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This chapter focuses specifically on components in the medium that are closely related to thermal radiation, how they emit and absorb thermal radiative rays, and how to quantify their characteristics in engineering practice.
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I will also describe the treatment of X-ray radiative effects of AGN and a more accurate black hole accretion rate prescription using the Bondi radius criterion.
Abel, T. & Wandelt, B. D. Adaptive ray tracing for radiative transfer around point sources.
We review the recent progress in modeling the influence of X-rays on the radiative equilibrium and on the radiative force.
Detailed mass and heat transfer analysis for a 5 kWth scale prototype was performed coupling Monte Carlo ray tracing for radiative heat exchange to the energy balances for the bed and the reactor.
The properties of the hot gas comparatively favor the cloudlet evaporation model as a main mechanism for the "thermal composite" X-ray appearance, though radiative rim and thermal conduction may also be effective.
It has been suggested that Ln3+ ions provide an effective mechanism for radiative emission by excitons generated by X-ray irradiation in a fluoride matrix.
The X-ray diffraction structure and radiative properties are compared to ab-initio quantum-computational predictions.
Experimental and numerical techniques were combined to solve the homogenised radiative transfer equations using Monte Carlo ray tracing in the limit of geometrical optics.
The spectroscopy response to gamma ray (an uncollimated 241Am radiative source with the principal energy of 59.5 keV) of the detectors shows that the energy resolution is 14.6% corresponding to FWHM ≈8.69 keV at room temperature.
It has been obtained by measuring the X-ray transition energy for radiative recombination into the 1s vacancy of bare rhodium and subtracting the electron beam energy from it.
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