2.3.0 spase://CNES/NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-omp channel P Ion Composition mode, Omnidirectional, channel P : High Energy Resolution Protons 2019-11-12T10:48:29Z Ion composition mode channel P. The available spectra are obtained by summing over all 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_omni PartOf ion composition mode : omni 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 psp_omic_PHf Proton omnidirectional flux 1/cm²/sr/s/(MeV/nuc) Spectrogram EnergyFlux h+ countrate psp_omic_PHcr Protons omnidirectional count rate cnts/sec Spectrogram CountRate