Fig. 4From: Akatsuki LIR observing system simulation experiments evaluated by thermal tides in the Venus atmosphereZonal–mean zonal wind (colors, m s−1) and temperature (white contours, K) in a latitude–height cross section at the final day. The cases of a frf, b h1, c h6, d h1_ds, e h1_ns, and f h24 are shownBack to article page