Global Positioning System Reference
In-Depth Information
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
[13
Fi gure 4.3
Limits on the a posteriori variance of unit weight. The figure refers to
α =
Lin
0.0
——
No
PgE
0 . 05.
The test statistics for testing groups of observations is based on v T Pv and the
change
v T Pv . According to Table 4.2 we have
= A 2 x + 2 T T A 2 x + 2
v T Pv
(4.269)
z 3 Tz 3
=
[13
Th e new random variable z 3 is a function of observations
1 and
2 . Applying the
la ws of propagation of mean and variance, one finds
A 2 E( x )
E( z 3 )
=
+
E(
2 )
=
A 2 x
A 2 x
=
o
(4.270)
T 1
Σ z 3 =
(4.271)
N o ,
0 T 1
2
z 3
σ
(4.272)
Carrying out the orthonormal transformation yields a random vector whose compo-
nents are stochastically independent and normally distributed. By standardizing these
distributions and summing the squares of these random variables, it follows that
v T Pv
σ
z 3 Tz 3
σ
n 2
=
∼ χ
(4.273)
2
0
2
0
has a chi-square distribution with n 2 degrees of freedom, where n 2 equals the number
of observations in the second group. The random variables (4.273) and (4.263) are
stochastically independent. To prove this, consider the new random variable z
=
 
Search WWH ::




Custom Search