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Explanation: actually, the amounts are just fractionally under the next integer
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{{otheruses|Intensity (disambiguation)}}
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In the field of [[heat transfer]], '''intensity of radiation''' <math>I</math> is a measure of the distribution of radiant heat flux per unit area and [[solid angle]], in a particular direction, defined according to
 
:<math>dq = I\, d\omega\, \cos \theta\, dA</math>
 
where
 
*<math>dA</math> is the infinitesimal source area
*<math>dq</math> is the ''outgoing'' heat transfer from the area <math>dA</math>
*<math>d\omega</math> is the [[solid angle]] subtended by the infinitesimal 'target' (or 'aperture') area <math>dA_a</math>
*<math>\theta</math> is the angle between the source area normal vector and the line-of-sight between the source and the target areas.
 
Typical units of intensity are W·m<sup>-2</sup>·sr<sup>-1</sup>.
 
Intensity can sometimes be called [[radiance]], especially in other fields of study.
 
The emissive power of a surface can be determined by integrating the intensity of emitted radiation over a hemisphere surrounding the surface:
 
:<math>q = \int_{\phi=0}^{2\pi} \int_{\theta=0}^{\pi/2} I \cos \theta \sin \theta d\theta d\phi</math>
 
For diffuse emitters, the emitted radiation intensity is the same in all directions, with the result that
 
:<math>E = \pi I</math>
 
The factor <math>\pi</math> (which really should have the units of [[steradian]]s) is a result of the fact that intensity is defined to exclude the effect of reduced [[view factor]] at large values <math>\theta</math>; note that the solid angle corresponding to a hemisphere is equal to <math>2\pi</math> steradians.
 
'''[[Specific radiative intensity|Spectral intensity]]''' <math>I_\lambda</math> is the corresponding spectral measurement of intensity; in other words, the intensity as a function of [[wavelength]].
 
== See also ==
* [[Non-ionising radiation]]
* [[Emissivity]]
 
== References ==
 
* Lienhard and Lienhard, ''[http://web.mit.edu/lienhard/www/ahtt.html A heat transfer textbook]'', 3rd Ed, 2008 (available for free online)
* J P Holman, '' Heat Transfer'' 9th Ed, McGraw Hill, 2002.
* [[F. P. Incropera]] and D. P. DeWitt, ''Fundamentals of Heat and Mass Transfer'', 4th Ed, Wiley, 1996.
 
[[Category:Heat transfer]]
[[Category:Radiation]]

Revision as of 09:50, 4 February 2014

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