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Willekeurig
In de buurt
Aanmelden
Voorkeuren
Doneren
Over Wikipedia
Disclaimers
Zoeken
Sjabloon
:
Tabel lichtgrootheden
Taal
Volgen
Bewerken
naam en symbool
definitie
eenheid
omrekening
Lichtsterkte
I
v
{\displaystyle I_{\mathrm {v} }}
I
=
∂
Φ
∂
Ω
{\displaystyle I={\frac {\partial \Phi }{\partial \Omega }}}
candela
c
d
{\displaystyle \mathrm {cd} }
1
c
d
=
1
l
m
s
r
{\displaystyle \mathrm {1\ cd=1\ {\frac {lm}{sr}}} }
Lichtstroom
Φ
v
{\displaystyle \Phi _{\mathrm {v} }}
Φ
v
=
K
m
∫
380
n
m
780
n
m
∂
Φ
e
(
λ
)
∂
λ
⋅
V
(
λ
)
d
λ
{\displaystyle \Phi _{\mathrm {v} }=K_{\mathrm {m} }\int _{380\ \mathrm {nm} }^{780\ \mathrm {nm} }{\frac {\partial \Phi _{\mathrm {e} }(\lambda )}{\partial \lambda }}\cdot V(\lambda )\ \mathrm {d} \lambda }
lumen
l
m
{\displaystyle \mathrm {lm} }
1
l
m
=
1
s
r
⋅
c
d
{\displaystyle \mathrm {1\ lm=1\ sr\cdot cd} }
Specifieke lichtstroom
of lichtrendement
η
{\displaystyle \eta }
of
Φ
s
{\displaystyle \Phi _{\mathrm {s} }}
η
=
Φ
P
{\displaystyle \eta ={\frac {\Phi }{P}}}
l
m
/
W
{\displaystyle \mathrm {lm/W} }
Verlichtingssterkte
:
E
{\displaystyle E}
E
=
∂
Φ
∂
A
{\displaystyle E={\frac {\partial \Phi }{\partial A}}}
lux
l
x
{\displaystyle \mathrm {lx} }
1
l
x
=
1
l
m
m
2
=
1
s
r
⋅
c
d
m
2
{\displaystyle \mathrm {1\ lx=1\ {\frac {lm}{m^{2}}}=1\ {\frac {sr\cdot cd}{m^{2}}}} }
Luminantie
L
{\displaystyle L}
L
=
∂
2
Φ
∂
Ω
⋅
∂
A
1
⋅
cos
ε
1
{\displaystyle L={\frac {\partial ^{2}\Phi }{\partial \Omega \cdot \partial A_{1}\cdot \cos \varepsilon _{1}}}}
c
d
m
2
{\displaystyle \mathrm {\frac {cd}{m^{2}}} }
1
c
d
m
2
=
1
l
m
s
r
⋅
m
2
{\displaystyle \mathrm {1\ {\frac {cd}{m^{2}}}} =\mathrm {1\ {\frac {lm}{sr\cdot m^{2}}}} }
Lichtenergie
Q
v
{\displaystyle Q_{\mathrm {v} }}
Q
v
=
∫
0
T
Φ
v
(
t
)
d
t
{\displaystyle Q_{\mathrm {v} }=\int _{0}^{T}\Phi _{\mathrm {v} }(t)\mathrm {d} t}
lumenseconde
l
m
⋅
s
{\displaystyle \mathrm {lm\cdot s} }
Ruimtehoek
Ω
{\displaystyle \Omega }
Ω
=
A
r
2
{\displaystyle \Omega ={\frac {A}{r^{2}}}}
steradiaal
s
r
{\displaystyle \mathrm {sr} }
1
s
r
=
1
m
2
m
2
=
[
o
p
p
e
r
v
l
a
k
]
[
s
t
r
a
a
l
]
2
{\displaystyle \mathrm {1\ sr=1\ {\frac {m^{2}}{m^{2}}}={\frac {\left[oppervlak\right]}{\left[straal\right]^{2}}}} }