What is the standard unit for luminous intensity?
Candela
Luminous intensity is a fundamental concept in photometry, the science of measuring light as perceived by the human eye. It describes the power emitted by a light source in a particular direction, based on the sensitivity of the human eye to different wavelengths of light.
The question asks for the standard unit used to measure luminous intensity. Let's examine the given options to identify the correct unit.
Based on the standard definitions of SI units, the candela is the unit specifically defined for luminous intensity.
| Unit | Quantity Measured | Relevance to Question |
|---|---|---|
| Tesla ($\text{T}$) | Magnetic Flux Density | Incorrect |
| Candela ($\text{cd}$) | Luminous Intensity | Correct |
| Steradian ($\text{sr}$) | Solid Angle | Incorrect (part of related definition) |
| Radian ($\text{rad}$) | Plane Angle | Incorrect |
Therefore, the standard unit for luminous intensity is the candela.
| Quantity | Symbol | SI Unit | SI Unit Symbol | Description |
|---|---|---|---|---|
| Luminous intensity | $I_v$ | Candela | cd | Luminous power per unit solid angle in a given direction. |
| Luminous flux | $\Phi_v$ | Lumen | lm | Total perceived power of light emitted by a source. ($1 \text{ lm} = 1 \text{ cd} \cdot \text{sr}$) |
| Luminance | $L_v$ | Candela per square meter | $\text{cd}/\text{m}^2$ | Luminous intensity per unit area of light traveling in a given direction. |
| Illuminance | $E_v$ | Lux | lx | Total luminous flux incident on a surface per unit area. ($1 \text{ lx} = 1 \text{ lm}/\text{m}^2$) |
The definition of the candela is based on a specific physical constant. The 26th General Conference on Weights and Measures (CGPM) in 2018 redefined the SI base units, including the candela. The candela is now defined by fixing the luminous efficacy of monochromatic radiation of frequency $540 \times 10^{12}$ Hz to be exactly 683 lumens per watt.
This definition means that one candela is the luminous intensity, in a given direction, of a source that emits monochromatic radiation of frequency $540 \times 10^{12}$ Hz and that has a radiant intensity in that direction of $(1/683)$ watt per steradian.
The frequency $540 \times 10^{12}$ Hz corresponds to a wavelength of about 555 nanometers, which is close to the peak sensitivity of the average human eye under bright conditions (photopic vision).
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