This is a list of some of the most commonly used coordinate transformations.
2-dimensional
Let
(
x
,
y
)
{\displaystyle (x,y)}
Cartesian coordinates , and
(
r
,
θ
)
{\displaystyle (r,\theta )}
polar coordinates .
To Cartesian coordinates
From polar coordinates
x
=
r
cos
θ
y
=
r
sin
θ
∂
(
x
,
y
)
∂
(
r
,
θ
)
=
[
cos
θ
−
r
sin
θ
sin
θ
−
r
cos
θ
]
Jacobian
=
det
∂
(
x
,
y
)
∂
(
r
,
θ
)
=
r
{\displaystyle {\begin{aligned}x&=r\cos \theta \\y&=r\sin \theta \\[5pt]{\frac {\partial (x,y)}{\partial (r,\theta )}}&={\begin{bmatrix}\cos \theta &-r\sin \theta \\\sin \theta &{\phantom {-}}r\cos \theta \end{bmatrix}}\\[5pt]{\text{Jacobian}}=\det {\frac {\partial (x,y)}{\partial (r,\theta )}}&=r\end{aligned}}}
From log-polar coordinates
x
=
e
ρ
cos
θ
,
y
=
e
ρ
sin
θ
.
{\displaystyle {\begin{aligned}x&=e^{\rho }\cos \theta ,\\y&=e^{\rho }\sin \theta .\end{aligned}}}
By using complex numbers
(
x
,
y
)
=
x
+
i
y
′
{\displaystyle (x,y)=x+iy'}
x
+
i
y
=
e
ρ
+
i
θ
{\displaystyle x+iy=e^{\rho +i\theta }}
That is, it is given by the complex exponential function.
From bipolar coordinates
x
=
a
sinh
τ
cosh
τ
−
cos
σ
y
=
a
sin
σ
cosh
τ
−
cos
σ
{\displaystyle {\begin{aligned}x&=a{\frac {\sinh \tau }{\cosh \tau -\cos \sigma }}\\y&=a{\frac {\sin \sigma }{\cosh \tau -\cos \sigma }}\end{aligned}}}
From 2-center bipolar coordinates
x
=
1
4
c
(
r
1
2
−
r
2
2
)
y
=
±
1
4
c
16
c
2
r
1
2
−
(
r
1
2
−
r
2
2
+
4
c
2
)
2
{\displaystyle {\begin{aligned}x&={\frac {1}{4c}}\left(r_{1}^{2}-r_{2}^{2}\right)\\y&=\pm {\frac {1}{4c}}{\sqrt {16c^{2}r_{1}^{2}-(r_{1}^{2}-r_{2}^{2}+4c^{2})^{2}}}\end{aligned}}}
x
=
∫
cos
[
∫
κ
(
s
)
d
s
]
d
s
y
=
∫
sin
[
∫
κ
(
s
)
d
s
]
d
s
{\displaystyle {\begin{aligned}x&=\int \cos \left[\int \kappa (s)\,ds\right]ds\\y&=\int \sin \left[\int \kappa (s)\,ds\right]ds\end{aligned}}}
To polar coordinates
From Cartesian coordinates
r
=
x
2
+
y
2
θ
′
=
arctan
|
y
x
|
{\displaystyle {\begin{aligned}r&={\sqrt {x^{2}+y^{2}}}\\\theta '&=\arctan \left|{\frac {y}{x}}\right|\end{aligned}}}
θ
′
{\displaystyle \theta '}
0
<
θ
<
π
2
{\textstyle 0<\theta <{\frac {\pi }{2}}}
θ
,
{\displaystyle \theta ,}
θ
{\displaystyle \theta }
θ
:
{\displaystyle \theta :}
θ
=
{
2
θ
′
(
for
θ
′
in QI:
I
I
V
0
<
θ
′
<
π
2
)
2
π
−
θ
′
(
for
θ
′
in QII:
I
V
π
2
<
θ
′
<
π
)
2
π
+
θ
′
(
for
θ
′
in QIII:
I
I
π
<
θ
′
<
3
π
2
)
2
π
−
θ
′
(
for
θ
′
in QIV:
I
3
π
2
<
θ
′
<
2
π
)
{\displaystyle \theta ={\begin{cases}{\hphantom {2}}\theta '&({\text{for }}\theta '{\text{ in QI: }}{\phantom {IIV}}0<\theta '<{\frac {\pi }{2}})\\{\hphantom {2}}\pi -\theta '&({\text{for }}\theta '{\text{ in QII: }}{\phantom {IV}}{\frac {\pi }{2}}<\theta '<\pi )\\{\hphantom {2}}\pi +\theta '&({\text{for }}\theta '{\text{ in QIII: }}{\phantom {II}}\pi <\theta '<{\frac {3\pi }{2}})\\2\pi -\theta '&({\text{for }}\theta '{\text{ in QIV: }}{\phantom {I}}{\frac {3\pi }{2}}<\theta '<2\pi )\end{cases}}}
