2.4.1 spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-anti sunward flow Ion Flux From AntiSun Direction 2022-09-04T20:38:56Z Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron and Proton Telescope, Rates. EPT measures electrons and ions in the lower part of the energetic particle spectrum. It effectuates measurements in 4 different fields of view : * Anti-Sunward Flow. Detector looks in the direction of the mean Parker spiral towards the Sun. * Sunward Flow. Detector looks opposite to the Sun direction. * Northward Flow. Detector looks towards the south ecliptic hemisphere. * Southward Flow. Detector looks towards the north ecliptic hemisphere. Parameter ID uses Detector looking directon. Additionally, EPT has 2 channels that separate electrons and ions: * Magnet channel. Uses a permanent magnet to deflect electrons. It measures protons with energies between 25 keV and 6.5 MeV and alpha particles up to 25 MeV. * Foil channel. Equipped with a foil that absorbs ions, it measures electrons in the energy range 25–500 keV. Ions with energies above 400 keV can penetrate the foil, contaminating the electron measurements. 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-eptsun PartOf L2 : ion flux spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server http://amda.irap.omp.eu/service/hapi 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 http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers. spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA Web application http://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 http://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-EPT EnergeticParticles 2020-05-13T00:00:03Z 2022-04-03T23:59:59Z PT5S PT30S Heliosphere.Inner Sun.Corona ion flux : sunward solo_ept_asun_iflux Particle flux in magnet channel 1/(s cm^2 sr MeV) Spectrogram 64 Ion EnergyFlux ion flux unc: sunward solo_ept_asun_iunc Uncertainty in ion flux 1/(s cm^2 sr MeV) Spectrogram 64 Ion EnergyFlux ion cntrate: sunward solo_ept_asun_irate Particle count rate in magnet channel cnts/s Spectrogram 64 Ion CountRate alpha flux: sunward solo_ept_asun_aflux High energy particle flux in magnet channel 1/(s cm^2 sr MeV) Spectrogram 8 Ion EnergyFlux alpha flux unc: sunward solo_ept_asun_aunc Uncertainty in alpha flux 1/(s cm^2 sr MeV) Spectrogram 8 Ion EnergyFlux alpha cntrate: sunward solo_ept_asun_arate High energy particle count rate in magnet channel cnts/s Spectrogram 8 Ion CountRate quality flag: sunward solo_ept_asun_qf 0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent TimeSeries DataQuality