How do we describe a travelling wave and the stationary waves it can form?
The travelling-wave equation, phase and phase difference, and the formation and properties of stationary waves.
An SQA Advanced Higher Physics answer on waves, covering the travelling-wave equation, the meaning of phase and phase difference, and the formation of stationary waves by superposition with their nodes and antinodes.
Reviewed by: AI editorial process; not yet individually human-reviewed
Have a quick question? Jump to the Q&A page
Jump to a section
What this key area is asking
The SQA wants you to use the travelling-wave equation to describe a wave and extract its amplitude, frequency and wavelength, understand phase and phase difference, and explain the formation and properties of stationary (standing) waves by superposition.
The travelling-wave equation
This equation describes the displacement of any point in the medium at any time. By comparing a given equation with the standard form you read the amplitude straight off, equate the time coefficient to find the frequency, and equate the space coefficient to find the wavelength. The wave speed follows from .
Phase and phase difference
Two points are in phase (moving identically) when their separation is a whole number of wavelengths, giving a phase difference of . They are in antiphase (exactly opposite) when separated by an odd number of half-wavelengths, a phase difference of . Phase difference is central to interference, where it decides whether waves reinforce or cancel.
Stationary waves
At a node the two waves always cancel, so the displacement is permanently zero; at an antinode they always reinforce, giving maximum amplitude. Nodes (and antinodes) are spaced half a wavelength apart, so measuring node spacing gives the wavelength. Stationary waves explain the resonant frequencies of strings and air columns: only wavelengths that fit the boundary conditions, with nodes at fixed ends, are allowed, producing the fundamental and its harmonics.
Examples in context
A guitar or violin string vibrates in stationary-wave patterns whose allowed wavelengths set the pitch, with the ends as nodes. An organ pipe or flute supports stationary sound waves in a column of air, with antinodes at open ends. Microwave ovens form stationary waves, which is why turntables are needed to even out the hot and cold spots at antinodes and nodes. Resonance in bridges and buildings, where a driving frequency matches a natural stationary-wave mode, is a design concern engineers must avoid.
Try this
Q1. State what the coefficient of in a travelling-wave equation represents. [1 mark]
- Cue. , so it gives the frequency.
Q2. State the phase difference, in radians, between two points one wavelength apart on a wave. [1 mark]
- Cue. (they are in phase).
Q3. State the distance between adjacent nodes on a stationary wave in terms of wavelength. [1 mark]
- Cue. Half a wavelength.
Exam-style practice questions
Practice questions written in the style of SQA exam questions on this dot point, with worked answer explainers. The year tag is the paper they imitate, not the source.
SQA AH style5 marksA travelling wave is described by , with all quantities in SI units. State the amplitude, and calculate the frequency and the wavelength.Show worked answer →
Compare with the standard form .
Amplitude: (the coefficient in front of the sine).
Frequency: , so .
Wavelength: , so .
Markers reward reading the amplitude directly, equating the time coefficient to find the frequency, and the space coefficient to find the wavelength, all with units.
SQA AH style4 marksExplain how a stationary wave is formed and describe what is meant by a node and an antinode.Show worked answer →
A stationary wave is formed when two waves of the same frequency and amplitude travel in opposite directions and superpose, for example an incident wave and its reflection.
A node is a point of permanently zero displacement, where the two waves always cancel (destructive interference).
An antinode is a point of maximum amplitude, where the two waves always reinforce (constructive interference).
Markers reward the superposition of two oppositely directed waves of equal frequency and amplitude, and the definitions of node and antinode in terms of cancellation and reinforcement.
Related dot points
- The definition of simple harmonic motion, displacement, velocity and acceleration as functions of time, energy in SHM, and damping.
An SQA Advanced Higher Physics answer on simple harmonic motion, covering the defining relationship a equals minus omega squared y, displacement, velocity and acceleration as functions of time, the interchange of kinetic and potential energy, and damping.
- Coherence and path difference, constructive and destructive interference, division of amplitude in thin films and wedges, and division of wavefront in Young's double-slit experiment.
An SQA Advanced Higher Physics answer on interference, covering coherence and path difference, the conditions for constructive and destructive interference, division of amplitude in thin films and wedges, and division of wavefront in Young's double-slit experiment.
- Plane polarisation of transverse waves, the action of polarisers and Malus's law, polarisation by reflection and Brewster's angle, and applications.
An SQA Advanced Higher Physics answer on polarisation, covering plane polarisation as a property of transverse waves, the action of polarisers and Malus's law, polarisation by reflection and Brewster's angle, and practical applications.
- Photons and quantised energy, wave-particle duality and the de Broglie wavelength, the uncertainty principle, and quantum tunnelling.
An SQA Advanced Higher Physics answer on quantum theory, covering photons and quantised energy, wave-particle duality and the de Broglie wavelength, the Heisenberg uncertainty principle, and quantum tunnelling.
- Cosmic rays and the solar wind, the motion of charged particles in magnetic fields, and the formation of aurorae.
An SQA Advanced Higher Physics answer on particles from space, covering cosmic rays and the solar wind, the helical motion of charged particles in magnetic fields, and how charged particles interacting with the Earth's magnetic field and atmosphere produce aurorae.
Sources & how we know this
- SQA Advanced Higher Physics Course Specification — SQA (2019)