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The uncertainty associated with using various methods to analyze hypersonic blunt body flows has been quantified through comparison to numerical solutions of the compressible Navier Stokes equations.
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The bacterial attachment and detachment were quantified through comparison of mass recoveries of bacterial breakthrough curves.
The effects of radiative loss and radiation absorption on large-scale spherical flame propagation are quantified through comparison among results predicted by these three models.
Genetic interactions were quantified through the comparison of fitness of double mutants and the expected phenotype based on the two single mutants.
These differences can be quantified through several different comparisons.
The strength of the strains is quantified through our analysis.
The latter can be quantified through various homogenization techniques.
These are quantified through the eco-indicator 99 method.
These effects are quantified through consequence analyses and probit models.
The resulting uncertainty is quantified through sensitivity analyses before making a recommendation regarding reimbursement.
The heating ability of MNPs was quantified through the specific power absorption (SPA) measurements.
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