Peacock jets observed in the Hα line on 2013 June 5 at 9:23 UT. a) Blue wing image at Δλ = −45 km s^-1; b) the line core; c) red wing image at Δλ = 45 km s^-1; d) co-temporal wide-band image in the SOT Ca ii H filter. The red and yellow dashed curves are the trajectories of the jets shown in Figs. 4 and 5. The red and green arrows point toward the solar disk center and the solar north pole, respectively. This figure is accompanied by an online animation that shows the temporal evolution of panels a)–c).