Metrology

Table of Contents

There is no unit in mathematics in the first place. By assigning units to quantities, you are endowing the quantity a physical significance. Therefore the physicality has to be taken into account thereon.

1. Commensurable

  • Two units are commensurable if they can added together.

2. Conversion Factor

  • A dimensionless number 1 that is a ratio of two measures.
    • e.g. \(1=100\, \mathrm{cm}/1\,\mathrm{m}\)
  • For incommensurable units, it depends on the context.
    • e.g. \(1=100\, \mathrm{km}/3\,\mathrm{h}\iff 100 \mathrm{km}=3\,\mathrm{h}\)
  • Degree, the unit of angle, can be thought of as a conversion factor.
    • \[^{\circ} =\frac{\pi}{180}\]

3. Common Units

3.1. SI Units

  • International System of Quantities (ISQ)

3.1.1. SI Base Units

Quantity Quantity Symbol Dimension SI Base Unit
Length \(l\) \(\sf L\) \(\rm m\)
Mass \(m\) \(\sf M\) \(\rm kg\)
Time \(t\) \(\sf T\) \(\rm s\)
Electric Current \(I\) \(\sf I\) \(\rm A\)
Thermodynamic Temperature \(T\) \(\sf \Theta\) \(\rm K\)
Amount of Substance \(n\) \(\sf N\) \(\rm mol\)
Luminous Intensity \(I_\mathrm{v}\) \(\sf J\) \(\rm cd\)

3.1.2. SI Derived Units

Name Symbol
radian \(\rm rad\)
steradian \(\rm sr\)
hertz \(\rm Hz\)
newton \(\rm N\)
pascal \(\rm Pa\)
joule \(\rm J\)
watt \(\rm W\)
coulomb \(\rm C\)
volt \(\rm V\)
farad \(\rm F\)
ohm \(\Omega\)
siemens \(\rm S\)
weber \(\rm Wb\)
tesla \(\rm T\)
henry \(\rm H\)
degree Celsius \(\rm ^\circ C\)
lumen \(\rm lm\)
lux \(\rm lx\)
becquerel \(\rm Bq\)
gray \(\rm Gy\)
sievert \(\rm Sv\)
katal \(\rm kat\)
  Unit
Electric Field \(\rm V/m\)
Permittivity \(\rm F/m\)

3.1.3. Prefixes

Name Symbol Base 10 Factor
quetta \(\rm Q\) \(10^{30}\)
ronna \(\rm R\) \(10^{27}\)
yotta \(\rm Y\) \(10^{24}\)
zetta \(\rm Z\) \(10^{21}\)
exa \(\rm E\) \(10^{18}\)
peta \(\rm P\) \(10^{15}\)
tera \(\rm T\) \(10^{12}\)
giga \(\rm G\) \(10^{9}\)
mega \(\rm M\) \(10^{6}\)
kilo \(\rm k\) \(10^3\)
hecto \(\rm h\) \(10^2\)
deca \(\rm da\) \(10^1\)
\(\text{--}\) \(\text{--}\) \(1\)
deci \(\rm d\) \(10^{-1}\)
centi \(\rm c\) \(10^{-2}\)
milli \(\rm m\) \(10^{-3}\)
micro μ \(10^{-6}\)
nano \(\rm n\) \(10^{-9}\)
pico \(\rm p\) \(10^{-12}\)
femto \(\rm f\) \(10^{-15}\)
atto \(\rm a\) \(10^{-18}\)
zepto \(\rm z\) \(10^{-21}\)
yocto \(\rm y\) \(10^{-24}\)
ronto \(\rm r\) \(10^{-27}\)
quecto \(\rm q\) \(10^{-30}\)

3.2. Avoirdupois

USimperial.png

3.2.1. Length

Yard

  • 0.9144 m
  • 3 feet

Mile

  • 1760 yards.
  • It originated from the different unit system, the Roman one.

