2.7.1 https://spdx.org/licenses/ SPDX CC0-1.0 https://spdx.org/licenses/CC0-1.0.html Creative Commons Zero v1.0 Universal CC0 1.0 Universal is the Creative Commons license applicable to all publicly available SPASE metadata descriptions spase://NASA/NumericalData/ACE/SEPICA/L2/PT1H NASA NumericalData ACE Solar Energetic Particle Ionic Charge Analyzer (SEPICA) Energetic Ion Flux Intensities Values and Uncertainties, Level 2 (H2), 1 h Data https://doi.org/10.48322/3086-yq22 2025-12-04T13:28:24Z 2021-04-27T15:38:11 Only known prior ReleaseDate of the metadata 2022-08-19T12:34:56.789 Added DOI and PublicationInfo minted by JMW on 20220808, updated two InformationURL URLs, updated the RepositoryID, updated the SPDF MetadataContact Person to Robert M. Candey, metadata updated to SPASE 2.4.1, reviewed by LFB 20220819 2025-09-30T14:27:18Z Updated PublishedBy name to match ROR Registry. Added ResourceType and NamingAuthority. Changed http to https in top-level schemaLocation attribute. Fixed version number separator in top-level schemaLocation attribute. Matched version number in schemaLocation attribute to updated value in Version tag. ZCB 2025-12-04T13:28:24Z Added MetadataRightsList and RightsList(s). Updated to 2.7.1. ZCB This Data Product contains Measurements from the ACE Solar Energetic Particle Ionic Charge Analyzer (SEPICA) Instrument. SEPICA is used to determine the Charge State Distribution of Energetic Particle Distributions. SEPICA is designed to measure the Ionic Charge State, Q, the Kinetic Energy, E, and the Nuclear Charge, Z, of Energetic Ions above 0.2 MeV/n. This includes Ions accelerated in Solar Flares as well as in Interplanetary Space during Energetic Storm Particle (ESP) Events and Co-rotating Interaction Region (CIR) Events. For low Mass Numbers, SEPICA also separates Isotopes such as 3He and 4He. The Quality of the ACE Level 2 Data are such that it is suitable for serious Scientific Study. However, to avoid Confusion and Misunderstanding, it is recommended that Users consult with the appropriate ACE Team Members before publishing Work derived from the Data. The ACE Team has worked hard to ensure that the Level 2 Data are free from Errors, but the Team cannot accept Responsibility for erroneous Data, or for Misunderstandings about how the Data may be used. This is especially true if the appropriate ACE Team Members are not consulted before Publication. At the very least, Preprints should be forwarded to the ACE Team before Publication. E.S. Moebius, Please acknowledge the Principal Investigator, E.S. Moebius, University of New Hampshire See the Rules of Use available from the ACE Science Center at http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html. Popecki, M., Klecker, B., Kistler, L., and E. Möbius 2022-01-01T00:00:00 Space Physics Data Facility spase://SMWG/Person/Eberhard.S.Moebius PrincipalInvestigator spase://SMWG/Person/Robert.M.Candey MetadataContact spase://SMWG/Person/Lee.Frost.Bargatze MetadataContact spase://SMWG/Person/James.M.Weygand MetadataContact ACE Science Center Home Page for Level 2 Data Release Notes https://izw1.caltech.edu/ACE/ASC/level2/index.html ACE Level 2 Data Release Notes Home Page ACE Science Center Home Page for Level 2 Rules of Use https://izw1.caltech.edu/ACE/ASC/level2/policy_lvl2.html ACE Level 2 Rules of Use Home Page ACE Solar Energetic Particle Ionic Charge Analyzer (SEPICA) Instrument Home Page at the University of New Hampshire http://www.ssg.sr.unh.edu/tof/Missions/Ace/index.html?sepicamain.html ACE SEPICA Instrument Home Page at UNH spase://VSPO/NumericalData/ACE/SEPICA/PT3600S spase://VSPO/NumericalData/P_ACE_HDR_SEPICA_1HR spase://VSPO/NumericalData/ACE/SEPICA/L2/PT1H spase://SMWG/Repository/NASA/GSFC/SPDF/CDAWeb Online Open https://spdx.org/licenses/ SPDX CC0-1.0 https://spdx.org/licenses/CC0-1.0.html Creative Commons Zero v1.0 Universal CC0 1.0 Universal is the Creative Commons license applicable to all publicly available NASA Heliophysics data products FTPS from SPDF (not with most browsers) ftps://spdf.gsfc.nasa.gov/pub/data/ace/sepica/level_2_cdaweb/sep_h2/ Access to Data in CDF Format via ftp from SPDF HTTPS from SPDF https://spdf.gsfc.nasa.gov/pub/data/ace/sepica/level_2_cdaweb/sep_h2/ Access to Data in CDF Format via http from SPDF CDAWeb https://cdaweb.gsfc.nasa.gov/cgi-bin/eval2.cgi?dataset=AC_H2_SEP&index=sp_phys AC_H2_SEP Access to ASCII, CDF, and Plots via NASA/GSFC CDAWeb CDF None https://cdaweb.gsfc.nasa.gov/pub/data/ace/sepica/level_2_cdaweb/sep_h2/$Y ac_h2_sep_$Y$m$d_$v.cdf E.S. Moebius, Please acknowledge the Principal Investigator, E.S. Moebius, University of New Hampshire See the Rules of Use available from the ACE Science Center at http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html. Please acknowledge the Data Providers and CDAWeb when using these Data. spase://SMWG/Repository/NASA/GSFC/SPDF Online Open CDAWeb Programmatic Data Access https://cdaweb.gsfc.nasa.gov/WS/cdasr/1/dataviews/sp_phys/datasets/AC_H2_SEP/clientLibraryExample/ AC_H2_SEP Access to this data from common programming environments. Note: this AccessInformation element was added by HDPWS. Binary E.S. Moebius, Please acknowledge the Principal Investigator, E.S. Moebius, University of New Hampshire See the Rules of Use available from the ACE Science Center at http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html. Please acknowledge the Data Providers and CDAWeb when using these Data. spase://SMWG/Repository/NASA/GSFC/SPDF/CDAWeb Online Open https://spdx.org/licenses/ SPDX CC0-1.0 