2.3.0 spase://CNES/NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-chp channel P High Energy Resolution Protons 2019-11-12T10:48:29Z Ion composition mode channel P. The available spectras are obtained by summing 80 directions by wedges of 10 detectors into producing 8 data with 8 looking directions. * Species : Protons * Nb of energy Bins : 48 * Energy range : 70 keV - 8.32 MeV * Nb of looking directions : 80 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_loic_wedge PartOf ion composition mode : wedges 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/epiLo EnergeticParticles 2018-09-02T00:00:12Z 2025-08-12T23:59:55Z PT60S PT1800S Heliosphere.Inner Sun.Corona h+ flux : 2D psp_loic_PHf Proton flux on 8 wedges 1/cm²/sr/s/(MeV/nuc) Spectrogram EnergyFlux h+ count rate : 2D psp_loic_PHcr Protons count rate on 8 wedges counts/sec Spectrogram CountRate