3.2.2. Weight

Pound

  • 0.454 kg

Ounce

  • oz, oz.
  • Alchemical symbol for an ounce ℥, and half an ounce 🝳.
  • 28.34 g

3.2.3. Volume

Fluid Ounce

  • fl oz, fl. oz.
  • US Customary: 29.57 mL
  • US Food Labelling: 30 mL

Gill

  • 4 US fluid ounces
  • 5 imperial fluid ounces

Pint

  • 4 gills

Quart

  • quarter gallon
  • 2 pints

Gallon

  • gal
  • US Gallon: 231 in³ (≈ 3.785 L)
  • 4 quarts

3.2.4. Point

  • The definition may vary.
3.2.4.1. DTP
  • desktop publishing point
  • 1/72 of an inch, 1/12 of a pica.
  • 0.3528 mm.
3.2.4.2. New Didot Point
  • nd
  • 3/8 mm, or 0.375 mm.
3.2.4.3. American Point

3.2.5. Horsepower

  • Watt determined that a horse could turn a mill wheel 144 times in an hour, or 2.4 times in a minute. The wheel was 12 feet (3.7 m) in radius, and Watt judged that the horse could pull with a force of 180 pounds-force (800 N).
  • \[ 1\,\mathrm{hp} = 180\,\mathrm{lbf}\cdot 2.4\,\mathrm{turn/min}\cdot (2\pi\cdot 12)\,\mathrm{ft/turn} = 32,572\,\mathrm{ft\,lbf/min} \]
3.2.5.1. Imperial Horsepower
  • \(1\,\mathrm{hp} = 745.7\,\mathrm{W}\)
3.2.5.2. Metric Horsepower
  • 735.5 W

3.3. Level

3.3.1. Decibel

  • dB (base quantity) is the unit of the level.

\[ L = 10 \log \frac{Q}{Q_0}\ \mathrm{dB} \]

  • A reference unit can be provided so that the quantity have a unit.
3.3.1.1. dBm
  • decibel-milliwatts
3.3.1.2. Root-Power Quantity
  • Often used for voltage.
  • 20 is used.

3.3.2. Neper

  • Np
  • natural logarithm is used.

3.4. Information

3.4.1. Shannon

  • Log 2 of probability

3.4.2. Nat

  • Natural log of probability

4. Centimeter-Gram-Second System of Units

  • CGS Units, CGS, cgs
Quantity Quantity Symbol Unit Name Unit Symbol Description
Acceleration \(a\) gal(galileo) \(\rm Gal\)  
Force \(F\) dyne \(\rm dyn\) From Greek, δύναμις, "power"
Energy \(E\) erg \(\rm erg\) From Greek, ἔργον, "work"
Pressure \(p\) barye \(\rm Ba\)  
Dynamic Viscosity \(\mu\) poise \(\rm P\) \(\rm cP\) is more common
Kinematic Viscosity \(\nu\) stokes \(\rm St\)  
Wavenumber \(k\) kayser \(\rm K\)  

For electromagnetic CGS units, we do not invent new units but simply measure it indirectly in conventional units.

4.1. Electrostatic Units

  • ESU, CGS-ESU

4.1.1. Statcoulomb

  • \(\rm statC\), \(\rm Fr\)
  • , esu charge

Electrostatic units first define the unit of charge, and derive other units from it.

It is defined by the Coulomb's law: \[ \mathbf{F} = \frac{q_1^\mathsf{ESU}q_2^\mathsf{ESU}}{r^2} \vu{r}. \] The unit of charge is called statcoulomb, and it is the amount of charge that exert one dyne of force when one centimeter apart from the same charge: \[ \rm statC = \sqrt{dyn \cdot cm^2} = cm^{3/2}\cdot g^{1/2}\cdot s^{-1} \] The point is to express charge entirely from mass, length, and time.

Statcoulomb is related to the SI unit coulomb by 1 C ≘ 10⁻¹ c statC, and the dimensions are related by: \[ q^\mathsf{ESU} = \frac{q^\mathsf{I}}{\sqrt{4\pi\varepsilon_0}} \]

Statcoulomb is related to the electromagnetic unit abcoulomb by c statC ≘ 1 abC, and the dimensions are also related by: \[ q^{\mathsf{ESU}} = c q^{\mathsf{EMU}}. \]

The factor of \(c\) between these units stayed mystery until the unification of electricity and magnetism.

