MAVEN Observations of H– Ions at Mars (Dataset)
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Datasets used in the analysis of Mars Atmosphere and Volatile EvoutioN (MAVEN)'s observations of H<sup>–</sup> ions at Mars, by Jones et al. Density data: Contains the orbit number, upstream solar wind energy (eV), upstream solar wind density (cm<sup>-3</sup>), H<sup>–</sup> ion density (cm<sup>-3</sup>), and H<sup>+</sup> ion density (cm<sup>-3</sup>) for observations made by MAVEN's Solar Wind Ion Analyzer (SWIA) and Solar Wind Electron Analyzer (SWEA). Solar longitude data: Contains the average Martian solar longitude (degrees) corresponding to each MAVEN orbit number. Sunward flux data: Contains differential energy fluxes (eV / (cm<sup>2</sup> sec sr eV)) for the sunward velocity direction, as measured at 64 detector energies (first row of dataset). Each row corresponds to a different MAVEN orbit. Anti–sunward flux data: Contains differential energy fluxes (eV / (cm<sup>2</sup> sec sr eV)) for the anti–sunward velocity direction, as measured at 64 detector energies (first row of dataset). Each row corresponds to a different MAVEN orbit. Orbit number data: Contains the MAVEN orbit numbers used in the analysis.



