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The hysteretic damping model cannot be applied to time domain dynamic simulations: this is a well-known feature that has been discussed in the literature since the time when analog computers were widespread.
Yes, if you're a fan of hardcore racing simulations, this isn't the game for you.
Note that in the presence of fading, some discrepancies can be observed between the analytical results and simulations; this is due to the additional source of randomness coming from the channel coefficients, making the "dominant interferer" approximation used in the derivations less accurate.
Although proton precipitation has already been modeled with hybrid simulations, this is the first study which examines the spatial precipitation patterns given by the solar wind protons and the protons of planetary origin, at different altitudes, for different energy ranges of precipitating protons.
As we noted above, the speed differences we used were too small to induce large changes in either the data or the simulations; this is reflected in the virtually constant viscoelastic ratios.
We also observe a significant effect of both arrangement and sex by arrangement interaction in about half of the simulations; this is consistent with the expected result if these two effects were independent.
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In our simulations, this was only the case at the very beginning of the simulation runs.
For the purpose of simulations, this was found to be not very relevant.
Due to the stochastic nature of these simulations, this was not always the first day of the epidemic.
In our simulation, this is suppressed by the tapered initial stresses towards the trench.
At low simulation temperatures, this is indeed the case.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com