4.1.2. Statampere

\[ \rm statA := \frac{statC}{s} = cm^{3/2}\cdot g^{1/2} \cdot s^{-2} = \sqrt{dyn} \cdot cm \cdot s^{-1} \]

4.1.3. Statvolt

\[ \rm statV := \frac{erg}{statC} = \frac{cm^2\cdot g\cdot s^{-2}}{cm^{3/2}\cdot g^{1/2}\cdot s^{-1}} = cm^{1/2}\cdot g^{1/2}\cdot s^{-1} = \sqrt{dyn} \]

4.1.4. Statvolt per Centimeter

\[ \rm statV \cdot cm^{-1} = \sqrt{dyn} \cdot cm^{-1} \]

The unit of electric filed is defined by the definition of electric field: \[ \mathbf{E}^\mathsf{ESU} = \frac{q^\mathsf{ESU}}{r^2}\mathbf{\hat{r}} = \frac{\mathbf{F}}{q^\mathsf{ESU}}. \]

The relation to the SI system is: \[ \mathbf{E}^\mathsf{ESU} = \sqrt{4\pi\varepsilon_0}\,\mathbf{E}^\mathsf{SI} \]

4.1.5. Statohm

\[ \rm stat \text{\Omega} := \frac{statV}{statA} = cm^{-1}\cdot s \]

4.1.6. Stattesla

  • \(\rm statT\)

It is defined by the Lorentz force: \[ \mathbf{F} = q^{\sf ESU}\mathbf{v}\times \mathbf{B}^{\sf ESU}. \]

\[ \rm statT := \frac{dyn\cdot s}{statC\cdot cm} = cm^{-3/2}\cdot g^{1/2} = \sqrt{dyn} \cdot s \cdot cm^{-2} \]

Stattesla is related to the SI unit tesla by 1T ≘ 10⁻⁴ c⁻¹ statT, and the dimensions are related by: \[ \mathbf{B}^{\sf ESU} = \sqrt{4\pi\varepsilon_0}\,\mathbf{B}^{\sf SI} = \sqrt{\frac{4\pi}{\mu_0}}\frac{\mathbf{B}^{\mathsf{SI}}}{c}. \]

It does not include the factor of \(c\), compared to Gauss.

4.1.7. Statweber

  • The unit of magnetic flux

\[ \rm statWb := statT \cdot cm^2 \]

4.2. Electromagnetic Units

  • EMU, CGS-EMU

4.2.1. Abampere

  • \(\rm abA\), \(\rm Bi\)
  • Biot, emu current

Electromagnetic units first define the unit of current, and derive other units from it.

It is defined by the force per centimeter \(f\) between two parallel wires of infinite length: \[ \frac{f}{2} =\frac{I_1^{\sf EMU}I_2^{\sf EMU}}{r}. \] The unit of current is called abampere, and it is the amount of current that exert two dyne per centimeter of force for two wires with same current are one centimeter apart from each other.

The factor of two is to cancel the two that arises for the magnetic field when applying the Biot-Savart law \[ \mathbf{B}^{\sf EMU} = \frac{I^{\sf EMU}\dd{\mathbf{l}}\times \mathbf{\hat{r}}}{r^2} \] for infinitely long wires, and applying the Lorentz force \[ \mathbf{F} = I^{\mathsf{EMU}} \dd{\mathbf{l}} \times \mathbf{B}^{\mathsf{EMU}}. \]

When represented with basis units: \[ \rm abA = \sqrt{dyn} = g^{1/2}\cdot cm^{1/2}\cdot s^{-1}. \]

Abampere is related to the SI unit ampere by 1 A ≘ 10⁻¹ abA and the dimensions are related by: \[ I^{\sf EMU} = \frac{I^{\sf SI}}{\sqrt{4\pi / \mu_0}} = \frac{I^{\sf SI}}{c\sqrt{4\pi\varepsilon_0}}. \]

4.2.2. Abcoulomb

\[ \rm abC := abA \cdot s = g^{1/2}\cdot cm^{1/2} = \sqrt{dyn} \cdot s \]

4.2.3. Gauss

  • Abtesla

Gauss is defined to be consistent with Biot-Savart law and Lorentz force, as explained above in abampere. \[ \rm G = \frac{dyn}{abA \cdot cm} = \frac{abA \cdot cm}{cm^2} = cm^{-1/2}\cdot g^{1/2}\cdot s^{-1} = \sqrt{dyn}\cdot cm^{-1} \]

The relation to the SI unit tesla is: 1 T ≘ 10⁴ G and the dimensions are related by: \[ \mathbf{B}^{\sf EMU} = c\sqrt{4\pi\varepsilon_0}\,\mathbf{B}^{\sf SI} = \sqrt{4\pi/\mu_0}\mathbf{B}^{\mathsf{SI}}. \]

It is related to the electrostatic unit stattesla by: 1 statT ≘ c G while the dimensions are related by: \[ c\mathbf{B}^{\mathsf{ESU}} = \mathbf{B}^{\mathsf{EMU}}. \]

