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2 ( y 2 - y 1 )
y 2
4
2
y 1
(a)
(b)
(c)
( 2 - 1 )(cos( 2 ) - cos( 1 ))
P
1
r
2
2
(1 - cos( r ))
2
/3
(d)
(e)
(f)
Figure 26.21: Various solid angles on the unit sphere.
( x , y , z ): x 2 + z 2 = 1, 0
Consider the upper half-cylinder H =
,
which projects to Ω under the axial projection map p . We can perform a change
of variables in the integral, and express B as
B =
( x , y , z ) H
{
y
1
}
Jp ( x , y , z )
dA ,
y
|
|
(26.24)
where ( x , y , z )= p ( x , y , z ) , and dA is area on H , and
is the Jacobian for
the change of variables (i.e., it represents how areas at ( x , y , z ) are stretched
or contracted to become areas at ( x , y , z )) . The theorem that p is area-preserving
means that
|
Jp
|
|
Jp
|
= 1, so the integral becomes
B =
ydA .
(26.25)
( x , y , z )
H
Figure 26.22: Horizontal radial
projection from the sphere to
the surrounding cylinder is area-
preserving.
Since in the formula for p , y does not change, we have y = y , so this becomes
B =
( x , y , z )
y dA .
(26.26)
H
times the integral of y from 0 to 1. That
By circular symmetry, this is just 2
π
2, so B = 2 ·
π
=
π
integral is 1
/
2
.
If instead we wanted to know the average of y over the upper hemisphere, we'd
need to divide its integral (
π
) by the area of the hemisphere (2
π
). The average is
1
thus
2 . This value comes up often, although it's usually in a slightly generalized
form: We have a hemisphere defined by
v ·
n
0, and we want to know the
average value of
n over this hemisphere. (Our instance is the special case
where n = 010 T .) We'll state this as a principle:
v ·
 
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