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NotesESS HLTopic 6.4
Unit 6 · Atmosphere and Climate Change · Topic 6.4

IB ESS HL — Stratospheric ozone

HL Topic 6.4 extends the study of ozone depletion with more detailed atmospheric chemistry, quantitative analysis of ozone trends, and deeper evaluation of the Montreal Protocol as a model for international environmental governance.

Higher Level students should use this topic hub as a map: start with the shared sub-topics, then follow the HL-only extensions and exam-skill links where this topic asks for deeper analysis.

6.4 FlashcardsExam technique guidePractice questions

Key concepts in Stratospheric ozone

Key Idea: Most marks in topic 6.4 come from the Montreal Protocol and the recovery of the ozone layer. At HL, also learn halogen chemistry, the polar ozone hole, HFCs and air conditioning.

1. The Montreal Protocol (most marks)

  • Signed in 1987; every UN member has ratified it.
  • It phased out CFCs and other ozone-depleting substances (ODSs), with later dates for poorer countries.
  • It worked: few producers, cheap alternatives, a fund to help, and rules tightened as science grew.

2. Depletion and recovery

  • CFCs from fridges, aerosols and foams release chlorine, which destroys ozone.
  • The Antarctic ozone hole grew fast in the 1980s and peaked at 26.6 million km² in 2006.
  • Ozone should return to 1980 levels around 2066 over Antarctica: CFCs last decades.

3. Why it matters and HL ideas

  • The ozone layer in the stratosphere absorbs most harmful UV radiation.
  • More UVB causes skin cancer and cataracts, and cuts phytoplankton photosynthesis.
  • At HL: halogen chemistry, the polar ozone hole in spring, HFCs and Kigali (2016), and air conditioning.

How it is examined:

QuestionHow to score
[1] to [2] Describe ozone-hole dataDirection, peak year and values, with units.
[1] Name the cause of the declineCFCs, or chlorine from ODSs.
[2] Outline the effects of ozone depletionMore UVB: skin cancer, cataracts, less phytoplankton growth.
[4] Explain how the data show the Protocol workedCompare before and after 1987, and note the time lag.
[7] to [9] Evaluate or discuss the Montreal ProtocolWhy it worked, its limits, a comparison with climate deals.

Key terms, one line each:

TermIn one line
Ozone-depleting substance (ODS)a chemical, such as a CFC, that destroys stratospheric ozone
CFCa chlorofluorocarbon once used in fridges, aerosols and foams
Ozone holean area where ozone is below 220 Dobson units
Dobson unit (DU)the unit for the amount of ozone in a column of air
UVBultraviolet radiation that damages DNA; ozone absorbs most of it
HFCa CFC replacement that spares ozone but is a strong greenhouse gas
Polar stratospheric cloudsclouds below about -78 °C on which chlorine is released

Last-minute check: answer, then tap to see.

Why does the Antarctic hole open in spring? Sunlight returns and splits chlorine stored on polar clouds.

How many ozone molecules can one chlorine atom destroy? Over 100,000: it is a catalyst.

Why were HFCs phased down at Kigali in 2016? They spare ozone but are potent greenhouse gases.

How does air conditioning harm the climate? High energy use and HFC leaks.

IB-style questionEvaluate[4 marks]

The Kigali Amendment (2016) added HFCs to the Montreal Protocol. Evaluate the replacement of CFCs with HFCs.

Model answer plan

See the mark-by-mark plan — for / against / judgement, with marking guidance — in study mode.

Claim your free topic →

Exam tips

  • For graph data, give the direction, the peak year and values with units.
  • Say chlorine from CFCs destroys ozone; do not blame carbon dioxide.
  • For the Protocol's success, compare the data before and after 1987.
  • Explain why the Antarctic hole opens in spring: cold, clouds, then sunlight.

What you'll learn in Topic 6.4

  • 6.4.1 Radiation from the Sun
  • 6.4.2 Ultraviolet radiation
  • 6.4.3 The ozone layer
  • 6.4.4 Harm from ultraviolet radiation
  • 6.4.5 A natural ozone balance
  • 6.4.6 Ozone-depleting substances
  • 6.4.7 Ozone depletion and its effects
  • 6.4.8 The Montreal Protocol
  • 6.4.9 The ozone planetary boundary
  • 6.4.10 Halogens and ozone
  • 6.4.11 The polar ozone hole
  • 6.4.12 HFCs: replacing CFCs
  • 6.4.13 Air conditioning and the climate

Exam relevance

At Higher Level, ESS includes an extended essay component and deeper analytical questioning. Expect longer data-response questions and more complex case study scenarios in both Paper 1 and Paper 2.

Suggested study order: Read the notes for each sub-topic below → test yourself with flashcards → attempt practice questions → review exam technique.

Study resources — 6.4 Stratospheric ozone

6.4.1

Radiation from the Sun

Notes
6.4.2

Ultraviolet radiation

Notes
6.4.3

The ozone layer

NotesFlashcards
6.4.4

Harm from ultraviolet radiation

Notes
6.4.5

A natural ozone balance

Notes
6.4.6

Ozone-depleting substances

NotesFlashcards
6.4.7

Ozone depletion and its effects

Notes
6.4.8

The Montreal Protocol

NotesFlashcards
6.4.9

The ozone planetary boundary

Notes
6.4.10

Halogens and ozone

Notes
6.4.11

The polar ozone hole

Notes
6.4.12

HFCs: replacing CFCs

Notes
6.4.13

Air conditioning and the climate

Notes

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Topic 6.4 Stratospheric ozone forms a core part of Unit 6: Atmosphere and Climate Change in IB ESS HL. Mastering these concepts will strengthen your understanding of connected topics across the syllabus and prepare you for exam questions that require analysis, evaluation, and real-world application.

Frequently asked questions

What does Topic 6.4 Stratospheric ozone cover in IB ESS?
Topic 6.4 covers stratospheric ozone as part of the IB ESS syllabus. Students learn key concepts, definitions, and real-world examples that are tested in Paper 1 and Paper 2 exams.
How should I revise Stratospheric ozone for IB ESS exams?
Start by reading the micro-topic notes to understand each concept, then use flashcards to memorise key terms. Practise exam-style questions to apply your knowledge under timed conditions and review the marking criteria.
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