# Recommended Reading - Mathematical Expression of Climate feedbacks

In this text we show how we can incorporate feedbacks in simple mathematical formulation of climate change and we will go through an example showing how the climate sensitivity due to doubling of CO changes as we introduce climate feedbacks.

Applying the concept of radiative forcing (), the total change in the surface temperature
when the surface temperature is in balance (equilibrium) with the new radiative forcing () is the direct change in temperature due to the radiative forcing plus the
contributions made up by the effect of the radiative forcing () on other climatic
parameters () such as snow, ice, humidity etc. that again affect temperature so the total
change in near surface temperature will be dependent on the radiatve forcing and changes
in other climatic parameters . We can approximate the total change in near surface temperature as:

Where the first term on the right hand side is the direct response and the second is the sum
of all the feedbacks.

To get some idea of the change in temperature if we have no feedbacks we need to know the
response of temperature to the radiative forcing (). We can do this by
consider the change in net radiation at the top of the atmosphere () if we impose a
radiative forcing (). At equilibrium the change in net radiation at the top of the
atmosphere given a change in radiative forcing (Q) is zero, using the chain rule we can then
write:

Noting that the direct response and rearranging to get we get

Thus we need to know the change in the net radiation at the top of the atmosphere due to
a change in equilibrium surface temperature () in order to get the temperature
sensitivity to a radiative forcing ().

### The case of no feedbacks

If temperature is the only climatic parameter that will change the the change in net
radiation at the top of the atmosphere due to a change in equilibrium surface temperature
is given by Stefan‐Boltzmann’s Law which states that the radiation from a body that absorbs
all incoming radiation is depending on the temperature in the power.

()

Where is the emission temperature of a blackbody (the temperature the body would
have if it absorbed all emission) and Stefan‐Boltzmann’s constant. If we further assume
that the sensitivity of the equilibrium surface temperature to a change in radiative forcing is
the same as the sensitivity of the emission temperature ( ) we get:

Inserting the emission temperature of the earth‐atmosphere system (255K) we get

[]

In other words, a 1 change in radiative forcing will induce a 0.26 equilibrium temperature change.

### Including feedbacks

If other variables than temperature are changing the calculation of is more
complicated.

Where are other climatic parameters such as such as clouds, water vapour, snow, ice etc
that again affect temperature.

In the literature the different terms in the denominator are often given as feedback
parameters (even if the first term, the direct response, is not a feedback) defined as:

The unit for the feedback parameters are ) and indicate how much the net energy at the top of the atmosphere is changed for a given feedback (in other words how much more or less energy remains in the earth-atmosphere system) for a 1 change in temperature . Using this notation a negative implies that the feedback is negative and positive values
that the feedback is positive. Note that in the literature
is sometimes defined without the minus sign. Using the above definition we get:

Inserting this into equation 1 gives

Thus the temperature change can be approximated by calculating the different feedback
parameters. The table below gives typical values for the different feedback parameters.

Table: Strength of individual feedback parameters [)] from different state of the art climate models. Values taken from Soden and Held (2006).

### Example: Calculating climate sensitivity due to doubling of CO

From the reading material for week 1 the radiative forcing of CO was given as:
where is the reference CO concentration (usually takes as 280 ppm) and C the
CO concentration. C and C0 must be given in ppm (parts per million).

A doubling of CO then gives a radiative forcing of which together with the average values
from the table above we can calculate the temperature change using:

The no feedback result:

With feedbacks:

© University of Bergen/Prof. Asgeir Sorteberg