2.4.1 spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-south.1 northward flow Electron HighEnergy ( 38-96 MeV ) / He3 / He4 From South Hemisphere Direction 2024-05-20T03:04:58Z 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-south.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: south solo_het_south_eheflux Electron flux in 38 - 96 MeV energy range 1/(s cm^2 sr MeV) TimeSeries EnergyFlux e- HE flux unc: northward solo_het_south_eheunc Uncertainty in electron flux 1/(s cm^2 sr MeV) TimeSeries EnergyFlux he3 flux: northward solo_het_south_he3flux He3 flux 1/(s cm^2 sr MeV) Spectrogram 9 EnergyFlux he3 flux unc: northward solo_het_south_he3unc Uncertainty in He3 flux 1/(s cm^2 sr MeV) Spectrogram 9 EnergyFlux he4 flux: northward solo_het_south_he4flux He4 flux 1/(s cm^2 sr MeV) Spectrogram 15 EnergyFlux he4 flux unc: northward solo_het_south_he4unc Uncertainty in He4 flux 1/(s cm^2 sr MeV) Spectrogram 15 EnergyFlux quality flag: northward solo_het_south_1_qf 0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent TimeSeries DataQuality