Projections
Projection:
Plate Carrée (Equirectangular, φ1 = 0°)
x
=
λ
2
⋅
π
y
=
φ
2
⋅
π
Equirectangular, φ1 = 15°
x
=
λ
2
⋅
π
y
=
φ
⋅
2
⋅
(
3
−
1
)
2
⋅
π
Equirectangular, φ1 = 30°
x
=
λ
2
⋅
π
y
=
φ
⋅
3
3
⋅
π
Plate Carrée (Equirectangular, φ1 = 45°)
x
=
λ
2
⋅
π
y
=
φ
⋅
2
2
⋅
π
Equirectangular, φ1 = 60°
x
=
λ
2
⋅
π
y
=
φ
π
Mercator
x
=
λ
2
⋅
π
y
=
ln
⁡
(
tan
⁡
(
π
4
+
φ
2
)
)
2
⋅
π
Gall Stereographic
x
=
λ
2
⋅
π
y
=
tan
⁡
(
φ
2
)
⋅
(
2
+
1
)
2
⋅
π
Miller
x
=
λ
2
⋅
π
y
=
5
⋅
ln
⁡
(
tan
⁡
(
π
4
+
2
⋅
φ
5
)
)
8
⋅
π
Lambert (Cylindrical Equal Area, φ1 = 0°)
x
=
λ
2
⋅
π
y
=
sin
⁡
(
φ
)
2
⋅
π
Behrmann (Cylindrical Equal Area, φ1 = 30°
x
=
λ
2
⋅
π
y
=
2
⋅
sin
⁡
(
φ
)
3
⋅
π
Hobo-Dyer (Cylindrical Equal Area, φ1 = 37°30'
x
=
λ
2
⋅
π
y
=
sin
⁡
(
φ
)
(
cos
⁡
(
5
⋅
π
24
)
)
2
⋅
2
⋅
π
Gall-Peters (Cylindrical Equal Area, φ1 = 45°)
x
=
λ
2
⋅
π
y
=
sin
⁡
(
φ
)
π
Balthasart (Cylindrical Equal Area, φ1 = 50°)
x
=
λ
2
⋅
π
y
=
sin
⁡
(
φ
)
(
cos
⁡
(
5
⋅
π
18
)
)
2
⋅
2
⋅
π
Sinusoidal
x
=
λ
⋅
cos
⁡
(
φ
)
2
⋅
π
y
=
φ
2
⋅
π
Mollweide
2
⋅
θ
+
sin
⁡
(
2
⋅
θ
)
=
π
⋅
sin
⁡
(
φ
)
x
=
λ
⋅
cos
⁡
(
θ
)
2
⋅
π
y
=
sin
⁡
(
θ
)
4
Robinson
Latitude
XScale
YScale
90°
0.5322
1.0000
85°
0.5722
0.9761
80°
0.6213
0.9394
75°
0.6732
0.8936
70°
0.7186
0.8435
65°
0.7597
0.7903
60°
0.7986
0.7346
55°
0.8350
0.6769
50°
0.8679
0.6176
45°
0.8962
0.5571
40°
0.9216
0.4958
35°
0.9427
0.4340
30°
0.9600
0.3720
25°
0.9730
0.3100
20°
0.9822
0.2480
15°
0.9900
0.1860
10°
0.9954
0.1240
5°
0.9986
0.0620
0°
1.0000
0.0000
-5°
0.9986
-0.0620
-10°
0.9954
-0.1240
-15°
0.9900
-0.1860
-20°
0.9822
-0.2480
-25°
0.9730
-0.3100
-30°
0.9600
-0.3720
-35°
0.9427
-0.4340
-40°
0.9216
-0.4958
-45°
0.8962
-0.5571
-50°
0.8679
-0.6176
-55°
0.8350
-0.6769
-60°
0.7986
-0.7346
-65°
0.7597
-0.7903
-70°
0.7186
-0.8435
-75°
0.6732
-0.8936
-80°
0.6213
-0.9394
-85°
0.5722
-0.9761
-90°
0.5322
-1.0000
x
=
XScale
⋅
λ
2
⋅
π
y
=
13523
⋅
YScale
16974
⋅
π
NaturalEarth
Latitude
XScale
YScale
90°
0.5630
1.0000
85°
0.6270
0.9761
80°
0.6754
0.9394
75°
0.7160
0.8936
70°
0.7525
0.8435
65°
0.7874
0.7903
60°
0.8196
0.7346
55°
0.8492
0.6769
50°
0.8763
0.6176
45°
0.9006
0.5571
40°
0.9222
0.4958
35°
0.9409
0.4340
30°
0.9570
0.3720
25°
