components of the earth's magnetic field
Measuring variation of field relative to arbitrary baseline. Accurate to 1nT
1 minute data representing 'spot' values of the 1Hz sampling
Ref: Satellite Experiments Simultaneous with Antarctic Measurements (SESAME), 
in GGS Instrument Papers, submitted to Space Science Reviews
Info:Keith Morrison,GGS Scientist,British Antarctic Survey,Cambridge,CB3 0ET,UK
E-mail: 19989::MORRISON
 
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SE_K0_RIO (spase://NASA/NumericalData/SESAME/KeyParameters/RIO/PT60S)
Description
Equivalent overhead absorption measured 45 degrees to vertical in N,S,E,W 
directions, but in an L-shell-aligned coordinate system (ie rotated 17 degrees 
anti-clockwise from geographic). Preliminary Quiet-Day Curve used.
1 minute data represent 'spot' values of the 1Hz sampling
Accurate to 0.05dB, but possible baseline uncertainties of +/-0.5dB
Ref1: The multiple riometer system at Halley, Antarctica, in 
British Antarctic Survey Bulletin, no 72, p13-23, 1986
Ref2: Satellite Experiments Simultaneous with Antarctic Measurements (SESAME), 
in GGS Instrument Papers, submitted to Space Science Reviews
Info:Keith Morrison,GGS Scientist,British Antarctic Survey,Cambridge,CB3 0ET,UK
E-mail: 19989::MORRISON
 
Dataset in CDAWeb
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SE_K0_VLF (spase://NASA/NumericalData/SESAME/KeyParameters/VLF-ELF/PT60S)
Description
Omni-directional intensities in 2 narrow passband filters centred on 1kHz & 3kHz
Ref1: Satellite Experiments Simultaneous with Antarctic Measurements (SESAME),
in GGS Instrument Papers submitted to Space Science Reviews.
Ref2: VERSIM Newsletter No.4, p7 1992.
Info:Keith Morrison,GGS Scientist,British Antarctic Survey,Cambridge,CB3 0ET,UK
E-mail: 19989::MORRISON
Modification History
05-Aug-92 Changed fill values to +10.0E+30 and -2147483648
08-Oct-92 Changed DATA ENCODING to NETWORK. Added Quality and Post Gap Flags
Plotting range changed to  10-80
27-Oct-92 Put in Logical_file_id, ADID_ref, DEPEND_i, VAR_TYPE
 
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SNOE_L3_GEO (spase://NASA/NumericalData/SNOE/UVS/GEO/PT1S)
Description
Barth, C. A. and S. M. Bailey, Comparison of a thermospheric photochemical model
with SNOE observations of nitric oxide, J. Geophys. Res.,
doi:10.1029/2003JA010227, 2004.
 
Dataset in CDAWeb
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SNOE_L3_MAG (spase://NASA/NumericalData/SNOE/UVS/MAG/PT1S)
Description
Barth, C. A. and S. M. Bailey, Comparison of a thermospheric photochemical model
with SNOE observations of nitric oxide, J. Geophys. Res.,
doi:10.1029/2003JA010227, 2004.
 
Dataset in CDAWeb
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SOHO_HELIO1DAY_POSITION (spase://NASA/NumericalData/SOHO/HelioWeb/Ephemeris/P1D)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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SOLO_HELIO1DAY_POSITION
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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SOLO_L2_EPD-EPT-ASUN-BURST-ELE-CLOSE
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Changes in metadata
 
Dataset in CDAWeb
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SOLO_L2_EPD-EPT-ASUN-BURST-ION
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Changes in metadata
 
Dataset in CDAWeb
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SOLO_L2_EPD-EPT-ASUN-HCAD
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Add new data
 
Dataset in CDAWeb
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SOLO_L2_EPD-EPT-ASUN-RATES
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Add new data
 
Dataset in CDAWeb
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SOLO_L2_EPD-EPT-NORTH-BURST-ELE-CLOSE
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Changes in metadata
 
Dataset in CDAWeb
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SOLO_L2_EPD-EPT-NORTH-BURST-ION
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Changes in metadata
 
Dataset in CDAWeb
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SOLO_L2_EPD-EPT-NORTH-HCAD
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Add new data
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-EPT-NORTH-RATES
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Add new data
 
Dataset in CDAWeb
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SOLO_L2_EPD-EPT-SOUTH-BURST-ELE-CLOSE
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Changes in metadata
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-EPT-SOUTH-BURST-ION
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Changes in metadata
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-EPT-SOUTH-HCAD
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Add new data
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-EPT-SOUTH-RATES
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Add new data
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-EPT-SUN-BURST-ELE-CLOSE
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Changes in metadata
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-EPT-SUN-BURST-ION
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Changes in metadata
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-EPT-SUN-HCAD
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Add new data
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-EPT-SUN-RATES
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Add new data
 
Dataset in CDAWeb
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SOLO_L2_EPD-HET-ASUN-BURST
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Changes in metadata
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-HET-ASUN-RATES
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Add new data
 
Dataset in CDAWeb
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SOLO_L2_EPD-HET-NORTH-BURST
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Changes in metadata
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-HET-NORTH-RATES
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Add new data
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-HET-SOUTH-BURST
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Changes in metadata
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-HET-SOUTH-RATES
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Add new data
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-HET-SUN-BURST
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Changes in metadata
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-HET-SUN-RATES
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Add new data
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-SIS-A-HEHIST
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-SIS-A-RATES-FAST
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V03: Changes in metadata
V04: New calibration (V04)
V05: New calibration (V05)
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-SIS-A-RATES-MEDIUM
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-SIS-A-RATES-SLOW
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-SIS-B-HEHIST
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-SIS-B-RATES-FAST
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V03: Changes in metadata
V04: New calibration (V04)
V05: New calibration (V05)
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-SIS-B-RATES-MEDIUM
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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SOLO_L2_EPD-SIS-B-RATES-SLOW
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
 
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SOLO_L2_EPD-STEP-BURST
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
 
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SOLO_L2_EPD-STEP-HCAD
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Add new data
 
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SOLO_L2_EPD-STEP-RATES
Description
Energetic Particle Detector (EPD). Instrument suite, part of the scientific
payload aboard the Solar Orbiter mission, dedicated to the study of solar
energetic particles. EPD measures electrons, protons and heavy ions with high
temporal resolution over a wide energy range, from suprathermal energies to
several hundreds of MeV/nucleon. It is composed of four units: SupraThermal
Electrons and Protons (STEP), Electron Proton Telescope (EPT), Suprathermal Ion
Spectrograph (SIS) and High Energy Telescope (HET).
https://doi.org/10.1051/0004-6361/201935287
Modification History
V02: Add new data
 
