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Polarized scattering of light for arbitrary magnetic fields with level-crossings from the combination of hyperfine and fine structure splittings

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dc.contributor.author Sowmya, K
dc.contributor.author Nagendra, K. N
dc.contributor.author Sampoorna, M
dc.contributor.author Stenflo, J. O
dc.date.accessioned 2020-11-17T14:00:26Z
dc.date.available 2020-11-17T14:00:26Z
dc.date.issued 2015-12-01
dc.identifier.citation The Astrophysical Journal, Vol. 814, No. 2, 127 en_US
dc.identifier.issn 0004-637X
dc.identifier.uri http://prints.iiap.res.in/handle/2248/7098
dc.description Restricted Access © The American Astronomical Society http://dx.doi.org/10.1088/0004-637X/814/2/127 en_US
dc.description.abstract Interference between magnetic substates of the hyperfine structure states belonging to different fine structure states of the same term influences the polarization for some of the diagnostically important lines of the Sun's spectrum, like the sodium and lithium doublets. The polarization signatures of this combined interference contain information on the properties of the solar magnetic fields. Motivated by this, in the present paper, we study the problem of polarized scattering on a two-term atom with hyperfine structure by accounting for the partial redistribution in the photon frequencies arising due to the Doppler motions of the atoms. We consider the scattering atoms to be under the influence of a magnetic field of arbitrary strength and develop a formalism based on the Kramers–Heisenberg approach to calculate the scattering cross section for this process. We explore the rich polarization effects that arise from various level-crossings in the Paschen–Back regime in a single scattering case using the lithium atomic system as a concrete example that is relevant to the Sun. en_US
dc.language.iso en en_US
dc.publisher IOP Publishing en_US
dc.subject Atomic processes en_US
dc.subject Line: formation en_US
dc.subject Polarization en_US
dc.subject Scattering en_US
dc.subject Sun: magnetic fields en_US
dc.title Polarized scattering of light for arbitrary magnetic fields with level-crossings from the combination of hyperfine and fine structure splittings en_US
dc.type Article en_US


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