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[en] Preliminary results of calculations aimed at assessing the potential value of resonance polarization observations for solar atmospheric diagnostics are presented. There are significant differences between the polarization profiles for three solar atmospheric models, especially near the core and wing maxima
Journal
Proceedings - Astronomical Society of Australia; ISSN 0066-9997; 
; v. 5(2); p. 186-188
; v. 5(2); p. 186-188