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In physics, a **transverse wave** is a wave whose oscillations are perpendicular to the direction of the wave's advance. This is in contrast to a longitudinal wave which travels in the direction of its oscillations. Water waves are an example of transverse wave.

- Mathematical formulation
- Superposition principle
- Circular polarization
- Power in a transverse wave in string
- See also
- References
- External links

A simple example is given by the waves that can be created on a horizontal length of string by anchoring one end and moving the other end up and down. Another example is the waves that are created on the membrane of a drum. The waves propagate in directions that are parallel to the membrane plane, but each point in the membrane itself gets displaced up and down, perpendicular to that plane. Light is another example of a transverse wave, where the oscillations are the electric and magnetic fields, which point at right angles to the ideal light rays that describe the direction of propagation.

Transverse waves commonly occur in elastic solids due to the shear stress generated; the oscillations in this case are the displacement of the solid particles away from their relaxed position, in directions perpendicular to the propagation of the wave. These displacements correspond to a local shear deformation of the material. Hence a transverse wave of this nature is called a **shear wave**. Since fluids cannot resist shear forces while at rest, propagation of transverse waves inside the bulk of fluids is not possible.^{ [1] } In seismology, shear waves are also called **secondary waves** or **S-waves**.

Transverse waves are contrasted with longitudinal waves, where the oscillations occur in the direction of the wave. The standard example of a longitudinal wave is a sound wave or "pressure wave" in gases, liquids, or solids, whose oscillations cause compression and expansion of the material through which the wave is propagating. Pressure waves are called "primary waves", or "P-waves" in geophysics.

Mathematically, the simplest kind of transverse wave is a **plane linearly polarized sinusoidal** one. "Plane" here means that the direction of propagation is unchanging and the same over the whole medium; "linearly polarized" means that the direction of displacement too is unchanging and the same over the whole medium; and the magnitude of the displacement is a sinusoidal function only of time and of position along the direction of propagation.

The motion of such a wave can be expressed mathematically as follows. Let *d* be the direction of propagation (a vector with unit length), and *o* any reference point in the medium. Let *u* be the direction of the oscillations (another unit-length vector perpendicular to *d*). The displacement of a particle at any point *p* of the medium and any time *t* (seconds) will be

where *A* is the wave's **amplitude** or **strength**, *T* is its **period**, *v* is the **speed** of propagation, and *φ* is its **phase** at *o*. All these parameters are real numbers. The symbol "•" denotes the inner product of two vectors.

By this equation, the wave travels in the direction *d* and the oscillations occur back and forth along the direction *u*. The wave is said to be linearly polarized in the direction *u*.

An observer that looks at a fixed point *p* will see the particle there move in a simple harmonic (sinusoidal) motion with period *T* seconds, with maximum particle displacement *A* in each sense; that is, with a **frequency** of *f* = 1/*T* full oscillation cycles every second. A snapshot of all particles at a fixed time *t* will show the same displacement for all particles on each plane perpendicular to *d*, with the displacements in successive planes forming a sinusoidal pattern, with each full cycle extending along *d* by the **wavelength***λ* = *v**T* = *v*/*f*. The whole pattern moves in the direction *d* with speed *V*.

The same equation describes a plane linearly polarized sinusoidal light wave, except that the "displacement" *S*(*p*, *t*) is the electric field at point *p* and time *t*. (The magnetic field will be described by the same equation, but with a "displacement" direction that is perpendicular to both *d* and *u*, and a different amplitude.)

In a homogeneous linear medium, complex oscillations (vibrations in a material or light flows) can be described as the superposition of many simple sinusoidal waves, either transverse or longitudinal.

The vibrations of a violin string, for example, can be analyzed as the sum of many transverse waves of different frequencies, that displace the string either up or down or left to right. The ripples in a pond can be analyzed as a combination of transverse and longitudinal waves (gravity waves) that propagate together.