https://spdx.org/licenses/CC0-1.0.html Creative Commons Zero v1.0 Universal CC0 1.0 Universal is the Creative Commons license applicable to all publicly available NASA Heliophysics data products CDAWeb HAPI Server https://cdaweb.gsfc.nasa.gov/hapi AC_H2_SEP Web Service to this product using the HAPI interface. CSV E.S. Moebius, Please acknowledge the Principal Investigator, E.S. Moebius, University of New Hampshire See the Rules of Use available from the ACE Science Center at http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html. Please acknowledge the Data Providers and CDAWeb when using these Data. Calibrated spase://SMWG/Instrument/ACE/SEPICA EnergeticParticles IonComposition 1997-10-08T00:00:00.000 -P14D The Data become available about two Weeks after Observation PT1H Heliosphere Heliosphere.Inner Heliosphere.NearEarth Level 2 Files produced prior to the Production of Version 4 Data used SEPICA Matrix and Sectored Rates alone. The Problem with this, is that the Matrix and Sectored Rates alone cannot be used to take into account the Results of Trails moving out of the Box Definitions in the Data Processing Unit (DPU). The Version 4 SEPICA Data are the first Version of the Level 2 Files created by using the more advanced Pulse Height Analysis/Basic Rate Normalization Method. The Software producing these Files could not reliably track Large-Scale Pressure Changes and it was possible for Trail Contamination across Boxes to occur. Version 5 takes into account Changes in Pressure and reliably keeps the proper Trails in the proper Boxes, but a Bug introduced in Version 5 Generation Code caused the Boxes to give improper Flux Readings for He5, He6, He7, and He8. The Version 6 SEPICA Data are virtually identical to the Version 5 SEPICA Data except for the Removal of the aforementioned Bug. Helium Rates: Two Helium Rates have special Significance because they include the Ions from the internal Americium 241 (Am241) Calibration Source in SEPICA. These are the Helium 4 Calibration (He4cal) Rate and the Helium Calibration Alpha Particle Check (HeCAck) Rate. The Difference between them is that HeCAck bounds the Alpha Particle Peak much more closely than He4cal. On Quiet Days, Alpha Particles from the Am241 Calibration Source dominate the Instrument Counting Rate. Excluding the He4cal Rate from a Spectrum substantially eliminates Contamination by the Calibration Alpha Particles. Alternatively, the external Helium Rate in He4cal may be calculated by subtracting an average Value of He4cal obtained on Quiet Days. Also beware that the He8 Data spans the Energy per Nucleon Ranges He3, He4cal and He5 Channels to provide a Helium Flux with a Mean Energy of 1.4 MeV/n. He8 also includes the Contribution from the Calibration Alpha Particle Rate. Heavy Ion Rates in the Solid State Detector (SSD) High-Gain Mode: When the Solid State Detectors are in High-Gain Mode instead of Low-Gain Mode, the maximum measurable Energy decreases. This enhances Detection of Helium at the Expense of High Energy Heavy Ions. The following Rates are available when the SSDs are in High-Gain Mode: Hydrogen - H1, H2, H3, Carbon - ClowE, C1, C2, Helium - He1, He2, He3, He4cal, He5, He6, He8, HeCAck, Oxygen - O1, O2, Neon - Ne1, Magnesium - Mg1, Iron - Fe1. In the Period from Year 2000, Day 070 to Year 2000, Day 318, the Instrument was in High-Gain Mode. Low Energy (lowE) Rates: The Rates with the lowE Designation should always be used with Caution. These Rates may be contaminated by other Ions, and the Level of Contamination may depend on the Pressure in the Proportional Counter. The Reason for this is as follows. The Instrument consists of a Proportional Counter/Solid State Detector Telescope. Ion Species are identified by the Energy they deposit in each Detector. At certain low Energies, the Ion Species are difficult to distinguish from one another. The lowE Rates extend as far as possible into this Energy Range. As the Pressure Changes, the Limiting Energy for Species Identification changes somewhat and the Automatic Flux Calculation Algorithm may improperly include other Species. Epoch Time Epoch Epoch Time, Beginning of Interval Average Type: standard This Parameter exhibits an increasing Monotonic Progression. PT1H ms 1.0e-3>s Epoch E14.8 6.2987652219904e+13 6.3745034619904e+13 LinearScale 01-Jan-1996 00:00:00.000 01-Jan-2020 00:00:00.000 -1.0e+31 Temporal Time PB5 Time Series defined by using: EPOCH Time_PB5 Time PB5, Time of Observation, Year, Day, and Milliseconds of Day This Parameter exhibits an increasing Monotonic Progression. PT1H LinearScale 3 Year 1 a 1997 2020 year 1997 2020 Day of Year (Jan 1 = Day 1) 2 d 1 366 day 1 366 Elapsed seconds of day 3 s 0 86400 sec 0 86400 -2147483648 Temporal Hydrogen Flux Intensity, H1 Time Series defined by using: EPOCH H1 Hydrogen Flux Intensity, Channel H1, 0.65 MeV/n to 0.86 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries H_0.65-0.86 MeV/n E11.4 LogScale 0.0 1.0e+06 -1.0e+31 Proton Scalar NumberFlux 1 0.65 0.86 MeV/n Hydrogen Flux Intensity, H2 Time Series defined by using: EPOCH H2 Hydrogen Flux Intensity, Channel H2, 0.86 MeV/n to 1.94 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries H_0.86-1.94 MeV/n E11.4 LogScale 0.0 1.0e+06 -1.0e+31 Proton Scalar NumberFlux 1 0.86 1.94 MeV/n Hydrogen Flux Intensity, H3 Time Series defined by using: EPOCH H3 Hydrogen Flux Intensity, Channel H3, 1.94 MeV/n to 3.07 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries H_1.94-3.07 MeV/n E11.4 LogScale 0.0 1.0e+06 -1.0e+31 Proton Scalar NumberFlux 1 1.94 3.07 MeV/n