Conduction–radiation interaction in 3D irregular enclosures using the finite volume method

Numerical analysis of solidification of a 3-D semitransparent medium in presence of volumetric radiation

“…2, with β = 1.0 and ω = 0.0, for conductionradiation parameter N = 1.0, 0.1 and 0.01, along z/Z direction at x/ X = 0.5 and y/Y = 0.5 the centreline non-dimensional temperature θ = T /T 0 have been compared. Results of the present work have been compared with those given in [33]. A very good agreement is observed.…”

“…The computer code for the present 3-D solidification problem has been validated against the results given in [33]. In [33], conduction-radiation problem in a 3-D cubical enclosure has been considered without any phase change.…”

“…In [33], conduction-radiation problem in a 3-D cubical enclosure has been considered without any phase change. The FVM has been used to compute radiative information and also to solve the energy equation.…”

Meshless Method for Solving Transient Radiative and Conductive Heat Transfer in Two-Dimensional Complex Geometries

“…Steady-state radiative and conductive heat transfer has been much studied because of the simplicity to deal with energy without time-dependent terms [1][2][3][4][5][6][7][8]. However, the transient effect is also very important and gaining more and more interest in many industrial applications, such as manufacture and heat processing of glass products, phase-change material melting and solidification in hightemperature thermal energy storage systems, etc.…”

Study on the Influence of Aerosol Radiation Balance in One-Dimensional Atmospheric Medium UsingPn-Approximation Method

“…Many numerical methods have been developed to solve the problem of radiative heat transfer, such as the discrete ordinates method (DOM) [6,7], finite volume method (FVM) [8], finite element method (FEM), Monte Carlo method (MCM) [9], and spherical harmonics method (SHM). The spherical harmonics method, also known as the -approximation method, was originally proposed by Jeans [10] for interstellar radiative transfer and further developed by Davison [11] and Kourganoff [12] for neutron transport.…”