The conversion factor \(10^4\) from gauss to tesla is particularly nice due to the value of permeability of the vacuum. \[ \frac{B^{\mathsf{EMU}}}{B^\mathsf{SI}} = \sqrt{\frac{4\pi}{\mu_0}} \approx \sqrt{\frac{4\pi}{4\pi\times 10^{-7}\ \mathrm{N/A^2}}} = 10^{\frac{7}{2}}\rm\ N^{-1/2}A = \frac{10^4\ G}{1\ T} \]

The digits of permeability of vacuum being so close to \(4\pi\) is in fact not a coincidence. Because the early definition (until 2019) of the unit of magnetic field was:

  • 1/(2⋅10⁻⁷) times
  • the magnetic field strength produced at one of the two identical infinitely long wire
  • with identical electric current flowing
  • separated by one meter
  • and exert force of 2⋅10⁻⁷ neuton per meter to each other (definition of 1 ampere).

Just like the defintiion of Gauss.

In order to cancel the inclusion of \(4\pi\) in the denominator of Biot-Savart law, \(4\pi\) is included in \(\mu_0\), and in order to reduce the effect of infinite wire to a infinitesimal segment, the force is halved, giving us the final formula for the familiar Biot-Savar law: \[ \mathbf{B} = \frac{\mu_0}{4\pi} \frac{I \dd{\mathbf{l}}\times \vu{\mathbf{r}}}{r^2} \] and the value of permeability of vacuum: \[ \mu_0 = 4\pi \times 10^{-7}\,\rm T\cdot m/A. \]

After 2019, ampere has been decoupled from the unit of force, and how much force it generates is now a matter of measurement.

4.2.4. Oersted

The unit of auxiliary magnetic field \(\mathbf{H}\) \[ \rm Oe := abA \cdot cm^{-1} \]

4.2.5. Maxwell

The unit of magnetic flux \(\Phi\) \[ \rm Mx := G \cdot cm^2 \]

4.3. Gaussian Units

  • CGS-Gaussian
  • Gaussian Unit System, Gaussian-CGS Units, CGS Units

Gaussian unit system follows ESU for electricity and EMU for magnetism. It choose Gauss for its unit of magnetic field, hence the name.

Quantity ESU EMU
Electric Charge Franklin  
Electric Current statA  
Electric Potential statV  
Electric Field statV/cm  
Electric Displacement Filed statC/cm²  
Electric Dipole Moment statC⋅cm  
Permittivity 4π⋅10¹¹⋅(c⋅s/cm)²  
Resistance statΩ  
Magnetic B Field   Gauss
Magnetic H Field   Oersted
Magnetic Dipole Moment   erg/G
Magnetic Flux   Maxwell
Permeability   10⁷/4π

Since two systems do not agree in its dimension, the equations related to electromagnetism are adjusted accordingly. Due to the fact that electric field and magnetic field having same dimension, the equations tends to simplify: Lorentz Force \[ \mathbf{F} = q^\mathrm{\mathsf{G}}\left(\mathbf{E}^\mathrm{\mathsf{G}} + \frac{1}{c}\mathbf{v}\times \mathbf{B}^\mathrm{\mathsf{G}}\right) \]

Maxwell's Equations \[ \nabla\cdot \mathbf{E}^\mathsf{G} = 4\pi \rho^\mathsf{G} \] \[ \nabla \cdot \mathbf{B}^\mathsf{G} = 0 \] \[ \nabla\times \mathbf{E}^\mathsf{G} + \frac{1}{c} \frac{\partial \mathbf{B}^\mathsf{G}}{\partial t} = 0 \] \[ \nabla\times \mathbf{B}^\mathsf{G} - \frac{1}{c}\frac{\partial \mathbf{E}^\mathsf{G}}{\partial t} = \frac{4\pi}{c}\mathbf{J}^\mathsf{G} \]

5. Radiometry and Photometry

Radiometry deals with raw electromagnetic radiation while photometry deals with how they are perceived. Radiometry uses subscript \(\rm e\) for "energetic" and photometry uses subscript \(\rm v\) to avoid confusion.