Hydrogen Flux Intensity, H1, Uncertainty Time Series defined by using: EPOCH unc_H1 Hydrogen Flux Intensity, Channel H1, 0.65 MeV/n to 0.86 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_H_0.65-0.86 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Proton Scalar Uncertainty NumberFlux 1 0.65 0.86 MeV/n Hydrogen Flux Intensity, H2, Uncertainty Time Series defined by using: EPOCH unc_H2 Hydrogen Flux Intensity, Channel H2, 0.86 MeV/n to 1.94 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_H_0.86-1.94 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Proton Scalar Uncertainty NumberFlux 1 0.86 1.94 MeV/n Hydrogen Flux Intensity, H3, Uncertainty Time Series defined by using: EPOCH unc_H3 Hydrogen Flux Intensity, Channel H3, 1.94 MeV/n to 3.07 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_H_1.94-3.07 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Proton Scalar Uncertainty NumberFlux 1 1.94 3.07 MeV/n Helium Flux Intensity, He1 Time Series defined by using: EPOCH He1 Helium Flux Intensity, Channel He1, 0.40 MeV/n to 0.64 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries He_0.40-0.64 MeV/n E11.4 LogScale 0.0 1.0e+06 -1.0e+31 Ion Scalar NumberFlux 2 0.40 0.64 MeV/n Helium Flux Intensity, He2 Time Series defined by using: EPOCH He2 Helium Flux Intensity, Channel He2, 0.64 MeV/n to 0.88 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries He_0.64-0.88 MeV/n E11.4 LogScale 0.0 1.0e+06 -1.0e+31 Ion Scalar NumberFlux 2 0.64 0.88 MeV/n Helium Flux Intensity, He3 Time Series defined by using: EPOCH He3 Helium Flux Intensity, Channel He3, 0.88 MeV/n to 1.19 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries He_0.88-1.19 MeV/n E11.4 LogScale 0.0 1.0e+06 -1.0e+31 Ion Scalar NumberFlux 2 0.88 1.19 MeV/n Helium Flux Intensity, He4cal Time Series defined by using: EPOCH He4cal Helium Flux Intensity, Channel He4cal, 1.19 MeV/n to 1.49 MeV/n Two Helium Rates have special Significance because they include the Ions from the internal Americium 241 (Am241) Calibration Source in SEPICA. These are the Helium 4 Calibration (He4cal) Rate and the Helium Calibration Alpha Particle Check (HeCAck) Rate. The Difference between them is that HeCAck bounds the Alpha Particle Peak much more closely than He4cal. On Quiet Days, Alpha Particles from the Am241 Calibration Source dominate the Instrument Counting Rate. Excluding the He4cal Rate from a Spectrum substantially eliminates Contamination by the Calibration Alpha Particles. Alternatively, the external Helium Rate in He4cal may be calculated by subtracting an average Value of He4cal obtained on Quiet Days. PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries He4cal_1.19-1.49 MeV/n E11.4 LogScale 0.0 1.0e+06 -1.0e+31 Ion Scalar NumberFlux 2 1.19 1.49 MeV/n Helium Flux Intensity, He5 Time Series defined by using: EPOCH He5 Helium Flux Intensity, Channel He5, 1.49 MeV/n to 1.92 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries He_1.49-1.92 MeV/n E11.4 LogScale 0.0 1.0e+06 -1.0e+31 Ion Scalar NumberFlux 2 1.49 1.92 MeV/n Helium Flux Intensity, He6 Time Series defined by using: EPOCH He6 Helium Flux Intensity, Channel He6, 1.92 MeV/n to 3.06 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries He_1.92-3.06 MeV/n E11.4 LogScale 0.0 1.0e+06 -1.0e+31 Ion Scalar NumberFlux 2 1.92 3.06 MeV/n Helium Flux Intensity, He7 Time Series defined by using: EPOCH He7 Helium Flux Intensity, Channel He7, 3.06 MeV/n to 6.00 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries He_3.06-6.00 MeV/n E11.4 LogScale 0.0 1.0e+06 -1.0e+31 Ion Scalar NumberFlux 2 3.06 6.00 MeV/n Helium Flux Intensity, He8 Time Series defined by using: EPOCH He8 Helium Flux Intensity, Channel He8, 0.88 MeV/n to 1.92 MeV/n The He8 Data spans the Energy per Nucleon Ranges He3, He4cal and He5 Channels to provide a Helium Flux with a Mean Energy of 1.4 MeV/n. He8 also includes the Contribution from the Calibration Alpha Particle Rate. PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries He_0.88-1.92 MeV/n E11.4 LogScale 0.0 1.0e+06 -1.0e+31 Ion Scalar NumberFlux 2 0.88 1.92 MeV/n Helium Flux Intensity, HeCAck Time Series defined by using: EPOCH HeCAck Helium Flux Intensity, Channel HeCAck, 1.15 MeV/n to 1.50 MeV/n Two Helium Rates have special Significance because they include the Ions from the internal Americium 241 (Am241) Calibration Source in SEPICA. These are the Helium 4 Calibration (He4cal) Rate and the Helium Calibration Alpha Particle Check (HeCAck) Rate. The Difference between them is that HeCAck bounds the Alpha Particle Peak much more closely than He4cal. On Quiet Days, Alpha Particles from the Am241 Calibration Source dominate the Instrument Counting Rate. Excluding the He4cal Rate from a Spectrum substantially eliminates Contamination by the Calibration Alpha Particles. Alternatively, the external Helium Rate in He4cal may be calculated by subtracting an average Value of He4cal obtained on Quiet Days. PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries HeCAck_1.15-1.50 MeV/n E11.4 LogScale 0.0 1.0e+06 -1.0e+31 Ion Scalar NumberFlux 2 1.15 1.50 MeV/n Helium Flux Intensity, He1, Uncertainty Time Series defined by using: EPOCH unc_He1 Helium Flux Intensity, Channel He1, 0.40 MeV/n to 0.64 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_He_0.40-0.64 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 2 0.40 0.64 MeV/n Helium Flux Intensity, He2, Uncertainty Time Series defined by using: EPOCH unc_He2 Helium Flux Intensity, Channel He2, 0.64 MeV/n to 0.88 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_He_0.64-0.88 