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6. Atmosphere and climate change
6.1

Introduction to the atmosphere

IB ESS Syllabus

SL & HL
Syllabus concepts to know
  • 6.1.1 The atmosphere forms the boundary between Earth and space.
  • 6.1.2 Differential heating of the atmosphere creates the tricellular model of atmospheric circulation that redistributes the heat from the equator to the poles.
  • 6.1.3 GHGs and aerosols in the atmosphere absorb and re-emit some of the infrared (long-wave) radiation emitted from the Earth’s surface, preventing it from being radiated out into space.
  • 6.1.4 The greenhouse effect keeps the Earth warmer than it otherwise would be due to the broad spectrum of the Sun’s radiation reaching the Earth’s surface and infrared radiation emitted by the warmed surface then being trapped and re-radiated by GHGs.
  • 6.1.5 The atmosphere is a dynamic system, and the components and layers are the result of continuous physical and chemical processes.
  • 6.1.6 Molecules in the atmosphere are pulled towards the Earth’s surface by gravity.
  • 6.1.7 Milankovitch cycles affect how much solar radiation reaches the Earth and lead to cycles in the
  • 6.1.8 Global warming is moving the Earth away from the glacial–interglacial cycle that has characterized the Quaternary period, toward new, hotter climatic conditions.
  • 6.1.9 The evolution of life on Earth changed the composition of the atmosphere, which in turn influences the evolution of life on Earth.

Study & practice 6.1 Introduction to the atmosphere

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Read Notes for 6.1

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5.2 Agriculture and food

6.2 Climate change—causes and impacts

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