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Atomic Orientation in Chromospheric Lines
Published online by Cambridge University Press: 12 April 2016
Abstract
Observations of the Stokes I and V profiles of the Ca II H and K lines in solar magnetic regions are presented. Least-squares fits of dI/dλ to V are obtained and the wavelength variation of the residuals, i. e. V-kdI/dλ, calculated. We find significant symmetric residuals in umbrae, which are in agreement with the effect on the V profiles due to atomic orientation, i.e. with the existence of an unequal population of the Zeeman sublevels with M>0 with respect to those with M<0.
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- Session 9. Convections and Oscillation in Active Regions
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- Copyright © Astronomical Society of the Pacific 1993
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