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 2 0.64 0.88 MeV/n Helium Flux Intensity, He3, Uncertainty Time Series defined by using: EPOCH unc_He3 Helium Flux Intensity, Channel He3, 0.88 MeV/n to 1.19 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_He_0.88-1.19 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 2 0.88 1.19 MeV/n Helium Flux Intensity, He4cal, Uncertainty Time Series defined by using: EPOCH unc_He4cal Helium Flux Intensity, Channel He4cal, 1.19 MeV/n to 1.49 MeV/n, Fractional Uncertainty Two Helium Rates have special Significance because they include the Ions from the internal Americium 241 (Am241) Calibration Source in SEPICA. These are the Helium 4 Calibration (He4cal) Rate and the Helium Calibration Alpha Particle Check (HeCAck) Rate. The Difference between them is that HeCAck bounds the Alpha Particle Peak much more closely than He4cal. On Quiet Days, Alpha Particles from the Am241 Calibration Source dominate the Instrument Counting Rate. Excluding the He4cal Rate from a Spectrum substantially eliminates Contamination by the Calibration Alpha Particles. Alternatively, the external Helium Rate in He4cal may be calculated by subtracting an average Value of He4cal obtained on Quiet Days. PT1H TimeSeries unc_He4cal_1.19-1.49 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 2 1.19 1.49 MeV/n Helium Flux Intensity, He5, Uncertainty Time Series defined by using: EPOCH unc_He5 Helium Flux Intensity, Channel He5, 1.49 MeV/n to 1.92 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_He_1.49-1.92 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 2 1.49 1.92 MeV/n Helium Flux Intensity, He6, Uncertainty Time Series defined by using: EPOCH unc_He6 Helium Flux Intensity, Channel He6, 1.92 MeV/n to 3.06 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_He_1.92-3.06 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 2 1.92 3.06 MeV/n Helium Flux Intensity, He7, Uncertainty Time Series defined by using: EPOCH unc_He7 Helium Flux Intensity, Channel He7, 3.06 MeV/n to 6.00 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_He_3.06-6.00 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 2 3.06 6.00 MeV/n Helium Flux Intensity, He8, Uncertainty Time Series defined by using: EPOCH unc_He8 Helium Flux Intensity, Channel He8, 0.88 MeV/n to 1.92 MeV/n, Fractional Uncertainty The He8 Data spans the Energy per Nucleon Ranges He3, He4cal and He5 Channels to provide a Helium Flux with a Mean Energy of 1.4 MeV/n. He8 also includes the Contribution from the Calibration Alpha Particle Rate. PT1H TimeSeries unc_He_0.88-1.92 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 2 0.88 1.92 MeV/n Helium Flux Intensity, HeCAck, Uncertainty Time Series defined by using: EPOCH unc_HeCAck Helium Flux Intensity, Channel HeCAck, 1.15 MeV/n to 1.50 MeV/n, Fractional Uncertainty Two Helium Rates have special Significance because they include the Ions from the internal Americium 241 (Am241) Calibration Source in SEPICA. These are the Helium 4 Calibration (He4cal) Rate and the Helium Calibration Alpha Particle Check (HeCAck) Rate. The Difference between them is that HeCAck bounds the Alpha Particle Peak much more closely than He4cal. On Quiet Days, Alpha Particles from the Am241 Calibration Source dominate the Instrument Counting Rate. Excluding the He4cal Rate from a Spectrum substantially eliminates Contamination by the Calibration Alpha Particles. Alternatively, the external Helium Rate in He4cal may be calculated by subtracting an average Value of He4cal obtained on Quiet Days. PT1H TimeSeries unc_HeCAck_1.15-1.50 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 2 1.15 1.50 MeV/n Carbon Flux Intensity, ClowE Time Series defined by using: EPOCH ClowE Carbon Flux Intensity, Channel ClowE, 0.33 MeV/n to 0.44 MeV/n Low Energy (lowE) Rates - The Rates with the lowE Designation should always be used with Caution. These Rates may be contaminated by other Ions, and the Level of Contamination may depend on the Pressure in the Proportional Counter. The Reason for this is as follows. The Instrument consists of a Proportional Counter/Solid State Detector Telescope. Ion Species are identified by the Energy they deposit in each Detector. At certain low Energies, the Ion Species are difficult to distinguish from one another. The lowE Rates extend as far as possible into this Energy Range. As the Pressure Changes, the Limiting Energy for Species Identification changes somewhat and the Automatic Flux Calculation Algorithm may improperly include other Species. PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Clo_0.33-0.44 MeV/n E11.4 LogScale 0.0 1.0e+08 -1.0e+31 Ion Scalar NumberFlux 6 0.33 0.44 MeV/n Carbon Flux Intensity, C1 Time Series defined by using: EPOCH C1 Carbon Flux Intensity, Channel C1, 0.45 MeV/n to 0.64 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries C_0.45-0.64 MeV/n E11.4 LogScale 0.0 1.0e+08 -1.0e+31 Ion Scalar NumberFlux 6 0.45 0.64 MeV/n Carbon Flux Intensity, C2 Time Series defined by using: EPOCH C2 Carbon Flux Intensity, Channel C2, 0.64 MeV/n to 0.86 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries C_0.64-0.86 MeV/n E11.4 LogScale 0.0 1.0e+08 -1.0e+31 Ion Scalar NumberFlux 6 0.64 0.86 MeV/n Carbon Flux Intensity, C3 Time Series defined by using: EPOCH C3 Carbon Flux Intensity, Channel C3, 0.86 MeV/n to 1.93 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries C_0.86-1.93 MeV/n E11.4 LogScale 0.0 1.0e+08 -1.0e+31 Ion Scalar NumberFlux 6 0.86 1.93 MeV/n Carbon Flux Intensity, C4 Time Series