Global Positioning System Reference
In-Depth Information
r X (τ )
(
0
,
1
)
τ
T
T
FIGURE 1.5. Autocorrelation function r X (τ ) for random sequence of pulses with ampli-
tude
±
1.
The ACF for the sample function x
(
t
)
of a process X
(
t
)
consisting of a random
sequence of pulses with amplitude
±
1 and with equal probability for the outcome
+
1and
1 is [see, e.g., Forssell (1991) or Haykin (2000)]
1
| τ T ,
for
| τ |≤
T ,
r X (τ ) =
(1.15)
0
,
otherwise.
The ACF is plotted in Figure 1.5. It follows that the power spectral density is
T
1
e j ωτ d
T sinc 2 ω
| τ |
T
T
2
S X (ω) =
τ =
,
(1.16)
T
which is plotted in Figure 1.6. The power spectral density of X
possesses a
main lope bounded by well-defined spectral nulls. Accordingly, the null-to-null
bandwidth provides a simple measure for the bandwidth of X
(
t
)
(
t
)
.
Note that the power spectral density S X (ω)
of a random sequence of pulses with
amplitude
±
1 differs from the energy spectral density
E f (ω)
,givenin(1.11),ofa
single rectangular pulse by only a scalar factor T .
1.2
Sampling
A crucial signal processing operation in a GPS or Galileo software-defined re-
ceiver is sampling . In the following we briefly review the sampling process.
Consider the signal x
. Suppose that we sample this signal at a uniform rate—
say once every T s seconds. Then we obtain an infinite sequence of samples, and
we denote this sequence by
(
t
)
,where n takes on all integer values. The
quantity T s is called the sampling period , and its reciprocal f s
{
x
(
nT s ) }
=
1
/
T s the sam-
pling rate .
The sampling operation is mathematically described by
x
δ (
t
) =
x
(
nT s )δ(
t
nT s ),
n
=−∞
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