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Polarization of resonance lines in the case of a Voigt absorption profile. / Dementyev, A. V.

в: Astronomy Letters, Том 34, № 8, 2008, стр. 574-580.

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Dementyev, A. V. / Polarization of resonance lines in the case of a Voigt absorption profile. в: Astronomy Letters. 2008 ; Том 34, № 8. стр. 574-580.

BibTeX

@article{5c64e638804a43ababb830c69afe1b0e,
title = "Polarization of resonance lines in the case of a Voigt absorption profile",
abstract = "Multiple resonance scattering of radiation in a spectral line is considered in the case of a Voigt absorption profile. The scattering is assumed to take place in a nonmagnetic semi-infinite atmosphere with uniformly distributed sources of unpolarized radiation. Polarization characteristics have been obtained for the emergent radiation by numerically solving the Ambartsumian-Chandrasekhar matrix integral equation.",
author = "Dementyev, {A. V.}",
year = "2008",
doi = "10.1134/S1063773708080094",
language = "English",
volume = "34",
pages = "574--580",
journal = "Astronomy Letters",
issn = "1063-7737",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "8",

}

RIS

TY - JOUR

T1 - Polarization of resonance lines in the case of a Voigt absorption profile

AU - Dementyev, A. V.

PY - 2008

Y1 - 2008

N2 - Multiple resonance scattering of radiation in a spectral line is considered in the case of a Voigt absorption profile. The scattering is assumed to take place in a nonmagnetic semi-infinite atmosphere with uniformly distributed sources of unpolarized radiation. Polarization characteristics have been obtained for the emergent radiation by numerically solving the Ambartsumian-Chandrasekhar matrix integral equation.

AB - Multiple resonance scattering of radiation in a spectral line is considered in the case of a Voigt absorption profile. The scattering is assumed to take place in a nonmagnetic semi-infinite atmosphere with uniformly distributed sources of unpolarized radiation. Polarization characteristics have been obtained for the emergent radiation by numerically solving the Ambartsumian-Chandrasekhar matrix integral equation.

U2 - 10.1134/S1063773708080094

DO - 10.1134/S1063773708080094

M3 - Article

VL - 34

SP - 574

EP - 580

JO - Astronomy Letters

JF - Astronomy Letters

SN - 1063-7737

IS - 8

ER -

ID: 5197098