defined by using: EPOCH C4 Carbon Flux Intensity, Channel C4, 1.93 MeV/n to 3.06 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries C_1.93-3.06 MeV/n E11.4 LogScale 0.0 1.0e+08 -1.0e+31 Ion Scalar NumberFlux 6 1.93 3.06 MeV/n Carbon Flux Intensity, C5 Time Series defined by using: EPOCH C5 Carbon Flux Intensity, Channel C5, 3.10 MeV/n to 7.15 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries C_3.10-7.15 MeV/n E11.4 LogScale 0.0 1.0e+08 -1.0e+31 Ion Scalar NumberFlux 6 3.10 7.15 MeV/n Carbon Flux Intensity, C6 Time Series defined by using: EPOCH C6 Carbon Flux Intensity, Channel C6, 7.15 MeV/n to 11.75 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries C_7.15-11.75 MeV/n E11.4 LogScale 0.0 1.0e+08 -1.0e+31 Ion Scalar NumberFlux 6 7.15 11.75 MeV/n Carbon Flux Intensity, ClowE, Uncertainty Time Series defined by using: EPOCH unc_ClowE Carbon Flux Intensity, Channel ClowE, 0.33 MeV/n to 0.44 MeV/n, Fractional Uncertainty Low Energy (lowE) Rates - The Rates with the lowE Designation should always be used with Caution. These Rates may be contaminated by other Ions, and the Level of Contamination may depend on the Pressure in the Proportional Counter. The Reason for this is as follows. The Instrument consists of a Proportional Counter/Solid State Detector Telescope. Ion Species are identified by the Energy they deposit in each Detector. At certain low Energies, the Ion Species are difficult to distinguish from one another. The lowE Rates extend as far as possible into this Energy Range. As the Pressure Changes, the Limiting Energy for Species Identification changes somewhat and the Automatic Flux Calculation Algorithm may improperly include other Species. PT1H TimeSeries unc_Clo_0.33-0.44 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 6 0.33 0.44 MeV/n Carbon Flux Intensity, C1, Uncertainty Time Series defined by using: EPOCH unc_C1 Carbon Flux Intensity, Channel C1, 0.45 MeV/n to 0.64 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_C_0.45-0.64 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 6 0.45 0.64 MeV/n Carbon Flux Intensity, C2, Uncertainty Time Series defined by using: EPOCH unc_C2 Carbon Flux Intensity, Channel C2, 0.64 MeV/n to 0.86 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_C_0.64-0.86 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 6 0.64 0.86 MeV/n Carbon Flux Intensity, C3, Uncertainty Time Series defined by using: EPOCH unc_C3 Carbon Flux Intensity, Channel C3, 0.86 MeV/n to 1.93 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_C_0.86-1.93 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 6 0.86 1.93 MeV/n Carbon Flux Intensity, C4, Uncertainty Time Series defined by using: EPOCH unc_C4 Carbon Flux Intensity, Channel C4, 1.93 MeV/n to 3.06 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_C_1.93-3.06 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 6 1.93 3.06 MeV/n Carbon Flux Intensity, C5, Uncertainty Time Series defined by using: EPOCH unc_C5 Carbon Flux Intensity, Channel C5, 3.10 MeV/n to 7.15 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_C_3.10-7.15 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 6 3.10 7.15 MeV/n Carbon Flux Intensity, C6, Uncertainty Time Series defined by using: EPOCH unc_C6 Carbon Flux Intensity, Channel C6, 7.15 MeV/n to 11.75 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_C_7.15-11.75 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 6 7.15 11.75 MeV/n Nitrogen Flux Intensity, N1 Time Series defined by using: EPOCH N1 Nitrogen Flux Intensity, Channel N1, 0.36 MeV/n to 0.49 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries N_0.36-0.49 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 7 0.36 0.49 MeV/n Nitrogen Flux Intensity, N2 Time Series defined by using: EPOCH N2 Nitrogen Flux Intensity, Channel N2, 0.49 MeV/n to 1.74 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries N_0.49-1.74 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 7 0.49 1.74 MeV/n Nitrogen Flux Intensity, N3 Time Series defined by using: EPOCH N3 Nitrogen Flux Intensity, Channel N3, 1.74 MeV/n to 2.60 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries N_1.74-2.60 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 7 1.74 2.60 MeV/n Nitrogen Flux Intensity, N4 Time Series defined by using: EPOCH N4 Nitrogen Flux Intensity, Channel N4, 2.60 MeV/n to 3.46 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries N_2.6-3.46 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 7 2.60 3.46 MeV/n Nitrogen Flux Intensity, N5 Time Series defined by using: EPOCH N5 Nitrogen Flux Intensity, Channel N5, 3.46 MeV/n to 7.73 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries N_3.46-7.73 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 7 3.46 7.73 MeV/n Nitrogen Flux Intensity, N6 Time Series defined by using: EPOCH N6 Nitrogen Flux Intensity, Channel N6, 7.73 MeV/n to 12.28 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries N_7.73-12.28 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 7 7.73 12.28 MeV/n Nitrogen Flux Intensity, N1, Uncertainty Time Series defined by using: EPOCH unc_N1 Nitrogen Flux Intensity, Channel N1, 0.36 MeV/n to 0.49 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_N_0.36-0.49 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 7 0.36 0.49 MeV/n Nitrogen Flux Intensity, N2, Uncertainty Time Series defined by using: EPOCH unc_N2 Nitrogen Flux Intensity, Channel N2, 0.49 MeV/n to 1.74 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_N_0.49-1.74 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 