2.3.2 spase://NASA/NumericalData/Wind/SMS/STICS/DistributionFunction/Level2/Magnetosphere/AlphaParticle/PT3M Wind SMS Suite, SupraThermal Ion Composition Spectrometer (SMS/STICS) Alpha Particle Distribution Function and Differential Flux, Magnetosphere, Level 2 (L2), PT3M Data 2021-04-27T15:38:11Z The Suprathermal Ion Composition Spectrometer (STICS) is a Time of Flight (TOF) Plasma Mass Spectrometer, capable of identifying Mass and Mass per Charge for incident Ions up to 200 keV/q. It uses an Electrostatic Analyzer to admit Ions of a particular Energy per Charge (E/Q) into the TOF Chamber. The E/Q Voltage is stepped through 32 Values, sitting at each Value for approximately 24 s, to measure Ions over the full E/Q Range of 6 keV/q to 200 keV/q. Ions then pass through a Carbon Foil and TOF Chamber, before finally impacting on a Solid-State Detector (SSD) for Energy Measurement. STICS combines these three Measurements of E/Q, TOF and Residual Energy, producing PHA Words. This Triple-Coincidence Technique greatly improves the Signal to Noise Ratio in the Data. Measurements of E/Q and TOF without Residual Energy also produce PHA Words. These Double-Coincidence Measurements are characterized by better Statistics since Ions whose Energy does not allow them to be registered by the SSD can still be counted in Double-Coincidence Measurements. However, Ion Identification in Double-Coincidence Measurements are limited to a select Number of Ions that are well separated in E/Q - TOF Space. The STICS Instrument provides full 3D Velocity Distribution Functions, through a Combination of multiple Telescopes and Spacecraft Spin. The Instrument includes three separate TOF Telescopes that view three separate Latitude Sectors, as shown in Figure 1. In addition, the WIND Spacecraft Spins, allowing the three Telescopes to trace out a nearly 4π sr Viewing Area. The Longitudinal Sectors are shown in Figure 2. The Solar Direction is in Sectors 8-10 while the Earthward Direction is in Sectors 0-2. Please acknowledge the Principal Investigator, G. Gloeckler, for providing the Data. spase://SMWG/Person/George.Gloeckler PrincipalInvestigator spase://SMWG/Person/Robert.M.Candey MetadataContact spase://SMWG/Person/Lee.Frost.Bargatze MetadataContact SMS Instrument Suite Home Page, UMD https://space.umd.edu/wind/ SMS (SWICS/MASS/STICS) Instrument Suite, Home Page, University of Maryland SMS Instrument Suite Web Page for Monthly and Daily Browse Plots, UMD https://space.umd.edu/wind/Data.html SMS (SWICS/MASS/STICS) Instrument Suite, Web Page for Monthly and Daily Browse Plots for SWICS up to February 1998 and STICS up to November 1998, University of Maryland WIND Instrument and Data Documentation Web Page, GSFC https://wind.nasa.gov/inst_info.php WIND Instrument and Data Documentation Web Page, Goddard Space Flight Center spase://VSPO/NumericalData/Wind/SMS/STICS/DistributionFunction/Level2/Magnetosphere/AlphaParticle/PT3M spase://SMWG/Repository/NASA/GSFC/SPDF Online Open FTPS from SPDF (not with most browsers) ftps://spdf.gsfc.nasa.gov/pub/data/wind/sms/l2/stics_cdf/he2plus_magnetosphere Access to Data in CDF Format via ftp from SPDF HTTPS from SPDF https://spdf.gsfc.nasa.gov/pub/data/wind/sms/l2/stics_cdf/he2plus_magnetosphere Access to Data in CDF Format via http from SPDF CDAWeb https://cdaweb.gsfc.nasa.gov/cgi-bin/eval2.cgi?dataset=WI_L2-HE2PLUS-3MIN_SMS-STICS-MAGNETOSPHERE&index=sp_phys WI_L2-HE2PLUS-3MIN_SMS-STICS-MAGNETOSPHERE Access to ASCII, CDF, and Plots via NASA/GSFC CDAWeb CDF None Please acknowledge the Principal Investigator, G. Gloeckler, for providing the Data. Please acknowledge the Data Providers and CDAWeb when using these Data. spase://SMWG/Repository/NASA/GSFC/SPDF Online Open CDAWeb HAPI Server https://cdaweb.gsfc.nasa.gov/hapi WI_L2-HE2PLUS-3MIN_SMS-STICS-MAGNETOSPHERE Web Service to this product using the HAPI interface. CSV Please acknowledge the Principal Investigator, G. Gloeckler, for providing the Data. Please acknowledge the Data Providers and CDAWeb when using these Data. Calibrated spase://SMWG/Instrument/Wind/SMS/STICS EnergeticParticles 1995-08-01T00:00:00.000 2004-04-28T23:59:59.999 