2.3.0 spase://CNES/NumericalData/CDPP-AMDA/PSP/epiLo/psp-loic-chd channel D Ion composition Group 2 (Si, Mg, C) 2019-11-12T10:48:29Z Ion composition mode channel D. The available spectra are obtained by summing 80 directions by wedges of 10 detectors into producing 8 data with 8 looking directions. * Species : Si, C, Mg * Nb of energy Bins : 192 * Energy range : 87 keV - 18.5 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 PT300S PT7200S Heliosphere.Inner Sun.Corona si count rate : 2D psp_loic_Sicr Silicon count rate on 8 wedges counts/sec Spectrogram CountRate c count rate : 2D psp_loic_Ccr Carbon count rate on 8 wedges counts/sec Spectrogram CountRate