Kinematics of the shock wave obtained using the type II burst frequency drift and coronal electron density models. The HF-type II was observed by both ground- and space-based instruments, while the LF-type II was observed only by space-based instruments. The HF-type II heights are obtained by using a 3.5-fold Saito density model, and the LF-type II heights are obtained using a 1-fold Leblanc density model. The spectral range of the bursts is emphasised by the error bars.