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== M&Mは配らウッドヒスイの手鏡 ==
'''Etendue''' or '''étendue''' ("ay-tahn-doo") is a property of [[light]] in an [[optics|optical system]], which characterizes how "spread out" the light is in area and angle.


M&Mは配らウッドヒスイの手鏡 [http://www.lamartcorp.com/modules/mod_menu/rakuten_cl_11.php クリスチャンルブタン 取扱店]。<br><br>は「私を与える? [http://www.lamartcorp.com/modules/mod_menu/rakuten_cl_14.php クリスチャンルブタン アウトレット] '秦ゆう心李チャン。<br>huanlingミラーを持つ<br>、すべての可能性で、この第二の場所が手にします [http://www.lamartcorp.com/modules/mod_menu/rakuten_cl_5.php クリスチャンルブタン スニーカー]。DUANMUジェイドは、このM&M以来ミラーに直接投入<br><br>があります [http://www.lamartcorp.com/modules/mod_menu/rakuten_cl_12.php クリスチャンルブタン ブーツ]。<br><br>(紳士教会http://www.junzitang.comを提供しています)<br><br>は 'あなたは?'秦Yuは尋ねた。<br><br>「結婚し参加していきます、私は、秦ゆう、あなたは私は神の女王に達すると思いますか? 'DUANMUジェイド」は、秦の微笑み<br><br>羽が、実際には、私はあなたが初めて競争する場所は、アウト '羅ゆうナイフ」であることを参照してください、私は知っている......あなたがかもしれ<br>18人、唯一の本当の愛JIANGを<br>し、彼女のためにすべてを与えて喜んで。 '<br><br>「JIANGはおそらく幸せになります。あなたと結婚し、M&Mのミラーは、私が与えたので、私はまた、あなたが成功することができますことを願っています<br>あなたを<br>。 [http://www.lamartcorp.com/modules/mod_menu/rakuten_cl_13.php クリスチャンルブタン サンダル] '<br><br>DUANMUジェイドはまだM&Mが利きミラー
From the source point of view, it is the area of the source times the [[solid angle]] the system's [[entrance pupil]] [[subtend]]s as seen from the source. From the system point of view, the etendue is the area of the entrance pupil times the solid angle the source subtends as seen from the pupil. These definitions must be applied for infinitesimally small "elements" of area and solid angle, which must then be summed over both the source and the diaphragm as shown below. Etendue may be considered to be a volume in [[Hamiltonian_optics#Phase_space|phase space]].
相关的主题文章:
<ul>
 
  <li>[http://globalvage.com/home.php?mod=space&uid=61393 http://globalvage.com/home.php?mod=space&uid=61393]</li>
 
  <li>[http://meilisheng.cn/plus/view.php?aid=245403 http://meilisheng.cn/plus/view.php?aid=245403]</li>
 
  <li>[http://www.louyuwang.com/bbs/home.php?mod=space&uid=106344 http://www.louyuwang.com/bbs/home.php?mod=space&uid=106344]</li>
 
</ul>


== 他の充電時 ==
Etendue is important because it never decreases in any optical system. A perfect optical system produces an image with the same etendue as the source. The etendue is related to the [[Lagrange invariant]] and the [[optical invariant]], which share the property of being constant in an ideal optical system. The [[radiance]] of an optical system is equal to the derivative of the [[radiant flux]] with respect to the etendue.