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SOLO_L2_MAG-RTN-BURST
Description
Dual-sensor, triaxial fluxgate magnetometer
doi:10.1051/0004-6361/201937257
Modification History
V01 2019/12/11 I. Carrasco: Initial release
V02 2019/12/18 I. Carrasco: Second release
V03 2020/03/17 H. O'Brien: Third release
V04 2020/03/27 V. Evans: Fourth release
V05 2020/03/30 V. Evans: Fifth release
V06 2020/03/31 V. Evans: Sixth release
V07 2020/05/01 V. Angelini: Seventh release
V08 2020/06/18 V. Angelini: Eighth release
V07 2020/07/27 V. Angelini: Ninth release
V10 2020/08/18 V. Angelini: Tenth release
V11 2020/09/11 V. Angelini: Eleventh release
 
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SOLO_L2_MAG-RTN-NORMAL
Description
Dual-sensor, triaxial fluxgate magnetometer
doi:10.1051/0004-6361/201937257
Modification History
V01 2019/12/11 I. Carrasco: Initial release
V02 2019/12/18 I. Carrasco: Second release
V03 2020/03/17 H. O'Brien: Third release
V04 2020/03/27 V. Evans: Fourth release
V05 2020/03/30 V. Evans: Fifth release
V06 2020/03/31 V. Evans: Sixth release
V07 2020/05/01 V. Angelini: Seventh release
V08 2020/06/18 V. Angelini: Eighth release
V07 2020/07/27 V. Angelini: Ninth release
V10 2020/08/18 V. Angelini: Tenth release
V11 2020/09/11 V. Angelini: Eleventh release
 
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SOLO_L2_MAG-RTN-NORMAL-1-MINUTE
Description
Dual-sensor, triaxial fluxgate magnetometer
doi:10.1051/0004-6361/201937257
Modification History
V01 2019/12/11 I. Carrasco: Initial release
V02 2019/12/18 I. Carrasco: Second release
V03 2020/03/17 H. O'Brien: Third release
V04 2020/03/27 V. Evans: Fourth release
V05 2020/03/30 V. Evans: Fifth release
V06 2020/03/31 V. Evans: Sixth release
V07 2020/05/01 V. Angelini: Seventh release
V08 2020/06/18 V. Angelini: Eighth release
V07 2020/07/27 V. Angelini: Ninth release
V10 2020/08/18 V. Angelini: Tenth release
V11 2020/09/11 V. Angelini: Eleventh release
 
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SOLO_L2_MAG-SRF-BURST
Description
Dual-sensor, triaxial fluxgate magnetometer
doi:10.1051/0004-6361/201937257
Modification History
V01 2019/12/10 I. Carrasco: Initial release
V02 2019/12/18 I. Carrasco: Second release
V03 2020/03/17 H. O'Brien: Third release
V04 2020/03/27 V. Evans: Fourth release
V05 2020/03/30 V. Evans: Fifth release
V06 2020/03/31 V. Evans: Sixth release
V07 2020/03/31 V. Angelini: Seventh release
V08 2020/06/18 V. Angelini: Eighth release
V09 2020/07/27 V. Angelini: Ninth release
V10 2020/08/18 V. Angelini: Tenth release
V11 2020/09/11 V. Angelini: Eleventh release
 
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SOLO_L2_MAG-SRF-NORMAL
Description
Dual-sensor, triaxial fluxgate magnetometer
doi:10.1051/0004-6361/201937257
Modification History
V01 2019/12/10 I. Carrasco: Initial release
V02 2019/12/18 I. Carrasco: Second release
V03 2020/03/17 H. O'Brien: Third release
V04 2020/03/27 V. Evans: Fourth release
V05 2020/03/30 V. Evans: Fifth release
V06 2020/03/31 V. Evans: Sixth release
V07 2020/03/31 V. Angelini: Seventh release
V08 2020/06/18 V. Angelini: Eighth release
V09 2020/07/27 V. Angelini: Ninth release
V10 2020/08/18 V. Angelini: Tenth release
V11 2020/09/11 V. Angelini: Eleventh release
 
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SOLO_L2_RPW-HFR-SURV
Description
This file contains RPW HFR level 2 science survey data for the current day.
 
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SOLO_L2_RPW-LFR-SURV-ASM
Description
This file contains RPW LFR level 2R survey ASM data of the current test.
 
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SOLO_L2_RPW-LFR-SURV-BP1
Description
This file contains RPW LFR level 2R Survey BP1 data of the current test.
 
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SOLO_L2_RPW-LFR-SURV-BP2
Description
This file contains RPW LFR level 2R Survey BP2 data of the current test.
 
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SOLO_L2_RPW-LFR-SURV-CWF-B
Description
This file contains RPW LFR level 2 continous waveform of magnetic data in survey
mode
Modification History
2017-12-15, J-Y Brochot (CNRS-LPC2E), initial release
V04: Update for solo data definition, X. BONNIN (CNRS-LESIA), April 2019
V05: Update to compliant with SOL-SGS-TN-0009 Issue 2, Rev 4 - X.Bonnin, 09/2019
V06: add B_RTN and MAG_LABEL_RTN variables, J-Y Brochot, 12/2019
V07: March 2020 : Standardize SAMPLING_RATE and delete Test_* g.attrs - X.Bonnin
(CNRS, LESIA)
V07: Suppress zVars POST_GAP_FLAG, ACQUISITION_TIME, ACQUISITION_TIME_UNITS and
ACQUISITION_TIME_LABEL - J-Y Brochot, March 2020
V08: Add gAttr SPICE_KERNELS - J-Y Brochot, April 2020
V09: Complete the zAttr of CALIBRATION_TABLE_INDEX - J-Y Brochot, May 2020
V10: Add zVar L2_QUALITY_BITMASK - J-Y Brochot, Aug 2020
V11: Suppress zVar SYNCHRO_FLAG - J-Y Brochot, Sept 2020
 
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SOLO_L2_RPW-LFR-SURV-CWF-E
Description
This file contains RPW LFR level 2 continuous waveform of electric data in
survey mode.
 
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SOLO_L2_RPW-LFR-SURV-SWF-B
Description
This file contains RPW LFR level 2 snapshot waveform of magnetic data in survey
mode
Modification History
2017-12-15, J-Y Brochot (CNRS-LPC2E), initial release
V04: Update for solo data definition, X. BONNIN (CNRS-LESIA), April 2019
V05: Update to compliant with SOL-SGS-TN-0009 Issue 2, Rev 4 - X.Bonnin, 09/2019
V06: add B_RTN and MAG_LABEL_RTN variables, J-Y Brochot, 12/2019
V07: March 2020 : Harmonize SAMPLING_RATE zvar and Test_* g.attrs - X.Bonnin
(CNRS, LESIA)
V07: Suppress zVars POST_GAP_FLAG, ACQUISITION_TIME, ACQUISITION_TIME_UNITS and
ACQUISITION_TIME_LABEL - J-Y Brochot, March 2020
V08: Add gAttr SPICE_KERNELS - J-Y Brochot, April 2020
V09: Complete the zAttr of CALIBRATION_TABLE_INDEX - J-Y Brochot, May 2020
V10: Add zVar L2_QUALITY_BITMASK - J-Y Brochot, Aug 2020
V11: Suppress zVar SYNCHRO_FLAG - J-Y Brochot, Sept 2020
 
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SOLO_L2_RPW-LFR-SURV-SWF-E
Description
This file contains RPW LFR level 2 snapshot waveform of electric data in survey
mode.
 