The value for
θ
{\displaystyle \theta }
θ
{\displaystyle \theta }
tan
θ
{\displaystyle \tan \theta }
−
π
2
<
θ
<
+
π
2
{\textstyle -{\frac {\pi }{2}}<\theta <+{\frac {\pi }{2}}}
π
{\displaystyle \pi }
Note that one can also use
r
=
x
2
+
y
2
θ
′
=
2
arctan
y
x
+
r
{\displaystyle {\begin{aligned}r&={\sqrt {x^{2}+y^{2}}}\\\theta '&=2\arctan {\frac {y}{x+r}}\end{aligned}}}
From 2-center bipolar coordinates
r
=
r
1
2
+
r
2
2
−
2
c
2
2
θ
=
arctan
[
8
c
2
(
r
1
2
+
r
2
2
−
2
c
2
)
r
1
2
−
r
2
2
−
1
]
{\displaystyle {\begin{aligned}r&={\sqrt {\frac {r_{1}^{2}+r_{2}^{2}-2c^{2}}{2}}}\\\theta &=\arctan \left[{\sqrt {{\frac {8c^{2}(r_{1}^{2}+r_{2}^{2}-2c^{2})}{r_{1}^{2}-r_{2}^{2}}}-1}}\right]\end{aligned}}}
Where 2c is the distance between the poles.
To log-polar coordinates from Cartesian coordinates
ρ
=
log
x
2
+
y
2
,
θ
=
arctan
y
x
.
{\displaystyle {\begin{aligned}\rho &=\log {\sqrt {x^{2}+y^{2}}},\\\theta &=\arctan {\frac {y}{x}}.\end{aligned}}}
Arc-length and curvature
In Cartesian coordinates
κ
=
x
′
y
″
−
y
′
x
″
(
x
′
2
+
y
′
2
)
3
2
s
=
∫
a
t
x
′
2
+
y
′
2
d
t
{\displaystyle {\begin{aligned}\kappa &={\frac {x'y''-y'x''}{({x'}^{2}+{y'}^{2})^{\frac {3}{2}}}}\\s&=\int _{a}^{t}{\sqrt {{x'}^{2}+{y'}^{2}}}\,dt\end{aligned}}}
In polar coordinates
κ
=
r
2
+
2
r
′
2
−
r
r
″
(
r
2
+
r
′
2
)
3
2
s
=
∫
a
φ
r
2
+
r
′
2
d
φ
{\displaystyle {\begin{aligned}\kappa &={\frac {r^{2}+2{r'}^{2}-rr''}{(r^{2}+{r'}^{2})^{\frac {3}{2}}}}\\s&=\int _{a}^{\varphi }{\sqrt {r^{2}+{r'}^{2}}}\,d\varphi \end{aligned}}}
3-dimensional
Let (x, y, z) be the standard Cartesian coordinates, and (ρ, θ, φ) the spherical coordinates , with θ the angle measured away from the +Z axis (as [1] , see conventions in spherical coordinates ). As φ has a range of 360° the same considerations as in polar (2 dimensional) coordinates apply whenever an arctangent of it is taken. θ has a range of 180°, running from 0° to 180°, and does not pose any problem when calculated from an arccosine, but beware for an arctangent.
If, in the alternative definition, θ is chosen to run from −90° to +90°, in opposite direction of the earlier definition, it can be found uniquely from an arcsine, but beware of an arccotangent. In this case in all formulas below all arguments in θ should have sine and cosine exchanged, and as derivative also a plus and minus exchanged.
All divisions by zero result in special cases of being directions along one of the main axes and are in practice most easily solved by observation.
