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Stability boundaries predicted by both linear and non-linear analysis were compared with field data published in a previous study; both types of analysis reproduced the data.
For calibration with EG, the instrument reproduced the data up to 99% precision.
Our calculations successfully reproduced the data within an experimental error of 15%.
Tyner and co-authors [ 36] reproduced the data set.
Structural equation modeling (SEM) was conducted to verify whether the proposed model reproduced the data.
In both cases, model output closely reproduced the data within Cohort E, including quantitative shedding frequency, as well as episode rate, median initiation to peak and peak to termination slopes, durations, and first, last, and peak HSV DNA copy numbers.
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Some salient information relevant to reproducing the data presented in this study are briefly stated below.
Various Monte Carlo generators, commonly used in heavy ion and cosmic ray physics, are found to reproduce the data within uncertainties.
Dispersion of the vibrational modes has to be taken into account in order to reproduce the data.
However, such models fail to reproduce the data completely, suggesting that thermal pressure plays an important role in the discs of dwarf galaxies.
Six firn air transport models are tuned to the NEEM site; all models successfully reproduce the data within a 1σ Gaussian distribution.
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CEO of Professional Science Editing for Scientists @ prosciediting.com