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SOLO_L2_RPW-TDS-SURV-HIST1D
Description
This file contains RPW TDS level 2 regular snapshot Histogram 1D data.
 
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SOLO_L2_RPW-TDS-SURV-HIST2D
Description
This file contains RPW TDS level 2 regular snapshot Histogram 2D data.
 
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SOLO_L2_RPW-TDS-SURV-MAMP
Description
This file contains RPW TDS level 2 regular snapshot waveform data.
 
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SOLO_L2_RPW-TDS-SURV-RSWF-B
Description
This file contains RPW TDS level 2 regular snapshot waveform of magnetic data in
survey mode
Modification History
2017-12-15, J-Y Brochot (CNRS-LPC2E), initial release
V04: Update for solo data definition, X. BONNIN (CNRS-LESIA), April 2019
V05: Update to compliant with SOL-SGS-TN-0009 Issue 2, Rev 4 - X.Bonnin, 09/2019
Uniformisation of the version, J-Y Brochot, 12/2019
V07: March 2020 : Harmonize SAMPLING_RATE zvar and Test_* g.attrs - X.Bonnin
(CNRS, LESIA)
V07: Suppress zVars POST_GAP_FLAG, ACQUISITION_TIME, ACQUISITION_TIME_UNITS and
ACQUISITION_TIME_LABEL - J-Y Brochot, March 2020
V08: Add gAttr SPICE_KERNELS - J-Y Brochot, April 2020
V09: Complete the zAttr of CALIBRATION_TABLE_INDEX - J-Y Brochot, May 2020
V10: Add zVar L2_QUALITY_BITMASK - J-Y Brochot, Aug 2020
V11: Suppress zVars CHANNEL_ON, RPW_STATUS_INFO, INPUT_CONFIG, SYNCHRO_FLAG,
BUFFER_OVERFLOW, CHANNEL_OVERFLOW, RPW_STATUS_INFO_LABEL, SNAPSHOT_SEQ_NR,
CHANNEL_CONFIG - J-Y Brochot, Sept 2020
 
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SOLO_L2_RPW-TDS-SURV-RSWF-E
Description
This file contains RPW TDS level 2 regular snapshot E waveform data.
 
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SOLO_L2_RPW-TDS-SURV-STAT
Description
This file contains RPW TDS level 2 survey mode statistics.
 
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SOLO_L2_RPW-TDS-SURV-TSWF-B
Description
This file contains RPW TDS level 2 triggered snapshot waveform of magnetic data
in survey mode
Modification History
2017-12-15, J-Y Brochot (CNRS-LPC2E), initial release
V04: Update for solo data definition, X. BONNIN (CNRS-LESIA), April 2019
V05: Update to compliant with SOL-SGS-TN-0009 Issue 2, Rev 4 - X.Bonnin, 09/2019
V06: Uniformisation of the version, J-Y Brochot, 12/2019
V07: March 2020 : Harmonize SAMPLING_RATE zvar and Test_* g.attrs - X.Bonnin
(CNRS, LESIA)
V07:  : Suppress zVars POST_GAP_FLAG, ACQUISITION_TIME, ACQUISITION_TIME_UNITS
and ACQUISITION_TIME_LABEL - J-Y Brochot, March 2020
V08: Add gAttr SPICE_KERNELS - J-Y Brochot, April 2020
V09: Complete the zAttr of CALIBRATION_TABLE_INDEX - J-Y Brochot, May 2020
V10: Add zVar L2_QUALITY_BITMASK - J-Y Brochot, Aug 2020
V11: Suppress zVars CHANNEL_ON, RPW_STATUS_INFO, INPUT_CONFIG, SYNCHRO_FLAG,
BUFFER_OVERFLOW, CHANNEL_OVERFLOW, RPW_STATUS_INFO_LABEL, SNAPSHOT_SEQ_NR,
CHANNEL_CONFIG - J-Y Brochot, Sept 2020
 
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SOLO_L2_RPW-TDS-SURV-TSWF-E
Description
This file contains RPW TDS level 2 triggered snapshot E waveform data.
 
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SOLO_LL02_EPD-EPT-ASUN-RATES
Description
No TEXT global attribute value.
 
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SOLO_LL02_EPD-EPT-NORTH-RATES
Description
No TEXT global attribute value.
 
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SOLO_LL02_EPD-EPT-SOUTH-RATES
Description
No TEXT global attribute value.
 
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SOLO_LL02_EPD-EPT-SUN-RATES
Description
No TEXT global attribute value.
 
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SOLO_LL02_EPD-HET-ASUN-RATES
Description
No TEXT global attribute value.
 
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SOLO_LL02_EPD-HET-NORTH-RATES
Description
No TEXT global attribute value.
 
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SOLO_LL02_EPD-HET-SOUTH-RATES
Description
No TEXT global attribute value.
 
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SOLO_LL02_EPD-HET-SUN-RATES
Description
No TEXT global attribute value.
 
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SOLO_LL02_EPD-SIS-A-RATES
Description
No TEXT global attribute value.
 
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SOLO_LL02_EPD-SIS-B-RATES
Description
No TEXT global attribute value.
 
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SOLO_LL02_EPD-STEP-RATES
Description
No TEXT global attribute value.
 
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SOLO_LL02_MAG
Description
Dual-sensor, triaxial fluxgate magnetometer
doi:10.1026/1234567
 
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SOLO_LL02_RPW-SBM1
Description
This file contains RPW Low latency SBM1 data produced by the RPW Low Latency
data Pipeline.
 
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SOLO_LL02_RPW-SBM2
Description
This file contains RPW Low latency SBM2 data produced by the RPW Low Latency
data Pipeline.
 
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SOLO_LL02_RPW-TNR
Description
This file contains RPW Low latency TNR spectral power data, produced by the RPW
Low Latency Data Pipeline (LLDP).
 
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SOLO_LL02_SWA-EAS-SS
Description
No TEXT global attribute value.
 
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SOLO_LL02_SWA-PAS-MOM
Description
No TEXT global attribute value.
 
