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        <title>en:yanding:imaging_basics:optics:radiometry_photometry:cie_luminous_efficiency_function</title>
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        <description>CIE Standard Luminous Efficiency Function

I. Definition

The CIE luminous efficiency function $V(\lambda)$ is a standard response function established by the International Commission on Illumination (CIE) to describe the relative visual sensitivity of the standard observer$\Phi_{e,\lambda}$$\lambda$$\Phi_{e,\lambda_m}$$\lambda_m$$\Phi_{e,\lambda_m}/\Phi_{e,\lambda}$$V(\lambda)$$L &gt; 5 cd·m⁻²$$V(\lambda)$$CIE 1988 (CIE 086-1990)$$4^\circ$\(V(\lambda)\)$4^\circ$\(V_{10}(\lambda)\)$L &lt; 0.005\ \math…</description>
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        <title>en:yanding:imaging_basics:optics:radiometry_photometry:illuminance</title>
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        <description>Illuminance

Illuminance

Illuminance is a physical quantity that characterizes the amount of luminous flux received per unit area of an illuminated surface, directly reflecting the degree to which the surface is illuminated. Its magnitude depends on the luminous intensity of the light source, the irradiation distance, and the angle (following the inverse square law and the cosine law), and is independent of the intrinsic properties of the illuminated object, such as its material and reflection …</description>
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        <description>Irradiance

I.Definition 

Irradiance (denoted by $E$) is the radiant flux incident on a surface per unit area. Its SI unit is $W\cdot m^{-2}$

Mathematical Expression: 

$$E = \frac{d\Phi}{d$}$$
where $\Phi$ is the radiant flux and $A$ is the surface area.


II.Irradiance from a point source

For an isotropic point source, the radiant intensity in a given direction is denoted by $I$$W\cdot sr^{-1}$$dA$$dA$$$d\Omega = \frac{dA}{r^2}$$$$d\Phi = I \cdot d\Omega = I \cdot \frac{dA}{r^2}$$$$E = \fra…</description>
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        <title>en:yanding:imaging_basics:optics:radiometry_photometry:luminance</title>
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        <description>Luminance

Luminance (symbol:$L$) is a photometric measure of the luminous intensity per unit area of light travelling in a given direction. It describes the amount of light that passes through, is emitted from, or is reflected off a particular surface. Luminance characterizes the human visual perception of $$L = \frac{I_\theta}{S \cdot \cos\theta}$$$L$$\mathrm{cd/m^2}$$I_\theta$$\mathrm{cd}$$S$$\mathrm{m^2}$$\theta$$\mathrm{rad}$$^\circ$$S \cdot \cos\theta$$\mathrm{cd/m^2}$</description>
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        <title>en:yanding:imaging_basics:optics:radiometry_photometry:luminous_efficacy</title>
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        <description>FIXME This page is not fully translated, yet. Please help completing the translation.

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Luminous Efficacy

1. Definition

Luminous efficacy is a metric that measures the efficiency of a light source in converting energy into visible light. It is defined as the ratio of luminous flux ($\Phi_V$${lm·W}^{-1}$$K(\lambda)$$$K = \frac{\Phi_V}{\Phi_e} = \frac{\int_0^\infty K(\lambda)\Phi_{e,\lambda}\mathrm{d}\lambda}{\int_0^\infty \Phi_{e,\lambd…</description>
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        <description>Luminous Exitance

Luminous exitance (symbol: $M_v$, $M$)is a fundamental physical quantity in photometry used to characterize the emission properties of a surface light source. It quantifies the capability of a surface to emit visible light outwards, describing the total luminous flux output per unit area, regardless of the directional distribution of the emitted light.$d\Phi_v$$2\pi$$dA$$d\Phi_v$$dA$$$M_v = \frac{d\Phi_v}{dA}$$$d\Phi_v$$dA$$lm$$dA$$m^2$$\text{lm/m}^2$$(M_v)$$(E)$$lx$$1\ \mathr…</description>
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        <description>Luminous Flux

Definition

Luminous flux (symbol:$\Phi_v$ ) is a photometric quantity that measures the light power perceived by the human eye.  It represents the total luminous energy emitted by a light source per unit time, and directly reflects the overall brightness of the source.$$1\ \text{lm} = 1\ \text{cd} \times 1\ \text{sr}$$$lm$$$\Phi_{v}(\lambda)=K_{m}V(\lambda)\Phi_{e}(\lambda)$$$K_{m}$$\Phi_{v}(\lambda)$$V(\lambda)$$\lambda$$\Phi_v$$$ \Phi_v = \int_{(\Omega)} I_v \, d\Omega$$$\Omega…</description>
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        <description>Luminous Intensity

Definition

Luminous intensity (symbol:$I_v$ ) describes the intensity of a light source in a given direction, defined as the luminous flux emitted per unit solid angle. It is an inherent property of the light source, independent of the source area and observation distance.$$ I_v = \frac{\mathrm{d}\Phi_v}{\mathrm{d}\Omega} $$$I_v$$\Phi_v$$\Omega$\(\mathrm{cd}\)\(540\times 10^{12}\ \mathrm{Hz}\)\(K_{\mathrm{cd}}\)\[
K_{\mathrm{cd}} = 683\ \mathrm{lm\,W^{-1}}.
\]\(\Phi_v\)\(I_v…</description>
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        <description>FIXME This page is not fully translated, yet. Please help completing the translation.

