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OCR GCSE Geography

GCSE · OCRGeography34 notes in 9 folders, 193 KB

Notes for OCR GCSE Geography B, Geography for Enquiring Minds (J384), in folders for the specification's eight topics in order (global hazards to resource reliance), then geographical skills and fieldwork. Each topic has notes on the processes and ideas, with worked case studies where the course asks for them. Where your school studied a different case study, keep the ideas and swap the place.

Adding them puts a copy in your notes, in a folder of its own with the folders below, for you to change and turn into flashcards or a question deck. Download gives you a zip of markdown files, which opens in any notes app.

What is inside

  • Global hazards
    • Global atmospheric circulation and weather extremes6 KB
    • Tropical storms, drought and El Niño6 KB
    • Case studies: weather hazards7 KB
    • Plate tectonics and plate boundaries6 KB
    • Earthquakes, volcanoes and living with tectonic hazards7 KB
  • Changing climate
    • Evidence and natural causes of climate change5 KB
    • The enhanced greenhouse effect and the impacts of climate change6 KB
  • Distinctive landscapes
    • Landscapes of the UK and the processes that shape them6 KB
    • Coastal and river landforms6 KB
    • Case studies: the Holderness coast and the River Tees7 KB
  • Sustaining ecosystems
    • Ecosystems and their global distribution4 KB
    • The tropical rainforest ecosystem5 KB
    • Exploiting and managing tropical rainforests6 KB
    • Polar environments6 KB
  • Urban futures
    • The changing global pattern of urbanisation3 KB
    • Rapid urbanisation in LIDCs and urban trends in ACs5 KB
    • Case study: London, a city in an advanced country5 KB
    • Case study: Lagos, a city in a low-income developing country5 KB
  • Dynamic development
    • Defining and measuring development5 KB
    • Causes of uneven development and breaking out of poverty5 KB
    • Ethiopia: development so far6 KB
    • Ethiopia: global connections and development strategies6 KB
  • UK in the 21st century
    • The UK today: human and physical characteristics4 KB
    • UK population change and an ageing population6 KB
    • The UK's changing economy6 KB
    • The UK's political and cultural role in the world5 KB
  • Resource reliance
    • Demand for food, energy and water5 KB
    • Food security and theories of population and food5 KB
    • Case study: food security in India8 KB
  • Geographical skills and fieldwork
    • Cartographic skills7 KB
    • Graphical skills6 KB
    • Numerical and statistical skills7 KB
    • Fieldwork enquiry7 KB
    • Enquiry and argument5 KB

The first note

Global hazards / Global atmospheric circulation and weather extremes

## Why the Earth has a circulation system The Sun heats the Earth unevenly. Near the equator the Sun's rays arrive almost overhead, so a given amount of energy is spread over a small area of surface and the ground gets very hot. Towards the poles the same rays arrive at a low angle, are spread over a much larger area and pass through more atmosphere, so they warm the surface far less. This difference in heating is the engine of the **global atmospheric circulation**, the large-scale movement of air that carries heat from the tropics towards the poles and so reduces what would otherwise be an even greater contrast in temperature. Air moves because of differences in pressure. Warm air is less dense, rises and leaves a region of **low pressure** at the surface. Cool air is denser, sinks and creates **high pressure** at the surface. Wind is air moving at the surface from high pressure to low pressure, and the Earth's rotation bends the path of that wind to the right in the northern hemisphere and to the left in the southern hemisphere. ## The three cells In each hemisphere the circulation is organised into three linked loops, called cells. - The **Hadley cell** lies between the equator and about 30° north and south. Air heated at the equator rises, cools as it climbs and forms towering clouds and heavy rain. At height the air spreads towards the poles, cools further and sinks at about 30°, then returns to the equator along the surface as the trade winds. - The **Ferrel cell**…

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