To Cartesian coordinates
From spherical coordinates
x
=
ρ
sin
θ
cos
φ
y
=
ρ
sin
θ
sin
φ
z
=
ρ
cos
θ
∂
(
x
,
y
,
z
)
∂
(
ρ
,
θ
,
φ
)
=
(
sin
θ
cos
φ
ρ
cos
θ
cos
φ
−
ρ
sin
θ
sin
φ
sin
θ
sin
φ
ρ
cos
θ
sin
φ
ρ
sin
θ
cos
φ
cos
θ
−
ρ
sin
θ
0
)
{\displaystyle {\begin{aligned}x&=\rho \,\sin \theta \cos \varphi \\y&=\rho \,\sin \theta \sin \varphi \\z&=\rho \,\cos \theta \\{\frac {\partial (x,y,z)}{\partial (\rho ,\theta ,\varphi )}}&={\begin{pmatrix}\sin \theta \cos \varphi &\rho \cos \theta \cos \varphi &-\rho \sin \theta \sin \varphi \\\sin \theta \sin \varphi &\rho \cos \theta \sin \varphi &\rho \sin \theta \cos \varphi \\\cos \theta &-\rho \sin \theta &0\end{pmatrix}}\end{aligned}}}
So for the volume element:
d
x
d
y
d
z
=
det
∂
(
x
,
y
,
z
)
∂
(
ρ
,
θ
,
φ
)
d
ρ
d
θ
d
φ
=
ρ
2
sin
θ
d
ρ
d
θ
d
φ
{\displaystyle dx\,dy\,dz=\det {\frac {\partial (x,y,z)}{\partial (\rho ,\theta ,\varphi )}}\,d\rho \,d\theta \,d\varphi =\rho ^{2}\sin \theta \,d\rho \,d\theta \,d\varphi }
From cylindrical coordinates
x
=
r
cos
θ
y
=
r
sin
θ
z
=
z
∂
(
x
,
y
,
z
)
∂
(
r
,
θ
,
z
)
=
(
cos
θ
−
r
sin
θ
0
sin
θ
r
cos
θ
0
0
0
1
)
{\displaystyle {\begin{aligned}x&=r\,\cos \theta \\y&=r\,\sin \theta \\z&=z\,\\{\frac {\partial (x,y,z)}{\partial (r,\theta ,z)}}&={\begin{pmatrix}\cos \theta &-r\sin \theta &0\\\sin \theta &r\cos \theta &0\\0&0&1\end{pmatrix}}\end{aligned}}}
So for the volume element:
d
V
=
d
x
d
y
d
z
=
det
∂
(
x
,
y
,
z
)
∂
(
r
,
θ
,
z
)
d
r
d
θ
d
z
=
r
d
r
d
θ
d
z
{\displaystyle dV=dx\,dy\,dz=\det {\frac {\partial (x,y,z)}{\partial (r,\theta ,z)}}\,dr\,d\theta \,dz=r\,dr\,d\theta \,dz}
To spherical coordinates
From Cartesian coordinates
ρ
=
x
2
+
y
2
+
z
2
θ
=
arctan
(
x
2
+
y
2
z
)
=
arccos
(
z
x
2
+
y
2
+
z
2
)
φ
=
arctan
(
y
x
)
=
arccos
(
x
x
2
+
y
2
)
=
arcsin
(
y
x
2
+
y
2
)
∂
(
ρ
,
θ
,
φ
)
∂
(
x
,
y
,
z
)
=
(
x
ρ
y
ρ
z
ρ
x
z
ρ
2
x
2
+
y
2
y
z
ρ
2
x
2
+
y
2
−
x
2
+
y
2
ρ
2
−
y
x
2
+
y
2
x
x
2
+
y
2
0
)
{\displaystyle {\begin{aligned}\rho &={\sqrt {x^{2}+y^{2}+z^{2}}}\\\theta &=\arctan \left({\frac {\sqrt {x^{2}+y^{2}}}{z}}\right)=\arccos \left({\frac {z}{\sqrt {x^{2}+y^{2}+z^{2}}}}\right)\\\varphi &=\arctan \left({\frac {y}{x}}\right)=\arccos \left({\frac {x}{\sqrt {x^{2}+y^{2}}}}\right)=\arcsin \left({\frac {y}{\sqrt {x^{2}+y^{2}}}}\right)\\{\frac {\partial \left(\rho ,\theta ,\varphi \right)}{\partial \left(x,y,z\right)}}&={\begin{pmatrix}{\frac {x}{\rho }}&{\frac {y}{\rho }}&{\frac {z}{\rho }}\\{\frac {xz}{\rho ^{2}{\sqrt {x^{2}+y^{2}}}}}&{\frac {yz}{\rho ^{2}{\sqrt {x^{2}+y^{2}}}}}&-{\frac {\sqrt {x^{2}+y^{2}}}{\rho ^{2}}}\\{\frac {-y}{x^{2}+y^{2}}}&{\frac {x}{x^{2}+y^{2}}}&0\\\end{pmatrix}}\end{aligned}}}
See also the article on atan2 for how to elegantly handle some edge cases.