If the medium is linear and allows multiple independent displacement directions for the same travel direction *d*, we can choose two mutually perpendicular directions of polarization, and express any wave linearly polarized in any other direction as a linear combination (mixing) of those two waves.

By combining two waves with same frequency, velocity, and direction of travel, but with different phases and independent displacement directions, one obtains a circularly or elliptically polarized wave. In such a wave the particles describe circular or elliptical trajectories, instead of moving back and forth.

It may help understanding to revisit the thought experiment with a taut string mentioned above. Notice that you can also launch waves on the string by moving your hand to the right and left instead of up and down. This is an important point. There are two independent (orthogonal) directions that the waves can move. (This is true for any two directions at right angles, up and down and right and left are chosen for clarity.) Any waves launched by moving your hand in a straight line are linearly polarized waves.

But now imagine moving your hand in a circle. Your motion will launch a spiral wave on the string. You are moving your hand simultaneously both up and down and side to side. The maxima of the side to side motion occur a quarter wavelength (or a quarter of a way around the circle, that is 90 degrees or π/2 radians) from the maxima of the up and down motion. At any point along the string, the displacement of the string will describe the same circle as your hand, but delayed by the propagation speed of the wave. Notice also that you can choose to move your hand in a clockwise circle or a counter-clockwise circle. These alternate circular motions produce right and left circularly polarized waves.

To the extent your circle is imperfect, a regular motion will describe an ellipse, and produce elliptically polarized waves. At the extreme of eccentricity your ellipse will become a straight line, producing linear polarization along the major axis of the ellipse. An elliptical motion can always be decomposed into two orthogonal linear motions of unequal amplitude and 90 degrees out of phase, with circular polarization being the special case where the two linear motions have the same amplitude.

(Let the linear mass density of the string be μ.)

The kinetic energy of a mass element in a transverse wave is given by:

In one wavelength, kinetic energy

Using Hooke's law the potential energy in mass element

And the potential energy for one wavelength

So, total energy in one wavelength

Therefore average power is ^{ [2] }

- Longitudinal wave
- Luminiferous aether – the postulated medium for light waves; accepting that light was a transverse wave prompted a search for evidence of this physical medium
- Shear wave splitting
- Sinusoidal plane-wave solutions of the electromagnetic wave equation
- Transverse mode
- Elastography
- Shear-wave elasticity imaging

In physics, mathematics, and related fields, a **wave** is a propagating dynamic disturbance of one or more quantities. Waves can be periodic, in which case those quantities oscillate repeatedly about an equilibrium (resting) value at some frequency. When the entire waveform moves in one direction, it is said to be a *traveling wave*; by contrast, a pair of superimposed periodic waves traveling in opposite directions makes a *standing wave*. In a standing wave, the amplitude of vibration has nulls at some positions where the wave amplitude appears smaller or even zero. Waves are often described by a *wave equation* or a one-way wave equation for single wave propagation in a defined direction.

**Polarization** is a property applying to transverse waves that specifies the geometrical orientation of the oscillations. In a transverse wave, the direction of the oscillation is perpendicular to the direction of motion of the wave. A simple example of a polarized transverse wave is vibrations traveling along a taut string *(see image)*; for example, in a musical instrument like a guitar string. Depending on how the string is plucked, the vibrations can be in a vertical direction, horizontal direction, or at any angle perpendicular to the string. In contrast, in longitudinal waves, such as sound waves in a liquid or gas, the displacement of the particles in the oscillation is always in the direction of propagation, so these waves do not exhibit polarization. Transverse waves that exhibit polarization include electromagnetic waves such as light and radio waves, gravitational waves, and transverse sound waves in solids.

The **propagation constant** of a sinusoidal electromagnetic wave is a measure of the change undergone by the amplitude and phase of the wave as it propagates in a given direction. The quantity being measured can be the voltage, the current in a circuit, or a field vector such as electric field strength or flux density. The propagation constant itself measures the change per unit length, but it is otherwise dimensionless. In the context of two-port networks and their cascades, **propagation constant **measures the change undergone by the source quantity as it propagates from one port to the next.