5.1. Radiant Flux

  • Radiant Power, Luminosity (in astronomy)
  • \(\rm W\)
  • Radiant energy emitted, reflected, transmitted, or received per unit time.

\[ \Phi_{\rm e} := \dv{Q_{\rm e}}{t} \] where \(Q_{\rm e}\) is the radiant energy passing a closed surface \(\Sigma\) in time interval \(T\): \[ Q_{\rm e} := \int_T\in_{\Sigma} \mathbf{S} \vdot \vu{n} \dd{A}\dd{t}. \]

Radiant flux can be either the average flux or the instantaneous flux.

5.2. Radiant Intensity

  • \(\rm W/sr\)
  • Radiant flux emitted, reflected, transmitted, or received per unit solid angle.

\[ I_{\rm e, \Omega} := \pdv{\Phi_{\rm e}}{\Omega} \]

5.2.1. Spectral Intensity

Spectral intensity in frequency \[ I_{\rm e, \Omega, \nu} := \pdv{I_{\rm e, \Omega}}{\nu} \]

Spectral intensity in frequency \[ I_{\rm e, \Omega, \lambda} := \pdv{I_{\rm e, \omega}}{\lambda} \]

5.3. Irradiance

  • \(\rm W/m^2\)
  • Radiant flux received by a surface per unit area.

\[ E_{\rm e} := \pdv{\Phi_{\rm e}}{A} \]

5.3.1. Spectral Irradiance

Spectral irradiance in frequency \[ E_{\rm e, \nu} := \pdv{E_{\rm e}}{\nu} \]

Spectral irradiance in wavelength \[ E_{\rm e, \lambda} := \pdv{E_{\rm e}}{\lambda} \]

5.4. Radiant Exposure

  • Fluence

Radiant energy received by a surface per unit area.

\[ H_{\rm e} := \pdv{Q_{\rm e}}{A} = \int_0^T E_{\rm e}(t)\dd{t} \] where \(T\) is the duration of irradiation.

5.4.1. Spectral Irradiance

Spectral exposure in frequency \[ H_{\rm e, \nu} := \pdv{H_{\rm e}}{\nu} \]

Spectral irradiance in wavelength \[ H_{\rm e, \lambda} := \pdv{H_{\rm e}}{\lambda} \]

5.5. Radiant Exitance

  • Radiant Emittance
  • \(\rm W/m^2\)
  • Radiant flux emitted by a surface per unit area.

\[ M_{\rm e} := \pdv{\Phi_{\rm e}}{A} \]

5.5.1. Spectral Exitance

Spectral exitance in frequency \[ M_{\rm e, \nu} := \pdv{M_{\rm e}}{\nu} \]

Spectral exitance in wavelength \[ M_{\rm e, \lambda} := \pdv{M_{\rm e}}{\lambda} \]

5.6. Radiosity

  • Radiant flux leaving (emitted, reflected, and transmitted by) a surface per unit area.

\[ J_{\rm e} := \pdv{\Phi_{\rm e}}{A} = J_{\rm e, em} + J_{\rm e, r} + J_{\rm e, tr} \] where \(J_{\rm e,em} = M_{\rm e}\) is the radiant exitance, \(J_{\rm e,r}\) is the reflected component, and \(J_{\rm e, tr}\) is the transmitted component.

5.6.1. Spectral Radiosity

Spectral radiosity in frequency \[ J_{\rm e, \nu} := \pdv{J_{\rm e}}{\nu} \]

Spectral radiosity in wavelength \[ J_{\rm e, \lambda} := \pdv{J_{\rm e}}{\lambda} \]

5.7. Radiance

  • Historically, "intensity" in heat transfer, astrophysics and astronomy

Radiant flux emitted, reflected, transmitted or received by a given surface, per unit solid angle per unit projected area.

\[ L_{\rm e, \Omega} := \frac{\partial^2\Phi_{\rm e}}{\partial\Omega\partial (A\cos\theta)} \] where \(\Omega\) is the solid angle, \(A\cos\theta\) is the projected area.

5.7.1. Spectral Radiance

Spectral radiance in frequency \[ L_{\rm e, \Omega,\nu} := \pdv{L_{\rm e, \Omega}}{\nu} \]

Spectral radiance in wavelength \[ L_{\rm e, \Omega, \lambda} := \pdv{L_{\rm e, \Omega}}{\lambda} \]

5.8. Luminous Efficacy

  • \(\rm lm/W\)
  • The efficiency of producing visible light.