どのように、セントはできる必要がありますか? [http://www.lamartcorp.com/modules/mod_menu/rakuten_cl_13.php クリスチャンルブタン 日本] '<br><br>「かもしれない」と青鳳最初に合意した [http://www.lamartcorp.com/modules/mod_menu/rakuten_cl_4.php クリスチャンルブタン パンプス]<br>青風水、デュZhongjun、3メッセンジャー目華ヤンにおけるhuan​​hangrnは、アーティファクトは、彼らが取得したいほとんどのものです [http://www.lamartcorp.com/modules/mod_menu/rakuten_cl_5.php クリスチャンルブタン ブーツ]<br><br>'それから私たちは、それを起動してください。「青風水は言った笑った。<br><br>「ジェントルメンウォーキング、私ははるかに送られました。「牙天軽く言った後、次の二つまたは三つのステップを向い明らかにキム·ウッド諸島指名手配金木島、牙天を飛ぶ、バックマロンタラの島に送られた。<br>レンヘンは、4つの直接北飛ん<br>華ヤン、デュZhongjunは、目標は、乾隆帝の大陸である [http://www.lamartcorp.com/modules/mod_menu/rakuten_cl_10.php クリスチャンルブタン 銀座]。九日の宮殿はあまり所持この9階宝物、秦Yuは息ほぼ千のトップグレードセントを受け取った、セント百個、各種貴重な万能薬が必要です。<br><br>「この限りトップグレードセントを持って、プラス私の中の神聖な獣「獣スペクトル '多数の十分な軍隊を作成します。 [http://www.lamartcorp.com/modules/mod_menu/rakuten_cl_3.php クリスチャンルブタン 靴] '秦ゆう英ムードは依然として非常に軽いです、彼は知らなかったものを外の世界。<br>他の充電時<br>
The term ''étendue'' comes from the French ''étendue géométrique'', meaning "geometrical extent". Other names for this property are '''acceptance''', '''throughput''', '''light-grasp''', '''collecting power''', '''optical extent''', and the '''A&Omega; product'''. ''Throughput'' and ''A&Omega; product'' are especially used in [[radiometry]] and radiative transfer where it is related to the [[view factor]] (or shape factor). It is a central concept in [[nonimaging optics]].<ref name="IntroductionNIO">Julio Chaves, ''Introduction to Nonimaging Optics'', CRC Press, 2008 [ISBN 978-1420054293]</ref><ref name="NIO">Roland Winston et al.,, ''Nonimaging Optics'', Academic Press, 2004 [ISBN 978-0127597515]</ref><ref name="Projection Displays">Matthew S. Brennesholtz, Edward H. Stupp, ''Projection Displays'', John Wiley & Sons Ltd, 2008 [ISBN 978-0470518038]</ref>
相关的主题文章:
 
<ul>
==Definition==
 
[[Image:Etendue-Definition.png|right|thumb|400px|Etendue for a [[differential element|differential surface element]] in 2D (left) and 3D (right).]]
  <li>[http://www.foreverexotic.com.au/6/index.cgi http://www.foreverexotic.com.au/6/index.cgi]</li>
 
 
An infinitesimal surface element, ''dS'', with normal '''n'''<sub>''S'' </sub> is immersed in a medium of [[refractive index]] ''n''. The surface is crossed by (or emits) light confined to a solid angle, ''d&Omega;'', at an angle &theta; with the normal '''n'''<sub>''S'' </sub>. The area of ''dS'' projected in the direction of the light propagation is<math>dS \cos{\theta}</math>. The etendue of this light crossing ''dS'' is defined in [[Two-dimensional space|2D]] as
  <li>[http://www.ccms.cc/forum.php?mod=viewthread&tid=93136&extra= http://www.ccms.cc/forum.php?mod=viewthread&tid=93136&extra=]</li>
 
 
:<math>d^2G := n dS \cos{\theta} d\theta \ </math>
  <li>[http://www.028dv.com/plus/feedback.php?aid=643 http://www.028dv.com/plus/feedback.php?aid=643]</li>
 
 
and in [[Three-dimensional space|3D]] as
  </ul>
 
:<math>d^2G := n^2 dS \cos{\theta} d\Omega \ </math>.
Because angles, solid angles, and refractive indices are [[dimensionless quantity|dimensionless quantities]], etendue has units of area (given by ''dS'').
 
==Conservation of etendue==
 
As shown below, etendue is conserved as light travels through free space and at  refractions or reflections. It is then also conserved as light travels through optical systems where it undergoes perfect reflections or refractions. However, if light was to hit, say, a [[Diffuser_(optics)|diffuser]], its solid angle would increase, increasing the etendue. Etendue can then remain constant or it can increase as light propagates through an optic, but it cannot decrease.
 