PT3M Heliosphere Heliosphere.Inner Heliosphere.NearEarth Epoch Time, Start of Interval Epoch Epoch Time at the Start of the Averaging Interval This Parameter exhibits an increasing Monotonic Progression. PT3M ms 1.0e-3>s Epoch 6.2924580219904e+13 6.3745034619904e+13 01-Jan-1994 00:00:00.000 01-Jan-2020 00:00:00.000 -1.0e+31 Temporal Energy per Unit Charge Time Series defined by using: EPOCH eoq Energy over Charge, EOQ PT3M keV/q 1.602176565e-16>J/q Energy per Charge E12.5 32 Element 1 1 1 Element 2 2 2 Element 3 3 3 Element 4 4 4 Element 5 5 5 Element 6 6 6 Element 7 7 7 Element 8 8 8 Element 9 9 9 Element 10 10 10 Element 11 11 11 Element 12 12 12 Element 13 13 13 Element 14 14 14 Element 15 15 15 Element 16 16 16 Element 17 17 17 Element 18 18 18 Element 19 19 19 Element 20 20 20 Element 21 21 21 Element 22 22 22 Element 23 23 13 Element 24 24 14 Element 25 25 15 Element 26 26 16 Element 27 27 17 Element 28 28 28 Element 29 29 29 Element 30 30 30 Element 31 31 31 Element 32 32 32 0.0 100000.0 -1.0e+31 AlphaParticle Array Energy 2 Ion Species, HE2+ Time Series defined by using: EPOCH ion Ion Species, HE2+ PT3M Ion Species, HE2+ A4 -1.0e+31 Other Distribution Function, HE2+ Time Series defined by using: EPOCH DF Distribution Function, Phase Space Density Value, HE2+. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16]. Column 2 Labels from TELESCOPE_INDEX: [ 1, 2, 3]. Column 3 Labels from STEP_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 13, 14, 15, 16, 17, 28, 29, 30, 31, 32]. PT3M s^3/km^6 1.0e-18>s^3/m^6 DF HE2+ E12.5 16 3 32 -1.0e+31 AlphaParticle Array PhaseSpaceDensity 2 Distribution Function, HE2+, Telescope 1 Time Series defined by using: EPOCH DF_T1 Distribution Function, Phase Space Density Value, HE2+, Telescope 1, Plasmagram Display Type. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ARR_SLICE with the following input parameters: DF. PT3M s^3/km^6 1.0e-18>s^3/m^6 DF HE2+ T2 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array PhaseSpaceDensity 2 Distribution Function, HE2+, Telescope 1, by Sector as Spectrograms by Step Time Series defined by using: EPOCH DF_T1_bySec_atStep Distribution Function, HE2+, Telescope 1, at 5 Sectors as Spectrograms by Step. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ALTERNATE_VIEW with the following input parameters: DF_T1. PT3M s^3/km^6 1.0e-18>s^3/m^6 Spectrogram DF HE2+ T1 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array PhaseSpaceDensity 2 Distribution Function, HE2+, Telescope 1, by Step as Spectrograms by Sector Time Series defined by using: EPOCH DF_T1_byStep_atSec Distribution Function, HE2+, Telescope 1, at 9 Steps as Spectrograms by Sector. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ALTERNATE_VIEW with the following input parameters: DF_T1. PT3M s^3/km^6 1.0e-18>s^3/m^6 Spectrogram DF HE2+ T1 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array PhaseSpaceDensity 2 Distribution Function, HE2+, Telescope 2 Time Series defined by using: EPOCH DF_T2 Distribution Function, Phase Space Density Value, HE2+, Telescope 2, Plasmagram Display Type. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ARR_SLICE with the following input parameters: DF. PT3M s^3/km^6 1.0e-18>s^3/m^6 DF HE2+ T2 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array PhaseSpaceDensity 2 Distribution Function, HE2+, Telescope 2, by Sector as Spectrograms by Step Time Series defined by using: EPOCH DF_T2_bySec_atStep Distribution Function, HE2+, Telescope 2, at 5 Sectors as Spectrograms by Step. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ALTERNATE_VIEW with the following input parameters: DF_T2. PT3M s^3/km^6 1.0e-18>s^3/m^6 Spectrogram DF HE2+ T2 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array PhaseSpaceDensity 2 Distribution Function, HE2+, Telescope 2, by Step as Spectrograms by Sector Time Series defined by using: EPOCH DF_T2_byStep_atSec Distribution Function, HE2+, Telescope 2, at 9 Steps as Spectrograms by Sector. