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