The new results from Curiosity will allow scientists to model the evolution of the Martian climate over time, and deduce whether the planet was warm and wet and if it might have had the right conditions for life.
Based on that model, the evolution of internal stresses and the macroscopic stress strain were simulated.
To monitor and model the evolution of urban landscapes, we develop a brightness darkness greenness (B D G) model.
We model the evolution of the solar wind with distance, using inner heliosphere data to predict plasma parameters at Voyager.
The focus of this paper is to model the evolution of traffic congestion caused by the demand from residential place to the famous resorts during public holidays.
In this paper a nonhomogeneous Markov chain (NHMC) model is proposed to model the evolution of maximum crackwidth with applied load cycles.
Third, we analyze the model transformations in MDA with respect to the abstract model, the evolution scenarios and the related crosscutting concerns.
We model the evolution of a quantitative trait under selection that fluctuates in space and time, and derive an analytical condition for when these fluctuations promote genetic diversification.
Reduced-order models are developed to model the evolution of microstructure described by an orientation distribution function using a finite element discretization of the orientation space.
Using this information as the input data to a thermal model, the evolution of the temperature field within the two components can be estimated.
By creating distinct classes of landowners, we will be able to model the evolution of (and between) classes over time.