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ALTERNATE_VIEW with the following input parameters: DF_T2. PT3M s^3/km^6 1.0e-18>s^3/m^6 Spectrogram DF HE2+ T2 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array PhaseSpaceDensity 2 Distribution Function, HE2+, Telescope 3 Time Series defined by using: EPOCH DF_T3 Distribution Function, Phase Space Density Value, HE2+, Telescope 3, Plasmagram Display Type. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ARR_SLICE with the following input parameters: DF. PT3M s^3/km^6 1.0e-18>s^3/m^6 DF HE2+ T3 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array PhaseSpaceDensity 2 Distribution Function, HE2+, Telescope 3, by Sector as Spectrograms by Step Time Series defined by using: EPOCH DF_T3_bySec_atStep Distribution Function, HE2+, Telescope 3, at 5 Sectors as Spectrograms by Step. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ALTERNATE_VIEW with the following input parameters: DF_T3. PT3M s^3/km^6 1.0e-18>s^3/m^6 Spectrogram DF HE2+ T3 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array PhaseSpaceDensity 2 Distribution Function, HE2+, Telescope 3, by Step as Spectrograms by Sector Time Series defined by using: EPOCH DF_T3_byStep_atSec Distribution Function, HE2+, Telescope 3, at 9 Steps as Spectrograms by Sector. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ALTERNATE_VIEW with the following input parameters: DF_T3. PT3M s^3/km^6 1.0e-18>s^3/m^6 Spectrogram DF HE2+ T3 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array PhaseSpaceDensity 2 Velocity Distribution Function Error, HE2+ Time Series defined by using: EPOCH DF_error Error in Velocity Distribution Function Value, HE2+. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16]. Column 2 Labels from TELESCOPE_INDEX: [ 1, 2, 3]. Column 3 Labels from STEP_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 13, 14, 15, 16, 17, 28, 29, 30, 31, 32]. PT3M s^3/km^6 1.0e-18>s^3/m^6 DF Error HE2+ E12.5 16 3 32 -1.0e+31 AlphaParticle Array Uncertainty PhaseSpaceDensity 2 Counts, HE2+ Time Series defined by using: EPOCH counts Counts, Phase Space Density Value, HE2+. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16]. Column 2 Labels from TELESCOPE_INDEX: [ 1, 2, 3]. Column 3 Labels from STEP_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 13, 14, 15, 16, 17, 28, 29, 30, 31, 32]. PT3M Counts HE2+ E12.5 16 3 32 -1.0e+31 AlphaParticle Array PhaseSpaceDensity 2 Counts Error, HE2+ Time Series defined by using: EPOCH counts_error Error in Counts estimated assuming Poisson Statistics, HE2+. The Error is equal to the Square Root of the Number of Counts. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16]. Column 2 Labels from TELESCOPE_INDEX: [ 1, 2, 3]. Column 3 Labels from STEP_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 13, 14, 15, 16, 17, 28, 29, 30, 31, 32]. PT3M Counts Error HE2+ E12.5 16 3 32 -1.0e+31 AlphaParticle Array Uncertainty PhaseSpaceDensity 2 Differential Flux, HE2+ Time Series defined by using: EPOCH dJ Differential Flux, dJ/dE, HE2+. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16]. Column 2 Labels from TELESCOPE_INDEX: [ 1, 2, 3]. Column 3 Labels from STEP_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 13, 14, 15, 16, 17, 28, 29, 30, 31, 32]. PT3M eV/(cm^2 s sr eV) 1.0e4>J/(m^2 s sr J) dJ HE2+ E12.5 16 3 32 -1.0e+31 AlphaParticle Array Differential EnergyFlux 2 Differential Flux, HE2+, Telescope 1 Time Series defined by using: EPOCH dJ_T1 Differential Flux, dJ/dE, HE2+, Telescope 1, Plasmagram Display Type. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ARR_SLICE with the following input parameters: dJ. PT3M eV/(cm^2 s sr eV) 1.0e4>J/(m^2 s sr J) dJ HE2+ T2 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array Differential EnergyFlux 2 Differential Flux, HE2+, Telescope 1, by Sector as Spectrograms by Step Time Series defined by using: EPOCH dJ_T1_bySec_atStep Differential Flux, dJ/dE, HE2+, Telescope 1, at 5 Sectors as Spectrograms by Step. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ALTERNATE_VIEW with the following input parameters: dJ_T1. PT3M eV/(cm^2 s sr eV) 1.0e4>J/(m^2 s sr J) Spectrogram dJ HE2+ T1 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array Differential EnergyFlux 2 Differential Flux, HE2+, Telescope 1, by Step as Spectrograms by Sector Time Series defined by using: EPOCH dJ_T1_byStep_atSec Differential Flux, dJ/dE, HE2+, Telescope 1, at 9 Steps as Spectrograms by Sector. