Stokes images of a spectral interval around the Sr I 4607 Å line. The spatial direction spans 47′′ on the solar disk. The observed region was near the est limb at μ ≃ 0.3, and the slit was placed parallel to the nearest limb. The reference direction for positive Stokes Q is the tangent to the nearest solar limb. These images are the result of a 2-minute observation average. The granulation pattern can be recognized in the intensity image, in particular in the continuum. The Q∕I image showsthe scattering polarization peak in the core of the Sr I line. Spatial variations at granular scales of this peak can be observed. Weak U∕I signals, just above the noise level, can be observed in the core of the Sr I line. In V∕I the typical antisymmetric Zeeman patterns can be easily recognized. Note in particular some small sized V∕I structures (for instance at spatial position 27′′).
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