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Cited article:

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GENERALIZATION OF THE LAST SCATTERING APPROXIMATION FOR THE SECOND SOLAR SPECTRUM MODELING: THE Ca I 4227 Å LINE AS A CASE STUDY

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Hanle effect in the solar Ba II D2 line: a diagnostic tool for chromospheric weak magnetic fields

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ORIGIN OF SPATIAL VARIATIONS OF SCATTERING POLARIZATION IN THE WINGS OF THE Ca I 4227 Å line

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Are collisions with neutral hydrogen important for modeling the second solar spectrum of Ti I and Ca II?

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