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SO_AT_DEF (spase://NASA/NumericalData/SOHO/Attitude/Definitive/PT10M)
Description
Data: 10 minute intervals
Modification History
5/6/94 - Original Implementation
1/25/96 - Added SARVariables for CCR 2189
 
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SO_K0_CEL (spase://NASA/NumericalData/SOHO/CELIAS/KP/PT5M)
Description
A description of the CELIAS instrument and scientific scope can be found on WWW 
at http://ubeclu.unibe.ch/phim/ms/soho/ or on the SOHO homepage 
http://sohowww.nascom.nasa.gov/
A written description of CELIAS will appear in the special issue of Solar 
Physics dedicated to SOHO 
Modification History
created Dec 1993
Modified by JT on 9/21/94
Modified by PW on 2/Mar/95
Modified by PW on 21/Jul/95
Modified by PW on 18/Aug/95
Modified by PW on 27/Nov/95
Modified by PW on 24/Jul/96
Modified by PW on  9/Jan/97
 
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SO_K0_CST (spase://NASA/NumericalData/SOHO/COSTEP/KP/PT5M)
Description
Data: 5 minute averages Time tag = center of interval 
References                    1.Kunow, H., et al., COSTEP -   Comprehensive
Suprathermal and  Energetic Particle Analyser for SOHO, in V. Domingo, editor,
The SOHO Mission - Scientific and  Technical Aspects of the        Instruments,
ESA SP-1104, pages 75 - 80, 1988 
2.Kunow, H., et al., COSTEP -  Comprehensive Suprathermal and  Energetic
Particle Analyser for SOHO - Scientific Goals and Data Description, Proc. First
SOHO  Workshop, ESA SP-348,           pages 43 - 46, 1992 
2.Mueller-Mellin, R., et al.,  COSTEP -                        Comprehensive
Suprathermal and  Energetic Particle Analyser,    to be published in            
 Solar Physics, 1995
 19 Dec 1996 Caveat: 1. The EPHIN E-detector developed gradually a noise problem
during 1996 and was switched off logically on 1996-305-14.40. Check EPHIN status
word >Ephin_Stat< bit 2 (2^2): if set to one: E detector  is on, if set to zero,
E detector is off. When off, the channels E3000, P41 and H41 show zero
intensity, the energy of the next lower channel E1300 is the average of E1300
and E3000, the width of channel E1300 is the sum of the  width E1300 and E3000;
P25, and H25 are changed accordingly.  Note: the KPGS calulates correctly the
new fluxes in channels E1300, P25, H25. Only their interpretation needs to be
changed by the user. 2. The geometric factor for the counting rate channels can
be changed either by ground command or autonomously by detecting high fluxes in
the center segment of detector A. Check EPHIN status word >Ephin_Stat<bits
9,10,11,12,13,17,18,19,20,21: if set to one: large geometric factor, if set to
zero: small geometric factor. Note: the KPGS software calculates correctly the
fluxes. No action needed by the user.
Modification History
 15 Feb 1994    Version  1.0 
 22 Nov 1994    Version  1.0                     Revision 1.0      new variables
COVER, DQF, STATUS
 28 Mar 1995    Version  1.0                     Revision 2.0      Energy ranges
updated           
 15 May 1995    Version  1.0                     Revision 3.0      Addition:
TEXT                   Correction: E_Energy [4]                     P_Energy [2]
                    P_Label             
 28 Nov 1995  Version  1.0.                    Revision 4.0        Correction: #
Var. from 24 to 25 Change: Descript. COST -> CST       Var_type data ->
support_data         at: Epoch, PB5                   at:  E_energy,  E_delta   
      at:  P_energy,  P_delta          at: He_energy, He_delta          at:
E_energy, E_delta  
 19 Dec 1996  Version  7.0. EPHIN E, P and He channel values adapted to new
investigations to geometry factors 
 
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SO_K0_ERN (spase://NASA/NumericalData/SOHO/ERNE/KP/PT128S)
Description
Data: 1 minute avarages Time tag = center of interval
Torsti et al.: ERNE - Energetic and Relativistic Nuclei and Electron experiment,
The SOHO Mission ESA SP-1104, 1988
Torsti et al.: Energetic Particle Experiment ERNEto be published in
SolarPhysics, 1995
M. Lumme and Eino Valtonen: CEPAC Experiment Operations Manual, November 1994 
ERNE WWW Home page  http://www.srl.utu.fi/projects/erne/erne.html  
Modification History
Version 01 19-Nov-1995. Modified by JT on Dec. 4, 1995Modified by TL on Aug 7
1996
 
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SO_OR_DEF (spase://NASA/NumericalData/SOHO/Ephemeris/Definitive/PT10M)
Description
TBS
Modification History
Originated Monday, May 13, 1991
Modified June 13, 1991 for version 2.1
Modified October 2,1991 for new global attributes, incr sizes
Modified 11/11/91 Add sun vector, replace space id with support id
Modified 1992 Feb 11 to use the variable name TIME and type CDF_INT4 instead of 
EPOCH and CDF_EPOCH for the time tags CCR 490
Modified 6/2/92 add project, discipline, source_name, data_version, title, and 
mods to global section; add validmin, validmax, labl_ptr_1 and monoton 
attributes to some variables; put epoch time back in, rename time to 
time_pb5; add label_time to variables
Modified 11/07/92 to use Epoch and Time_PB5 variable name
Modified 6/2/93 add ADID_ref and Logical_file_id
7/5/94 - CCR ISTP 1852 updated CDHF skeleton to CDF standards - JT
9/21/94 - Added 24 new global attributes to log the ephemeris 
comparison summary report from the definitive FDF orbit file.  CCR 1932
11/7/94 - Merged CCR 1852 changes and corrected errors 
made in CCR 1852.  ICCR 1884
12/7/94 - Modified MODS to follow ISTP standards.  ICCR 1885
01/05/95 - add heliocentric coordinate system.  CCR 1889
2/28/95 - added COMMENT1 and COMMENT2 for CCR 
11/03/95 - deleted crn_space for CCR 2154 - RM
09/20/96 - changed CRN to CRN_EARTH for CCR 2269
 
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SO_OR_PRE (spase://NASA/NumericalData/SOHO/Ephemeris/Predicted/PT10M)
Description
TBS
Modification History
Originated Monday, May 13, 1991
Modified June 13, 1991 for version 2.1
Modified October 2,1991 for new global attributes, incr sizes
Modified 11/11/91 Add sun vector, replace space id with support id
Modified 1992 Feb 11 to use the variable name TIME and type CDF_INT4 instead of 
EPOCH and CDF_EPOCH for the time tags CCR 490
Modified 6/2/92 add project, discipline, source_name, data_version, title, and 
mods to global section; add validmin, validmax, labl_ptr_1 and monoton 
attributes to some variables; put epoch time back in, rename time to 
time_pb5; add label_time to variables
Modified 11/07/92 to use Epoch and Time_PB5 variable name
Modified 6/2/93 add ADID_ref and Logical_file_id
7/5/94 - CCR ISTP 1852 updated CDHF skeleton to CDF standards - JT
9/21/94 - Added 24 new global attributes to log the ephemeris 
comparison summary report from the definitive FDF orbit file.  CCR 1932
11/7/94 - Merged CCR 1852 changes and corrected errors 
made in CCR 1852.  ICCR 1884
12/7/94 - Modified MODS to follow ISTP standards.  ICCR 1885
01/05/95 - add heliocentric coordinate system.  CCR 1889
2/28/95 - added COMMENT1 and COMMENT2 for CCR 
11/03/95 - deleted crn_space for CCR 2154 - RM
 
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ST5-094_1SEC_MAG (spase://NASA/NumericalData/ST5-094/Ephemeris/PT1M)
Description
Tri-axial magnetometer data from NASA Space Technology 5.
Modification History

Mon Dec  8 16:21:55 2014: in-place replacement of missing Gjerloev correction
values.
 
