Vincent Eymet

TL;DR: In this article, a general circulation model (GCM) was developed for the Venus atmosphere, from the surface up to 100 km altitude, based on the GCM developed for Earth at their laboratory.

TL;DR: This review puts forward the practical consequences of writing down and handling the integral formulation associated to each Monte Carlo algorithm and tries to argue that these formulations are very much accessible to the non specialist and that they allow a straightforward entry to sensitivity computations and convergence enhancement techniques involving subtle concepts such as control variate and zero variance.

TL;DR: In this article, a net exchange formulation was used to analyze the thermal radiation within the Venus atmosphere, which is based on a set of gaseous and cloud optical data chosen among available referenced data.

TL;DR: In this article, the authors illustrate the practice of integral formulation, zero-variance approaches and sensitivity evaluations in the field of radiative transfer Monte Carlo simulation, as well as the practical implementation of the corresponding algorithms, for such realistic systems as photobioreactors involving spectral integration, multiple scattering and complex geometries.

TL;DR: A detailed one-dimensional analysis of the energy balance in the Venus atmosphere is proposed in this article, based on the Net Exchange Rate formalism that allows the identification in each altitude region of the dominant energy exchanges controlling the temperature.