7 0.49 1.74 MeV/n Nitrogen Flux Intensity, N3, Uncertainty Time Series defined by using: EPOCH unc_N3 Nitrogen Flux Intensity, Channel N3, 1.74 MeV/n to 2.60 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_N_1.74-2.60 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 7 1.74 2.60 MeV/n Nitrogen Flux Intensity, N4, Uncertainty Time Series defined by using: EPOCH unc_N4 Nitrogen Flux Intensity, Channel N4, 2.60 MeV/n to 3.46 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_N_2.6-3.46 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 7 2.60 3.46 MeV/n Nitrogen Flux Intensity, N5, Uncertainty Time Series defined by using: EPOCH unc_N5 Nitrogen Flux Intensity, Channel N5, 3.46 MeV/n to 7.73 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_N_3.46-7.73 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 7 3.46 7.73 MeV/n Nitrogen Flux Intensity, N6, Uncertainty Time Series defined by using: EPOCH unc_N6 Nitrogen Flux Intensity, Channel N6, 7.73 MeV/n to 12.28 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_N_7.73-12.28 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 7 7.73 12.28 MeV/n Oxygen Flux Intensity, OlowE Time Series defined by using: EPOCH OlowE Oxygen Flux Intensity, Channel OlowE, 0.05 MeV/n to 0.43 MeV/n Low Energy (lowE) Rates - The Rates with the lowE Designation should always be used with Caution. These Rates may be contaminated by other Ions, and the Level of Contamination may depend on the Pressure in the Proportional Counter. The Reason for this is as follows. The Instrument consists of a Proportional Counter/Solid State Detector Telescope. Ion Species are identified by the Energy they deposit in each Detector. At certain low Energies, the Ion Species are difficult to distinguish from one another. The lowE Rates extend as far as possible into this Energy Range. As the Pressure Changes, the Limiting Energy for Species Identification changes somewhat and the Automatic Flux Calculation Algorithm may improperly include other Species. PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Olo_0.05-0.43 MeV/n E11.4 LogScale 0.0 1.0e+07 -1.0e+31 Ion Scalar NumberFlux 8 0.05 0.43 MeV/n Oxygen Flux Intensity, O1 Time Series defined by using: EPOCH O1 Oxygen Flux Intensity, Channel O1, 0.43 MeV/n to 0.65 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries O_0.43-0.65 MeV/n E11.4 LogScale 0.0 1.0e+07 -1.0e+31 Ion Scalar NumberFlux 8 0.43 0.65 MeV/n Oxygen Flux Intensity, O2 Time Series defined by using: EPOCH O2 Oxygen Flux Intensity, Channel O2, 0.65 MeV/n to 0.86 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries O_0.65-0.86 MeV/n E11.4 LogScale 0.0 1.0e+07 -1.0e+31 Ion Scalar NumberFlux 8 0.65 0.86 MeV/n Oxygen Flux Intensity, O3 Time Series defined by using: EPOCH O3 Oxygen Flux Intensity, Channel O3, 0.86 MeV/n to 1.93 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries O_0.86-1.93 MeV/n E11.4 LogScale 0.0 1.0e+07 -1.0e+31 Ion Scalar NumberFlux 8 0.86 1.93 MeV/n Oxygen Flux Intensity, O4 Time Series defined by using: EPOCH O4 Oxygen Flux Intensity, Channel O4, 1.93 MeV/n to 3.07 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries O_1.93-3.07 MeV/n E11.4 LogScale 0.0 1.0e+07 -1.0e+31 Ion Scalar NumberFlux 8 1.93 3.07 MeV/n Oxygen Flux Intensity, O5 Time Series defined by using: EPOCH O5 Oxygen Flux Intensity, Channel O5, 3.08 MeV/n to 7.19 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries O_3.08-7.19 MeV/n E11.4 LogScale 0.0 1.0e+07 -1.0e+31 Ion Scalar NumberFlux 8 3.08 7.19 MeV/n Oxygen Flux Intensity, OlowE, Uncertainty Time Series defined by using: EPOCH unc_OlowE Oxygen Flux Intensity, Channel OlowE, 0.05 MeV/n to 0.43 MeV/n, Fractional Uncertainty Low Energy (lowE) Rates - The Rates with the lowE Designation should always be used with Caution. These Rates may be contaminated by other Ions, and the Level of Contamination may depend on the Pressure in the Proportional Counter. The Reason for this is as follows. The Instrument consists of a Proportional Counter/Solid State Detector Telescope. Ion Species are identified by the Energy they deposit in each Detector. At certain low Energies, the Ion Species are difficult to distinguish from one another. The lowE Rates extend as far as possible into this Energy Range. As the Pressure Changes, the Limiting Energy for Species Identification changes somewhat and the Automatic Flux Calculation Algorithm may improperly include other Species. PT1H TimeSeries unc_Olo_0.05-0.43 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 8 0.05 0.43 MeV/n Oxygen Flux Intensity, O1, Uncertainty Time Series defined by using: EPOCH unc_O1 Oxygen Flux Intensity, Channel O1, 0.43 MeV/n to 0.65 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_O_0.43-0.65 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 8 0.43 0.65 MeV/n Oxygen Flux Intensity, O2, Uncertainty Time Series defined by using: EPOCH unc_O2 Oxygen Flux Intensity, Channel O2, 0.65 MeV/n to 0.86 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_O_0.65-0.86 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 8 0.65 0.86 MeV/n Oxygen Flux Intensity, O3, Uncertainty Time Series defined by using: EPOCH unc_O3 Oxygen Flux Intensity, Channel O3, 0.86 MeV/n to 1.93 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_O_0.86-1.93 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 8 0.86 1.93 MeV/n Oxygen Flux Intensity, O4, Uncertainty Time Series defined by using: EPOCH unc_O4 Oxygen Flux Intensity, Channel O4, 1.93 MeV/n to 3.07 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_O_1.93-3.07 