From left to right slit-reconstructed images from the Tenerife Infrared Polarimeter (TIP-II) at different times. From top to bottom several wavelengths are presented that represent different layers in the atmosphere, from the photosphere to the chromosphere: continuum, Si i 10 827 Å line center and He i 10 830 Å red core intensities. The panels are located at different positions to approximately represent the alignment of their respective FOVs. The small white arrows indicate the position of the Stokes profiles presented in Figs. 7–9.