Conservation of etendue can be derived in different contexts, such as from optical first principles, from [[Hamiltonian optics]] or from the [[second law of thermodynamics]].<ref name="IntroductionNIO"/>
 
===In free space===
 
[[Image:Etendue-Free_space.png|right|thumb|300px|Etendue in free space]]
 
Consider a light source, &Sigma;, and a light "receiver", S, both of which are extended surfaces (rather than differential elements), and which are separated by a [[medium (optics)|medium]] of refractive index ''n'' that is perfectly [[transparency (optics)|transparent]] (shown). To compute the etendue of the system, one must consider the contribution of each point on the surface of the light source as they cast rays to each point on the receiver.<ref name="Wikilivre">[[Wikibooks:fr:Photographie/Photom%C3%A9trie/Notion_d%27%C3%A9tendue_g%C3%A9om%C3%A9trique|''Wikilivre de Photographie'']], ''Notion d'étendue géométrique'' (in French). Accessed 27 Jan 2009.</ref>
 
According to the definition above, the etendue of the light crossing ''d''&Sigma; towards ''dS'' is given by:
 
:<math>d^2G_\Sigma =n^2 d\Sigma \cos{\theta_\Sigma} d\Omega_\Sigma = n^2 d\Sigma \cos{\theta_\Sigma} \frac{dS \cos{\theta_S}}{d^2}</math>
 
where <math>d\Omega_\Sigma</math> is the solid angle defined by area ''dS'' at area ''d''&Sigma;. Accordingly, the etendue of the light crossing ''dS'' coming from ''d''&Sigma; is given by:
 
:<math>d^2G_S =n^2 dS \cos{\theta_S} d\Omega_S = n^2 dS \cos{\theta_S} \frac{d\Sigma \cos{\theta_\Sigma}}{d^2}</math>
 
where <math>d\Omega_S</math> is the solid angle defined by area ''d''&Sigma;. These expressions result in <math>d^2G_\Sigma = d^2G_S </math> showing that etendue is conserved as light propagates in free space.
 
The etendue of the whole system is then:
 
:<math>G = \int_\Sigma \!\int_S d^2G \ </math> <!--I hope this is right!-->
 
If both surfaces ''d''<sub>&Sigma;</sub> and ''dS'' are immersed in air (or in vacuum), ''n''=1 and the expression above for the etendue may be written as
 
:<math>d^2G = d\Sigma \cos{\theta_\Sigma} \frac{dS \cos{\theta_S}}{d^2}= \pi d\Sigma\left(\frac{\cos{\theta_\Sigma}\cos{\theta_S}}{\pi d^2} dS \right)=\pi d\Sigma F_{d\Sigma \rarr dS}</math>
 
where <math>F_{d\Sigma \rarr dS}</math> is the [[view factor]] between differential areas ''d''<sub>&Sigma;</sub> and ''dS''. Integration on ''d''<sub>&Sigma;</sub> and ''dS'' results in <math>G =\pi \Sigma F_{\Sigma \rarr S}</math> which allows the etendue between two surfaces to be obtained from the view factors between those surfaces, as provided in a [http://www.me.utexas.edu/~howell/tablecon.html list of view factors for specific geometry cases] or in several [[heat transfer]] textbooks.
 
The conservation of etendue in free space is related to the [[View_factor#View_factors_of_differential_areas|reciprocity theorem for view factors]].
 
===In refractions and reflections===
 
The conservation of etendue discussed above applies to the case of light propagation in free space, or more generally, in a medium in which the [[refractive index]] is constant. However, etendue is also conserved in refractions and reflections.<ref name="IntroductionNIO"/> Figure "etendue in refraction" shows an infinitesimal surface ''dS'' on the ''xy'' plane separating two media of refractive indices ''n''<sub>&Sigma;</sub> and ''n''<sub>S</sub>.
 
[[Image:Etendue-Refraction.png|right|thumb|300px|Etendue in refraction]]
 
The normal to ''dS'' points in the direction of the ''z'' axis. Incoming light is confined to a solid angle ''d''&Omega;<sub>&Sigma;</sub> and reaches ''dS'' at an angle ''&theta;''<sub>&Sigma;</sub> to its normal. Refracted light is confined to a solid angle ''d''&Omega;<sub>S</sub> and leaves ''dS'' at an angle ''&theta;''<sub>S</sub> to its normal. The directions of the incoming and refracted light are contained in a plane making an angle ''&phi;'' to the ''x'' axis, defining these directions in a [[spherical coordinate system]]. With these definitions, [[Snell's law]] of refraction can be written as
 
:<math>n_\Sigma \sin\theta_\Sigma=n_S \sin\theta_S \ </math>
 
and its derivative relative to ''&theta;''
 
