2) Radiation & The Greenhouse Effect

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15 Terms

1
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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)

2
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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

3
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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

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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

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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’

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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

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Describe the water vapour feedback

  • Positive

  • Warming → more evaporation → more water vapour → more warming

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Describe the ice-albedo feedback

  • Positive

  • Ice melts → albedo drops → more absorption → more warming

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Describe the lapse rate feedback

  • Negative

  • Warmer air emits more IR → increased radiation loss → cooling

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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

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Describe the carbon cycle feedback

  • Positive

  • Warming → permafrost melts → CO₂ & CH₄ release → more warming

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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).

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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

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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

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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