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Improving the Ni I atomic model for solar and stellar atmospheric models
(IOP Publishing, 2013-05-10)
Neutral nickel (Ni I) is abundant in the solar atmosphere and is one of the important elements that contribute to the emission and absorption of radiation in the spectral range between 1900 and 3900 Å. Previously, the Solar ...
Radiative constraints on the hydrological cycle in an idealized radiative-convective equilibrium model
(American Meteorological Society, 2009-01)
The radiative constraints on the partitioning of the surface energy budget and, hence, on the strength of the hydrological cycle are analyzed in an idealized one-dimensional radiative–convective equilibrium model formulated ...
Effects of temperature and geometry on the heat transfer from turbulent flow of a participating gas through a duct
(Hemisphere Publ CorpBristolEUA, 1998)
Non-gray radiative convective conductive modeling of a double glass window with a cavity filled with a mixture of absorbing gases
(Pergamon-elsevier Science LtdOxfordInglaterra, 2006)
Light transport with the equation of radiative transfer: The Fourier Continuation – Discrete Ordinates (FC–DOM) Method
(Pergamon-Elsevier Science Ltd, 2019-10)
We present a method for the treatment of the time dependent radiative transfer equation under the discrete ordinate approximation. The novelty of the proposed approach stems, in part, from the incorporation of a spectral ...
Polarization in Monte Carlo radiative transfer and dust scattering polarization signatures of spiral galaxies
(EDP Sciences, 2017-05)
Polarization is an important tool to further the understanding of interstellar dust and the sources behind it. In this paper we describe
our implementation of polarization that is due to scattering of light by spherical ...