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MAVEN Observations of H– Ions at Mars (Dataset)

<p>Datasets used in the analysis of Mars Atmosphere and Volatile EvoutioN (MAVEN)&#39;s observations of H<sup>&ndash;</sup>&nbsp;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>&ndash;</sup>&nbsp;ion density (cm<sup>-3</sup>), and H<sup>+</sup>&nbsp;ion density (cm<sup>-3</sup>) for observations made by MAVEN&#39;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>&nbsp;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&ndash;sunward flux data: Contains differential energy fluxes (eV / (cm<sup>2</sup>&nbsp;sec sr eV)) for the anti&ndash;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