So for the element:
d
ρ
d
θ
d
φ
=
det
∂
(
ρ
,
θ
,
φ
)
∂
(
x
,
y
,
z
)
d
x
d
y
d
z
=
1
x
2
+
y
2
x
2
+
y
2
+
z
2
d
x
d
y
d
z
{\displaystyle d\rho \,d\theta \,d\varphi =\det {\frac {\partial (\rho ,\theta ,\varphi )}{\partial (x,y,z)}}\,dx\,dy\,dz={\frac {1}{{\sqrt {x^{2}+y^{2}}}{\sqrt {x^{2}+y^{2}+z^{2}}}}}\,dx\,dy\,dz}
From cylindrical coordinates
ρ
=
r
2
+
h
2
θ
=
arctan
r
h
φ
=
φ
∂
(
ρ
,
θ
,
φ
)
∂
(
r
,
h
,
φ
)
=
(
r
r
2
+
h
2
h
r
2
+
h
2
0
h
r
2
+
h
2
−
r
r
2
+
h
2
0
0
0
1
)
det
∂
(
ρ
,
θ
,
φ
)
∂
(
r
,
h
,
φ
)
=
1
r
2
+
h
2
{\displaystyle {\begin{aligned}\rho &={\sqrt {r^{2}+h^{2}}}\\\theta &=\arctan {\frac {r}{h}}\\\varphi &=\varphi \\{\frac {\partial (\rho ,\theta ,\varphi )}{\partial (r,h,\varphi )}}&={\begin{pmatrix}{\frac {r}{\sqrt {r^{2}+h^{2}}}}&{\frac {h}{\sqrt {r^{2}+h^{2}}}}&0\\{\frac {h}{r^{2}+h^{2}}}&{\frac {-r}{r^{2}+h^{2}}}&0\\0&0&1\\\end{pmatrix}}\\\det {\frac {\partial (\rho ,\theta ,\varphi )}{\partial (r,h,\varphi )}}&={\frac {1}{\sqrt {r^{2}+h^{2}}}}\end{aligned}}}
To cylindrical coordinates
From Cartesian coordinates
r
=
x
2
+
y
2
θ
=
arctan
(
y
x
)
z
=
z
{\displaystyle {\begin{aligned}r&={\sqrt {x^{2}+y^{2}}}\\\theta &=\arctan {\left({\frac {y}{x}}\right)}\\z&=z\quad \end{aligned}}}
∂
(
r
,
θ
,
h
)
∂
(
x
,
y
,
z
)
=
(
x
x
2
+
y
2
y
x
2
+
y
2
0
−
y
x
2
+
y
2
x
x
2
+
y
2
0
0
0
1
)
{\displaystyle {\frac {\partial (r,\theta ,h)}{\partial (x,y,z)}}={\begin{pmatrix}{\frac {x}{\sqrt {x^{2}+y^{2}}}}&{\frac {y}{\sqrt {x^{2}+y^{2}}}}&0\\{\frac {-y}{x^{2}+y^{2}}}&{\frac {x}{x^{2}+y^{2}}}&0\\0&0&1\end{pmatrix}}}
From spherical coordinates
r
=
ρ
sin
φ
h
=
ρ
cos
φ
θ
=
θ
∂
(
r
,
h
,
θ
)
∂
(
ρ
,
φ
,
θ
)
=
(
sin
φ
ρ
cos
φ
0
cos
φ
−
ρ
sin
φ
0
0
0
1
)
det
∂
(
r
,
h
,
θ
)
∂
(
ρ
,
φ
,
θ
)
=
−
ρ
{\displaystyle {\begin{aligned}r&=\rho \sin \varphi \\h&=\rho \cos \varphi \\\theta &=\theta \\{\frac {\partial (r,h,\theta )}{\partial (\rho ,\varphi ,\theta )}}&={\begin{pmatrix}\sin \varphi &\rho \cos \varphi &0\\\cos \varphi &-\rho \sin \varphi &0\\0&0&1\\\end{pmatrix}}\\\det {\frac {\partial (r,h,\theta )}{\partial (\rho ,\varphi ,\theta )}}&=-\rho \end{aligned}}}
s
=
∫
0
t
x
′
