2.3.0 spase://CNES/NumericalData/CDPP-AMDA/PSP/epiLo/psp-lope-omg channel G Particle Energy mode, Omnidirectional, channel G : High Anglular Resolution Electrons 2019-11-12T10:48:29Z Particle Energy mode channel G. The available spectra are obtained by summing over all 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_omni PartOf particle energy mode (electrons) : 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 PT300S PT3000S Heliosphere.Inner Sun.Corona e- countrate psp_ompe_Gecr Electrons omnidirectional count rate cnts/sec Spectrogram CountRate