2.4.1 spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/solo-sisa-slow slow mode SIS-A ion anti-sunward flux 2024-05-20T02:47:15Z Solar Orbiter, Level 2 Data, Energetic Particle Detector, Suprathermal Ion Spectrograph, Rates. SIS relies in the time-of-flight technique for identifying ions, providing particle counts for several ion species in the energy range between 14 keV/n and 20 MeV/n. It consists of 2 telescopes: SIS-A looking in the sunward direction, along the mean Parker spiral and SIS-B looking anti-sunward. The main scientific measurements that SIS provides are: * Particle rates. Count rates of 12 ion species (H, He3, He4, C, N, O, Ne, Mg, Si, S, Ca and Fe) in 21 energy channels. * Helium histogram. Helium events is collected in a mass histogram for better separation of He3 and He4 intensities. * PHA data with information about individual events. 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-sisa PartOf L2 : sis-a ; anti-sunward flow spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi solo-sisa-slow 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-SIS EnergeticParticles 2020-04-02T10:52:18Z 2024-02-29T23:50:37Z PT30M Heliosphere.Inner Sun.Corona h flux: anti-sunward solo_sisa_slow_hflux Hydrogen flux 1/(s cm^2 sr MeV/n) Spectrogram 11 EnergyFlux he3 flux: anti-sunward solo_sisa_slow_he3flux Helium-3 flux 1/(s cm^2 sr MeV/n) Spectrogram 12 EnergyFlux he4 flux: anti-sunward solo_sisa_slow_he4flux Heliun-4 flux 1/(s cm^2 sr MeV/n) Spectrogram 13 EnergyFlux c flux: anti-sunward solo_sisa_slow_cflux Carbon flux 1/(s cm^2 sr MeV/n) Spectrogram 16 EnergyFlux n flux: anti-sunward solo_sisa_slow_nflux Nitrogen flux 1/(s cm^2 sr MeV/n) Spectrogram 16 EnergyFlux o flux: anti-sunward solo_sisa_slow_oflux Oxygen flux 1/(s cm^2 sr MeV/n) Spectrogram 16 EnergyFlux ne flux: anti-sunward solo_sisa_slow_neflux Neon flux 1/(s cm^2 sr MeV/n) Spectrogram 16 EnergyFlux mg flux: anti-sunward solo_sisa_slow_mgflux Magnesium flux 1/(s cm^2 sr MeV/n) Spectrogram 16 EnergyFlux si flux: anti-sunward solo_sisa_slow_siflux Silicium flux 1/(s cm^2 sr MeV/n) Spectrogram 17 EnergyFlux s flux: anti-sunward solo_sisa_slow_sflux Sulfur flux 1/(s cm^2 sr MeV/n) Spectrogram 17 EnergyFlux ca flux: anti-sunward solo_sisa_slow_caflux Calcium flux 1/(s cm^2 sr MeV/n) Spectrogram 16 EnergyFlux fe flux: anti-sunward solo_sisa_slow_feflux Ferrum flux 1/(s cm^2 sr MeV/n) Spectrogram 15 EnergyFlux quality flag: anti-sunward solo_sisa_slow_qf 0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent TimeSeries DataQuality