Fluence
{{#invoke:Hatnote|hatnote}} Template:Expert-subject In physics, fluence is the flux (either particle or radiative flux) integrated over time. For particles, it is defined as the total number of particles that intersect a unit area in a specific time interval of interest, and has units of m^{–2} (number of particles per meter squared). Fluence can also be used to describe the energy delivered per unit area, in which case it has units of J/m^{2}.
Definition
It has two equivalent definitions:
1. Suppose N particles pass through an area A. The particle fluence for the area A is defined as:
In the limit of infinitesimal area, this is:
2. Imagine an infinitesimal volume dV with particles passing through it. The particle fluence can be defined as
where is the sum of all the path lengths of the particles that traverse the volume. These definitions are equivalent as can be seen by multiplying the first definition by where dx is the typical path length of a particle in the volume. The numerator () then gives the total path length traced out by the dN particles in the volume () while the denominator () gives the volume dV.
Uses
In visible light based medicine and dentistry, fluence, which may be more properly referred to as radiant exposure, is a measurement of energy over area. The area is usually the spot size of the light device.
It is considered one of the fundamental units in dosimetry. The attached diagram shows its relationship to other radiation quantities.
References
- ICRU 33: Radiation Quantities and Units, April, 1980. (www.icru.org)
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Quantity | Unit | Dimension | Notes | |||||
---|---|---|---|---|---|---|---|---|
Name | Symbol^{[nb 1]} | Name | Symbol | Symbol | ||||
Radiant energy | Q_{e}^{[nb 2]} | joule | J | M⋅L^{2}⋅T^{−2} | energy | |||
Radiant flux | Φ_{e}^{[nb 2]} | watt | W or J/s | M⋅L^{2}⋅T^{−3} | radiant energy per unit time, also called radiant power. | |||
Spectral power | Φ_{eλ}^{[nb 2]}^{[nb 3]} | watt per metre | W⋅m^{−1} | M⋅L⋅T^{−3} | radiant power per wavelength. | |||
Radiant intensity | I_{e} | watt per steradian | W⋅sr^{−1} | M⋅L^{2}⋅T^{−3} | power per unit solid angle. | |||
Spectral intensity | I_{eλ}^{[nb 3]} | watt per steradian per metre | W⋅sr^{−1}⋅m^{−1} | M⋅L⋅T^{−3} | radiant intensity per wavelength. | |||
Radiance | L_{e} | watt per steradian per square metre | W⋅sr^{−1}⋅m^{−2} | M⋅T^{−3} | power per unit solid angle per unit projected source area. confusingly called "intensity" in some other fields of study. | |||
Spectral radiance | L_{eλ}^{[nb 3]} or L_{eν}^{[nb 4]} |
watt per steradian per metre^{3} or watt per steradian per square |
W⋅sr^{−1}⋅m^{−3} or W⋅sr^{−1}⋅m^{−2}⋅Hz^{−1} |
M⋅L^{−1}⋅T^{−3} or M⋅T^{−2} |
commonly measured in W⋅sr^{−1}⋅m^{−2}⋅nm^{−1} with surface area and either wavelength or frequency. | |||
Irradiance | E_{e}^{[nb 2]} | watt per square metre | W⋅m^{−2} | M⋅T^{−3} | power incident on a surface, also called radiant flux density. sometimes confusingly called "intensity" as well. | |||
Spectral irradiance | E_{eλ}^{[nb 3]} or E_{eν}^{[nb 4]} |
watt per metre^{3} or watt per square metre per hertz |
W⋅m^{−3} or W⋅m^{−2}⋅Hz^{−1} |
M⋅L^{−1}⋅T^{−3} or M⋅T^{−2} |
commonly measured in W⋅m^{−2}⋅nm^{−1} or 10^{−22} W⋅m^{−2}⋅Hz^{−1}, known as solar flux unit.^{[nb 5]} | |||
Radiant exitance / Radiant emittance |
M_{e}^{[nb 2]} | watt per square metre | W⋅m^{−2} | M⋅T^{−3} | power emitted from a surface. | |||
Spectral radiant exitance / Spectral radiant emittance |
M_{eλ}^{[nb 3]} or M_{eν}^{[nb 4]} |
watt per metre^{3} or watt per square |
W⋅m^{−3} or W⋅m^{−2}⋅Hz^{−1} |
M⋅L^{−1}⋅T^{−3} or M⋅T^{−2} |
power emitted from a surface per unit wavelength or frequency. | |||
Radiosity | J_{e} | watt per square metre | W⋅m^{−2} | M⋅T^{−3} | emitted plus reflected power leaving a surface. | |||
Spectral radiosity | J_{eλ}^{[nb 3]} | watt per metre^{3} | W⋅m^{−3} | M⋅L^{−1}⋅T^{−3} | emitted plus reflected power leaving a surface per unit wavelength | |||
Radiant exposure | H_{e} | joule per square metre | J⋅m^{−2} | M⋅T^{−2} | also referred to as fluence | |||
Radiant energy density | ω_{e} | joule per metre^{3} | J⋅m^{−3} | M⋅L^{−1}⋅T^{−2} | ||||
See also: SITemplate:· RadiometryTemplate:· Photometry |
- ↑ Standards organizations recommend that radiometric quantities should be denoted with a suffix "e" (for "energetic") to avoid confusion with photometric or photon quantities.
- ↑ ^{2.0} ^{2.1} ^{2.2} ^{2.3} ^{2.4} Alternative symbols sometimes seen: W or E for radiant energy, P or F for radiant flux, I for irradiance, W for radiant emittance.
- ↑ ^{3.0} ^{3.1} ^{3.2} ^{3.3} ^{3.4} ^{3.5} Spectral quantities given per unit wavelength are denoted with suffix "λ" (Greek) to indicate a spectral concentration. Spectral functions of wavelength are indicated by "(λ)" in parentheses instead, for example in spectral transmittance, reflectance and responsivity.
- ↑ ^{4.0} ^{4.1} ^{4.2} Spectral quantities given per unit frequency are denoted with suffix "ν" (Greek)—not to be confused with the suffix "v" (for "visual") indicating a photometric quantity.
- ↑ NOAA / Space Weather Prediction Center includes a definition of the solar flux unit (SFU).