Three-dimensional simulation outputs for three of the eight hot Jupiters in this study. From left to right, the panels showcase (1) a zonal jet-dominated flow, (2) an intermediate transitional regime, and (3) a day-to-night flow pattern. Each column plots the line-of-sight velocity at the P ≈ 0.1 bar atmospheric layer for a single planet. Negative values (blue) denote winds moving toward the observer, while positive values (red) denote winds moving away. The results shown are time-averaged over the last 500 days of their corresponding simulation times. Top: view from the north pole with the SS point and AS point marked. Bottom: view from the dayside.