:<math>n_\Sigma \cos\theta_\Sigma d \theta_\Sigma=n_S \cos\theta_S d \theta_S \ </math>
 
multiplied by each other result in
 
:<math>n_\Sigma^2 \cos\theta_\Sigma \left (\sin\theta_\Sigma d \theta_\Sigma d \varphi \right )=n_S^2 \cos\theta_S \left (\sin\theta_S d \theta_S d \varphi \right )</math>
 
where both sides of the equation were also multiplied by ''d&phi;'' which does not change on refraction. This expression can now be written as
 
:<math>n_\Sigma^2 \cos\theta_\Sigma d \Omega_\Sigma=n_S^2 \cos\theta_S d \Omega_S</math>
 
and multiplying both sides by ''dS'' we get
 
:<math>n_\Sigma^2 d S \cos\theta_\Sigma d \Omega_\Sigma=n_S^2 d S \cos\theta_S d \Omega_S</math>  &hArr;  <math>d^2G_\Sigma=d^2G_S \ </math>
 
showing that the etendue of the light refracted at ''dS'' is conserved. The same result is also valid for the case of a reflection at a surface ''dS'', in which case ''n''<sub>&Sigma;</sub>=''n''<sub>S</sub> and ''&theta;''<sub>&Sigma;</sub>=''&theta;''<sub>S</sub>.
 
==Conservation of basic radiance==
 
[[Radiance]] is defined by
 
:<math>L = \frac{d^2 \Phi}{dS \cos \theta d\Omega } = n^2 \frac{d^2 \Phi}{d^2 G}</math>
 
where ''n'' is the refractive index in which ''dS'' is immersed and ''d''<sup>2</sup>&Phi; is the [[radiant flux]] emitted by or crossing surface ''dS'' inside solid angle ''d''&Omega;. As light travels through an ideal optical system, both the etendue and the energy flux are conserved. Therefore, the basic radiance defined as<ref>William Ross McCluney, ''Introduction to Radiometry and Photometry'', Artech House, Boston, MA, 1994 [ISBN 978-0890066782]</ref>
 
:<math>L^* = \frac{L}{n^2}</math>
 
is also conserved. In real systems etendue may increase (for example due to diffusion) or the light flux may decrease (for example due to absorption) and, therefore, basic radiance may decrease. However, etendue may not decrease and energy flux may not increase and, therefore, basic radiance may not increase.
 
==Etendue as a volume in phase space==
 
In the context of [[Hamiltonian optics]], at a point in space, a light ray may be completely defined by a point '''P'''=(''x'',''y'',''z''), a unit [[Euclidean vector]] <math>\mathbf{v}=(\cos \alpha_X,\cos \alpha_Y,\cos \alpha_Z)</math> indicating its direction and the refractive index ''n'' at point '''P'''. The optical momentum of the ray at that point is defined by
 
:<math>\mathbf{p} = n (\cos \alpha_X,\cos \alpha_Y,\cos \alpha_Z)=(p,q,r)</math>
 
with <math>\|\mathbf{p}\|=n</math>. The geometry of the optical momentum vector is illustrated in figure "optical momentum".
 
[[Image:Etendue-Optical_Momentum.png|200px|thumb|right|Optical momentum]]
 
In a [[spherical coordinate system]] '''p''' may be written as
 
:<math> \mathbf{p} =n \left ( \sin \theta \cos \varphi, \sin \theta \sin \varphi, \cos \theta \right) \ </math>
 
from which
 
:<math> d p\, d q =\frac{\partial(p,q)}{\partial(\theta,\varphi)} d \theta \,d \varphi = \left ( \frac{\partial p}{\partial \theta} \frac{\partial q}{\partial \varphi} - \frac{\partial p}{\partial \varphi} \frac{\partial q}{\partial \theta}\right) d \theta\, d \varphi \ </math>
:<math>= n^2 \cos \theta \sin \theta \,d \theta d \varphi = n^2 \cos \theta d \Omega</math>
 
and therefore, for an infinitesimal area ''dS''=''dxdy'' on the ''xy'' plane immersed in a medium of refractive index ''n'', the etendue is given by
 
:<math>d^2G =n^2 dS \cos{\theta} d\Omega = d x\, d y\, d p\, d q  \ </math>
 
which is an infinitesimal volume in phase space ''x'',''y'',''p'',''q''. Conservation of etendue in phase space is the equivalent in optics to [[Liouville's_theorem_(Hamiltonian)|Liouville's theorem]] in classical mechanics.<ref name="IntroductionNIO"/> Etendue as volume in phase space is commonly used in [[nonimaging optics]].
 