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ALTERNATE_VIEW with the following input parameters: dJ_T1. PT3M eV/(cm^2 s sr eV) 1.0e4>J/(m^2 s sr J) Spectrogram dJ HE2+ T1 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array Differential EnergyFlux 2 Differential Flux, HE2+, Telescope 2 Time Series defined by using: EPOCH dJ_T2 Differential Flux, dJ/dE, HE2+, Telescope 2, Plasmagram Display Type. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ARR_SLICE with the following input parameters: dJ. PT3M eV/(cm^2 s sr eV) 1.0e4>J/(m^2 s sr J) dJ HE2+ T2 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array Differential EnergyFlux 2 Differential Flux, HE2+, Telescope 2, by Sector as Spectrograms by Step Time Series defined by using: EPOCH dJ_T2_bySec_atStep Differential Flux, dJ/dE, HE2+, Telescope 2, at 5 Sectors as Spectrograms by Step. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ALTERNATE_VIEW with the following input parameters: dJ_T2. PT3M eV/(cm^2 s sr eV) 1.0e4>J/(m^2 s sr J) Spectrogram dJ HE2+ T2 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array Differential EnergyFlux 2 Differential Flux, HE2+, Telescope 2, by Step as Spectrograms by Sector Time Series defined by using: EPOCH dJ_T2_byStep_atSec Differential Flux, dJ/dE, HE2+, Telescope 2, at 9 Steps as Spectrograms by Sector. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ALTERNATE_VIEW with the following input parameters: dJ_T2. PT3M eV/(cm^2 s sr eV) 1.0e4>J/(m^2 s sr J) Spectrogram dJ HE2+ T2 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array Differential EnergyFlux 2 Differential Flux, HE2+, Telescope 3 Time Series defined by using: EPOCH dJ_T3 Differential Flux, dJ/dE, HE2+, Telescope 3, Plasmagram Display Type. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ARR_SLICE with the following input parameters: dJ. PT3M eV/(cm^2 s sr eV) 1.0e4>J/(m^2 s sr J) dJ HE2+ T3 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array Differential EnergyFlux 2 Differential Flux, HE2+, Telescope 3, by Sector as Spectrograms by Step Time Series defined by using: EPOCH dJ_T3_bySec_atStep Differential Flux, dJ/dE, HE2+, Telescope 3, at 5 Sectors as Spectrograms by Step. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ALTERNATE_VIEW with the following input parameters: dJ_T3. PT3M eV/(cm^2 s sr eV) 1.0e4>J/(m^2 s sr J) Spectrogram dJ HE2+ T3 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array Differential EnergyFlux 2 Differential Flux, HE2+, Telescope 3, by Step as Spectrograms by Sector Time Series defined by using: EPOCH dJ_T3_byStep_atSec Differential Flux, dJ/dE, HE2+, Telescope 3, at 9 Steps as Spectrograms by Sector. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16] This parameter is virtual. It is calculated by calling the function ALTERNATE_VIEW with the following input parameters: dJ_T3. PT3M eV/(cm^2 s sr eV) 1.0e4>J/(m^2 s sr J) Spectrogram dJ HE2+ T3 E12.5 LogScale 16 32 -1.0e+31 AlphaParticle Array Differential EnergyFlux 2 Differential Flux, Error, HE2+ Time Series defined by using: EPOCH dJ_error Differential Flux, dJ/dE, Error, HE2+. Column 1 Labels from SECTOR_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16]. Column 2 Labels from TELESCOPE_INDEX: [ 1, 2, 3]. Column 3 Labels from STEP_INDEX: [ 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 13, 14, 15, 16, 17, 28, 29, 30, 31, 32]. PT3M eV/(cm^2 s sr eV) 1.0e4>J/(m^2 s sr J) dJ Error HE2+ E12.5 16 3 32 -1.0e+31 AlphaParticle Array Differential EnergyFlux 2 Delta Time, HE2+ Time Series defined by using: EPOCH delT Delta Time, HE2+ PT3M delT HE2+ E12.5 0.0 100000.0 -1.0e+31 Scalar Temporal Sector Index Time Series defined by using: EPOCH SECTOR_index Sector Index PT3M Sector Index I2 LinearScale 16 1 16 -9 Other Telescope Index Time Series defined by using: EPOCH TELESCOPE_index Telescope Index PT3M I2 LinearScale 3 1 3 -9 Other Step Index Time Series defined by using: EPOCH STEP_index Step Index PT3M I2 LinearScale 32 1 32 -9 Other