On the solution of the radiative transfer equations for polarized radiation.

Bibliographic Details
Title: On the solution of the radiative transfer equations for polarized radiation.
Authors: Degl'innocenti, E., Degl'innocenti, M.
Source: Solar Physics; Jun1985, Vol. 97 Issue 2, p239-250, 12p
Abstract: A general formalism is presented to obtain an analytical solution of the radiative transfer equations for polarized radiation when the absorption Mueller matrix for the Stokes parameters is constant along the ray-path. The formalism is then applied to find an analytical approximation of the Stokes parameters profiles for a typical chromospheric line having an optical-depth dependence of the source function of the form S(τ) = (ɛ + δ)(1 + ɛ). [ABSTRACT FROM AUTHOR]
Copyright of Solar Physics is the property of Springer Nature and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: On the solution of the radiative transfer equations for polarized radiation.
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  Data: <searchLink fieldCode="AR" term="%22Degl'innocenti%2C+E%2E%22">Degl'innocenti, E.</searchLink><br /><searchLink fieldCode="AR" term="%22Degl'innocenti%2C+M%2E%22">Degl'innocenti, M.</searchLink>
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  Data: Solar Physics; Jun1985, Vol. 97 Issue 2, p239-250, 12p
– Name: Abstract
  Label: Abstract
  Group: Ab
  Data: A general formalism is presented to obtain an analytical solution of the radiative transfer equations for polarized radiation when the absorption Mueller matrix for the Stokes parameters is constant along the ray-path. The formalism is then applied to find an analytical approximation of the Stokes parameters profiles for a typical chromospheric line having an optical-depth dependence of the source function of the form S(τ) = (ɛ + δ)(1 + ɛ). [ABSTRACT FROM AUTHOR]
– Name: Abstract
  Label:
  Group: Ab
  Data: <i>Copyright of Solar Physics is the property of Springer Nature and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1007/BF00165988
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      – Code: eng
        Text: English
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              Text: Jun1985
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              Y: 1985
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              Value: 97
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              Value: 2
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