MAVEN Observations of H– Ions at Mars (Dataset)
<p>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.</p> <p>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).</p> <p>Solar longitude data: Contains the average Martian solar longitude (degrees) corresponding to each MAVEN orbit number.</p> <p>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.</p> <p>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.</p> <p>Orbit number data: Contains the MAVEN orbit numbers used in the analysis.</p>
ShareScore
36/100
Overall dataset sharing score
Score breakdown
These five areas show where the dataset supports — or may limit — practical reuse.
- Stewardship
- 4
- Harmonization
- 4
- Access
- 20
- Reuse readiness
- 8
- Engagement
- 0