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

Research output: Contribution to journal › Article › peer-review

51 Scopus citations

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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10.1007/BF00683336

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title = "Radiation from a strongly-magnetized plasma: The case of predominant scattering",

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,",

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year = "1982",

month = sep,

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pages = "249--297",

journal = "Astrophysics and Space Science: An International Journal of Astronomy, Astrophysics and Space Science",

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T1 - Radiation from a strongly-magnetized plasma

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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U2 - 10.1007/BF00683336

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SN - 0004-640X

VL - 86

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JO - Astrophysics and Space Science: An International Journal of Astronomy, Astrophysics and Space Science

JF - Astrophysics and Space Science: An International Journal of Astronomy, Astrophysics and Space Science

IS - 2

ER -

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

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