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Fig. 4


Maps of a) Magnetic field strength B, b) inclination angle, γ, of the magnetic field vector with respect to the solar surface normal, c) azimuth direction, φ, of the magnetic field vector and d) line-of-sight velocity obtained from the observations recorded on 14 November 2010. Left and right maps in all panels represent atmospheric parameters obtained in the photosphere and upper chromosphere, respectively. An arrow in the left map of panel d indicates the disk center direction and three arrows in the right map point three downflow intrusions in the penumbra.

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