Radiation from a strongly-magnetized plasma

The case of predominant scattering

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

Research output: Contribution to journalArticle

37 Citations (Scopus)

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, kTe≩mc2,

Original languageEnglish (US)
Pages (from-to)249-297
Number of pages49
JournalAstrophysics and Space Science: An International Journal of Astronomy, Astrophysics and Space Science
Volume86
Issue number2
DOIs
StatePublished - Jan 1 1982

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radiative transfer
scattering
plasma
radiation
cold plasmas
polarization
magnetic field
photons
coefficients
magnetic fields
cold

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

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Radiation from a strongly-magnetized plasma : The case of predominant scattering. / Kaminker, A. D.; Pavlov, George; Shibanov, Yu A.

In: Astrophysics and Space Science: An International Journal of Astronomy, Astrophysics and Space Science, Vol. 86, No. 2, 01.01.1982, p. 249-297.

Research output: Contribution to journalArticle

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