output voltage of an oscillator can be expressed as:
v(t) = [V
o
+ ε(t)] sin [2πν
0
t + φ(t)] , (1)
where V
o
is the nominal peak voltage amplitude, ε(t)
is the deviation from the nominal amplitude, ν
0
is the
name-plate frequency, and φ(t) is the phase deviation
from the ideal phase 2πν
0
t. Changes in the peak value
of the signal is the amplitude instability. Fluctuations
in the zero crossings of the voltage is the phase insta-
bility. The so-called frequency instability is depicted
by the fluctuations in the period of the voltage. The
situation is depicted in figure 1
3
.
0 0.01 0.02 0.03 0.04 0.05 0.06 0.07 0.08 0.09 0.1
-2
-1.5
-1
-0.5
0
0.5
1
1.5
2
Time (s)
Voltage (V)
Amplitude instability
Phase instability
Frequency instability
Figure 1: Simulated types of instabilities in a 25 Hz si-
nusoidal output with additive noise. The noise process has
a power spectral density proportional to the inverse of the
frequency (flicker phase modulation).
The impacts of oscillator noise and the causes of
short term instabilities have been described in many
research works and tutorials like (Howe et al., 1999),
(Vig, 2001) and (Sullivan et al., 1990). The short-term
stability measures most frequently found on oscillator
specification sheets is the two-sample deviation, also
called Allan deviation, σ
2
y
(τ).
Classical variance in non-stationary noise
processes don’t converge to concrete values. It
diverges for some noise processes, such as random
walk, i.e., the variance increases with increasing
number of data points. This is the reason whereby
non-classical statistics are used to characterize short
term instability.
AVAR and MVAR have proven their adequacy
in characterizing frequency phase and instabilities.
These easy-to-compute variances converge for all
noise processes observed in precision frequency
sources, have a straightforward relationship to power
3
A similar example was provided by Prof. Eva Ferre-
Pikal (Univ. of Wyoming) and used by John R. Vig in (Vig,
2001).
law spectral density of noise processes, and are faster
and more accurate in than the FFT (Lesage and Ayi,
1984).
The estimates of AVAR and MVAR for a given cali-
bration time τ for a m-data series of phase differences,
x, are given by equations 2 and 3, (Greenhall, 1988):
AV AR ≡ σ
2
y
(τ, m) =
1
2(m − 1)
m
X
j=2
y
j
− y
j−1
2
=
1
2τ
2
(m − 1)
m
X
j=2
∆
2
τ
x(jτ )
2
(2)
MV AR ≡
1
2τ
2
h∆
2
τ
xi
2
, (3)
where the bar over x denotes the average in the
time interval τ (averaging time), and ∆
2
τ
x = x
i+2
−
2x
i+1
+ x
i
, is the so called second difference of
x. The fractional frequency deviation is the relative
phase difference in an interval τ. It is defined by equa-
tion 4:
y =
1
τ
Z
t
t−τ
y(s)ds =
x(t) − x(t − τ )
τ
=
∆
τ
x(t)
τ
.
(4)
Non-classical statistics estimators, defined above, in
equations 2 and 3, for non-stationary series charac-
terization, give an average dispersion of the fractional
frequency deviation due to the noise processes cou-
pled to the oscillator. As a consequence time do-
main instability (two-sample variance) is related to
the noise spectral density via (Rutman and Walls,
1991):
σ
2
y
(τ) =
2
(πν
0
τ)
2
Z
f
h
0
S
φ
(f)sin
4
(πfτ)df, (5)
where ν
0
is the carrier frequency and f is the Fourier
frequency (the variable), and f
h
is the band-width of
the measurement system. S
φ
(f) is the spectral den-
sity of phase deviations, which is in turn related to
the spectral density of fractional frequency deviations
by(Rutman and Walls, 1991):
S
φ
(f) =
ν
2
0
f
2
S
y
(f), (6)
The classical power-law noise model is a sum of the
five common spectral densities. The model can be de-
scribed by the one-sided phase spectral density S
φ
(f)
via (IEEE, 1988), (Greenhall, 1988):
S
φ
(f) =
ν
2
0
f
2
2
X
α=−2
h
α
f
α
= ν
2
0
4
X
β=0
h
β
f
β
, (7)
for 0 ≤ f ≤ f
h
. Where, again, f
h
is the high-
frequency cut-off of the measurement system (the
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311