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Encyclopedia > Radiant intensity

In physics, intensity is a measure of the time-averaged energy flux. To find the intensity, take the energy density (that is, the energy per unit volume) and multiply it by the velocity at which the energy is moving. The resulting vector has the units of power divided by area (i.e. watt/mē). It is possible to define the intensity of the water coming from a garden sprinkler, but intensity is used most frequently with waves (i.e. sound or light).


The word "intensity" in physics is not synonymous with "strength", "amplitude", or "level", as it sometimes is in colloquial speech. For example, "the intensity of pressure" is physical nonsense.


If a point source is radiating energy in three dimensions, and there is no energy lost to the medium, then the intensity drops off as the distance from the object squared. The reason for this is one part physics, one part geometry. The physics comes from the conservation of energy (i.e. if the energy isn't being lost to the medium, it can't just disappear). The consequence of this is that the net power coming from the source must be constant, thus:

where P is the net power radiated, I is the intensity as a function of position, and dA is a differential element of a closed surface that contains the source. That P is a constant. If the source is radiating uniformly, that is, the same in all directions, and we take A to be a sphere centered on the source (so that I will be constant on its surface), the equation becomes:

where I is the intensity at the surface of the sphere, and r is the radius of the sphere (note: enclosed in parentheses is the expression for the surface area of a sphere). Solving for I, we get:

Anything that can carry energy can have an intensity associated with it.


If the medium is damped (i.e. both sound and light in air slowly lose energy), then the intensity drops off more quickly than the above equation suggests.


"No energy can get lost", not even slowly.


See also

SI light units

edit  (http://en.wikipedia.org/w/index.php?title=Template:SI_light_units&action=edit)

Quantity SI unit Symbol Notes
Luminous energy joule J
Luminous flux lumen or ( candela · steradian ) lm also called Luminous power
Luminous intensity candela cd
Luminance candela / square metre cd/m2 also called Luminosity
Illuminance lux or (lumen / square metre) lx
Luminous efficacy lumens per watt lm/w
SI radiometry units

edit  (http://en.wikipedia.org/w/index.php?title=Template:SI_radiometry_units&action=edit)

Quantity SI unit Symbol Notes
radiant energy joule J energy
radiant flux watt W radiant energy per unit time, also called radiant power
radiant intensity watts per steradian W · sr-1 power per unit solid angle
radiance watts per steradian per square metre W · sr-1 · m-2 power per unit solid angle per unit area
irrradiance watts per square metre W · m-2 power per unit area, also called radiant emittance or radiant exitance
spectral radiance watt per steradian per cubic metre W · sr-1 · m-3 commonly measured in W sr-1m-2nm-1
spectral irradiance watt per cubic metre W · m-3 commonly measured in W m-2 nm-1

  Results from FactBites:
 
Luminous intensity - Wikipedia, the free encyclopedia (210 words)
Luminous intensity should not be confused with luminous flux, which is the total perceived power emitted across all directions.
Luminous intensity is not the same as the radiant intensity, the corresponding objective physical quantity.
In 1881, Jules Violle proposed the Violle as a unit of luminous intensity, and it was notable as the first unit of light intensity that did not depend on the properties of a particular lamp.
  More results at FactBites »


 

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