Ratio of luminous flux to power. The power can be either the radiant flux of the source's output, or the total power (electric, chemical, or others) consumed by the source. The former sense is sometimes called the luminous efficacy of radiation \(K\), and the latter luminous efficacy of a light source \(\eta\) or overall luminous efficacy.

\[ K = \frac{\Phi_{\rm v}}{\Phi_{\rm e}} = \frac{\int_0^{\infty} K(\lambda) \Phi_{\rm e, \lambda}\dd{\lambda}}{\Phi_{\rm e, \lambda}\dd{\lambda}} \] where \(K(\lambda) = K_{\rm m} \bar{y}(\lambda)\) is the spectral luminous efficacy, consisting of maximum spectral luminous efficacy \(K_{\rm m} = 683.002\, \mathrm{lm/W}\) and luminous efficiency function defined by CIE.

5.9. Luminous Flux

  • Luminous Power

Perceived power of light

lumen \(\rm lm\) Luminous flux of light produced by a light source that emits one candela of luminous intensity over a solid angle of one steradian.

\[ 1\, \mathrm{lm} = 1\, \mathrm{cd} \cdot 1 \, \mathrm{sr}. \]

It is wavelength-weighted power by the luminous efficiency function \(\bar{y}(\lambda)\) (sometimes \(V(\lambda)\)): \[ \Phi_{\rm v} = (683.002\, \mathrm{lm/W}) \int_0^{\infty} \bar{y}(\lambda) \Phi_{\rm e, \lambda} (\lambda) \dd{\lambda} \] where \(\Phi_{\rm e, \lambda}\) is the spectral radiant flux.

5.10. Luminous Intensity

Perceived power of light per solid angle.

candela \(\rm cd\) SI Base Units

5.11. Illuminance

Total luminous flux incident on a surface per unit area.

lux \(\rm lx\)

5.12. Luminous Exposure

  • \(\rm lx\cdot s\)

\[ H_{\rm v} := \int_0^T E_{\rm v}(t)\dd{t} \]

5.13. Luminous Exitance

  • Luminous Emittance

Luminous flux emitted from a surface per unit area

5.14. Luminance

Luminous intensity per unit area.

\[ L_{\rm v} = \frac{\dd[2]\Phi_{\rm v}}{\dd{\Sigma}\dd{\Omega_{\Sigma}}\cos\theta_{\Sigma}} \] where \(\dd[2]{\Phi_{\rm v}}\) is the luminous flux leaving the area \(\dd{\Sigma}\) in any direction contained inside the solid angle \(\dd{\Omega}_{\Sigma}\), \(\dd{\Sigma}\) is an infinitesimal area of the source, \(\dd{\Omega_{\Sigma}}\) is an infinitesimal solid angle containing the specified direction, \(\theta_{\Sigma}\) is the angle between the normal \(\vu{n}_{\Sigma}\) to the surface \(\dd{\Sigma}\) and the specified direction.

In a lossless medium, the luminance does not change along a given light ray. For an arbitrary surface \(S\) being illuminated, the luminance is given by: \[ L_{\rm v} = \frac{\dd[2]\Phi_{\rm v}}{\dd{S}\dd{\Omega_{S}}\cos\theta_{S}} \] where \(\dd{S}\) is the infinitesimal area of \(S\) seem from the source inside the solid angle \(\dd{\Omega_{\Sigma}}\), \(\dd{\Omega_S}\) is the infinitesimal solid angle subteded by \(\dd{\Sigma}\) as seen from \(\dd{S}\), \(\theta_S\) is the angle between the normal \(\vu{n}_S\) to \(\dd{S}\) and the direction of the light.

More generally, the luminance along a light ray is defined as: \[ L_{\rm v} = n^2 \dv{\Phi_{\rm v}}{G} \] where \(\dd{G}\) is the etendue of an infinitesimally narrow beam containing the specified ray, \( \dd{\Phi_{\rm v}} \) is the luminous flux carried by this beam, and \(n\) is the index of refraction of the medium.

nit

  • \(\rm nt\), \(\rm cd/m^2\)
  • The name probably come from Latin nitēre "to shine".

stilb

  • \(\rm sb\), \(\rm cd/cm^2\)
  • CGS unit

lambert

  • \(1/\pi\) candela per square centimeter

apostilb, bril, skot are obsolete units

6. Dosimetry

6.1. Activity

Number of radioactive transformations per second on average.

Becquerel \(\rm Bq\) One decay per second.

