The climatic influence of clouds is a combination of their influence on the planetary albedo and the IR budget. These two influences depend a great deal on the cloud properties. In class I described two extreme clases of clouds - high thin and low thick.
The schematics show cloud influences on the solar and IR
fluxes for
thin high clouds (left) and low thick clouds (right). On the left we
see
much of the solar flux passes through the thin high cloud and the IR
emitted
from this cloud is relatively small compared to Earth's surface. Thus
the
outgoing IR flux escaping from the planet is relatively low (and made
so
by the thin high cloud). In contrast the thick low cloud blocks a lot
of
solar radiation and emits an IR flux similar to that of the surface.
Consequently
the thick cloud mostly reduces absorbed solar flux but has little
influence
on the outgoing longwave radiation. Overall the thin high cloud has a
warming
influence on the surface and the thick low cloud has a cooling
influence
compared to cloud-free conditions. Remember clouds are fairly good blackbody emitter/absorbers
but their
height in Earth's atmosphere has a strong influence on the strength of
their
greenhouse effect. High clouds tend to have a stronger greenhouse
effect.
This is analogous in some ways to a thick versus thin atmosphere (think
greenhouse
effect of Venus compared to Mars ). The average effect of clouds (not the change in clouds in the future) is easier to understand. We think, based on the average characteristic of clouds, that clouds have an overal cooling effect on the average climate today. Hence if Earth lost all its clouds, the planet would warm. Please read the notes on convection. I'll include a few a few illustrations here. ![]() The lapse rate is defined to be the temperature decrease with height. It is defined to be positive for the typical atmospheric condition of a temperature DECREASE with height. When parcels of air move up or down they must follow the dry adiabatic lapse rate, provided they exchange no heat with their surroundings, which is normally a good approximation, and there temperature has not reached the saturation point for the concentration of vapor contained in the parce. The real atmosphere does not necessarily follow the dry adiabatic lapser rate because the real atmosphere is also influenced by IR absorption and emission and condensation. This brings us to the end of Chapter 3 and we return to the feedback loops we brought up in chapter 2 again. I talked about a water vapor feedback loop that is positive: ![]() Remember I said that something else prevented a runaway greenhouse effect on Earth. This something else is the strong negative feedback from IR radiation emitted by Earth's surface. It is sometimes called the most fundamental feedback on Earth. It is so fundamental that sometimes we forget that it is a feedback at all: Recall that it defined the effective radiating temperature of the planet. ![]() |
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