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 8 1.93 3.07 MeV/n Oxygen Flux Intensity, O5, Uncertainty Time Series defined by using: EPOCH unc_O5 Oxygen Flux Intensity, Channel O5, 3.08 MeV/n to 7.19 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_O_3.08-7.19 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 8 3.08 7.19 MeV/n Neon Flux Intensity, Ne1 Time Series defined by using: EPOCH Ne1 Neon Flux Intensity, Channel Ne1, 0.64 MeV/n to 0.86 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Ne_0.64-0.86 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 10 0.64 0.86 MeV/n Neon Flux Intensity, Ne2 Time Series defined by using: EPOCH Ne2 Neon Flux Intensity, Channel Ne2, 0.86 MeV/n to 1.94 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Ne_0.86-1.94 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 10 0.86 1.94 MeV/n Neon Flux Intensity, Ne3 Time Series defined by using: EPOCH Ne3 Neon Flux Intensity, Channel Ne3, 1.94 MeV/n to 3.07 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Ne_1.94-3.07 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 10 1.94 3.07 MeV/n Neon Flux Intensity, Ne4 Time Series defined by using: EPOCH Ne4 Neon Flux Intensity, Channel Ne4, 3.07 MeV/n to 7.19 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Ne_3.07-7.19 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 10 3.07 7.19 MeV/n Neon Flux Intensity, Ne1, Uncertainty Time Series defined by using: EPOCH unc_Ne1 Neon Flux Intensity, Channel Ne1, 0.64 MeV/n to 0.86 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Ne_0.64-0.86 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 10 0.64 0.86 MeV/n Neon Flux Intensity, Ne2, Uncertainty Time Series defined by using: EPOCH unc_Ne2 Neon Flux Intensity, Channel Ne2, 0.86 MeV/n to 1.94 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Ne_0.86-1.94 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 10 0.86 1.94 MeV/n Neon Flux Intensity, Ne3, Uncertainty Time Series defined by using: EPOCH unc_Ne3 Neon Flux Intensity, Channel Ne3, 1.94 MeV/n to 3.07 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Ne_1.94-3.07 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 10 1.94 3.07 MeV/n Neon Flux Intensity, Ne4, Uncertainty Time Series defined by using: EPOCH unc_Ne4 Neon Flux Intensity, Channel Ne4, 3.07 MeV/n to 7.19 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Ne_3.07-7.19 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 10 3.07 7.19 MeV/n Magnesium Flux Intensity, Mg1 Time Series defined by using: EPOCH Mg1 Magnesium Flux Intensity, Channel Mg1, 0.81 MeV/n to 0.90 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Mg_0.81-0.90 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 12 0.81 0.90 MeV/n Magnesium Flux Intensity, Mg2 Time Series defined by using: EPOCH Mg2 Magnesium Flux Intensity, Channel Mg2, 0.90 MeV/n to 1.92 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Mg_0.90-1.92 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 12 0.90 1.92 MeV/n Magnesium Flux Intensity, Mg3 Time Series defined by using: EPOCH Mg3 Magnesium Flux Intensity, Channel Mg3, 1.92 MeV/n to 3.07 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Mg_1.92-3.07 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 12 1.92 3.07 MeV/n Magnesium Flux Intensity, Mg4 Time Series defined by using: EPOCH Mg4 Magnesium Flux Intensity, Channel Mg4, 3.07 MeV/n to 6.02 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Mg_3.07-6.02 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 12 3.07 6.02 MeV/n Magnesium Flux Intensity, Mg1, Uncertainty Time Series defined by using: EPOCH unc_Mg1 Magnesium Flux Intensity, Channel Mg1, 0.81 MeV/n to 0.90 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Mg_0.81-0.90 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 12 0.81 0.90 MeV/n Magnesium Flux Intensity, Mg2, Uncertainty Time Series defined by using: EPOCH unc_Mg2 Magnesium Flux Intensity, Channel Mg2, 0.90 MeV/n to 1.92 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Mg_0.90-1.92 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 12 0.90 1.92 MeV/n Magnesium Flux Intensity, Mg3, Uncertainty Time Series defined by using: EPOCH unc_Mg3 Magnesium Flux Intensity, Channel Mg3, 1.92 MeV/n to 3.07 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Mg_1.92-3.07 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 12 1.92 3.07 MeV/n Magnesium Flux Intensity, Mg4, Uncertainty Time Series defined by using: EPOCH unc_Mg4 Magnesium Flux Intensity, Channel Mg4, 3.07 MeV/n to 6.02 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Mg_3.07-6.02 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 12 3.07 6.02 MeV/n Silicon Flux Intensity, Si1 Time Series defined by using: EPOCH Si1 Silicon Flux Intensity, Channel Si1, 0.76 MeV/n to 0.89 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Si_0.76-0.89 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 14 0.76 0.89 MeV/n Silicon Flux Intensity, Si2 Time Series defined by using: EPOCH Si2 Silicon Flux Intensity, Channel Si2, 0.89 MeV/n to 1.93 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Si_0.89-1.93 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 14 0.89 1.93 MeV/n Silicon Flux Intensity, Si3 Time Series defined by using: EPOCH Si3 Silicon Flux Intensity, Channel Si3, 1.93 MeV/n to 3.07 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Si_1.93-3.07 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 14 1.93 3.07 MeV/n Silicon Flux Intensity, Si4 Time Series defined by using: EPOCH Si4 Silicon Flux Intensity, Channel Si4, 