2.4.1 spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-anti.1 sunward flow Electron HighEnergy ( 38-96 MeV ) / He3 / He4 From Antisun Direction ( mean Parker spiral ) 2024-05-20T03:04:16Z 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://CNES/Person/CDPP-AMDA/J.Rodrigues-Pacheco PrincipalInvestigator SolO Archive Support Data https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data solo-epd-het.1 PartOf L2 : e- 38-96 MeV / he3 / he4 flux spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi so-het-anti.1 Web Service to this product using the HAPI interface. CSV Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA Web application https://amda.cdpp.eu Access to Data via CDPP/AMDA Web application. CSV VOTable CDF PNG Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. http://soar.esac.esa.int/soar EPD-EPT-SUN-RATES spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET EnergeticParticles 2020-05-13T00:00:03Z 2024-02-29T23:59:59Z PT5S PT30S Heliosphere.Inner Sun.Corona e- HE flux: sunward solo_het_asun_eheflux Electron flux in 38 - 96 MeV energy range 1/(s cm^2 sr MeV) TimeSeries Electron EnergyFlux e- HE flux unc: sunward solo_het_asun_eheunc Uncertainty in electron flux 1/(s cm^2 sr MeV) TimeSeries Electron EnergyFlux he3 flux: sunward solo_het_asun_he3flux He3 flux 1/(s cm^2 sr MeV) Spectrogram 9 Ion EnergyFlux he3 flux unc: sunward solo_het_asun_he3unc Uncertainty in He3 flux 1/(s cm^2 sr MeV) Spectrogram 9 Ion EnergyFlux he4 flux: sunward solo_het_asun_he4flux He4 flux 1/(s cm^2 sr MeV) Spectrogram 15 Ion EnergyFlux he4 flux unc: sunward solo_het_asun_he4unc Uncertainty in He4 flux 1/(s cm^2 sr MeV) Spectrogram 15 Ion EnergyFlux quality flag: sunward solo_het_asun_1_qf 0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent TimeSeries DataQuality