In physics, a **standing wave**, also known as a **stationary wave**, is a wave that oscillates in time but whose peak amplitude profile does not move in space. The peak amplitude of the wave oscillations at any point in space is constant with respect to time, and the oscillations at different points throughout the wave are in phase. The locations at which the absolute value of the amplitude is minimum are called nodes, and the locations where the absolute value of the amplitude is maximum are called antinodes.

**Longitudinal waves** are waves in which the vibration of the medium is parallel ("along") to the direction the wave travels and displacement of the medium is in the same direction of the wave propagation. Mechanical longitudinal waves are also called *compressional* or **compression waves**, because they produce compression and rarefaction when traveling through a medium, and **pressure waves**, because they produce increases and decreases in pressure. A wave along the length of a stretched Slinky toy, where the distance between coils increases and decreases, is a good visualization. Real-world examples include sound waves and seismic P-waves.

In the physical sciences, the **wavenumber** is the *spatial frequency* of a wave, measured in cycles per unit distance or radians per unit distance. It is analogous to temporal frequency, which is defined as the number of wave cycles per unit time or radians per unit time.

A **sine wave**, **sinusoidal wave**, or just **sinusoid** is a mathematical curve defined in terms of the *sine* trigonometric function, of which it is the graph. It is a type of continuous wave and also a smooth periodic function. It occurs often in mathematics, as well as in physics, engineering, signal processing and many other fields.

A **normal mode** of a dynamical system is a pattern of motion in which all parts of the system move sinusoidally with the same frequency and with a fixed phase relation. The free motion described by the normal modes takes place at fixed frequencies. These fixed frequencies of the normal modes of a system are known as its natural frequencies or resonant frequencies. A physical object, such as a building, bridge, or molecule, has a set of normal modes and their natural frequencies that depend on its structure, materials and boundary conditions.

In physics, a **wave vector** is a vector which helps describe a wave. Like any vector, it has a magnitude and direction, both of which are important. Its magnitude is either the wavenumber or angular wavenumber of the wave, and its direction is ordinarily the direction of wave propagation.

In the physical sciences and electrical engineering, **dispersion relations** describe the effect of dispersion on the properties of waves in a medium. A dispersion relation relates the wavelength or wavenumber of a wave to its frequency. Given the dispersion relation, one can calculate the phase velocity and group velocity of waves in the medium, as a function of frequency. In addition to the geometry-dependent and material-dependent dispersion relations, the overarching Kramers–Kronig relations describe the frequency dependence of wave propagation and attenuation.

In seismology and other areas involving elastic waves, **S waves**, **secondary waves**, or **shear waves** are a type of elastic wave and are one of the two main types of elastic body waves, so named because they move through the body of an object, unlike surface waves.

In elastodynamics, **Love waves**, named after Augustus Edward Hough Love, are horizontally polarized surface waves. The Love wave is a result of the interference of many shear waves (S-waves) guided by an elastic layer, which is *welded* to an elastic half space on one side while bordering a vacuum on the other side. In seismology, **Love waves** are surface seismic waves that cause horizontal shifting of the Earth during an earthquake. Augustus Edward Hough Love predicted the existence of Love waves mathematically in 1911. They form a distinct class, different from other types of seismic waves, such as P-waves and S-waves, or Rayleigh waves. Love waves travel with a lower velocity than P- or S- waves, but faster than Rayleigh waves. These waves are observed only when there is a low velocity layer overlying a high velocity layer/ sub–layers.

