•
..
urements on non-Gaussian nois
e,
it
is
necessary to
use
a true-
rms instrument.
3.3.4 Measuring
Amplitude
Distribution.
The amplitude
distribution,
P(v),
can
be
measured by
means
of
a
circuit
that
measures
the percentage
of
time during
which the noise voltage exceeds (or does
not
exceed) the volt-
age
level,
v.
Apparatus
for
this purpose generally includes
some
form
of
level-crossing detector and,
for
high-speed opera-
tion,
Schmitt-circuit
wave-sh
apers.
The measurement must
be
made by averaging over a time long enough
to
smooth the
fluctuations in the indication
to
negligible
size.
The amplitude density
distribution,
p(v),
can
be
meas-
ured
by
similar,
but
somewhat more complicated, apparatus
that indicates the percentage
of
time that the noise voltage
exists
within
the range
from
v to
(v
+ dv). In making any
of
these measurements, averaging
is
important,
bacause
only
the
av
erage
characteristics
of
the noise
can
be
measured meaning-
fully.
In the present state
of
the art, l
eve
l-
crossing detector cir-
cuits
can
not
be
made
to
operate fast enough
for
measurements
on random noise containing such high frequencies
as
those pro-
duced by the 1383. However, measurements
can
be
made
by
sampling the noise at a lower-frequency rate,
such
as
50 or
100 kHz.
If
the sampling efficiency
is
unity,
the sampled-and-
held waveform
has
the
same
amplitude
distribution
as
the high-
frequency random noise,
but
it
contains much lower frequency
components, and
it
can
be
applied successfully
to
the l
eve
l-
crossing detector circuits mentioned above.
3.3.5
Amplitude
Distribution
of
the Type 1383.
The noise source
used
in the 1383
is
a thermionic diode.
The noise
is
generated
as
shot noise in the plate current
of
the
diode, the amp
litud
e
distribution
of
which
is
definitely
Gaussi-
an
because
the total current
is
the sum
of
a very large number
of
,independent pulses.2 The amplifiers in the 1383
have
been
specia
lly
des
ig
ned
so
that, at
full
output
amp I itude, pulses
be-
low 3a
will
not
be
clipped.
3.4 SPECTRUM.
3.4. 1 General.
The spectrum
of
a random signal
is
different
from
that
of
a periodic signal, which
is
composed
of
one or more discrete
lin
es,
each
of
which corresponds
to
a frequency component
of
the periodic signal. A
truly
random signal contains no peri-
odic
fr
equency components, and
has
a spectrum that
is
a con-
tinuous function
of
frequency.
3.4.2 Spectrum Functions.
The frequency content
of
a random noise
is
described by
a
function
called the spectral intensity, which
has
the dimen-
sions
of
voltage squared per
unit
bandwidth. (When divided
2Bennett
, W.
R.
,
"Electrical
Noise",
McGraw-Hill
Book
Co.,
New
York
(1960),
p.40.
by a value
of
resistance,
it
is
equal
to
the power that voltage
would dissipate in that resistance, per
unit
bandwidth). The
spectral intensity
is
the Fourier transform
of
the autocorrela-
tion
function,
and
is
the spectrum function most often
used
in
mathematical analysis
of
random noise.
It
is
not
the most co
n-
venient function
for
practical
use,
~owever,
because
spectra
are
usually measured
as
voltage, rather than voltage
squa
r
ed
, in a
given bandwidth, and
filter
r
esponses,
used
in shaping noise
spectra,
are
usually
measu
r
ed
as
voltage functions. Therefor
e,
for
practical
use,
we
define the voltage spectrum
as
numerical-
ly equal to the square
root
of
the
spec
tral intensity.
It
has
units
of
voltage per
squa
re
root
of
bandwi
dth,
but
may
be
spoken
of
as
voltage in a given bandwidth. Spect
ra
shown in
Figure 3-3
are
plotted
as
vo
lt
age
spectra.
3.4.3 White Noise.
Noise whose spect
ral
intens
it
y
is
constant
ov~r
a range of
frequencies
is
called white noise, by
ana
logy with
white
light,
which contains more or l
ess
equal
int
ens
iti
es
of
all visible
colors.3 White noise cannot contain equal amplitudes at
al
l
frequencies,
for
then the total power in t
he
noise would
be
in-
finite. White noise, therefore,
means
that
the spectrum
is
flat
over the range
of
interest,
for
example,
throughout
the audi
o-
frequency rang
e.
Because
of
it
s
flat
spec
trum,
whit
e noise
,i
s
particularly convenient
as
a
sta
rting point
for
many experi-
ments.
3.4.4 Importance
of
Knowing the Spectrum.
In most experiments involving random noise, knowl
edge
of
the spectrum
of
the noise being
used
is vitally
necessa
ry.
When
noise
is
used
as
a driving-po
int
signa
l
to
determine the
response
of
some
sys
tem, the response is meaningful
only
when
the
input
spect
ru
m
is
known, and
is
usual
ly most conveniently
studied when the
input
spectrum is flat. There are,
of
cou
rse,
cases
where other spectra are more convenient.
If,
in such
cases
, a
filter
can
be
constructed whose r
espo
nse has
the
shape
of
the desired spectrum,
white
noise
is
the proper
input
fo
r
that
filter
to
produce the desired spectrum at its
output
3.4.5 Noise-Spectra Measurements.
The spectrum
of
a noise
can
be
measured
with
any
wave
analyzer whose frequency
range
is
appropriat
e.
For the out-
put
indication to
be
free
of
fluctuat
i
ons
th
at
might
ca
use
reading errors, the product
of
ana
ly
sis
bandwidth and the
av-
eraging time must
be
large. As in the
meas
ur
eme
nt
of
the
amplitude
distribution,
the spectrum
ca
n only
be
measured
accurately
by
ave
ra
ging
ove
r a relatively long
tim
e interval.
Wave
analyzers generally indi
ca
te the vol
tage
in the
ana
l-
ysis passband. The indication
is
therefore propo
rti
onal
to
w(f)
,
not
W(f).
It
is
convenient
to
reduce all measurements
to
a
3Aithough,
as
Bennett
(op.cit.,
p.
14)
points
out,
the
analogy
has
been
drawn
inco
rr
ect
ly
,
because
spec
troscopists
were
measuring
Intensity
as
a
function
of
wa
ve
length
,
and
found
it
to
be
substantially
con
sta
nt
per
unit
wavelength,
not
per
unit
frequency.
PROPERTIES OF RANDOM NOISE 3-3