Atmospheric Circulation on Venus Research Paper

Atmospheric Circulation on Venus - Research Paper usageThe Venus air is in a condition of vigorous circulation and super-rotation (Hunten, et al. 685). In just 4 days, the holy atmosphere circles the planet which is faster than the sidereal day of 243 days of the planet. The super rotation is supported by the plucks and they blow as fast as 100 m/s (360 km/h or 220 mph). Winds move up to 60 times of the rotation of the planet. On the other hand, the speed of wind becomes greatly slower as the elevation from the surface becomes smaller, with the breeze rarely reaching the speed of 10 km/h on the surface. Anticyclonic structures are near the poles and they are called vortices. Every vortex is double-eyed and exhibits a character S-shaped pattern of clouds. These Venus dont have a magnetic field. Its ionosphere disconnects the atmosphere from the solar wind and outer space. This layer that is ionized includes the solar magnetic field, providing Venus with a distinct magnetic enviro nment. This is believed to be Venuss induced magnetosphere. Gases that are lighter including water vapor, keeps on being blown away by the solar wind through the induced magnetotail. It is believed that Venuss atmosphere up to some 4 billion years ago was similar to that of the earth containing water on the surface. A play greenhouse effect may have been brought by surface water evaporation and subsequent show of the levels of other greenhouse gases.Despite the severe conditions on the surface, the pressure and temperature of the atmosphere at approximately 50km to 65km in a higher place the planets surface is around the same as that of the Earth, hence its upper atmosphere near the same as the earths in the Solar System, even more than the Mars surface. Because of the resemblance in temperature and pressure and the fact that breathable air is a lifting gas on earth, the upper part of the atmosphere has been proposed as a section for both colonization and