Geography Reference
In-Depth Information
Along the orthonormal base
{
e 1 ,e 2 |O}
attached to the origin
O
, the center of the “one-sphere”,
2 = x 2 + y 2 = r 2 > 0. A point P
of the “one-sphere” is orthogonally projected on the x axis such that p = π ( P ). Refer to Fig. 3.1
for an illustration. The unit vector e x := x /
2
we define a Cartesian coordinate system
{
x, y
}
such that
x
x
2 and the unit base vector e 1 include the angle
λ =
( e x , e 1 ), an element of the open interval λ
∈{ R |
0 <λ < 2 π
}
.
Φ 1 ( x ): x ( λ )= e 1 r cos λ + e 2 r sin λ,
Φ ( x )= λ ( x )
(3.3)
Φ 1 ( x )= r cos λ
,
(3.4)
sin λ
d( x 1 , x 2 )= r (cos λ 1
cos λ 2 ) 2 +(sin λ 1
sin λ 2 ) 2 =
= r 2 1
(cos λ 1 cos λ 2 +sin λ 1 sin λ 2 ) =
(3.5)
= r 2 1
cos( λ 1
λ 2 ) .
We apologize for our sloppy notation x ( λ ) meaning x =
κ
( λ ), but introduced for economical
reason: save extra symbols.
arctan( y/x )
for x> 0
arctan( y/x )+ π
for x< 0
λ ( x )=
.
(3.6)
( π/ 2) sgn y
for x =0and y
=0
undefined
for x =0and y =0
Note that =0or2 π} or, equivalently, {x = r, y =0 } is the exceptional point which is not
curved by the angular parameter λ !
1
(ii) Topology on Φ ( S
r ) .
The topology on Φ ( S
r ) is defined by the Euclidean metric, namely the distance function
d( y 1 , y 2 ):=
y 1
y 2 2 =
|
λ 1
λ 2 |
.
(3.7)
End of Example.
r , two-dimensional manifold, topology).
Example 3.2 (Sphere
S
2
2
First, we present the topology on
S
r . Second, we present the topology on φ (
S
r ). The “two-sphere”
2
S
r (sphere of radius r ) is defined as the manifold
2
3
x 2 + y 2 + z 2 = r 2 ,r
+ ,r> 0
S
r :=
{
x
R
|
R
}
.
(3.8)
2
(i) Topology on
S
r .
2
The topology on
S
r is defined by the Euclidean metric , namely the distance function of the
3 , i.e. d( x 1 , x 2 ):=
ambient space
R
x 1
x 2
2 . Along the orthonormal base
{
e 1 , e 2 , e 3
|O}
attached to the origin
O
, the center of the “two-sphere”, we define a Cartesian coordinate system
2 = x 2 + y 2 + z 2 = r 2 > 0. A point P of the “two-sphere” is
orthogonally projected on the ( x, y ) plane, which is also called the equatorial plane , such that
p = π ( P ). Refer to Fig. 3.2 for an illustration. The straight line p - O is oriented with respect to
the unit vector e 1 or the x axis by the angular parameter “spherical longitude” λ ,anelement
{
x, y, z
}
in such a way that
x
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