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ST5-155_1SEC_MAG (spase://NASA/NumericalData/ST5-155/Ephemeris/PT1M)
Description
Tri-axial magnetometer data from NASA Space Technology 5.
Modification History

Mon Dec  8 16:24:50 2014: in-place replacement of missing Gjerloev correction
values.
 
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ST5-224_1SEC_MAG (spase://NASA/NumericalData/ST5-224/Ephemeris/PT1M)
Description
Tri-axial magnetometer data from NASA Space Technology 5.
Modification History

Mon Dec  8 16:27:59 2014: in-place replacement of missing Gjerloev correction
values.
 
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STA_COHO1HR_MERGED_MAG_PLASMA (spase://NASA/NumericalData/STEREO-A/IMPACT_PLASTIC/COHOWEB/PT1H)
Description
The Solar-Terrestrial Relations Observatory (STEREO) mission includes two
spacecraft respectively lagging (STEREO A) and leading (STEREO B) the Earth in
heliocentric orbit around the Sun for remote 3-D imaging and radio observations
of coronal mass ejections (CMEs).  These events are responsible for large solar
energetic particle events in interplanetary space and are the primary cause of
major geomagnetic storms at Earth. The two spacecraft are launched to drift
slowly away from the Earth in opposite directions at about 10 degrees per year
for the lagging spacecraft and 20 degrees per year for the leading one. Optimal
longitudinal separation of about sixty degrees is achieved after two years.
Afterwards the separation gradually increases beyond the design lifetime of two
years with the possibility of extended mission observations at larger angles.
Science instruments selected for STEREO include the Sun Earth Connection Coronal
and Heliospheric Investigation (SECCHI) for extreme ultraviolet (EUV),
white-light coronographic, and heliospheric imaging, the STEREO/WAVES (SWAVES)
interplanetary radio burst tracker, the In situ Measurements of Particles and
CME Transients (IMPACT) investigation for in-situ sampling the 3-D distribution
and plasma characteristics of solar energetic particles and the interplanetary
magnetic field, and the PLAsma and SupraThermal Ion and Composition (PLASTIC)
experiment to measure elemental and charge composition of ambient and CME plasma
ions. STEREO data recorded and stored onboard each spacecraft will be downlinked
through the NASA Deep Space Network on a daily schedule. Real-time space weather
data will be continuously transmitted through a separate beacon system to NASA
and non-NASA receiving stations.
 About STEREO data in COHOWEB STEREO-A and -B data are from the magnetometer of
the IMPACT package and from the PLASTIC plasma detector.  Principal
Investigators for these packages are Janet Luhmann (UCB) and Antoinette Galvin
(UNH), respectively.  Magnetic field  data were obtained as 10-min averages from
the UCLA web site at
http://aten.igpp.ucla.edu/forms/stereo/ascii_PLASTIC_10m_new.html, courtesy of
C.T. Russell.  Proton Fluxes from .http://www.srl.caltech.edu/STEREO/.  COHOWeb's 
magnetic field hourly averages were created at GSFC/SPDF by averaging over the
six 10-min averages falling within each hour.  Hourly plasma parameter data,
including plasma flow direction angles for STEREO-A but not yet for STEREO B (as
of 7/11/2010), were obtained from UNH via .http://fiji.sr.unh.edu/1dmax_ascii/. 
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_HELIO1DAY_POSITION (spase://NASA/NumericalData/STEREO-A/HelioWeb/Ephemeris/P1D)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L1_IMPACT_BURST (spase://NASA/NumericalData/STEREO-A/IMPACT/Burst/L1/PT2S)
Description
The file contains burst criteria values from the IMPACT instrument on the STEREO
Ahead spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L1_IMPACT_HKP (spase://NASA/NumericalData/STEREO-A/IMPACT/Housekeeping/L1/PT2S)
Description
The file contains state of health data from the IMPACT instrument on the STEREO
Ahead spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L1_LET (spase://NASA/NumericalData/STEREO-A/IMPACT/LET/L1/PT1M)
Description
The file contains Level 1 IMPACT/LET data from the STEREO Ahead spacecraft.
Modification History
Version 5 changes made to new sectored fluxes
 
Dataset in CDAWeb
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STA_L1_MAGB_RTN (spase://NASA/NumericalData/STEREO-A/IMPACT/MAG/L1/Burst/RTN/PT0.031S)
Description
The file contains Level 1 magnetic field vectors from the IMPACT/MAG instrument
on the STEREO Ahead spacecraft.
Modification History
Version 1: Used internally at UCB and UCLA ONLY. No corrections applied to raw
MAG data.

Version 2: Offset correction applied to MAG data.

Version 3: Initial
algorithm for correcting glitches in the X sensor on STEREO Ahead
applied.

Version 4: Improvement in glitch correction algorithm
applied.

Version 5: Further refinement of glitch correction for X sensor on
STEREO Ahead. Also, two timing issues resolved: a) applying a 6ms time shift to
account for time lag between IMPACT IDPU and MAG, b) fixing an occasional 1
second "glitch".

Version 6: Added "FILTER_VALUE" variable
 
Dataset in CDAWeb
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STA_L1_MAGB_SC (spase://NASA/NumericalData/STEREO-A/IMPACT/MAG/L1/Burst/SC/PT0.031S)
Description
The file contains Level 1 magnetic field vectors from the IMPACT/MAG instrument
on the STEREO Ahead spacecraft.
Modification History
Version 1: Used internally at UCB and UCLA ONLY. No corrections applied to raw
MAG data.

Version 2: Offset correction applied to MAG data.

Version 3: Initial
algorithm for correcting glitches in the X sensor on STEREO Ahead
applied.

Version 4: Improvement in glitch correction algorithm
applied.

