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Ulysses Cosmic Ray and Solar Particle Investigation (COSPIN) Kiel Electron Telescope (KET) Proton, Helium, and Electron Spin-Integrated Counting Rates Data, 10 min Average Data

ResourceID
spase://VSPO/NumericalData/Ulysses/COSPIN/KET/Rates/PT10M

Description

This Data Set contains 10 min Averages of: (a) Spin-Integrated Count Rates of Protons (2.7-5.4, 5.4-23.1, 34.1-125.0, 125.0-320.0, 320.0-2100 and >2100.0 MeV), Alpha Particles (6.0-20.4, 34.2-125.0, 125.0-320.0, 320.0-2100.0 and >2100.0 MeV/n), and Electrons (2.5-7.0, 7.0-170.0 and >170.0 MeV). (b) Eight-Sectored Count Rates of Protons (5.4-23.1 MeV) and Electrons (2.5-7.0 MeV). (c) Count Rates of D10, D20, C10, C20 and A01 single Detector Sensors. The Parameter Keys in the Parameter Level Segments below are specifically relevant to the UFA accessible Versions of the Data.

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Details

Version:2.2.9

NumericalData

ResourceID
spase://VSPO/NumericalData/Ulysses/COSPIN/KET/Rates/PT10M
ResourceHeader
ResourceName
Ulysses Cosmic Ray and Solar Particle Investigation (COSPIN) Kiel Electron Telescope (KET) Proton, Helium, and Electron Spin-Integrated Counting Rates Data, 10 min Average Data
AlternateName
COSPIN-KET-RAT-10M
ReleaseDate
2019-08-05 15:03:35Z
Description

This Data Set contains 10 min Averages of: (a) Spin-Integrated Count Rates of Protons (2.7-5.4, 5.4-23.1, 34.1-125.0, 125.0-320.0, 320.0-2100 and >2100.0 MeV), Alpha Particles (6.0-20.4, 34.2-125.0, 125.0-320.0, 320.0-2100.0 and >2100.0 MeV/n), and Electrons (2.5-7.0, 7.0-170.0 and >170.0 MeV). (b) Eight-Sectored Count Rates of Protons (5.4-23.1 MeV) and Electrons (2.5-7.0 MeV). (c) Count Rates of D10, D20, C10, C20 and A01 single Detector Sensors. The Parameter Keys in the Parameter Level Segments below are specifically relevant to the UFA accessible Versions of the Data.

Acknowledgement
Please acknowledge the COSPIN PI, R. Bruce McKibben, the KET Co-PI, Bernd Heber, and the UDS and/or NSSDC
Contacts
RolePerson
1.PrincipalInvestigatorspase://SMWG/Person/R.Bruce.McKibben
2.CoInvestigatorspase://SMWG/Person/Bernd.Heber
3.ArchiveSpecialistspase://SMWG/Person/Cecil.Tranquille
InformationURL
Name
The Ulysses Cosmic Ray and Solar Particle Investigation, COSPIN
URL
http://ufa.esac.esa.int/ufa/#instruments
Description

Published Description of the COSPIN Instrumentation, J.A. Simpson et al., Astron. Astrophys. Suppl. Ser. 92, 365-399, 1992. See especially Section 4.5 for a detailed Description of the High Energy Telescopes, HET. An electronic Copy of this Paper is available at http://adsbit.harvard.edu/cgi-bin/nph-iarticle_query?1992A%26AS...92..365S&defaultprint=YES&filetype=.pdf.

