The temperature profile of the atmosphere is a result of an interaction between
radiation and
convection. Sunlight in the
visible spectrum hits the ground and heats it. The ground then heats the air at the surface. If
radiation were the only way to transfer heat from the ground to space, the
greenhouse effect of gases in the atmosphere would keep the ground at roughly , and the temperature would decay exponentially with height. However, when air is hot, it tends to expand, which lowers its density. Thus, hot air tends to rise and transfer heat upward. This is the process of
convection. Convection comes to equilibrium when a parcel of air at a given altitude has the same density as its surroundings. Air is a poor conductor of heat, so a parcel of air will rise and fall without exchanging heat. This is known as an
adiabatic process, which has a characteristic pressure-temperature curve. As the pressure gets lower, the temperature decreases. The rate of decrease of temperature with elevation is known as the
adiabatic lapse rate, which is approximately 9.8 °C per kilometer (or 5.4 °F per 1000 feet) of altitude. The actual lapse rate, called the
environmental lapse rate, is not constant (it can fluctuate throughout the day or seasonally and also regionally), but a normal lapse rate is 5.5 °C per 1,000 m (3.57 °F per 1,000 ft). Therefore, moving up on a mountain is roughly equivalent to moving 80 kilometres (50 miles or 0.75° of
latitude) towards the pole. This relationship is only approximate, however, since local factors, such as proximity to
oceans, can drastically modify the climate. As the altitude increases, the main form of
precipitation becomes
snow and the
winds increase. The temperature continues to drop until the
tropopause, at , where it does not decrease further. This is higher than the highest
summit. ==Distribution==