Radiation and Waves (OCR)

What are the Risks and Benefits of Using Radiations?

Radiation as a Model
  • A model of radiation helps explain how energy is transferred from a source to an object some distance away.

  • The source emits radiation, which spreads out and carries energy through space.

  • This radiation can interact with matter by being transmitted, reflected, or absorbed.

The Electromagnetic Spectrum
  • Light is a type of electromagnetic radiation.

  • The electromagnetic spectrum includes several types of radiation, all of which travel at the same speed in a vacuum (approximately 3 × 10⁸ m/s).

  • The spectrum consists of:

    • Radio waves

    • Microwaves

    • Infrared

    • Visible light (red to violet)

    • Ultraviolet

    • X-rays

    • Gamma rays

  • These are ordered from:

    • Long to short wavelength

    • Low to high frequency

    • Low to high energy

Interaction with Matter
  • When radiation strikes an object, it may:

    • Be transmitted (pass through)

    • Be reflected (bounce off)

    • Be absorbed (energy taken in)

  • When absorbed, the radiation usually heats the object.

  • Some forms of electromagnetic radiation have enough energy to cause ionisation:

    • X-rays, gamma rays, and high-energy ultraviolet radiation can remove electrons from atoms or molecules.

    • This ionisation can lead to chemical changes or biological effects.

Risks and Benefits of Electromagnetic Radiation

Benefits
  • Used in medical imaging (e.g., X-rays)

  • Communication technologies (e.g., radio, microwaves)

  • Infrared radiation for heating

  • Gamma rays for sterilisation of medical equipment

Risks
  • Ionising radiation (X-rays, gamma rays, and high-energy ultraviolet rays) can damage living tissue.

  • May lead to mutations or increase cancer risk.

  • Excessive exposure to ultraviolet can cause skin damage or eye problems.

Effects of Ionising Radiation on Living Cells
  • High doses of ionising radiation can damage or destroy living cells, potentially leading to radiation sickness or death.

  • Smaller doses can cause mutations or changes in DNA, which may cause cells to grow uncontrollably, leading to cancer.

Protection from Harmful Radiation
  • In the upper atmosphere, oxygen is affected by radiation and forms ozone (O₃).

  • This ozone layer absorbs harmful ultraviolet (UV) radiation from the sun.

  • The ozone layer protects animals and other living organisms on Earth by reducing their exposure to UV radiation.

Production and Detection of Radio Waves
  • Radio waves are produced by oscillating currents in electrical circuits.

  • These waves are detected when they cause an oscillating current in a receiver circuit (e.g., an aerial or antenna).

Uses of the Electromagnetic Spectrum
  • Different parts of the electromagnetic spectrum are suited to different tasks because of how materials absorb, reflect, or transmit them.

  • For example:

    • Microwaves are absorbed by water molecules and used for heating.

    • X-rays pass through soft tissue but are absorbed by bone, making them useful in medical imaging.

Evaluation of New Technologies
  • Advances in technology use all parts of the electromagnetic spectrum.

  • When assessing new technologies, it is important to:

    • Consider both benefits and potential risks.

    • Use data and scientific explanations, not opinions, to justify decisions about their use.

What is Climate Change and What is the Evidence for It?

  • All objects emit electromagnetic radiation.

  • The type (wavelength) and intensity (strength) of radiation depend on the temperature of the object:

    • Cooler objects emit longer wavelengths (infrared).

    • Hotter objects emit shorter wavelengths (visible or ultraviolet).

  • The higher the temperature, the:

    • Greater the intensity of radiation emitted.

    • Peak wavelength of the radiation shifts to shorter wavelengths.

  • This is known as black body radiation – an ideal object that absorbs and emits all radiation perfectly.

Energy Balance and Temperature:
  • The temperature of an object depends on the balance between:

    1. Incoming radiation (e.g. from the Sun)

    2. Absorbed radiation

    3. Radiation emitted by the object

  • If an object absorbs more radiation than it emits → it gets hotter.

  • If an object emits more radiation than it absorbs → it gets cooler.

  • When the rates are equal, the object’s temperature stays constant.

The Earth’s Energy Balance and the Greenhouse Effect:
  • The Earth receives short-wavelength radiation (mostly visible light) from the Sun.

  • Some of this radiation is:

    • Reflected by clouds or the surface (especially ice and snow).

    • Absorbed by the surface, warming the planet.

  • The Earth emits longer-wavelength infrared radiation back into space.

  • Some gases in the atmosphere (e.g. carbon dioxide, methane, water vapour) absorb and re-emit this infrared radiation in all directions.

    • This traps heat and keeps Earth warmer than it would be without an atmosphere.

    • This is called the greenhouse effect.

Factors that Determine the Earth’s Temperature:
  • The amount of greenhouse gases – more gases = more heat trapped.

