Here we systematically examine the correlation among the modal properties (density and radiative loss) of leaky modes, physical features, and solar absorption of dielectric antenna structures.
This means that the red shifted emission occurred with suppressed high-energy features and a small radiative rate, in other words, indicating the presence of intermolecular interaction in the solid-state aggregated environments, as explained by Varghese et al. [31] and Kabe et al. [6].
A detailed numerical simulation of the burning process is also presented that features detailed MD combustion chemistry, radiative heat transfer, species diffusion, and phase change effects to predict the evolution of droplet and flame diameter.
This dispersion feature of ω(k) for radiative modes is caused by a reduction in size of Au NPs.
All the features above makes it an "invisible" radiative cooling coat by taking advantage of the atmospheric transparency window.
Our simulation is a magnetohydrodynamic simulation including anisotropic thermal conduction, optically thin radiative losses, and parametrised heating as main thermodynamical features to construct a realistic arcade configuration from chromospheric to coronal heights.
From this figure, we can see several interesting features about the time evolution of radiative cooling by NO.
The new generation of the SCIATRAN model comprises all features of the latest SCIATRAN 1.2 RTM supporting additionally radiative transfer calculations in a spherical atmosphere.
The features related to the interdot-chain, long-range radiative coupling are explored by means of time-resolved PL spectroscopy.
For example, Wright et al. (2011) recently modeled the planetary nebula NGC 6302, an object that shows spectral features attributable to forsterite, using the 3D photoionization and radiative transfer Monte Carlo code MOCASSIN (Ercalano et al., 2003, 2005).