2
+
y
′
2
+
z
′
2
d
t
κ
=
(
z
″
y
′
−
y
″
z
′
)
2
+
(
x
″
z
′
−
z
″
x
′
)
2
+
(
y
″
x
′
−
x
″
y
′
)
2
(
x
′
2
+
y
′
2
+
z
′
2
)
3
2
τ
=
x
‴
(
y
′
z
″
−
y
″
z
′
)
+
y
‴
(
x
″
z
′
−
x
′
z
″
)
+
z
‴
(
x
′
y
″
−
x
″
y
′
)
(
x
′
y
″
−
x
″
y
′
)
2
+
(
x
″
z
′
−
x
′
z
″
)
2
+
(
y
′
z
″
−
y
″
z
′
)
2
{\displaystyle {\begin{aligned}s&=\int _{0}^{t}{\sqrt {{x'}^{2}+{y'}^{2}+{z'}^{2}}}\,dt\\[3pt]\kappa &={\frac {\sqrt {(z''y'-y''z')^{2}+(x''z'-z''x')^{2}+(y''x'-x''y')^{2}}}{({x'}^{2}+{y'}^{2}+{z'}^{2})^{\frac {3}{2}}}}\\[3pt]\tau &={\frac {x'''(y'z''-y''z')+y'''(x''z'-x'z'')+z'''(x'y''-x''y')}{{(x'y''-x''y')}^{2}+{(x''z'-x'z'')}^{2}+{(y'z''-y''z')}^{2}}}\end{aligned}}}
See also
References
![{\displaystyle {\begin{aligned}x&=r\cos \theta \\y&=r\sin \theta \\[5pt]{\frac {\partial (x,y)}{\partial (r,\theta )}}&={\begin{bmatrix}\cos \theta &-r\sin \theta \\\sin \theta &{\phantom {-}}r\cos \theta \end{bmatrix}}\\[5pt]{\text{Jacobian}}=\det {\frac {\partial (x,y)}{\partial (r,\theta )}}&=r\end{aligned}}}](/media/api/rest_v1/media/math/render/svg/a9005464a89553d80be52a7b3c648717e7efc509)
![{\displaystyle {\begin{aligned}x&=\int \cos \left[\int \kappa (s)\,ds\right]ds\\y&=\int \sin \left[\int \kappa (s)\,ds\right]ds\end{aligned}}}](/media/api/rest_v1/media/math/render/svg/0cf415cca15fe7faf409efdfa8323225993978f8)
![{\displaystyle {\begin{aligned}r&={\sqrt {\frac {r_{1}^{2}+r_{2}^{2}-2c^{2}}{2}}}\\\theta &=\arctan \left[{\sqrt {{\frac {8c^{2}(r_{1}^{2}+r_{2}^{2}-2c^{2})}{r_{1}^{2}-r_{2}^{2}}}-1}}\right]\end{aligned}}}](/media/api/rest_v1/media/math/render/svg/40fd7b0ef6f1fea0e4467981685d16feb513186d)
![{\displaystyle {\begin{aligned}s&=\int _{0}^{t}{\sqrt {{x'}^{2}+{y'}^{2}+{z'}^{2}}}\,dt\\[3pt]\kappa &={\frac {\sqrt {(z''y'-y''z')^{2}+(x''z'-z''x')^{2}+(y''x'-x''y')^{2}}}{({x'}^{2}+{y'}^{2}+{z'}^{2})^{\frac {3}{2}}}}\\[3pt]\tau &={\frac {x'''(y'z''-y''z')+y'''(x''z'-x'z'')+z'''(x'y''-x''y')}{{(x'y''-x''y')}^{2}+{(x''z'-x'z'')}^{2}+{(y'z''-y''z')}^{2}}}\end{aligned}}}](/media/api/rest_v1/media/math/render/svg/439b196b830ab79231f87b27a17af5ed4cf5f4e4)
![[1]](/wiki/File:3D_Spherical.svg){kind=link}