Time Dependent Evolution from SMIN to SMAX

Equatorial Vertical Winds for Venus, Earth, and Mars vs. Height


Venus
VTGCM equatorial fields and their time-dependent evolution from SMIN to SMAX conditions, showing vertical winds at noon (LT = 12) over 100-200 km for 1-day integration.

Earth:
TIEGCM equatorial fields and their time-dependent evolution from SMIN to SMAX conditions, showing vertical winds at mid-afternoon (LT = 16) over 100-500 km for 10-days integration.

Mars:
MTGCM equatorial fields and their time-dependent evolution from SMIN to SMAX conditions, showing vertical winds at mid-afternoon (LT = 15) over 100-220 km for 1-day integration.