The **electromagnetic wave equation** is a second-order partial differential equation that describes the propagation of electromagnetic waves through a medium or in a vacuum. It is a three-dimensional form of the wave equation. The homogeneous form of the equation, written in terms of either the electric field **E** or the magnetic field **B**, takes the form:

The **linear attenuation coefficient**, **attenuation coefficient**, or **narrow-beam attenuation coefficient** characterizes how easily a volume of material can be penetrated by a beam of light, sound, particles, or other energy or matter. A coefficient value that is large represents a beam becoming 'attenuated' as it passes through a given medium, while a small value represents that the medium had little effect on loss. The SI unit of attenuation coefficient is the reciprocal metre (m^{−1}). **Extinction coefficient** is another term for this quantity, often used in meteorology and climatology. Most commonly, the quantity measures the exponential decay of intensity, that is, the value of downward *e*-folding distance of the original intensity as the energy of the intensity passes through a unit thickness of material, so that an attenuation coefficient of 1 m^{−1} means that after passing through 1 metre, the radiation will be reduced by a factor of *e*, and for material with a coefficient of 2 m^{−1}, it will be reduced twice by *e*, or *e*^{2}. Other measures may use a different factor than *e*, such as the *decadic attenuation coefficient* below. The **broad-beam attenuation coefficient** counts forward-scattered radiation as transmitted rather than attenuated, and is more applicable to radiation shielding.

**Lamb waves** propagate in solid plates or spheres. They are elastic waves whose particle motion lies in the plane that contains the direction of wave propagation and the direction perpendicular to the plate. In 1917, the English mathematician Horace Lamb published his classic analysis and description of acoustic waves of this type. Their properties turned out to be quite complex. An infinite medium supports just two wave modes traveling at unique velocities; but plates support two infinite sets of Lamb wave modes, whose velocities depend on the relationship between wavelength and plate thickness.

The **acoustoelastic effect** is how the sound velocities of an elastic material change if subjected to an initial static stress field. This is a non-linear effect of the constitutive relation between mechanical stress and finite strain in a material of continuous mass. In classical linear elasticity theory small deformations of most elastic materials can be described by a linear relation between the applied stress and the resulting strain. This relationship is commonly known as the generalised Hooke's law. The linear elastic theory involves second order elastic constants and yields constant longitudinal and shear sound velocities in an elastic material, not affected by an applied stress. The acoustoelastic effect on the other hand include higher order expansion of the constitutive relation between the applied stress and resulting strain, which yields longitudinal and shear sound velocities dependent of the stress state of the material. In the limit of an unstressed material the sound velocities of the linear elastic theory are reproduced.

In fluid dynamics, **Green's law**, named for 19th-century British mathematician George Green, is a conservation law describing the evolution of non-breaking, surface gravity waves propagating in shallow water of gradually varying depth and width. In its simplest form, for wavefronts and depth contours parallel to each other, it states:

In fluid dynamics, **Stokes problem** also known as **Stokes second problem** or sometimes referred to as **Stokes boundary layer** or **Oscillating boundary layer** is a problem of determining the flow created by an oscillating solid surface, named after Sir George Stokes. This is considered one of the simplest unsteady problem that have exact solution for the Navier-Stokes equations. In turbulent flow, this is still named a Stokes boundary layer, but now one has to rely on experiments, numerical simulations or approximate methods in order to obtain useful information on the flow.

In physics, a **sinusoidal****plane wave** is a special case of plane wave: a field whose value varies as a sinusoidal function of time and of the distance from some fixed plane.

- ↑ "Fluid Mechanics II: Viscosity and Shear stresses" (PDF).
`{{cite web}}`

: CS1 maint: url-status (link) - ↑ "16.4 Energy and Power of a Wave - University Physics Volume 1 | OpenStax".
*openstax.org*. Retrieved 2022-01-28.

- Interactive simulation of transverse wave
- Wave types explained with high speed film and animations
- Weisstein, Eric Wolfgang (ed.). "Transverse Wave".
*ScienceWorld*. - Transverse and Longitudinal Waves Introductory module on these waves at Connexions

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