2.3.0 spase://CNES/NumericalData/CDPP-AMDA/PSP/epiLo/psp-lope-chg channel G High Look Resolution Electrons 2019-11-12T10:48:29Z Particle Energy mode channel G. The available spectra are obtained by summing 80 directions by wedges of 10 detectors into producing 8 data with 8 looking directions. * Species : Electrons * Nb of energy Bins : 48 * Energy range : 30 keV - 325 keV * 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_lope_wedge PartOf particle energy mode (electrons) : 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 PT3000S Heliosphere.Inner Sun.Corona e- count rate : 2D psp_lope_Gecr Electrons count rate on 8 wedges counts/sec Spectrogram CountRate