3.07 MeV/n to 5.24 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Si_3.07-5.24 MeV/n E11.4 LogScale 0.0 100000.0 -1.0e+31 Ion Scalar NumberFlux 14 3.07 5.24 MeV/n Silicon Flux Intensity, Si1, Uncertainty Time Series defined by using: EPOCH unc_Si1 Silicon Flux Intensity, Channel Si1, 0.76 MeV/n to 0.89 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Si_0.76-0.89 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 14 0.76 0.89 MeV/n Silicon Flux Intensity, Si2, Uncertainty Time Series defined by using: EPOCH unc_Si2 Silicon Flux Intensity, Channel Si2, 0.89 MeV/n to 1.93 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Si_0.89-1.93 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 14 0.89 1.93 MeV/n Silicon Flux Intensity, Si3, Uncertainty Time Series defined by using: EPOCH unc_Si3 Silicon Flux Intensity, Channel Si3, 1.93 MeV/n to 3.07 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Si_1.93-3.07 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 14 1.93 3.07 MeV/n Silicon Flux Intensity, Si4, Uncertainty Time Series defined by using: EPOCH unc_Si4 Silicon Flux Intensity, Channel Si4, 3.07 MeV/n to 5.24 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Si_3.07-5.24 MeV/n E11.4 LogScale 0.0001 10.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 14 3.07 5.24 MeV/n Iron Flux Intensity, FeloE Time Series defined by using: EPOCH FeloE Iron Flux Intensity, Channel FeloE, 0.12 MeV/n to 0.43 MeV/n Low Energy (lowE) Rates - The Rates with the lowE Designation should always be used with Caution. These Rates may be contaminated by other Ions, and the Level of Contamination may depend on the Pressure in the Proportional Counter. The Reason for this is as follows. The Instrument consists of a Proportional Counter/Solid State Detector Telescope. Ion Species are identified by the Energy they deposit in each Detector. At certain low Energies, the Ion Species are difficult to distinguish from one another. The lowE Rates extend as far as possible into this Energy Range. As the Pressure Changes, the Limiting Energy for Species Identification changes somewhat and the Automatic Flux Calculation Algorithm may improperly include other Species. PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Felo_0.12-0.43 MeV/n E11.4 LogScale 0.0 1.0e+07 -1.0e+31 Ion Scalar NumberFlux 26 0.12 0.43 MeV/n Iron Flux Intensity, Fe1 Time Series defined by using: EPOCH Fe1 Iron Flux Intensity, Channel Fe1, 0.43 MeV/n to 0.64 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Fe_0.43-0.64 MeV/n E11.4 LogScale 0.0 1.0e+07 -1.0e+31 Ion Scalar NumberFlux 26 0.43 0.64 MeV/n Iron Flux Intensity, Fe2 Time Series defined by using: EPOCH Fe2 Iron Flux Intensity, Channel Fe2, 0.65 MeV/n to 0.86 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Fe_0.65-0.86 MeV/n E11.4 LogScale 0.0 1.0e+07 -1.0e+31 Ion Scalar NumberFlux 26 0.65 0.86 MeV/n Iron Flux Intensity, Fe3 Time Series defined by using: EPOCH Fe3 Iron Flux Intensity, Channel Fe3, 0.86 MeV/n to 1.93 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Fe_0.86-1.93 MeV/n E11.4 LogScale 0.0 1.0e+07 -1.0e+31 Ion Scalar NumberFlux 26 0.86 1.93 MeV/n Iron Flux Intensity, Fe4 Time Series defined by using: EPOCH Fe4 Iron Flux Intensity, Channel Fe4, 1.93 MeV/n to 3.07 MeV/n PT1H (cm^2 s sr MeV/n)^-1 6.24161e-19>(m^2 s sr J/n)^-1 TimeSeries Fe_1.93-3.07 MeV/n E11.4 LogScale 0.0 1.0e+07 -1.0e+31 Ion Scalar NumberFlux 26 1.93 3.07 MeV/n Iron Flux Intensity, FeloE, Uncertainty Time Series defined by using: EPOCH unc_FeloE Iron Flux Intensity, Channel FeloE, 0.12 MeV/n to 0.43 MeV/n, Fractional Uncertainty Low Energy (lowE) Rates - The Rates with the lowE Designation should always be used with Caution. These Rates may be contaminated by other Ions, and the Level of Contamination may depend on the Pressure in the Proportional Counter. The Reason for this is as follows. The Instrument consists of a Proportional Counter/Solid State Detector Telescope. Ion Species are identified by the Energy they deposit in each Detector. At certain low Energies, the Ion Species are difficult to distinguish from one another. The lowE Rates extend as far as possible into this Energy Range. As the Pressure Changes, the Limiting Energy for Species Identification changes somewhat and the Automatic Flux Calculation Algorithm may improperly include other Species. PT1H TimeSeries unc_Felo_0.12-0.43 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 26 0.12 0.43 MeV/n Iron Flux Intensity, Fe1, Uncertainty Time Series defined by using: EPOCH unc_Fe1 Iron Flux Intensity, Channel Fe1, 0.43 MeV/n to 0.64 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Fe_0.43-0.64 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 26 0.43 0.64 MeV/n Iron Flux Intensity, Fe2, Uncertainty Time Series defined by using: EPOCH unc_Fe2 Iron Flux Intensity, Channel Fe2, 0.65 MeV/n to 0.86 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Fe_0.65-0.86 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 26 0.65 0.86 MeV/n Iron Flux Intensity, Fe3, Uncertainty Time Series defined by using: EPOCH unc_Fe3 Iron Flux Intensity, Channel Fe3, 0.86 MeV/n to 1.93 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Fe_0.86-1.93 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 26 0.86 1.93 MeV/n Iron Flux Intensity, Fe4, Uncertainty Time Series defined by using: EPOCH unc_Fe4 Iron Flux Intensity, Channel Fe4, 1.93 MeV/n to 3.07 MeV/n, Fractional Uncertainty PT1H TimeSeries unc_Fe_1.93-3.07 MeV/n E11.4 LogScale 1.0e-5 1.0 -1.0e+31 Ion Scalar Uncertainty NumberFlux 26 1.93 3.07 MeV/n