Abstract

Radiative Transfer (RT) in a continuous spectrum in plasmas is caused by the emission and absorption of electromagnetic waves (EM) by free electrons. For a wide class of problems, the deviation of the velocity distribution function (VDF) of free electrons from the thermodynamic equilibrium, the Maxwellian VDF, can be neglected. In this case, RT in the geometric optics approximation is reduced to a single transport equation for the intensity of EM waves with source and sink functions dependent on the macroscopic parameters of the plasma (temperature and density of electrons). Integration of this equation for RT of radio-frequency EM waves in laboratory plasmas with highly reflecting metallic walls is substantially complicated by the multiple reflections which make the waves with the long free path the dominant contributors to the power balance profile. This in turn makes the RT substantially nonlocal with the spatial–spectral profile of the power balance determined by the spatial integrals of the plasma parameters. The geometric symmetry of the bounding walls, especially when enhanced by the diffuse reflectivity, provides a semi-analytic description of the RT problem. Analysis of the accuracy of such an approach reveals an approximate self-similarity of the power balance profile and the radiation intensity spectrum in both approximate and ab initio modeling. This phenomenon is shown here for a wide range of plasma parameters and wall reflectivity, including data from various numeric codes. The relationship between the revealed self-similarity and the accuracy of numeric codes is discussed.

Highlights

  • Self-similarity phenomena in the theory of the radiative transfer in plasmas play an important role in identifying the main scalings and elaborating on the approaches to solving the problems of time-consuming numerical modeling

  • The similarity of the radiative transfer (RT) in continuous spectrum in plasmas with highly reflecting walls is shown here for the main characteristics of RT, namely the spectral distribution of the radiation intensity escaping from a toroidal plasma, Jesc(ω), defined in (18), and the spatial distribution of the net power loss PEC(ρ), defined in (4)

  • The results are presented for the transport of electron cyclotron radiation (ECR) in hot Maxwellian plasmas under conditions of a thermonuclear fusion tokamak-reactor and for RT with model functions of absorption and emission of radiation, connected by Kirchhoff’s law at low frequencies

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Summary

Introduction

Self-similarity phenomena in the theory of the radiative transfer in plasmas play an important role in identifying the main scalings and elaborating on the approaches to solving the problems of time-consuming numerical modeling An example of such self-similarity is presented in [1], where it is shown that the Green’s function of the non-stationary radiative transfer (RT) in the spectral lines of atoms and ions in plasma and gases has an approximate self-similarity in a wide range of RT problems. In the case of electromagnetic radiation in spectral lines, the radiation is emitted and absorbed by bound electrons in atoms and ions Another type of RT is associated with radiation emission and absorption by free electrons in plasmas.

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