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Conversion between Lv, Luminance, and Luminous Exitance

Background: Expressing Film Speed on a Logarithmic Scale$$S_v = \log_2 (N S_x) \tag{1}$$$S_x$$S_v$$S_x$$S_v$$$E_v = A_v + T_v = B_v + S_v \tag{2}$$$A_v$$T_v$$B_v$$S_v$$$2^{E_v} = \frac{A^2}{T} = \frac{B S_x}{K} \tag{3}$$$$B = \frac{2^{E_v} \cdot K}{S_x} \quad (\textrm{fL}) \tag{4}$$$$1 \space\te…</description>
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        <title>en:yanding:imaging_basics:optics:radiometry_photometry:radiance</title>
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        <description>Radiance

Definition

Radiance(symbol: $L$) is the radiant flux emitted, reflected, transmitted, or received by a surface, per unit solid angle per unit projected area in a specified direction.As the fundamental property of extended sources, it characterizes the radiant intensity per unit projected area of a surface element along a given line of sight. \(\mathrm{W \cdot sr^{-1} \cdot m^{-2}}\)$L$$$L = \frac{dI}{dA \cos\theta} = \frac{d^2 \Phi}{dA \cos\theta \, d\Omega}$$$L$$I$$\Phi$$A$$\theta$$\…</description>
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        <description>FIXME This page is not fully translated, yet. Please help completing the translation.

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Radiant Energy

I. Definition

Radiant Energy is the energy carried by electromagnetic radiation during its emission, propagation, or absorption. It is a fundamental energy quantity in radiometry, used to characterize the total energy transferred by radiation, and is denoted by the symbol: $Q_e$$$Q_e = \int_{t_1}^{t_2} \Phi_e(t) dt$$$\Phi_e(t)$$t_1-t_…</description>
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        <description>FIXME This page is not fully translated, yet. Please help completing the translation.

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Radiant Energy Density

I. Definition

Radiant energy density is defined as the electromagnetic radiant energy stored per unit volume of space\(w\)\(u\)\(J/m^3\)\([M L^{-1} T^{-2}]\)$$w = \frac{dQ}{dV}$$\(dQ\)\(dV\)$Q = 8000 J$$V= 23 L= 0.023 {m}^3$$w \approx 347\,826.09 {J/m}^3$\(E\)\(B\)$$w = \frac{1}{2}\left(\varepsilon E^2 + \frac{1}{\mu} B^2\righ…</description>
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Radiant Exitance

Radiant exitance, denoted as $M$, refers to the radiant flux emitted per unit time from a unit area of a surface into the outward hemispherical space, with the unit being $W/m^2$$$M = \frac{d\Phi}{dA}$$$$M = \int_{\Omega} L(\omega) \cos\theta \, d\omega$$$L(\omega)$$\omega$$\theta$$\Omega$$$M = \rho E$$$\rho$$E$$\mathrm{W/m^2}$$$M = …</description>
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        <description>Radiant Flux

I.Definition

Radiant flux ($\Phi_e$), also known as radiant power, is the time rate of change of radiant energy. It represents the total radiant energy emitted, transferred, or received per unit time. The quantity is denoted by $\Phi_e$ or $P$ and is defined as:$$\Phi_\text{e} = \frac{\mathrm{d}Q_\text{e}}{\mathrm{d}t}$$$Q_\text{e}$$t$$\Phi_e$$\Phi_e$$$\Phi_e = K \cdot S$$$S$$K$$$\Phi_e = \int_{\lambda_1}^{\lambda_2} \Phi_{e,\lambda}(\lambda) d\lambda$$$I(\theta,\varphi)$$$  \Phi …</description>
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Radiant Intensity

Definition: The radiant flux emitted by a radiation source in a specific direction per unit solid angle, denoted by the symbol $I$$$I = \frac{d\Phi}{d\Omega}$$$\Omega$$A$$r$$\Omega = \frac{A}{r^2}$$\Phi $$\Omega$$ I = \frac{d\Phi}{d\Omega}$$D$$ I = \frac{d\Phi}{d\Omega}$</description>
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        <dc:date>2026-07-22T09:45:23+00:00</dc:date>
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        <title>en:yanding:imaging_basics:optics:radiometry_photometry:solid_angle</title>
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        <description>Solid Angle

Definition:

In geometry and radiometry, a solid angle is a measure of the amount of the field of view from some particular point that a given object covers.

For an arbitrary surface that subtends a region at a point (the vertex), the solid angle $\Omega$$A$$r$$$\Omega = \frac{A}{r^2}$$$\Omega$$A$$r$$r$$sr$$4\pi$</description>
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