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Precision in Thinking

B.2 Greenhouse Effect

This topic links simple energy-balance physics to climate: how incoming solar power, reflection, emission and greenhouse gases together set a planet’s temperature.


Energy balance and radiative terms

  • In steady state, the average power absorbed by Earth equals the average power it emits, an application of the conservation of energy.
  • The solar constant SS is the intensity of solar radiation at Earth’s orbit on a surface normal to the Sun’s rays.
  • Because Earth is spherical and spins, the mean incoming intensity over the whole surface is Iin=S/4I_{\text{in}} = S/4.

Albedo and emissivity

  • Albedo is the fraction of incident radiation that is scattered or reflected, α=Preflected/Pincident\alpha = P_{\text{reflected}}/P_{\text{incident}}; snow and cloud have high albedo, oceans and forests have low albedo.
  • Earth’s albedo changes daily with cloud cover, ice extent, vegetation and surface type, so absorbed solar power is not constant.
  • Emissivity compares a surface’s thermal emission to that of an ideal black body; the radiated power per unit area is P=eσT4P = e\sigma T^{4}.

Greenhouse gases and warming

  • Main greenhouse gases in the atmosphere include H2O, CO2, CH4, N2O\text{H}_{2}\text{O},\ \text{CO}_{2},\ \text{CH}_{4},\ \text{N}_{2}\text{O}, along with others in smaller amounts.
  • These molecules have vibrational and rotational energy level spacings that resonate with outgoing infrared radiation from the surface, so they absorb and then re‑emit this energy in all directions.
  • Human activities such as burning fossil fuels, large‑scale agriculture and deforestation increase greenhouse gas concentrations, strengthening this effect and leading to the enhanced greenhouse effect.

Important formulas

Pout=PinP_{\text{out}} = P_{\text{in}}

Energy balance in steady state (conservation of energy).

α=PreflectedPincident\alpha = \dfrac{P_{\text{reflected}}}{P_{\text{incident}}}

Albedo of a planet or system.

Pemit=eσAT4P_{\text{emit}} = e\sigma A T^{4}

Thermal power radiated by a surface of emissivity e.

SS

Solar constant: intensity of solar radiation at Earth’s mean distance, on a surface normal to the rays.

Iin=S4I_{\text{in}} = \dfrac{S}{4}

Average incoming solar intensity over the whole Earth’s surface.


Practice problems

Albedo from reflected power

Sunlight of intensity 500\ \mathrm{W\,m^{-2}} falls on two surfaces. Surface A reflects 150\ \mathrm{W\,m^{-2}} and surface B reflects 350\ \mathrm{W\,m^{-2}}. Calculate the albedo of each surface and state which one cools more effectively.

Why the factor of four?

The solar constant S is about 1.36\times10^{3}\ \mathrm{W\,m^{-2}} at Earth’s orbit. Explain why the average incoming solar intensity over the entire Earth surface is S/4.

Simple energy balance model

Assume the Earth behaves like a uniform sphere with albedo 0.30 and emissivity e = 1. Take S = 1.36\times10^{3}\ \mathrm{W\,m^{-2}}. Estimate the equilibrium surface temperature T from a one-layer energy balance model.

Emissivity and surface type

Two flat surfaces, concrete and fresh snow, receive the same downwards infrared intensity. Concrete has emissivity e = 0.90 and snow has e = 0.60. Which surface emits more thermal radiation at the same temperature, and why does that not automatically mean it is cooler?

Greenhouse gas absorption

Explain qualitatively how greenhouse gases such as CO_{2}, CH_{4} and H_{2}O vapour warm the lower atmosphere, referring to infrared absorption, molecular energy levels and re‑emission.

Enhanced greenhouse effect

State one main human activity that increases each of the greenhouse gases CO_{2} and CH_{4}, and describe one climate impact that is linked to the enhanced greenhouse effect.


Clarity tip: For B.2 questions, start by sketching the energy flows — incoming solar, reflection, emission and greenhouse trapping — then write a simple power balance before substituting numbers.


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Sessions use careful diagrams and worked problems so that B.2 questions become straightforward applications of conservation of energy.