==Maximum concentration==
 
[[Image:Etendue-Large_solid_angle.png|right|thumb|200px|Etendue for a large solid angle]]
 
Consider an infinitesimal area, ''dS'', immersed in a medium of refractive index ''n'' crossed by (or emitting) light inside a cone of angle ''&alpha;''. The etendue of this light is given by
:<math>dG=n^2 dS\int\cos\theta\,d\Omega = n^2 \int_{0}^{2\pi}\int_{0}^{\alpha}\cos \theta \sin \theta \, d\theta\, d\varphi</math> <math>=\pi n^2 dS \sin^2 \alpha \ </math>
Noting that <math>n \sin \alpha</math> is the [[numerical aperture]], NA, of the beam of light, this can also be expressed as
:<math>dG = \pi dS \mathrm{NA}^2</math>.
 
Note that ''d''&Omega; is expressed in a [[spherical coordinate system]]. Now, if a large surface ''S'' is crossed by (or emits) light also confined to a cone of angle ''&alpha;'', the etendue of the light crossing ''S'' is
 
:<math>G=\pi n^2 \sin^2 \alpha \int \,dS = \pi n^2 S \sin^2 \alpha = \pi S \mathrm{NA}^2</math>
 
[[Image:Etendue-Ideal_Concentration.png|left|thumb|250px|Etendue and ideal concentration]]
 
The limit on maximum concentration (shown) is an optic with an entrance aperture, ''S'', in air (''n<sub>I</sub>''=1) collecting light within a solid angle of angle 2''&alpha;'' (its [[Acceptance_angle_(solar_concentrator)|acceptance angle]]) and sending it to a smaller area receiver &Sigma; immersed in a medium of refractive index ''n'', whose points are illuminated within a solid angle of angle 2''&beta;''. From the above expression, the etendue of the incoming light is
 
:<math>G_I= \pi S \sin^2 \alpha \ </math>
 
and the etendue of the light reaching the receiver is
 
:<math>G_R= \pi n^2 \Sigma \sin^2 \beta \ </math>
 
Conservation of etendue ''G''<sub>I</sub>=''G''<sub>R</sub> then gives
 
:<math>C= \frac{S}{\Sigma}=n^2 \frac{\sin^2 \beta}{\sin^2 \alpha} \ </math>
 
where ''C'' is the concentration of the optic. For a given angular aperture, ''&alpha;'', of the incoming light, this concentration will be maximum for the maximum value of ''&beta;'', that is ''&beta;''=''&pi;''/2. The maximum possible concentration is then<ref name="IntroductionNIO"/><ref name="NIO"/>
 
:<math>C_\mathrm{max}= \frac{n^2}{\sin^2 \alpha} \ </math>
 
In the case that the incident index is not unity, we have
:<math>G_I = \pi n_I S \sin^2 \alpha=G_R = \pi n_R \Sigma \sin^2 \beta</math>
and so
:<math>C=\left(\frac{\mathrm{NA}_R}{\mathrm{NA}_I}\right)^2</math>
and in the best-case limit of <math>\beta=\pi/2</math>, this becomes
:<math>C_\mathrm{max}=\frac{n_R^2}{\mathrm{NA}_I^2}</math>.
 
If the optic were a [[collimator]] instead of a concentrator, the light direction is reversed and conservation of etendue gives us the minimum aperture, ''S'', for a given output full angle 2''&alpha;''.
 
==References==
{{Reflist}}
==See also==
*[[Light field]]
*[[Symplectic geometry]]
*[[Noether's theorem]]
 
==Further reading==
*{{cite book | first=John E. | last=Greivenkamp | year=2004 | title=Field Guide to Geometrical Optics | publisher=SPIE | others=SPIE Field Guides vol. '''FG01''' | isbn=0-8194-5294-7 }}
*Xutao Sun ''et al.'', 2006, "Etendue analysis and measurement of light source with elliptical reflector", ''Displays'' (27), 56–61.
 