InformationURL
Name
User Notes for the COSPIN/KET Data Files
URL
http://ufa.esac.esa.int/ufa-sl-server/data-action?PROTOCOL=HTTP&PRODUCT_TYPE=ALL&FILE_NAME=cospin_ket_un.html&FILE_PATH=/ufa/HiRes/doc/cospin
Description

The User Notes File at the Ulysses Final Archive (UFA) describes the Format of the ASCII Data Files for the COSPIN Kiel Electron Telescope Telescope, KET, 10 min Average Proton, Helium and Electron Count Rates and detector Count Rates

PriorIDs
spase://VEPO/NumericalData/Ulysses/COSPIN/KET/RATES/PT10M
AccessInformation
RepositoryID
spase://SMWG/Repository/ESA/ESAC/UlyssesFinalArchive
Availability
Online
AccessRights
Open
AccessURL
Name
Ulysses Final Archive Access to COSPIN/KET 10 min Average Proton, Helium, and Electron Spin-Integrated Counting Rates Data
URL
http://ufa.esac.esa.int/ufa/#data
Description

Parent Directory containing compressed Ulysses COSPIN/KET 10 min Average Rates Data organized in Daily ASCII Files ucosketaYYDOY.dat (YY and DOY are the two digit Year and the Day of Year, respectively) grouped together into Yearly Files (cosketYY.zip, where YY is the two digit Year)

Format
Text
Encoding
ZIP
Acknowledgement
Please acknowledge the COSPIN KET Co-PI, Bernd Heber, CAU Kiel
AccessInformation
RepositoryID
spase://SMWG/Repository/NASA/GSFC/SPDF
Availability
Online
AccessRights
Open
AccessURL
Name
FTP Access to CDF Files at SPDF
URL
ftps://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin_cdaweb/ket/
Description

KET Data Access via FTP in CDF Format from SPDF

AccessURL
Name
HTTP Access to CDF Files at SPDF
URL
https://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin_cdaweb/ket/
Description

KET Data Access via HTTP in CDF Format from SPDF

Format
CDF
Acknowledgement
Please acknowledge the Space Physics Data Facility at NASA/GSFC
AccessInformation
RepositoryID
spase://SMWG/Repository/NASA/GSFC/SPDF
Availability
Online
AccessRights
Open
AccessURL
Name
CDAWeb
URL
https://cdaweb.sci.gsfc.nasa.gov/cgi-bin/eval2.cgi?dataset=UY_M0_KET&index=sp_phys
ProductKey
UY_M0_KET
Description

Subset, Plot, List via CDAWeb

AccessURL
Name
FTP Access to ASCII Files at SPDF
URL
ftps://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin/ket/10_min/
Description

KET Data Access via FTP in ASCII Format from SPDF

AccessURL
Name
HTTP Access to ASCII Files at SPDF
URL
https://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin/ket/10_min/
Description

KET Data Access via HTTP in ASCII Format from SPDF

Format
Text
Acknowledgement
Please acknowledge the Space Physics Data Facility at NASA/GSFC
InstrumentIDs
spase://SMWG/Instrument/Ulysses/COSPIN/KET
MeasurementType
EnergeticParticles
TemporalDescription
TimeSpan
StartDate
1990-10-23 00:00:00.000
StopDate
2008-12-31 23:59:59.999
Cadence
PT10M
ObservedRegion
Heliosphere.Outer
Parameter #1
Name
Time for the record
ParameterKey
Time_PG1
Description

Time for the record given in Year, Day of Year, Hour, Minute, Seconds and coverage in percent. The given time represents the start of the averaging interval.

Cadence
PT10M
Structure
Size
6
Element
Name
Year
Index
1
ValidMin
1990
ValidMax
2008
Element
Name
Day of Year
Index
2
ValidMin
1
ValidMax
366
Element
Name
Hour of Day
Index
3
ValidMin
0
ValidMax
23
Element
Name
Minute of Hour
Index
4
ValidMin
0
ValidMax
59
Element
Name
Seconds of Minute
Index
5
ValidMin
0
ValidMax
59
Element
Name
Coverage
Index
6
ValidMin
0
ValidMax
100
Support
SupportQuantity
Temporal
Parameter #2
Name
COSPIN/KET 10-Minute Average 2.7-5.4 MeV Proton Spin-Averaged Count Rates (K1)
ParameterKey
K1
Description