Curie \(\rm Ci\) Originally the quantity or mass of radium emanation in equilibrium with one gram of radium, but now redefined as \[ 1\, \rm Ci = 3.7\times 10^{10}\, \text{decay/s}. \]

Rutherford \(\rm Rd\)

6.2. Radiation Exposure

  • \(\rm C/kg\)

Ionization of air due to ionizing radiation from photons, measured in electric charge freed by such radiation within a region of air divided by the mass of that air.

6.3. Absorbed Dose

  • \(\rm Gy = J/kg\)

Energy per unit mass (specific energy) deposited by ionizing radiation.

6.4. Equivalent Dose

  • \(\rm Sv\)

\[ H_T := \sum_R W_R D_{T,R} \] where \(W_R\) is the radiation weighting factor defined by regulation, \(D_{T,R}\) is the absorbed dose in tissue \(T\) by radiation type \(R\),

6.5. Effective Dose

  • \(\rm Sv\)
\begin{align*} E := \sum_T W_T\cdot H_T \\ &= \sum_T W_T \sum_R W_R \cdot \bar{D}_{T,R} \\ &= \sum_T W_T\sum_R W_R \cdot \frac{\displaystyle \int_T D_R(\mathbf{x}) \rho(\mathbf{x}) \dd{V}}{\displaystyle \int_T \rho(\mathbf{x}) \dd{V}}. \end{align*}

where \(E\) is the effective dose to the entire organism, \(H_T\) is the equivalent dose absorbed by tissue \(T\), \(W_T\) is the tissue weighting factor defined by regulation, \(W_R\) is the radiation weighting factor defined by regulation, \(\bar{D}_{T,R}\) is the mass-averaged absorbed dose in tissue \(T\) by radiation type \(R\), \(D_R(\mathbf{x})\) is the absorbed dose from radiation type \(R\) as a function of location, \(\rho(\mathbf{x})\) is the density as a function of location, \(V\) is volume, and \(T\) is the tissue or organ of interest.

6.6. Dose Equivalent

  • Operational Quantity

7. Natural Units

7.1. Planck Units

7.1.1. Quantities

  • Every quantities are scaled by the factor of plank quantities, yielding dimensionless quantities that corresponds to the normal quantities.
Name Expression
Plank length \(l_\text{P} = \sqrt{\dfrac{\hbar G}{c^3}}\)
Plank mass \(m_\text{P} = \sqrt{\dfrac{\hbar c}{G}}\)
Plank time \(t_\text{P} = \sqrt{\dfrac{\hbar G}{c^5}}\)
Plank temperature \(T_\text{P} = \sqrt{\dfrac{\hbar c^5}{Gk_\text{B}^2}}\)
Plank charge \(q_\text{P} = \sqrt{4\pi\varepsilon_0\hbar c}\ (k_\text{B} = 1)\quad\text{or}\quad \sqrt{\varepsilon_0\hbar c}\ (\varepsilon_0 = 1)\)

7.1.2. Units

  • The units can be thought of as the ratio to the Plank quantities.
    • e.g.
      • \[ [\text{length}] = \frac{\rm m}{l_\text{P}} \]

7.1.3. Implications

  • The effect is equivalent to setting \(c = G = \hbar = k_\text{B} = 1\)
  • \[ F = \frac{m_1m_2}{r^2} \]

7.2. Heaviside-Lorentz Units

7.2.1. Quantities

  • Only the \(\varepsilon_0\) is removed compared to the Gaussian units.
  • \[ q^{\sf HL} := \frac{q^{\sf SI}}{\sqrt{\varepsilon_0}} \]
  • \[ \mathbf{E}^{\sf HL} := \sqrt{\varepsilon_0}\,\mathbf{E}^{\sf SI} \]
  • \[ \mathbf{B}^{\sf HL} := c\sqrt{\varepsilon_0}\,\mathbf{B}^{\sf SI} = \frac{1}{\sqrt{\mu_0}}\mathbf{B}^{\sf SI} \]

7.3. Atomic Units

7.3.1. Quantities

  • Similar to Planck units, but set \(\hbar = e = m_\text{e} = 4\pi\varepsilon_0 = 1\).

8. Obscure Units

8.1. Airwatt

\( \rm AW, airW \)

The product of suction pressure (in Pascal) and air flow rate (in cubic meter per second): \[ P = p\cdot Q. \]

9. See Also

10. Reference

Footnotes:

Author: Jeemin Kim

Created: 2026-09-14 Mon 06:07