2.2.2 spase://VSPO/NumericalData/MarsExpress/ASPERA3/IMA/EDR/PT1S Mars Express ion mass distribution functions 2012-06-13T00:00:00 The data consist of arrays of counts of ions at 96 energy steps spanning 0.01-40 keV/q and 32 mass channels giving good coverage for H+, He+, He++, O+. Temporal separation between arrays is ~12 sec (in the arrays sampled). The data are organized in csv ASCII format for spreadsheet usage. No spacecraft trajectory data are included in these experiment data records, but see http://www.rssd.esa.int/index.php?project=PSA&page=ancillary. As of June 2012, these data were available for mid-2003 through Jun 2011, although for the 2003 cruise phase, a total of only several hours of data were generated and are available. The Mars Express ASPERA team, R. Lundin, Swedish Institute of Space Physics, PI, and the European Space Agency spase://SMWG/Person/Rickard.Lundin PrincipalInvestigator Project-Archive Interface Control Document http://pds-ppi.igpp.ucla.edu/search/view/?f=yes&id=pds://PPI/MEXASP_1100/DOCUMENT/MEX_ASPERA3_PSA_ICD_V01_02 spase://SMWG/Repository/ESA/ESAC/PlanetaryScienceArchive Online Open Planetary Science Archive ftp://psa.esac.esa.int/pub/mirror/MARS-EXPRESS/ASPERA-3/ See the subdirectories whose names include "EDR-IMA" Text The Mars Express ASPERA team, R. Lundin, Swedish Institute of Space Physics, Kiruna, PI, the European Space Agency and the ESA Planetary Science Archive spase://SMWG/Repository/PDS/PPI Online Open PDS/PPI http://pds-ppi.igpp.ucla.edu/search/?t=Mars&sc=Mars%20Express&i=Energetic%20Particle%20and%20Plasma%20Spectrometer&title=Mars%20:%20Mars%20Express%20:%20Energetic%20Particle%20and%20Plasma%20Spectrometer PDS/PPI site, is currently not be as complete as ESA's Planetary Science Archive Text The Mars Express ASPERA team, R. Lundin, Swedish Institute of Space Physics, Kiruna, PI, the European Space Agency and the NASA Planetary Data System spase://SMWG/Instrument/MarsExpress/ASPERA3/IMA EnergeticParticles 2003-06-23T00:00:00 2007-06-30T00:00:00 PT12S Mars