2.3.1 spase://CNES/NumericalData/CDPP-AMDA/VEX/ELS/vex-els-all electron energy spectra : 16 anodes 2016-10-13T17:00:00 Level2 data. This dataset is generated directly from the VEX telemetry with IRAP software The Venus Express ASPERA team, S.Barabash, Swedish Institute of Space Physics, PI, and the European Space Agency spase://SMWG/Person/Stas.Barabash PrincipalInvestigator spase://CNES/Person/Andrew.J.Coates GeneralContact ELS data analysis at PSA ftp://psa.esac.esa.int/pub/mirror/VENUS-EXPRESS/ASPERA4/VEX-V-SW-ASPERA-2-ELS-V1.0/DOCUMENT/ELS_DATA_ANALYSIS_SUMMARY.PDF spase://SMWG/Repository/CNES/CDPP-AMDA Online Open http://amda.cdpp.eu NetCDF IRAP spase://CNES/Instrument/CDPP-AMDA/VEX/ELS ThermalPlasma 2005-03-03T01:48:33Z 2014-05-26T11:44:31Z PT1S PT64S Venus Anode selection : Anodes 5-12 have unobstructed views. Anodes 11 and 12 provide the best views and are the most commonly used in data analysis. plasma electron counts : per anode ##anode## vex_els_spec Averaged energy-time spectrogram of electron counts phys.count;phys.electron cnts Spectrogram 128 Electron Counts counts : sum over anodes vex_els_spec_sum energy spectrogram of electron counts phys.count;phys.electron cnts Spectrogram 128 Electron Counts