What Is the Intensity of a Travelling Plane Electromagnetic Wave

Power transferred per unit area

In physics, the intensity or flux of radiant energy is the power transferred per unit area, where the area is measured on the plane perpendicular to the management of propagation of the energy. In the SI system, it has units watts per square metre (West/10002), or kg⋅s−3 in base units. Intensity is used almost frequently with waves such equally acoustic waves (sound) or electromagnetic waves such equally light or radio waves, in which case the average power transfer over one period of the wave is used. Intensity can be practical to other circumstances where energy is transferred. For instance, one could calculate the intensity of the kinetic energy carried by drops of water from a garden sprinkler.

The give-and-take "intensity" as used here is not synonymous with "force", "amplitude", "magnitude", or "level", equally it sometimes is in colloquial spoken communication.

Intensity can be found by taking the free energy density (free energy per unit volume) at a bespeak in infinite and multiplying information technology past the velocity at which the energy is moving. The resulting vector has the units of power divided by area (i.eastward., surface ability density).

Mathematical description [edit]

If a point source is radiating free energy in all directions (producing a spherical moving ridge), and no free energy is captivated or scattered by the medium, then the intensity decreases in proportion to the distance from the object squared. This is an example of the inverse-square police.

Applying the law of conservation of free energy, if the net power emanating is constant,

P = I d A , {\displaystyle P=\int \mathbf {I} \,\cdot d\mathbf {A} ,}

where P is the internet ability radiated, I is the intensity vector equally a function of position, the magnitude | I | is the intensity equally a office of position, and d A is a differential element of a airtight surface that contains the source.

If one integrates a compatible intensity, | I | = abiding, over a surface that is perpendicular to the intensity vector, for case over a sphere centered around the point source, the equation becomes

P = | I | A s u r f = | I | 4 π r ii , {\displaystyle P=|I|\cdot A_{\mathrm {surf} }=|I|\cdot iv\pi r^{ii}\,,}

where | I | is the intensity at the surface of the sphere, r is the radius of the sphere, and A southward u r f = 4 π r 2 {\displaystyle A_{\mathrm {surf} }=iv\pi r^{2}} is the expression for the surface area of a sphere.

Solving for | I | gives

| I | = P A s u r f = P iv π r two . {\displaystyle |I|={\frac {P}{A_{\mathrm {surf} }}}={\frac {P}{4\pi r^{2}}}.}

If the medium is damped, then the intensity drops off more quickly than the in a higher place equation suggests.

Anything that can transmit energy can have an intensity associated with it. For a monochromatic propagating electromagnetic moving ridge, such as a aeroplane wave or a Gaussian beam, if Due east is the complex amplitude of the electric field, then the time-averaged energy density of the wave, travelling in a non-magnetic material, is given past:

U = due north 2 ε 0 2 | E | 2 , {\displaystyle \left\langle U\right\rangle ={\frac {due north^{2}\varepsilon _{0}}{two}}|E|^{ii},}

and the local intensity is obtained past multiplying this expression by the moving ridge velocity, c/northward:

I = c n ε 0 2 | E | 2 , {\displaystyle I={\frac {\mathrm {c} n\varepsilon _{0}}{two}}|E|^{2},}

where northward is the refractive index, c is the speed of lite in vacuum and ε 0 {\displaystyle \varepsilon _{0}} is the vacuum permittivity.

For non-monochromatic waves, the intensity contributions of different spectral components can but be added. The treatment above does non concur for capricious electromagnetic fields. For instance, an evanescent wave may have a finite electrical aamplitude while not transferring any power. The intensity should and so be divers as the magnitude of the Poynting vector.[1]

Alternative definitions [edit]

In photometry and radiometry intensity has a unlike significant: it is the luminous or radiant ability per unit solid bending. This tin can crusade confusion in optics, where intensity can mean whatsoever of radiant intensity, luminous intensity or irradiance, depending on the groundwork of the person using the term. Radiance is as well sometimes called intensity, particularly past astronomers and astrophysicists, and in oestrus transfer.

Run into also [edit]

  • Field strength
  • Sound intensity
  • Magnitude (astronomy)

References [edit]

  1. ^ Paschotta, Rüdiger. "Optical Intensity". Encyclopedia of Laser Physics and Technology. RP Photonics.

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