Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6659
Title: The Quantum Interference Effects in the Sc II 4247 Å Line of the Second Solar Spectrum
Authors: Smitha, H. N
Nagendra, K. N
Stenflo, J. O
Bianda, M
Ramelli, R
Keywords: Line: profiles;Methods: numerical;Polarization;Radiative transfer;Scattering;Sun: atmosphere
Issue Date: 10-Oct-2014
Publisher: IOP Publishing
Citation: The Astrophysical Journal, Vol. 794, No. 1, 30
Abstract: The Sc II 4247 Å line formed in the chromosphere is one of the lines well known, like the Na I D2 and Ba II D2, for its prominent triple-peak structure in Q/I and the underlying quantum interference effects governing it. In this paper, we try to study the nature of this triple-peak structure using the theory of F-state interference including the effects of partial frequency redistribution (PRD) and radiative transfer (RT). We compare our results with the observations taken in a quiet region near the solar limb. In spite of accounting for PRD and RT effects, it has not been possible to reproduce the observed triple-peak structure in Q/I. While the two wing PRD peaks (on either side of central peak) and the near wing continuum can be reproduced, the central peak is completely suppressed by the enhanced depolarization resulting from the hyperfine structure splitting. This suppression remains for all the tested widely different one-dimensional model atmospheres or for any multi-component combinations of them. While multidimensional RT effects may improve the fit to the intensity profiles, they do not appear capable of explaining the enigmatic central Q/I peak. This leads us to suspect that some aspect of quantum physics is missing.
Description: Open Access
URI: http://hdl.handle.net/2248/6659
ISSN: 0004-637X
???metadata.dc.rights???: © IOP Publishing
???metadata.dc.relation.uri???: http://iopscience.iop.org/0004-637X/794/1/30/
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