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Asymmetric Stokes Q, U and V Line Profiles Observed in Sunspots
Published online by Cambridge University Press: 12 April 2016
Abstract
We present a systematic description of the asymmetric shapes the Stokes line profiles exhibit in sunspots. These asymmetries seem to be caused by gradients of both magnetic field and velocity in the photospheres of sunspots.
- Type
- Session 3. Techniques of Magnetic Field Measurements
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- Copyright © Astronomical Society of the Pacific 1993