2.3.0 spase://CNES/NumericalData/CDPP-AMDA/PSP/epiHi/psp-het-1min HET 1min High Energy Telescope 1 min rate 2019-11-12T10:48:29Z 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 spase://SMWG/Repository/CNES/CDPP-AMDA Online Open AMDA at CDPP http://amda.cdpp.eu Text AMDA is a science analysis system provided by the Centre de Donnees de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Universite Paul Sabatier, Toulouse SPDF Please acknowledge the CDAWeb team at GSFC/SPDF. spase://CNES/Instrument/CDPP-AMDA/PSP/epiHi EnergeticParticles 2018-09-02T00:00:12Z 2025-08-12T23:59:55Z 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+ flux side B psp_het_1min_BHf Proton flux side B 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 flux side B psp_het_1min_BHef Helium flux side B 1/cm²/sr/s/(MeV/nuc) Spectrogram EnergyFlux