2.3.0 spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-anti.2 sunward flow C / N / O 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.2 PartOf L2 : c / n / o 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 PT1M PT5M Heliosphere.Inner Sun.Corona c flux: sunward solo_het_asun_cflux Carbon flux 1/(s cm^2 sr MeV/n) Spectrogram 17 c flux unc: sunward solo_het_asun_cunc Uncertainty in Carbon flux 1/(s cm^2 sr MeV) Spectrogram 17 n flux: sunward solo_het_asun_nflux Nytrogen flux 1/(s cm^2 sr MeV/n) Spectrogram 17 n flux unc: sunward solo_het_asun_nunc Uncertainty in Nytrogen flux 1/(s cm^2 sr MeV) Spectrogram 17 o flux: sunward solo_het_asun_oflux Oxygen Flux 1/(s cm^2 sr MeV/n) Spectrogram 17 o flux unc: sunward solo_het_asun_ounc Uncertainty in Oxygen flux 1/(s cm^2 sr MeV) Spectrogram 17 quality flag: sunward solo_het_asun_2_qf 0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent TimeSeries