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Results obtained in these simulations are less precise that those obtained for e=32 and e=7.63·10−6, but they highlight that the slope is controlled by the value of e.
The orbits of particles at typical cosmic ray energies in the GeV range, however, are influenced mainly by the inner magnetosphere where the magnetic field is strong, and where MHD simulations are less helpful because of their limited spatial resolution.
The findings indicate that the outdoor climatic conditions developed for cooling load estimation via the simulations are less stringent than the current outdoor design data and approaches adopted by local architectural and engineering practices.
Interestingly, in tau oligomers consisting of repeats R3 and R4, the percentage of hydrogen bonds that are retained during the simulations are less than 60% for R3 and less than 50% for R4, while in repeat R2, >70% of the hydrogen bonds are retained.
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Note that such queries against a single simulation are typical in MS applications as comparing multiple simulations is less popular.
Some previous authors have pointed to simulations being less costly than some comparable physical lab activities that require expensive equipment, supplies, or animals (Dewhurst et al. 1994; Wiesner and Lan 2004), but this was not a concern with the physical natural selection simulation used here as it uses cheap and readily available materials.
As shown in Fig. 3G, the variation in cell volume during these simulations was less than 1%.
The largest log likelihood ratio for our simulated data sets was 5.506 and the likelihood ratio for over 96% of our simulations was less than 0.001, whereas the likelihood ratio for our actual data was 18.064.
We also derive the probability distribution of the first passage time by using Kolmogorov's backward equation in Appendix E, but the fit of the shape of the probability distribution of waiting times to the distribution observed in individual-based simulations is less than perfect.
The errors of the grain size between the experiment and simulation are less than 20%.
Hence, the results of the simulation are less reliable in the western area which is still actively being explored.
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Justyna Jupowicz-Kozak
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