2.4.1 spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-step-rates flux Flux averaged over sectors 2022-01-17T05:52:44Z Solar Orbiter, Level 2 Data, Energetic Particle Detector, SupraThermal Electrons and Protons, Rates. STEP is designed to measure electrons and ions in the suprathermal energy range (280 keV). To allow for the separation of electrons and ions, STEP has 2 different channels, each equipped with its own solid state detectors for detecting particles: * Magnet channel. Uses a permanent magnet to deflect electrons, measuring only ions (mostly protons). * Integral channel. Measures all incoming particles. The electron flux is recovered by subtracting the magnet channel measurements from the integral channel ones. Each channel is divided in 15 sectors, disposed in 3 rows of 5 pixels, providing directional information of the incoming particles within the field of view. An additional pixel, not directly exposed to the incoming flux, measures the cosmic ray background. 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-step PartOf L2 : rates spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi so-step-rates 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-STEP-RATES spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-STEP EnergeticParticles 2020-04-30T00:00:11Z 2021-10-22T11:48:29Z PT10S PT60S Heliosphere.Inner Sun.Corona ion flux solo_step_mflux Magnet channel. Uses a permanet magnet to deflect electrons. Measuring only ions (mostly protons) 1/(s cm^2 sr MeV) Spectrogram 48 EnergyFlux ion flux unc solo_step_munc Uncertainty in sector averaged magnet channel flux 1/(s cm^2 sr MeV) Spectrogram 48 EnergyFlux ion cntrate solo_step_mrate Sector averaged magnet channel count rate cnts/s Spectrogram 48 CountRate el flux solo_step_eflux The electron flux is recovered by subtracting the magnet channel measurements from the integral channel ones 1/(s cm^2 sr MeV) Spectrogram 48 EnergyFlux total flux solo_step_iflux Integral channel. Measures all incoming particles 1/(s cm^2 sr MeV) Spectrogram 48 EnergyFlux total flux unc solo_step_iunc Uncertainty in sector averaged integral channel flux 1/(s cm^2 sr MeV) Spectrogram 48 EnergyFlux total cntrate solo_step_irate Sector averaged integral channel count rate cnts/s Spectrogram 48 CountRate quality flag solo_step_qf 0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent TimeSeries DataQuality