Version 5: Further refinement of glitch correction for X sensor on
STEREO Ahead. Also, two timing issues resolved: a) applying a 6ms time shift to
account for time lag between IMPACT IDPU and MAG, b) fixing an occasional 1
second "glitch".

Version 6: Added "FILTER_VALUE" variable
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L1_MAG_RTN (spase://NASA/NumericalData/STEREO-A/IMPACT/MAG/L1/PT0.125S)
Description
The file contains Level 1 magnetic field vectors from the IMPACT/MAG instrument
on the STEREO Ahead spacecraft.
Modification History
Version 1: Used internally at UCB and UCLA ONLY. No corrections applied to raw
MAG data.

Version 2: Offset correction applied to MAG data.

Version 3: Initial
algorithm for correcting glitches in the X sensor on STEREO Ahead
applied.

Version 4: Improvement in glitch correction algorithm
applied.

Version 5: Further refinement of glitch correction for X sensor on
STEREO Ahead. Also, two timing issues resolved: a) applying a 6ms time shift to
account for time lag between IMPACT IDPU and MAG, b) fixing an occasional 1
second "glitch".

Version 6: Added "FILTER_VALUE" variable
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L1_MAG_SC (spase://NASA/NumericalData/STEREO-A/IMPACT/MAG/SC/L1/PT0.125S)
Description
The file contains Level 1 magnetic field vectors from the IMPACT/MAG instrument
on the STEREO Ahead spacecraft.
Modification History
Version 1: Used internally at UCB and UCLA ONLY. No corrections applied to raw
MAG data.

Version 2: Offset correction applied to MAG data.

Version 3: Initial
algorithm for correcting glitches in the X sensor on STEREO Ahead
applied.

Version 4: Improvement in glitch correction algorithm
applied.

Version 5: Further refinement of glitch correction for X sensor on
STEREO Ahead. Also, two timing issues resolved: a) applying a 6ms time shift to
account for time lag between IMPACT IDPU and MAG, b) fixing an occasional 1
second "glitch".

Version 6: Added "FILTER_VALUE" variable
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L1_SEPT (spase://NASA/NumericalData/STEREO-A/IMPACT/SEPT/L1/PT1M)
Description
The file contains Level 1 IMPACT/SEPT data from the STEREO Ahead spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L1_SIT (spase://NASA/NumericalData/STEREO-A/IMPACT/SIT/L1/PT1M)
Description
The file contains Level 1 IMPACT/SIT data from the STEREO Ahead spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L1_STE (spase://NASA/NumericalData/STEREO-A/IMPACT/STE/L1/PT10S)
Description
The file contains Level 1 electron spectra from the IMPACT/STE instrument on the
STEREO Ahead spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L1_SWEA_DISB (spase://NASA/NumericalData/STEREO-A/IMPACT/SWEA/L1/PT2S)
Description
The file contains Level 1 3D burst mode electron distributions from the
IMPACT/SWEA instrument on the STEREO Ahead spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L1_SWEA_DIST (spase://NASA/NumericalData/STEREO-A/IMPACT/SWEA/L1/PT30S)
Description
The file contains Level 1 3D electron distributions from the IMPACT/SWEA
instrument on the STEREO Ahead spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L1_SWEA_SPEC (spase://NASA/NumericalData/STEREO-A/IMPACT/SWEA/Spectra/L1/PT10S)
Description
The file contains Level 1 spectra from the IMPACT/SWEA instrument on the STEREO
Ahead spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L2_MAGPLASMA_1M (spase://NASA/NumericalData/STEREO-A/MAGPLASMA/L2/PT1M)
Description
The file contains Level 2 magnetic field vectors from the IMPACT/MAG instrument
and solar wind parameters from the PLASTIC instrument on the STEREO Ahead
spacecraft.
Modification History
Version 1: Used internally at UCB and UCLA ONLY. No corrections applied to raw
MAG data...Version 2: Offset correction applied to MAG data...Version 3: Initial
algorithm for correcting glitches in the X sensor on STEREO Ahead
applied...Version 4: Improvement in glitch correction algorithm
applied...Version 5: Further refinement of glitch correction for X sensor on
STEREO Ahead. Also, two timing issues resolved: a) applying a 6ms time shift to
account for time lag between IMPACT IDPU and MAG, b) fixing an occasional 1
second "glitch"...Version 6: Added "FILTER_VALUE" variable
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L2_PLA_1DMAX_10MIN (spase://NASA/NumericalData/STEREO-A/PLASTIC/Protons/PT10M)
Description
PLASTIC - Plasma and Suprathermal Ion Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
Modification History
Initial Release 02/16/09. 
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L2_PLA_1DMAX_1HR (spase://NASA/NumericalData/STEREO-A/PLASTIC/Protons/PT1H)
Description
PLASTIC - Plasma and Suprathermal Ion Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
Modification History
Initial Release 02/16/09. 
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L2_PLA_1DMAX_1MIN (spase://NASA/NumericalData/STEREO-A/PLASTIC/Protons/PT1M)
Description
PLASTIC - Plasma and Suprathermal Ion Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
Modification History
Initial Release 02/16/09. 
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L2_PLA_IRON_Q_2HR (spase://NASA/NumericalData/STEREO-A/PLASTIC/Fe-abundance/PT2H)
Description
PLASTIC - Plasma and Suprathermal Ion Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
Modification History
Initial Release 08/16/10. 
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L3_PLA_HE2PL_F_VSW_01HR (spase://NASA/NumericalData/STEREO-A/PLASTIC/AlphaParticle/PhaseSpaceDensities/PT1H)
Description
PLASTIC - Plasma and Suprathermal Ion Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
Modification History
Initial Release 03/06/14. 
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L3_PLA_HEPLUS_24HR (spase://NASA/NumericalData/STEREO-A/PLASTIC/HeliumPlusParameter/P1D)
Description
PLASTIC - Plasma and Suprathermal Ion Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
Modification History
Initial Release 03/06/14. 
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L3_PLA_HEPLUS_F_VSW_01HR (spase://NASA/NumericalData/STEREO-A/PLASTIC/L3/PT1H)
Description
PLASTIC - Plasma and Suprathermal Ion Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
Modification History
Initial Release 03/06/14. 
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L3_PLA_HEPLUS_F_VSW_10MIN (spase://NASA/NumericalData/STEREO-A/PLASTIC/HeliumPlus/PhaseSpaceDensities/PT10M)
Description
PLASTIC - Plasma and Suprathermal Ion Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
Modification History
Initial Release 10/02/19. 
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L3_PLA_HEPLUS_F_VSW_24HR (spase://NASA/NumericalData/STEREO-A/PLASTIC/L3/P1D)
Description
PLASTIC - Plasma and Suprathermal Ion Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
Modification History
Initial Release 03/06/14. 
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_L3_PLA_HEPLUS_SW_VELCTDIST_5MIN (spase://NASA/NumericalData/STEREO-A/PLASTIC/HeliumPlus/VelocityCountDistributions/PT5M)
Description
PLASTIC - Plasma and Suprathermal Ion Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
Modification History
Initial Release 07/31/19. 
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_LB_IMPACT (spase://NASA/NumericalData/STEREO-A/IMPACT/LB/PT1M)
Description
This file contains Beacon data from the IMPACT experiment on the STEREO Ahead
spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_LB_MAG_RTN (spase://NASA/NumericalData/STEREO-A/IMPACT/MAG/RTN/LevelBeacon/PT0.125S)
Description
The file contains Level 1 magnetic field vectors from the IMPACT/MAG instrument
on the STEREO Ahead spacecraft.
Modification History
Version 1: Used internally at UCB and UCLA ONLY. No corrections applied to raw
MAG data.

