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A Benchmark Model for the Sunlit Martian Ionosphere: Structure, Composition, and Energetics

  • Authors: Yanxing Liu, Xiaoshu Wu, Jun Cui, Haoyu Lu, Yutian Cao, Jianyang Li

Yanxing Liu et al 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure 3.

Comparison between modeled ion and electron density profiles from the nominal simulation (solid lines) and mean MAVEN NGIMS measurements (open circles) during the DD2 period. (a) Results for O﹩{}_{2}^{+}﹩, O+, CO﹩{}_{2}^{+}﹩, NO+, HCO+, N﹩{}_{2}^{+}﹩, CO+, and electrons. (b) Results for OH+, H2O+, H3O+, Ar+, and C+. Electron densities are derived by assuming charge neutrality. The modeled sum of CO+ and N﹩{}_{2}^{+}﹩ densities is displayed for comparison with the mean NGIMS measurements at the M/Z = 28 channel, where M/Z denotes the mass-to-charge ratio.

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