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Radiation Laws
Warmer objects emit more intensely than cold objects. (Stefan-Boltzmann Law)
Warmer objects emit a higher proportion of their energy at short wavelengths than cold objects. (Wien’s Law)
Why does effective temperature have small changes year to year?
The system is in equilibrium: the energy inputs must be balanced approximately by energy losses.
It has increased due to industrial activity
Natural fluctuations due to El Niño
Calculation for incoming solar radiation
Incoming = (1-α) x S0 x A
Incoming = 1361 x πre2
Where:
S0 = solar constant (W/m2)
A = area
α = albedo
Calculation for outgoing radiation
Outgoing = σT4 × 4πre2
Where:
T = Temperature (K)
σ = Stefan-Boltzmann constant (5.67 x 10-8 W m-2 K-4).
4πre2 = Surface area of Earth
Describe the atmosphere’s transmission characteristics
Atmosphere is nearly transparent to shortwave radiation but almost opaque to the earth’s ‘longwave’ radiation
These characteristics explain how the atmosphere absorbs, emits and transmits radiation
The trapping of the ‘longwave’ radiation by the atmosphere is the ‘greenhouse effect’
Describes what happens to the incoming solar radiation
Albedo means 30% reflected.
Of the 70% absorbed:
51% is absorbed by land/water
Some (15%) is absorbed and then re-radiated by the Earth as IR radiation.
Some (16%) is absorbed and re-radiated by the atmosphere as longwave IR radiation.
This radiation is absorbed and re-radiated by greenhouse gases. This leads to a warming the atmosphere (troposphere) and the earth.
19% is absorbed by the atmosphere & clouds
Describe the water vapour feedback
Positive
Warming → more evaporation → more water vapour → more warming
Describe the ice-albedo feedback
Positive
Ice melts → albedo drops → more absorption → more warming
Describe the lapse rate feedback
Negative
Warmer air emits more IR → increased radiation loss → cooling
Describe cloud feedback
Mixed
Negative caused by low-level clouds (e.g. stratocumulus)
As temperatures rise, more low clouds can form
These reflect more incoming solar radiation → dampening the warming
Positive caused by high-level clouds (e.g. cirrus clouds)
With warming, the atmosphere can hold more moisture → more high clouds
These trap more outgoing radiation → further warming
Describe the carbon cycle feedback
Positive
Warming → permafrost melts → CO₂ & CH₄ release → more warming
What is effective radiative forcing?
Change in Earth’s energy balance after fast (days-months) atmospheric adjustments but before full surface temperature response.
ERF accounts for short-term feedbacks (e.g., cloud and stratospheric changes).
What is equilibrium climate sensitivity (ECS)?
Long-term temperature change from a doubling of CO₂ after the climate system reaches equilibrium
Includes slow feedbacks like ice sheet response and deep ocean warming
Estimated: ~1.5–4.5°C
Important for long-term climate risk projections
Not directly observable, inferred from palaeoclimate records, models, and energy balance approaches
What is transient climate response (TCR)?
TCR is the global temperature increase at the time of CO₂ doubling, assuming it increases 1% per year (which takes ~70 years).
Captures shorter-term warming with less involvement of slow-acting feedbacks.
Estimated range: ~1.0–2.5°C
More relevant for policy decisions over the next 50–100 years
Observationally constrained
Describe the relationship between TCR and ECS?
TCR < ECS, because ECS includes slow components that don’t respond immediately
ECS is what we expect eventually, TCR is what we see within a century