2.4.1 spase://CNES/NumericalData/CDPP-AMDA/PSP/epiHi/psp-het-1min HET 1min High Energy Telescope 1 min rate 2023-03-06T20:40:41Z 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 Please acknowledge the National Aeronautics and Space Administration, NASA spase://SMWG/Person/David.J.McComas PrincipalInvestigator spase://SMWG/Person/Eric.R.Christian DeputyPI PSP/ISoIS Energetic Particle Data - User Guide https://spdf.sci.gsfc.nasa.gov/pub/data/psp/isois/ISOIS_Data_Glossary.pdf Parker Solar Probe Mission Instrument web page, JPL http://parkersolarprobe.jhuapl.edu/Spacecraft/index.php#Instruments psp-isois-het PartOf HET spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server http://amda.irap.omp.eu/service/hapi Web Service to this product using the HAPI interface. CSV 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 http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers. spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA Web application http://amda.cdpp.eu Access to Data via CDPP/AMDA Web application. CSV VOTable CDF PNG 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 http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers. SPDF spase://CNES/Instrument/CDPP-AMDA/PSP/epiHi EnergeticParticles 2018-09-28T00:00:26Z 2022-11-14T23:59:32Z PT60S Heliosphere.Inner Sun.Corona h+ flux side A psp_het_1min_AHf Proton flux side A 1/cm²/sr/s/(MeV/nuc) Spectrogram EnergyFlux h+ A uncertainty psp_het_1min_AHfu Proton flux side A uncertainty 1/cm²/sr/s/(MeV/nuc) Spectrogram EnergyFlux h+ flux side B psp_het_1min_BHf Proton flux side B 1/cm²/sr/s/(MeV/nuc) Spectrogram EnergyFlux h+ B uncertainty psp_het_1min_BHfu Proton flux side B uncertainty 1/cm²/sr/s/(MeV/nuc) Spectrogram EnergyFlux he flux side A psp_het_1min_AHef Helium flux side A 1/cm²/sr/s/(MeV/nuc) Spectrogram EnergyFlux he A uncertainty psp_het_1min_AHefu Helium flux side A uncertainty 1/cm²/sr/s/(MeV/nuc) Spectrogram EnergyFlux he flux side B psp_het_1min_BHef Helium flux side B 1/cm²/sr/s/(MeV/nuc) Spectrogram EnergyFlux he B uncertainty psp_het_1min_BHefu Helium flux side B uncertainty 1/cm²/sr/s/(MeV/nuc) Spectrogram EnergyFlux