2.3.0 spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-anti.3 sunward flow Fe Flux From Antisun Direction ( mean Parker spiral ) 2019-11-12T10:48:29Z Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Rates. HET measures the upper part of the energetic particle spectrum. It is equipped with several solid state detectors and a BGO crystal to provide identification of particle species from the relative energy deposited in the different detectors. Thus, HET measures count rates for different ion species, as well as electrons. HET provides measurements in the same 4 fields of view covered by EPT (Sun, Anti-Sun, North and South) Parameter ID uses Detector looking directon. See http://espada.uah.es/epd/EPD_data.php spase://CDPP/Person/J.Rodrigues-Pacheco PrincipalInvestigator SolO Archive Support Data https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data solo-epd-het.3 PartOf L2 : fe flux 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 http://soar.esac.esa.int/soar EPD-EPT-SUN-RATES spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET EnergeticParticles 2018-09-02T00:00:12Z 2025-08-12T23:59:55Z PT5M PT10M Heliosphere.Inner Sun.Corona fe flux: sunward solo_het_asun_feflux Ferrum flux 1/(s cm^2 sr MeV/n) Spectrogram 16 fe flux unc: sunward solo_het_asun_feunc Ferrum flux uncertainty 1/(s cm^2 sr MeV/n) Spectrogram 16 quality flag: sunward solo_het_asun_3_qf 0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent TimeSeries