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We also present a mass loading simulation which corresponds to a 2D version of the interaction between the solar wind and a comet.
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The current simulation shows that mass loading by pickup ions H+,H+2, CH+4 and N+2 is stronger than in the previous simulations when O+ ions are introduced into the background plasma.
However, unlike our previous simulations, the most polar profile no longer exhibits the largest mass loading achieved in the model domain, nor the largest particle effective radius.
The conditions in the magnetosheath are modeled by a semi-analytical MHD simulation that includes mass loading.
In Fig. 16, we show the mass loading and effective radius for this simulation.
The mid-latitude and polar profiles exhibit a much greater recurrence of significant variability in both mass loading and effective radius than previous simulations.
Consistent with the results of the simulations in which the mass loading and effective radius were found to increase in response to an increase in photochemical production rates, this simulation in which the photochemical production rate was decreased results in decreases of photochemical cloud mass and effective radius.
Fig. 13 Contour plots of mass loading and effective radius for the nominal simulation containing photochemistry, displayed over the domain from 40 to 70 km.
In general, this simulation appears to underestimate the mass loading and overestimate the effective radius of the aerosol in the upper cloud region.
The contour plots of the mass loading and effective radius with time in this simulation (Fig. 13) demonstrate that we are at or near steady state.
However, these simulations also severely underestimate the mass loading.
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