10-minute average KET spin-averaged proton count rates between 2.7 and 5.4 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K1 18 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter. Background fluxes of K1 are a combination of components, including a high RTG background rate. This channel should be used only during event times.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
2.7
High
5.4
Units
MeV
Parameter #3
Name
COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 1 (K21)
ParameterKey
K21
Description

10-minute average KET proton count rates in spin sector 1 (of 8) between 5.4 and 23.1 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K21-K28 120 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
5.4
High
23.1
Units
MeV
Parameter #4
Name
COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 2 (K22)
ParameterKey
K22
Description

10-minute average KET proton count rates in spin sector 2 (of 8) between 5.4 and 23.1 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K21-K28 120 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
5.4
High
23.1
Units
MeV
Parameter #5
Name
COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 3 (K23)
ParameterKey
K23
Description

10-minute average KET proton count rates in spin sector 3 (of 8) between 5.4 and 23.1 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K21-K28 120 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
5.4
High
23.1
Units
MeV
Parameter #6
Name
COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 4 (K24)
ParameterKey
K24
Description

10-minute average KET proton count rates in spin sector 4 (of 8) between 5.4 and 23.1 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K21-K28 120 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
5.4
High
23.1
Units
MeV
Parameter #7
Name
COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 5 (K25)
ParameterKey
K25
Description

10-minute average KET proton count rates in spin sector 5 (of 8) between 5.4 and 23.1 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K21-K28 120 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
5.4
High
23.1
Units
MeV
Parameter #8
Name
COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 6 (K26)
ParameterKey
K26
Description

10-minute average KET proton count rates in spin sector 6 (of 8) between 5.4 and 23.1 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K21-K28 120 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
5.4
High
23.1
Units
MeV
Parameter #9
Name
COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 7 (K27)
ParameterKey
K27
Description

10-minute average KET proton count rates in spin sector 7 (of 8) between 5.4 and 23.1 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K21-K28 120 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
5.4
High
23.1
Units
MeV
Parameter #10
Name
COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Count Rates in Spin Sector 8 (K28)
ParameterKey
K28
Description

10-minute average KET proton count rates in spin sector 8 (of 8) between 5.4 and 23.1 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K21-K28 120 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
5.4
High
23.1
Units
MeV
Parameter #11
Name
COSPIN/KET 10-Minute Average 5.4-23.1 MeV Proton Spin-Averaged Count Rates (P4)
ParameterKey
P4
Description

10-minute average KET spin-averaged proton count rates between 5.4 and 23.1 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= P4 120 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
5.4
High
23.1
Units
MeV
Parameter #12
Name
COSPIN/KET 10-Minute Average 34.1-125.0 MeV Proton Spin-Averaged Count Rates (K3)
ParameterKey
K3
Description

10-minute average KET spin-averaged proton count rates between 34.1 and 125.0 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K3 70.0 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
34.1
High
125.0
Units
MeV
Parameter #13
Name
COSPIN/KET 10-Minute Average 125.0-320.0 MeV Proton Spin-Averaged Count Rates (K34)
ParameterKey
K34
Description

10-minute average KET spin-averaged proton count rates between 125.0 and 320.0 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K34 152.0 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
125.0
High
320.0
Units
MeV
Parameter #14
Name
COSPIN/KET 10-Minute Average 320.0-2100.0 MeV Proton Spin-Averaged Count Rates (K12)
ParameterKey
K12
Description

10-minute average KET spin-averaged proton count rates between 320.0 and 2100.0 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K12 3300.0 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
320.0
High
2100.0
Units
MeV
Parameter #15
Name
COSPIN/KET 10-Minute Average >2100.0 MeV Proton Spin-Averaged Count Rates (K10)
ParameterKey
K0
Description

10-minute average KET spin-averaged proton count rates >2100.0 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K10 N/A On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
2100.0
High
INF
Units
MeV
Parameter #16
Name
COSPIN/KET 10-Minute Average 6.0-20.4 MeV/n Helium Spin-Averaged Count Rates (K2)
ParameterKey
K2
Description