Version 2: Offset correction applied to MAG data.

Version 3: Initial
algorithm for correcting glitches in the X sensor on STEREO Ahead
applied.

Version 4: Improvement in glitch correction algorithm
applied.

Version 5: Further refinement of glitch correction for X sensor on
STEREO Ahead. Also, two timing issues resolved: a) applying a 6ms time shift to
account for time lag between IMPACT IDPU and MAG, b) fixing an occasional 1
second "glitch".

Version 6: Added "FILTER_VALUE" variable
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STA_LB_PLA_BROWSE (spase://NASA/NumericalData/STEREO-A/PLASTIC/LB/Browse/PT1M)
Description
PLASTIC - Plasma and Suprathermal Ion and Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
PLASTIC Beacon data has not been validated and 
should not be used for publication purposes.
Modification History
Initial Release 06/14/2011.
 
Dataset in CDAWeb
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STB_COHO1HR_MERGED_MAG_PLASMA (spase://NASA/NumericalData/STEREO-B/IMPACT_PLASTIC/COHOWEB/PT1H)
Description
The Solar-Terrestrial Relations Observatory (STEREO) mission includes two
spacecraft respectively lagging (STEREO A) and leading (STEREO B) the Earth in
heliocentric orbit around the Sun for remote 3-D imaging and radio observations
of coronal mass ejections (CMEs).  These events are responsible for large solar
energetic particle events in interplanetary space and are the primary cause of
major geomagnetic storms at Earth. The two spacecraft are launched to drift
slowly away from the Earth in opposite directions at about 10 degrees per year
for the lagging spacecraft and 20 degrees per year for the leading one. Optimal
longitudinal separation of about sixty degrees is achieved after two years.
Afterwards the separation gradually increases beyond the design lifetime of two
years with the possibility of extended mission observations at larger angles.
Science instruments selected for STEREO include the Sun Earth Connection Coronal
and Heliospheric Investigation (SECCHI) for extreme ultraviolet (EUV),
white-light coronographic, and heliospheric imaging, the STEREO/WAVES (SWAVES)
interplanetary radio burst tracker, the In situ Measurements of Particles and
CME Transients (IMPACT) investigation for in-situ sampling the 3-D distribution
and plasma characteristics of solar energetic particles and the interplanetary
magnetic field, and the PLAsma and SupraThermal Ion and Composition (PLASTIC)
experiment to measure elemental and charge composition of ambient and CME plasma
ions. STEREO data recorded and stored onboard each spacecraft will be downlinked
through the NASA Deep Space Network on a daily schedule. Real-time space weather
data will be continuously transmitted through a separate beacon system to NASA
and non-NASA receiving stations.
 About STEREO data in COHOWEB STEREO-A and -B data are from the magnetometer of
the IMPACT package and from the PLASTIC plasma detector.  Principal
Investigators for these packages are Janet Luhmann (UCB) and Antoinette Galvin
(UNH), respectively.  Magnetic field  data were obtained as 10-min averages from
the UCLA web site at
http://aten.igpp.ucla.edu/forms/stereo/ascii_PLASTIC_10m_new.html, courtesy of
C.T. Russell. Proton Fluxes from .http://www.srl.caltech.edu/STEREO/.  COHOWeb's 
magnetic field hourly averages were created at GSFC/SPDF by averaging over the
six 10-min averages falling within each hour.  Hourly plasma parameter data,
including plasma flow direction angles for STEREO-A but not yet for STEREO B (as
of 7/11/2010), were obtained from UNH via .http://fiji.sr.unh.edu/1dmax_ascii/. 
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_HELIO1DAY_POSITION (spase://NASA/NumericalData/STEREO-B/HelioWeb/Ephemeris/P1D)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L1_IMPACT_BURST (spase://NASA/NumericalData/STEREO-B/IMPACT/Burst/L1/PT2S)
Description
The file contains burst criteria values from the IMPACT instrument on the STEREO
Behind spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L1_IMPACT_HKP (spase://NASA/NumericalData/STEREO-B/IMPACT/Housekeeping/L1/PT2S)
Description
The file contains state of health data from the IMPACT instrument on the STEREO
Behind spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L1_LET (spase://NASA/NumericalData/STEREO-B/IMPACT/LET/L1/PT1M)
Description
The file contains Level 1 IMPACT/LET data from the STEREO Behind spacecraft.
Modification History
Version 5 changes made to new sectored fluxes
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L1_MAGB_RTN (spase://NASA/NumericalData/STEREO-B/IMPACT/MAG/L1/Burst/RTN/PT0.031S)
Description
The file contains Level 1 magnetic field vectors from the IMPACT/MAG instrument
on the STEREO Behind spacecraft.
Modification History
Version 1: Used internally at UCB and UCLA ONLY. No corrections applied to raw
MAG data.

Version 2: Offset correction applied to MAG data.

Version 3: Initial
algorithm for correcting glitches in the X sensor on STEREO Ahead
applied.

Version 4: Improvement in glitch correction algorithm
applied.

Version 5: Further refinement of glitch correction for X sensor on
STEREO Ahead. Also, two timing issues resolved: a) applying a 6ms time shift to
account for time lag between IMPACT IDPU and MAG, b) fixing an occasional 1
second "glitch".

Version 6: Added "FILTER_VALUE" variable

 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L1_MAGB_SC (spase://NASA/NumericalData/STEREO-B/IMPACT/MAG/L1/Burst/SC/PT0.031S)
Description
The file contains Level 1 magnetic field vectors from the IMPACT/MAG instrument
on the STEREO Behind spacecraft.
Modification History
Version 1: Used internally at UCB and UCLA ONLY. No corrections applied to raw
MAG data.

Version 2: Offset correction applied to MAG data.

Version 3: Initial
algorithm for correcting glitches in the X sensor on STEREO Ahead
applied.

Version 4: Improvement in glitch correction algorithm
applied.

