Radiation from a strongly-magnetized plasma: The case of predominant scattering

A. D. Kaminker; G. G. Pavlov; Yu A. Shibanov

doi:10.1007/BF00683336

Radiation from a strongly-magnetized plasma: The case of predominant scattering

A. D. Kaminker, G. G. Pavlov, Yu A. Shibanov

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Abstract

On the basis of diffusion approach for normal modes, solutions of the radiative transfer problem are obtained and analysed for an optically thick tenuous plasma with a strong magnetic field. The case is considered when the scattering processes without change of photon frequency ω are dominant. The radiative transfer coefficients as well as spectra, angular dependences and polarization of the outgoing radiation are investigated in detail for a ‘cold’ plasma, kT_e≩mc²,

Original language	English (US)
Pages (from-to)	249-297
Number of pages	49
Journal	Astrophysics and Space Science: An International Journal of Astronomy, Astrophysics and Space Science
Volume	86
Issue number	2
DOIs	https://doi.org/10.1007/BF00683336
State	Published - Sep 1982

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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abstract = "On the basis of diffusion approach for normal modes, solutions of the radiative transfer problem are obtained and analysed for an optically thick tenuous plasma with a strong magnetic field. The case is considered when the scattering processes without change of photon frequency ω are dominant. The radiative transfer coefficients as well as spectra, angular dependences and polarization of the outgoing radiation are investigated in detail for a {\textquoteleft}cold{\textquoteright} plasma, kTe≩mc2,",

author = "Kaminker, {A. D.} and Pavlov, {G. G.} and Shibanov, {Yu A.}",

year = "1982",

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T2 - The case of predominant scattering

AU - Kaminker, A. D.

AU - Pavlov, G. G.

AU - Shibanov, Yu A.

PY - 1982/9

Y1 - 1982/9

N2 - On the basis of diffusion approach for normal modes, solutions of the radiative transfer problem are obtained and analysed for an optically thick tenuous plasma with a strong magnetic field. The case is considered when the scattering processes without change of photon frequency ω are dominant. The radiative transfer coefficients as well as spectra, angular dependences and polarization of the outgoing radiation are investigated in detail for a ‘cold’ plasma, kTe≩mc2,

AB - On the basis of diffusion approach for normal modes, solutions of the radiative transfer problem are obtained and analysed for an optically thick tenuous plasma with a strong magnetic field. The case is considered when the scattering processes without change of photon frequency ω are dominant. The radiative transfer coefficients as well as spectra, angular dependences and polarization of the outgoing radiation are investigated in detail for a ‘cold’ plasma, kTe≩mc2,

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Radiation from a strongly-magnetized plasma: The case of predominant scattering

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