2.4.1 spase://CNES/NumericalData/CDPP-AMDA/MESSENGER/EPS/mess-eps-spec pitch-angle distribution 2019-06-11T16:04:45Z The particle measurements are averaged in 120-second bins. Pitch angle bins are 11.25 degrees wide, and run from 0 to 180 degrees. Please note that the D03 detector on EPS has a very high background and is not useable for any science data product. spase://SMWG/Person/George.Ho DataProducer Data product PDS description https://pds-ppi.igpp.ucla.edu/data/MESS-E_V_H_SW-EPPS-3-EPS-DDR-V1.0/DOCUMENT/DDR_SIS/EPPS_DDR_SIS.HTM spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi mess-eps-spec 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. Calibrated PDS MESS-E_V_H_SW-EPPS-3-EPS-DDR-V1.0/EPS_PA_DAILY_SPECTROGRAM spase://CNES/Instrument/CDPP-AMDA/MESSENGER/EPS EnergeticParticles 2011-03-23T00:00:00Z 2015-04-30T23:59:58Z PT120S Mercury EPS PDS data products are derivate from the “Shaped” channel on EPS which is an integrated (hardware) channel. The hardware channel responded to all particles (ion and electron) that are above the threshold (~30 keV). Our experience at Mercury’s magnetosphere is that the primary particles are mostly energetic electrons. Please note that the D03 detector on the EPS has a very high background and is not useable for any of these science data products. countrate mes_eps_pad cnts/s Spectrogram 16 Electron EnergyFlux