10-minute average KET spin-averaged helium count rates between 6.0 and 20.4 MeV/n

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K2 120 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
AlphaParticle
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
6.0
High
20.4
Units
MeV/n
Parameter #17
Name
COSPIN/KET 10-Minute Average 34.2-125.0 MeV/n Helium Spin-Averaged Count Rates (K33)
ParameterKey
K33
Description

10-minute average KET spin-averaged helium count rates between 34.2 and 125.0 MeV/n

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K33 70.0 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
AlphaParticle
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
34.2
High
125.0
Units
MeV/n
Parameter #18
Name
COSPIN/KET 10-Minute Average 125.0-320.0 MeV/n Helium Spin-Averaged Count Rates (K29)
ParameterKey
K29
Description

10-minute average KET spin-averaged helium count rates between 125.0 and 320.0 MeV/n

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K29 88.0 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
AlphaParticle
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
125.0
High
320.0
Units
MeV/n
Parameter #19
Name
COSPIN/KET 10-Minute Average 320.0-2100.0 MeV/n Helium Spin-Averaged Count Rates (K31)
ParameterKey
K31
Description

10-minute average KET spin-averaged helium count rates between 320.0 and 2100.0 MeV/n

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K31 3200.0 On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
AlphaParticle
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
320.0
High
2100.0
Units
MeV/n
Parameter #20
Name
COSPIN/KET 10-Minute Average >2100.0 MeV/n Helium Spin-Averaged Count Rates (K30)
ParameterKey
K30
Description

10-minute average KET spin-averaged helium count rates >2100.0 MeV/n

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K30 N/A On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
AlphaParticle
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
2100.0
High
INF
Units
MeV/n
Parameter #21
Name
COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 1 (K13)
ParameterKey
K13
Description

10-minute average KET electron count rates in spin sector 1 (of 8) between 2.5 and 7.0 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K13-K20 N/A On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Electron
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
2.5
High
7.0
Units
MeV
Parameter #22
Name
COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 2 (K14)
ParameterKey
K14
Description

10-minute average KET electron count rates in spin sector 2 (of 8) between 2.5 and 7.0 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K13-K20 N/A On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Electron
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
2.5
High
7.0
Units
MeV
Parameter #23
Name
COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 3 (K15)
ParameterKey
K15
Description

10-minute average KET electron count rates in spin sector 3 (of 8) between 2.5 and 7.0 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K13-K20 N/A On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Electron
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
2.5
High
7.0
Units
MeV
Parameter #24
Name
COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 4 (K16)
ParameterKey
K16
Description

10-minute average KET electron count rates in spin sector 4 (of 8) between 2.5 and 7.0 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K13-K20 N/A On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Electron
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
2.5
High
7.0
Units
MeV
Parameter #25
Name
COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 5 (K17)
ParameterKey
K17
Description

10-minute average KET electron count rates in spin sector 5 (of 8) between 2.5 and 7.0 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K13-K20 N/A On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Electron
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
2.5
High
7.0
Units
MeV
Parameter #26
Name
COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 6 (K18)
ParameterKey
K18
Description

10-minute average KET electron count rates in spin sector 6 (of 8) between 2.5 and 7.0 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K13-K20 N/A On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Electron
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
2.5
High
7.0
Units
MeV
Parameter #27
Name
COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 7 (K19)
ParameterKey
K19
Description

10-minute average KET electron count rates in spin sector 7 (of 8) between 2.5 and 7.0 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K13-K20 N/A On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Electron
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
2.5
High
7.0
Units
MeV
Parameter #28
Name
COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Count Rates in Spin Sector 8 (K20)
ParameterKey
K20
Description

10-minute average KET electron count rates in spin sector 8 (of 8) between 2.5 and 7.0 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K13-K20 N/A On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Electron
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
2.5
High
7.0
Units
MeV
Parameter #29
Name
COSPIN/KET 10-Minute Average 2.5-7.0 MeV Electron Spin-Averaged Count Rates (E4)
ParameterKey
E4
Description

