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Geoscience Letters

Official Journal of the Asia Oceania Geosciences Society (AOGS)

Figure 8 | Geoscience Letters

Figure 8

From: Current understanding of the aeronomy of Mars

Figure 8

MHD 3-D ion model. Viking 1 ion density measurements are compared to model calculations of [19]. The lack of good agreement in O+ is the result of the uncertainty in neutral O densities; excellent agreement could be achieved by adjusting the neutral O density values, which were originally obtained by fitting a different model.

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