Version 5: Further refinement of glitch correction for X sensor on
STEREO Ahead. Also, two timing issues resolved: a) applying a 6ms time shift to
account for time lag between IMPACT IDPU and MAG, b) fixing an occasional 1
second "glitch".

Version 6: Added "FILTER_VALUE" variable
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L1_MAG_RTN (spase://NASA/NumericalData/STEREO-B/IMPACT/MAG/L1/PT0.125S)
Description
The file contains Level 1 magnetic field vectors from the IMPACT/MAG instrument
on the STEREO Behind spacecraft.
Modification History
Version 1: Used internally at UCB and UCLA ONLY. No corrections applied to raw
MAG data.

Version 2: Offset correction applied to MAG data.

Version 3: Initial
algorithm for correcting glitches in the X sensor on STEREO Ahead
applied.

Version 4: Improvement in glitch correction algorithm
applied.

Version 5: Further refinement of glitch correction for X sensor on
STEREO Ahead. Also, two timing issues resolved: a) applying a 6ms time shift to
account for time lag between IMPACT IDPU and MAG, b) fixing an occasional 1
second "glitch".

Version 6: Added "FILTER_VALUE" variable

 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L1_MAG_SC (spase://NASA/NumericalData/STEREO-B/IMPACT/MAG/SC/L1/PT0.125S)
Description
The file contains Level 1 magnetic field vectors from the IMPACT/MAG instrument
on the STEREO Behind spacecraft.
Modification History
Version 1: Used internally at UCB and UCLA ONLY. No corrections applied to raw
MAG data.

Version 2: Offset correction applied to MAG data.

Version 3: Initial
algorithm for correcting glitches in the X sensor on STEREO Ahead
applied.

Version 4: Improvement in glitch correction algorithm
applied.

Version 5: Further refinement of glitch correction for X sensor on
STEREO Ahead. Also, two timing issues resolved: a) applying a 6ms time shift to
account for time lag between IMPACT IDPU and MAG, b) fixing an occasional 1
second "glitch".

Version 6: Added "FILTER_VALUE" variable
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L1_SEPT (spase://NASA/NumericalData/STEREO-B/IMPACT/SEPT/L1/PT1M)
Description
The file contains Level 1 IMPACT/SEPT data from the STEREO Behind spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L1_SIT (spase://NASA/NumericalData/STEREO-B/IMPACT/SIT/L1/PT1M)
Description
The file contains Level 1 IMPACT/SIT data from the STEREO Behind spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L1_STE (spase://NASA/NumericalData/STEREO-B/IMPACT/STE/L1/PT10S)
Description
The file contains Level 1 electron spectra from the IMPACT/STE instrument on the
STEREO Behind spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L1_SWEA_DISB (spase://NASA/NumericalData/STEREO-B/IMPACT/SWEA/L1/PT2S)
Description
The file contains Level 1 3D burst mode electron distributions from the
IMPACT/SWEA instrument on the STEREO Behind spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L1_SWEA_DIST (spase://NASA/NumericalData/STEREO-B/IMPACT/SWEA/L1/PT30S)
Description
The file contains Level 1 3D electron distributions from the IMPACT/SWEA
instrument on the STEREO Behind spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L1_SWEA_SPEC (spase://NASA/NumericalData/STEREO-B/IMPACT/SWEA/Spectra/L1/PT10S)
Description
The file contains Level 1 spectra from the IMPACT/SWEA instrument on the STEREO
Behind spacecraft.
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L2_MAGPLASMA_1M (spase://NASA/NumericalData/STEREO-B/MAGPLASMA/L2/PT1M)
Description
The file contains Level 2 magnetic field vectors from the IMPACT/MAG instrument
and solar wind parameters from the PLASTIC instrument on the STEREO Behind
spacecraft.
Modification History
Version 1: Used internally at UCB and UCLA ONLY. No corrections applied to raw
MAG data...Version 2: Offset correction applied to MAG data...Version 3: Initial
algorithm for correcting glitches in the X sensor on STEREO Ahead
applied...Version 4: Improvement in glitch correction algorithm
applied...Version 5: Further refinement of glitch correction for X sensor on
STEREO Ahead. Also, two timing issues resolved: a) applying a 6ms time shift to
account for time lag between IMPACT IDPU and MAG, b) fixing an occasional 1
second "glitch"...Version 6: Added "FILTER_VALUE" variable
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L2_PLA_1DMAX_10MIN (spase://NASA/NumericalData/STEREO-B/PLASTIC/Protons/PT10M)
Description
PLASTIC - Plasma and Suprathermal Ion Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
Modification History
Initial Release 02/16/09. 
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L2_PLA_1DMAX_1HR (spase://NASA/NumericalData/STEREO-B/PLASTIC/Protons/PT1H)
Description
PLASTIC - Plasma and Suprathermal Ion Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
Modification History
Initial Release 02/16/09. 
 
Dataset in CDAWeb
Python/ IDL  Data Access Code Examples
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STB_L2_PLA_1DMAX_1MIN (spase://NASA/NumericalData/STEREO-B/PLASTIC/Protons/PT1M)
Description
PLASTIC - Plasma and Suprathermal Ion Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
Modification History
Initial Release 02/16/09. 
 
Dataset in CDAWeb
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STB_L2_PLA_IRON_Q_2HR (spase://NASA/NumericalData/STEREO-B/PLASTIC/Fe-abundance/PT2H)
Description
PLASTIC - Plasma and Suprathermal Ion Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
Modification History
Initial Release 08/16/10. 
 
Dataset in CDAWeb
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STB_LB_IMPACT (spase://NASA/NumericalData/STEREO-B/IMPACT/LB/PT1M)
Description
This file contains Beacon data from the IMPACT experiment on the STEREO Behind
spacecraft.
 
Dataset in CDAWeb
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STB_LB_PLA_BROWSE (spase://NASA/NumericalData/STEREO-B/PLASTIC/LB/Browse/PT1M)
Description
PLASTIC - Plasma and Suprathermal Ion and Composition.
References: .http://stereo.sr.unh.edu/stereo.html. 
PLASTIC Beacon data has not been validated and 
should not be used for publication purposes.
Modification History
Initial Release 06/14/2011.
 
Dataset in CDAWeb
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STEREO_LEVEL2_SWAVES (spase://NASA/NumericalData/STEREO/SWAVES/DS/Combined/PT1M)
Description
The file contains 1 minute averaged radio intensity data.
 
Dataset in CDAWeb
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SUISEI_HELIO1DAY_POSITION (spase://NASA/NumericalData/Suisei/HelioWeb/Ephemeris/P1D)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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SX_K0_30F (spase://NASA/NumericalData/SAMPEX/PT30.00S)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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SX_K0_POF (spase://NASA/NumericalData/SAMPEX/PCA/PT48M)
Description
No TEXT global attribute value.
 
Dataset in CDAWeb
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