[[Category:Optics]]

Latest revision as of 00:05, 3 November 2013

Etendue or étendue ("ay-tahn-doo") is a property of light in an optical system, which characterizes how "spread out" the light is in area and angle.

From the source point of view, it is the area of the source times the solid angle the system's entrance pupil subtends as seen from the source. From the system point of view, the etendue is the area of the entrance pupil times the solid angle the source subtends as seen from the pupil. These definitions must be applied for infinitesimally small "elements" of area and solid angle, which must then be summed over both the source and the diaphragm as shown below. Etendue may be considered to be a volume in phase space.

Etendue is important because it never decreases in any optical system. A perfect optical system produces an image with the same etendue as the source. The etendue is related to the Lagrange invariant and the optical invariant, which share the property of being constant in an ideal optical system. The radiance of an optical system is equal to the derivative of the radiant flux with respect to the etendue.

The term étendue comes from the French étendue géométrique, meaning "geometrical extent". Other names for this property are acceptance, throughput, light-grasp, collecting power, optical extent, and the AΩ product. Throughput and AΩ product are especially used in radiometry and radiative transfer where it is related to the view factor (or shape factor). It is a central concept in nonimaging optics.[1][2][3]

Definition

File:Etendue-Definition.png
Etendue for a differential surface element in 2D (left) and 3D (right).

An infinitesimal surface element, dS, with normal nS is immersed in a medium of refractive index n. The surface is crossed by (or emits) light confined to a solid angle, , at an angle θ with the normal nS . The area of dS projected in the direction of the light propagation is. The etendue of this light crossing dS is defined in 2D as

and in 3D as

.

Because angles, solid angles, and refractive indices are dimensionless quantities, etendue has units of area (given by dS).

Conservation of etendue

As shown below, etendue is conserved as light travels through free space and at refractions or reflections. It is then also conserved as light travels through optical systems where it undergoes perfect reflections or refractions. However, if light was to hit, say, a diffuser, its solid angle would increase, increasing the etendue. Etendue can then remain constant or it can increase as light propagates through an optic, but it cannot decrease.

Conservation of etendue can be derived in different contexts, such as from optical first principles, from Hamiltonian optics or from the second law of thermodynamics.[1]

In free space

Etendue in free space

Consider a light source, Σ, and a light "receiver", S, both of which are extended surfaces (rather than differential elements), and which are separated by a medium of refractive index n that is perfectly transparent (shown). To compute the etendue of the system, one must consider the contribution of each point on the surface of the light source as they cast rays to each point on the receiver.[4]

According to the definition above, the etendue of the light crossing dΣ towards dS is given by:

where is the solid angle defined by area dS at area dΣ. Accordingly, the etendue of the light crossing dS coming from dΣ is given by:

where is the solid angle defined by area dΣ. These expressions result in showing that etendue is conserved as light propagates in free space.

The etendue of the whole system is then:

If both surfaces dΣ and dS are immersed in air (or in vacuum), n=1 and the expression above for the etendue may be written as

where is the view factor between differential areas dΣ and dS. Integration on dΣ and dS results in which allows the etendue between two surfaces to be obtained from the view factors between those surfaces, as provided in a list of view factors for specific geometry cases or in several heat transfer textbooks.

The conservation of etendue in free space is related to the reciprocity theorem for view factors.

In refractions and reflections

The conservation of etendue discussed above applies to the case of light propagation in free space, or more generally, in a medium in which the refractive index is constant. However, etendue is also conserved in refractions and reflections.[1] Figure "etendue in refraction" shows an infinitesimal surface dS on the xy plane separating two media of refractive indices nΣ and nS.

File:Etendue-Refraction.png
Etendue in refraction

The normal to dS points in the direction of the z axis. Incoming light is confined to a solid angle dΩΣ and reaches dS at an angle θΣ to its normal. Refracted light is confined to a solid angle dΩS and leaves dS at an angle θS to its normal. The directions of the incoming and refracted light are contained in a plane making an angle φ to the x axis, defining these directions in a spherical coordinate system. With these definitions, Snell's law of refraction can be written as

and its derivative relative to θ

multiplied by each other result in

where both sides of the equation were also multiplied by which does not change on refraction. This expression can now be written as

and multiplying both sides by dS we get

showing that the etendue of the light refracted at dS is conserved. The same result is also valid for the case of a reflection at a surface dS, in which case nΣ=nS and θΣ=θS.

