2.4.1 spase://CNES/NumericalData/CDPP-AMDA/Cassini/MIMI-LEMMS/cass-lemms-pha1min 1min One minute average particle intensity from PHA 2021-10-11T16:26:54Z One minute average particle intensity data for PHA (Pulse Height Analysis) ion and electron channels. There are three types of channels included in these averages: the A channels, the E channels and the F1 channels. The A channels measure ions, mostly protons. The E and F1 channels measure electrons. For the A channels, channel indices 8 through 62 are present (energies of 26-758 keV). For the E channels, indices 15 to 62 (20-410 keV), and for F1, 26 through 59 (206-1717 keV). spase://SMWG/Person/Jon.Vandegriff DataProducer cass-lemms-pha PartOf flux from PHA data spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi cass-lemms-pha1min 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. PDS CO-S-MIMI-4-LEMMS-CALIB-V1.0/LPHAAVG0_1MIN spase://CNES/Instrument/CDPP-AMDA/Cassini/MIMI-LEMMS EnergeticParticles 2004-01-01T00:00:30Z 2017-09-15T23:59:30Z PT60S Saturn The data is background subtracted, and thus occasionally there will be negative values when the count rate falls below the background level. Also, the uncertainties are based on the counting statistics, and thus because of the background subtraction, the uncertainties can be larger than the data value. ions A cass_lemms_pha1mina phot.count;phys.atmol.ionStage cm-2.sr-1.s-1.keV-1 Spectrogram Ion NumberFlux electrons E cass_lemms_pha1mine phot.count;phys.electron cm-2.sr-1.s-1.keV-1 Spectrogram Electron NumberFlux electrons F1 cass_lemms_pha1minf1 phot.count;phys.electron cm-2.sr-1.s-1.keV-1 Spectrogram Electron NumberFlux