HDPWS

PSP - IS⊙IS EPI-Hi - HET - HET 1min

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/PSP/epiHi/psp-het-1min

Description
The HET is a cylinder containing a central stack of detector disks and two single detector disks, one at each end. The individual detectors in the central stack have thicknesses of 1000 microns. Three of the detectors in the central stack comprise two 1000-micron disks connected to act as single 2000 micron detectors. The end detector disks are 500 microns thick. The front end detector and the outermost detectors at each end of the central stack are each divided into five active elements, a central bulls-eye and four quadrants, each of equal area. Which active area hit on different disks gives directional information on the particle. An outer annular segment of each detector acts as an anti-coincidence shield to detect particles that exit the cylinder before passing through all the detectors. The HET covers electrons up to approximately 6 MeV and protons and heavy ions to at least 100 MeV/n. The lower range overlaps the high end of the Low Energy Telescopes. The measurements are divided into two different sides of the instrument, A and B

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Version:2.4.1

NumericalData

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/PSP/epiHi/psp-het-1min
ResourceHeader
ResourceName
PSP - IS⊙IS EPI-Hi - HET - HET 1min
AlternateName
High Energy Telescope 1 min rate
ReleaseDate
2024-09-24 09:17:28Z
Description
The HET is a cylinder containing a central stack of detector disks and two single detector disks, one at each end. The individual detectors in the central stack have thicknesses of 1000 microns. Three of the detectors in the central stack comprise two 1000-micron disks connected to act as single 2000 micron detectors. The end detector disks are 500 microns thick. The front end detector and the outermost detectors at each end of the central stack are each divided into five active elements, a central bulls-eye and four quadrants, each of equal area. Which active area hit on different disks gives directional information on the particle. An outer annular segment of each detector acts as an anti-coincidence shield to detect particles that exit the cylinder before passing through all the detectors. The HET covers electrons up to approximately 6 MeV and protons and heavy ions to at least 100 MeV/n. The lower range overlaps the high end of the Low Energy Telescopes. The measurements are divided into two different sides of the instrument, A and B
Acknowledgement
Please acknowledge the National Aeronautics and Space Administration, NASA
Contacts
Role Person StartDate StopDate Note
1. PrincipalInvestigator spase://SMWG/Person/David.J.McComas
2. DeputyPI spase://SMWG/Person/Eric.R.Christian

InformationURL
Name
PSP/ISoIS Energetic Particle Data - User Guide
URL
InformationURL
Name
Parker Solar Probe Mission Instrument web page, JPL
URL
Association
AssociationID
AssociationType
PartOf
Note
HET
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA HAPI Server
URL
Style
HAPI
ProductKey
psp-het-1min
Description
Web Service to this product using the HAPI interface.
Format
CSV
Acknowledgement
Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA Web application
URL
Description
Access to Data via CDPP/AMDA Web application.
Format
CSV
Format
VOTable
Format
CDF
Format
PNG
Acknowledgement
Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.
ProviderName
SPDF
InstrumentIDs
MeasurementType
EnergeticParticles
TemporalDescription
TimeSpan
StartDate
2018-09-28 00:00:26Z
StopDate
2024-06-16 23:59:39Z
Cadence
PT60S
ObservedRegion
Heliosphere.Inner
ObservedRegion
Sun.Corona
Parameter #1
Name
h+ flux side A
ParameterKey
psp_het_1min_AHf
Description
Proton flux side A
Units
1/cm²/sr/s/(MeV/nuc)
RenderingHints
DisplayType
Spectrogram
Particle
ParticleQuantity
EnergyFlux
Parameter #2
Name
h+ A uncertainty
ParameterKey
psp_het_1min_AHfu
Description
Proton flux side A uncertainty
Units
1/cm²/sr/s/(MeV/nuc)
RenderingHints
DisplayType
Spectrogram
Particle
ParticleQuantity
EnergyFlux
Parameter #3
Name
h+ flux side B
ParameterKey
psp_het_1min_BHf
Description
Proton flux side B
Units
1/cm²/sr/s/(MeV/nuc)
RenderingHints
DisplayType
Spectrogram
Particle
ParticleQuantity
EnergyFlux
Parameter #4
Name
h+ B uncertainty
ParameterKey
psp_het_1min_BHfu
Description
Proton flux side B uncertainty
Units
1/cm²/sr/s/(MeV/nuc)
RenderingHints
DisplayType
Spectrogram
Particle
ParticleQuantity
EnergyFlux
Parameter #5
Name
he flux side A
ParameterKey
psp_het_1min_AHef
Description
Helium flux side A
Units
1/cm²/sr/s/(MeV/nuc)
RenderingHints
DisplayType
Spectrogram
Particle
ParticleQuantity
EnergyFlux
Parameter #6
Name
he A uncertainty
ParameterKey
psp_het_1min_AHefu
Description
Helium flux side A uncertainty
Units
1/cm²/sr/s/(MeV/nuc)
RenderingHints
DisplayType
Spectrogram
Particle
ParticleQuantity
EnergyFlux
Parameter #7
Name
he flux side B
ParameterKey
psp_het_1min_BHef
Description
Helium flux side B
Units
1/cm²/sr/s/(MeV/nuc)
RenderingHints
DisplayType
Spectrogram
Particle
ParticleQuantity
EnergyFlux
Parameter #8
Name
he B uncertainty
ParameterKey
psp_het_1min_BHefu
Description
Helium flux side B uncertainty
Units
1/cm²/sr/s/(MeV/nuc)
RenderingHints
DisplayType
Spectrogram
Particle
ParticleQuantity
EnergyFlux