0.9703
0.3100
20°
0.9811
0.2480
15°
0.9894
0.1860
10°
0.9953
0.1240
5°
0.9988
0.0620
0°
1.0000
0.0000
-5°
0.9988
-0.0620
-10°
0.9953
-0.1240
-15°
0.9894
-0.1860
-20°
0.9811
-0.2480
-25°
0.9703
-0.3100
-30°
0.9570
-0.3720
-35°
0.9409
-0.4340
-40°
0.9222
-0.4958
-45°
0.9006
-0.5571
-50°
0.8763
-0.6176
-55°
0.8492
-0.6769
-60°
0.8196
-0.7346
-65°
0.7874
-0.7903
-70°
0.7525
-0.8435
-75°
0.7160
-0.8936
-80°
0.6754
-0.9394
-85°
0.6270
-0.9761
-90°
0.5630
-1.0000
x
=
XScale
⋅
λ
2
⋅
π
y
=
13
⋅
YScale
50
Kavrayskiy VII
x
=
λ
⋅
1
−
3
⋅
(
φ
π
)
2
2
⋅
π
y
=
φ
⋅
3
3
⋅
π
Wagner VI
x
=
λ
⋅
1
−
3
⋅
(
φ
π
)
2
2
⋅
π
y
=
φ
2
⋅
π
Aitoff
α
=
arccos
⁡
(
cos
⁡
(
φ
)
⋅
cos
⁡
(
λ
2
)
)
x
=
cos
⁡
(
φ
)
⋅
sin
⁡
(
λ
2
)
sinc
⁡
(
α
)
⋅
π
y
=
sin
⁡
(
φ
)
sinc
⁡
(
α
)
⋅
2
⋅
π
Hammer
x
=
cos
⁡
(
φ
)
⋅
sin
⁡
(
λ
2
)
2
⋅
1
+
cos
⁡
(
φ
)
⋅
cos
⁡
(
λ
2
)
y
=
sin
⁡
(
φ
)
4
⋅
1
+
cos
⁡
(
φ
)
⋅
cos
⁡
(
λ
2
)
Winkel I
x
=
λ
⋅
(
cos
⁡
(
φ
)
⋅
π
+
2
)
2
⋅
π
⋅
(
π
+
2
)
y
=
φ
π
+
2
Winkel Tripel
α
=
arccos
⁡
(
cos
⁡
(
φ
)
⋅
cos
⁡
(
λ
2
)
)
x
=
sinc
⁡
(
α
)
⋅
λ
+
cos
⁡
(
φ
)
⋅
sin
⁡
(
λ
2
)
⋅
π
sinc
⁡
(
α
)
⋅
π
⋅
(
π
+
2
)
y
=
sin
⁡
(
φ
)
+
φ
⋅
sinc
⁡
(
α
)
2
⋅
sinc
⁡
(
α
)
⋅
(
π
+
2
)
Van der Grinten
θ
=
arcsin
⁡
(
|
2
⋅
φ
π
|
)
A
=
|
π
λ
−
λ
π
|
2
G
=
cos
⁡
(
θ
)
sin
⁡
(
θ
)
+
cos
⁡
(
θ
)
−
1
P
=
G
⋅
(
2
sin
⁡
(
θ
)
−
1
)
Q
=
A
2
+
G
x
=
{
λ
2
⋅
π
,
φ
=
0
0
,
λ
=
0
∨
φ
=
±
π
2
sign
⁡
(
λ
)
⋅
|
A
⋅
(
G
−
P
2
)
+
A
2
⋅
(
G
−
P
2
)
2
−
(
P
2
+
A
2
)
⋅
(
G
2
⋅
P
2
)
|
2
⋅
(
P
2
+
A
2
)
,
otherwise
y
=
{
0
,
φ
=
0
sign
⁡
(
φ
)
⋅
tan
⁡
(
θ
2
)
2
,
λ
=
0
∨
φ
=
±
π
2
sign
⁡
(
φ
)
⋅
|
P
⋅
Q
−
A
⋅
(
A
2
+
1
)
⋅
(
P
2
+
A
2
)
−
Q
2
|
2
⋅
(
P
2
+
A
2
)
,
otherwise
Eckert II
x
=
λ
⋅
4
−
3
⋅
sin
⁡
(
|
φ
|
)
4
⋅
π
y
=
sgn
⁡
(
φ
)
⋅
(
2
−
4
−
3
⋅
sin
⁡
(
|
φ
|
)
)
4
Eckert V
x
=
λ
⋅
(
1
+
cos
⁡
(
φ
)
)
4
⋅
π
y
=
φ
2
⋅
π
Azimuthal Equidistant (Polar)
x
=
sin
⁡
(
λ
)
⋅
(
0.25
−
φ
2
⋅
π
)
y
=
-
cos
⁡
(
λ
)
⋅
(
0.25
−
φ
2
⋅
π
)
Definitions and Notes
φ
=
latitude in radians
λ
=
longitude in radians
sinc
⁡
(
x
)
=
{
1
,
x
=
0
sin
⁡
(
x
)
x
,
otherwise
The formulae listed here for the projections are scaled to assume a circumfrence of 1. The formulae may not match their traditional definitions.