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On nonstationary radiative transfer in a spectral line in stellar atmospheres. / Grachev, S. I.

In: Astrophysics, Vol. 37, No. 3, 07.1994, p. 243-246.

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@article{66aa37c82e9540e59af4e60a9ab31ab1,
title = "On nonstationary radiative transfer in a spectral line in stellar atmospheres",
abstract = "We consider nonstationary radiative transfer in a line in stellar atmospheres simulated as a stationary semi-infinite plane-parallel medium. We assume complete frequency redistribution in the elementary act of scattering. We assume that the time a photon spends in the medium is determined only by the mean time spent in the absorbed state. We obtain an explicit expression for the resolvent of the nonstationary integral equation of transfer, which is a bilinear expansion with respect to the eigenfunctions found in [12] for the corresponding stationary transfer equation.",
author = "Grachev, {S. I.}",
note = "Copyright: Copyright 2019 Elsevier B.V., All rights reserved.",
year = "1994",
month = jul,
doi = "10.1007/BF02058779",
language = "English",
volume = "37",
pages = "243--246",
journal = "Astrophysics",
issn = "0571-7256",
publisher = "Wolters Kluwer",
number = "3",

}

RIS

TY - JOUR

T1 - On nonstationary radiative transfer in a spectral line in stellar atmospheres

AU - Grachev, S. I.

N1 - Copyright: Copyright 2019 Elsevier B.V., All rights reserved.

PY - 1994/7

Y1 - 1994/7

N2 - We consider nonstationary radiative transfer in a line in stellar atmospheres simulated as a stationary semi-infinite plane-parallel medium. We assume complete frequency redistribution in the elementary act of scattering. We assume that the time a photon spends in the medium is determined only by the mean time spent in the absorbed state. We obtain an explicit expression for the resolvent of the nonstationary integral equation of transfer, which is a bilinear expansion with respect to the eigenfunctions found in [12] for the corresponding stationary transfer equation.

AB - We consider nonstationary radiative transfer in a line in stellar atmospheres simulated as a stationary semi-infinite plane-parallel medium. We assume complete frequency redistribution in the elementary act of scattering. We assume that the time a photon spends in the medium is determined only by the mean time spent in the absorbed state. We obtain an explicit expression for the resolvent of the nonstationary integral equation of transfer, which is a bilinear expansion with respect to the eigenfunctions found in [12] for the corresponding stationary transfer equation.

UR - http://www.scopus.com/inward/record.url?scp=34249755390&partnerID=8YFLogxK

U2 - 10.1007/BF02058779

DO - 10.1007/BF02058779

M3 - Article

AN - SCOPUS:34249755390

VL - 37

SP - 243

EP - 246

JO - Astrophysics

JF - Astrophysics

SN - 0571-7256

IS - 3

ER -

ID: 74196601