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- W1855300055 abstract "This paper considers the problem of modeling the light polarization that emerges from an astrophysical plasma composed of atoms whose excitation state is significantly influenced by the anisotropy of the incident radiation field. In particular, it highlights how radiative transfer simulations in three-dimensional models of the quiet solar atmosphere may help us to probe its thermal and magnetic structure, from the near equilibrium photosphere to the highly non-equilibrium upper chromosphere. The paper finishes with predictions concerning the amplitudes and magnetic sensitivities of the linear polarization signals produced by scattering processes in two transition region lines, which should encourage us to develop UV polarimeters for sounding rockets and space telescopes with the aim of opening up a new diagnostic window in astrophysics." @default.
- W1855300055 created "2016-06-24" @default.
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- W1855300055 date "2011-05-02" @default.
- W1855300055 modified "2023-09-27" @default.
- W1855300055 title "Modeling Scattering Polarization for Probing Solar Magnetism" @default.
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- W1855300055 hasPublicationYear "2011" @default.
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