  • Cloud cover – can reflect or trap radiation depending on type and height.

  • Surface reflectivity (albedo) – ice reflects more radiation than oceans or forests.

  • Solar activity – changes in the Sun’s output affect incoming energy.

  • Volcanic activity – can increase atmospheric particles that reflect sunlight.

Evidence for Climate Change:
  • Carbon dioxide levels have been rising due to:

    • Burning fossil fuels (coal, oil, gas).

    • Deforestation (reduces CO₂ absorption by trees).

  • Computer climate models:

    • Use data from satellites, weather stations, and ocean buoys.

    • Predict temperature rises and help understand long-term climate trends.

    • Support the conclusion that human activity is contributing to global warming.

Everyday Example:
  • A car parked in the sun:

    • Absorbs visible light.

    • Re-emits it as infrared radiation.

    • Glass windows trap infrared, warming the interior — similar to the greenhouse effect.

How Do Waves Behave?

1. Wave Basics

  • A wave is a regular disturbance that transfers energy through a medium or space.

  • Waves do not transfer matter, only energy.

  • The disturbance in the medium moves differently depending on the type of wave:

    • Transverse wave: the medium moves perpendicular to the direction of wave travel.

    • Longitudinal wave: the medium moves parallel to the direction of wave travel.

2. Types of Waves

Transverse Waves:

  • Particles move at right angles to the wave direction.

  • Examples:

    • Waves on a rope

    • Ripples on water

    • Light and other electromagnetic waves

Longitudinal Waves:

  • Particles move in the same direction as the wave.

  • Examples:

    • Sound waves in air

    • Compression waves in a slinky spring

3. Wave Properties

Amplitude:

  • The maximum displacement from the rest position.

  • Linked to the energy carried by the wave.

Wavelength (λ):

  • The distance between two matching points on a wave (e.g., crest to crest or compression to compression).

Frequency (f):

  • The number of waves passing a point each second.

  • Measured in Hertz (Hz).

Period (T):

  • The time it takes for one wave to pass a point.

  • Formula:

Wave Speed (v):

  • The speed at which the wave moves through a medium.

  • Formula:


    where
    v = speed (m/s),
    f = frequency (Hz),
    λ = wavelength (m)

4. Wave Behaviour

  • It is the wave that travels, not the medium itself.

  • In both water ripples and sound waves, the particles oscillate but stay in place.

5. Reflection and Refraction

Reflection:

  • Waves bounce back when they hit a surface.

  • Example: light reflecting off a mirror.

Refraction:

  • Waves change direction and speed when passing from one medium to another.

  • Example: light bending when it enters glass from air.

These behaviours can be demonstrated using water waves, making them a useful model for understanding light and sound.

6. Measuring Waves (PAG4 and PAG8)

PAG4 – Using a ripple tank:

  • Measure the speed, frequency, and wavelength of waves.

  • Observe transverse wave behaviour.

PAG8 – Light waves:

  • Measure refraction using a prism.

  • Investigate reflection using a plane mirror.

7. Practical Applications

  • A wave model helps predict and explain the behaviour of light and sound:

    • How they travel

    • How they interact with surfaces (reflection and refraction)

Refraction of Light and Sound

What is Refraction?
  • Refraction is the bending of a wave when it enters a different medium at an angle.

  • It occurs due to a change in wave speed in different substances.

Why Does Refraction Happen?
  • When a wave moves from one material to another (e.g., air to glass):

    • The speed of the wave changes.

    • This causes a change in wavelength, because the frequency stays the same.

    • The change in wavelength leads to a change in direction (refraction).

Key Points:
  • Frequency stays constant during refraction.

  • Wavelength and speed change depending on the medium.

  • Angle of incidence and angle of refraction are used to describe the direction change.


Electromagnetic Waves

11. Light as an Electromagnetic Wave

  • Light is part of the electromagnetic spectrum.

  • It does not need a medium to travel; it can move through a vacuum.

  • Electromagnetic waves include:

    • Radio waves

    • Microwaves

    • Infrared

    • Visible light

    • Ultraviolet

    • X-rays

    • Gamma rays

12. Nature of Electromagnetic Waves

  • All electromagnetic waves are transverse.

    • This means the electric and magnetic fields oscillate at right angles to the direction of wave travel.

  • They all travel at the same speed in a vacuum (approximately 3.0×1083.0 \times 10^83.0×108 m/s).

Summary

Concept

Explanation

Refraction

Bending of waves due to change in speed when entering a new medium

Speed and Medium

Wave speed varies depending on the substance

Wavelength Change

Caused by a change in speed; frequency remains constant

Light

Electromagnetic, does not need a medium

Electromagnetic Waves

All are transverse and include light, microwaves, etc.