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All the model results shown below are averages over the last model cycle.
This is consistent with the model results shown in Fig. 3.
The model results shown in Fig. 3 give ion densities in good agreement with Cassini and Voyager observations (cf. Keller et al., 1998; Cravens et al., 2004).
When model results shown in Figure 4, tested for fluid composition from Straub and Layne ([2003]), are plotted in the Cl versus F diagram (Figure 5B), the direction of melting trends is determined by the value of α, whereas the extent of the trends are determined by the degree of melting.
Model results shown in Figure 5 reveal a clear effect of ozone on upper stratospheric and mesospheric temperatures; first, a strengthening of cooling after 1980 and then after the mid-1990s, a leveling-off of the trend, if not a slight statistically insignificant heating in the mesosphere.
The regression line shown in Figure 2 corresponds to the primary model results shown in Table 4.
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Finite element model results showed good agreement with experimental results.
The model results showed reasonable agreements under different operating conditions.
Model results show that magnetite is the main corrosion product.
The model results showed an excellent agreement with experimental values.
However, model results show that proppant settling velocity depends on fluid viscosity (Fig. 21).
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