Conservation of basic radiance

Radiance is defined by

where n is the refractive index in which dS is immersed and d2Φ is the radiant flux emitted by or crossing surface dS inside solid angle dΩ. As light travels through an ideal optical system, both the etendue and the energy flux are conserved. Therefore, the basic radiance defined as[5]

is also conserved. In real systems etendue may increase (for example due to diffusion) or the light flux may decrease (for example due to absorption) and, therefore, basic radiance may decrease. However, etendue may not decrease and energy flux may not increase and, therefore, basic radiance may not increase.

Etendue as a volume in phase space

In the context of Hamiltonian optics, at a point in space, a light ray may be completely defined by a point P=(x,y,z), a unit Euclidean vector indicating its direction and the refractive index n at point P. The optical momentum of the ray at that point is defined by

with . The geometry of the optical momentum vector is illustrated in figure "optical momentum".

File:Etendue-Optical Momentum.png
Optical momentum

In a spherical coordinate system p may be written as

from which

and therefore, for an infinitesimal area dS=dxdy on the xy plane immersed in a medium of refractive index n, the etendue is given by

which is an infinitesimal volume in phase space x,y,p,q. Conservation of etendue in phase space is the equivalent in optics to Liouville's theorem in classical mechanics.[1] Etendue as volume in phase space is commonly used in nonimaging optics.

Maximum concentration

File:Etendue-Large solid angle.png
Etendue for a large solid angle

Consider an infinitesimal area, dS, immersed in a medium of refractive index n crossed by (or emitting) light inside a cone of angle α. The etendue of this light is given by

Noting that is the numerical aperture, NA, of the beam of light, this can also be expressed as

.

Note that dΩ is expressed in a spherical coordinate system. Now, if a large surface S is crossed by (or emits) light also confined to a cone of angle α, the etendue of the light crossing S is

File:Etendue-Ideal Concentration.png
Etendue and ideal concentration

The limit on maximum concentration (shown) is an optic with an entrance aperture, S, in air (nI=1) collecting light within a solid angle of angle 2α (its acceptance angle) and sending it to a smaller area receiver Σ immersed in a medium of refractive index n, whose points are illuminated within a solid angle of angle 2β. From the above expression, the etendue of the incoming light is

and the etendue of the light reaching the receiver is

Conservation of etendue GI=GR then gives

where C is the concentration of the optic. For a given angular aperture, α, of the incoming light, this concentration will be maximum for the maximum value of β, that is β=π/2. The maximum possible concentration is then[1][2]

In the case that the incident index is not unity, we have

and so

and in the best-case limit of , this becomes

.

If the optic were a collimator instead of a concentrator, the light direction is reversed and conservation of etendue gives us the minimum aperture, S, for a given output full angle 2α.

References

43 year old Petroleum Engineer Harry from Deep River, usually spends time with hobbies and interests like renting movies, property developers in singapore new condominium and vehicle racing. Constantly enjoys going to destinations like Camino Real de Tierra Adentro.

See also

Further reading

  • 20 year-old Real Estate Agent Rusty from Saint-Paul, has hobbies and interests which includes monopoly, property developers in singapore and poker. Will soon undertake a contiki trip that may include going to the Lower Valley of the Omo.

    My blog: http://www.primaboinca.com/view_profile.php?userid=5889534
  • Xutao Sun et al., 2006, "Etendue analysis and measurement of light source with elliptical reflector", Displays (27), 56–61.
  1. 1.0 1.1 1.2 1.3 1.4 Julio Chaves, Introduction to Nonimaging Optics, CRC Press, 2008 [ISBN 978-1420054293]
  2. 2.0 2.1 Roland Winston et al.,, Nonimaging Optics, Academic Press, 2004 [ISBN 978-0127597515]
  3. Matthew S. Brennesholtz, Edward H. Stupp, Projection Displays, John Wiley & Sons Ltd, 2008 [ISBN 978-0470518038]
  4. Wikilivre de Photographie, Notion d'étendue géométrique (in French). Accessed 27 Jan 2009.
  5. William Ross McCluney, Introduction to Radiometry and Photometry, Artech House, Boston, MA, 1994 [ISBN 978-0890066782]