10-minute average KET spin-averaged electron count rates between 2.5 and 7.0 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= E4 N/A On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Electron
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
2.5
High
7.0
Units
MeV
Parameter #30
Name
COSPIN/KET 10-Minute Average 7.0-170.0 MeV Electron Spin-Averaged Count Rates (K11)
ParameterKey
K11
Description

10-minute average KET spin-averaged electron count rates between 7.0 and 170.0 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K11 N/A On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Electron
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
7.0
High
170.0
Units
MeV
Parameter #31
Name
COSPIN/KET 10-Minute Average >170.0 MeV Electron Spin-Averaged Count Rates (K32)
ParameterKey
K32
Description

10-minute average KET spin-averaged electron count rates >170.0 MeV

Caveats
Only rates C are given, since no simple estimates of the intensities can be done Intensities (I) must be derived by dividing through the integral geometric factor Gi, and by correcting through Pulse Height Analysis. I=C/Gi Values of the geometrical Factor Gi = (counting rate)/(Intensity): KET Channel Gi ============================= K32 N/A On 10 min averages some of the channels have limitations because of RTG background. Very slow increases are a sign that backgrounf levels are reached (a few percent per year). Get Low Flux Values from the PI for longer Accumulation Time Periods when KET is saturated or is working in a "calibration mode" have been omitted: eg. March event 1991 peak fluxes in the June to August period 1991 Jovian encounter.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Electron
Qualifier
Average
ParticleQuantity
CountRate
EnergyRange
Low
170.0
High
INF
Units
MeV
Parameter #32
Name
COSPIN/KET 10-Minute Average D10 Detector Counting Rate (D10)
ParameterKey
D10
Description

10-minute average KET D10 detector counting rate

Caveats
Rate channel D10 includes all particles depositing energy greater than the minimum discriminator level.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
ParticleType
AlphaParticle
ParticleType
Ion
ParticleType
Electron
Qualifier
Average
ParticleQuantity
Counts
Parameter #33
Name
COSPIN/KET 10-Minute Average D20 Detector Counting Rate (D20)
ParameterKey
D20
Description

10-minute average KET D20 detector counting rate

Caveats
Rate channel D20 includes all particles depositing energy greater than the minimum discriminator level.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
ParticleType
AlphaParticle
ParticleType
Ion
ParticleType
Electron
Qualifier
Average
ParticleQuantity
Counts
Parameter #34
Name
COSPIN/KET 10-Minute Average C10 Detector Counting Rate (D10)
ParameterKey
C10
Description

10-minute average KET C10 detector counting rate

Caveats
Rate channel C10 includes all particles depositing energy greater than the minimum discriminator level.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
ParticleType
AlphaParticle
ParticleType
Ion
ParticleType
Electron
Qualifier
Average
ParticleQuantity
Counts
Parameter #35
Name
COSPIN/KET 10-Minute Average C20 Detector Counting Rate (D10)
ParameterKey
C20
Description

10-minute average KET C20 detector counting rate

Caveats
Rate channel C20 includes all particles depositing energy greater than the minimum discriminator level.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
ParticleType
AlphaParticle
ParticleType
Ion
ParticleType
Electron
Qualifier
Average
ParticleQuantity
Counts
Parameter #36
Name
COSPIN/KET 10-Minute Average A01 Detector Counting Rate (A01)
ParameterKey
A01
Description

10-minute average KET A01 detector counting rate

Caveats
Rate channel A01 includes all particles depositing energy greater than the minimum discriminator level.
Cadence
PT10M
Units
s^-1
ValidMin
0.0
ValidMax
1000000
FillValue
-707
Particle
ParticleType
Proton
ParticleType
AlphaParticle
ParticleType
Ion
ParticleType
Electron
Qualifier
Average
ParticleQuantity
Counts