Operating
Instructions-PG
506 (SN 8040000 & up)
REFERENCE EDGE
;;;'
1 V
+TRIG
~
FIXED
OUT
AMPLITUDE
__
0 V
REFERENCE EDGE
-
-fO
V
HIGH
-t
AMPLITUDE
VARIABLE
SQUARE WAVE
REFERENCE EDGE
)
FAST RISE
~
OUTPUT
REFERENCE
EDGE
FAST RISE
-~
-r
OUTPUT
1740-02
Ag. 2-3. Output signals from the PG 506 Calibration Generator.
Fast Rise Outputs
To
use the
PG
506 Pulse
Generator
system
to
produce
low
amplitude
, fast-rise square-waves, set
the
mode
swtich
to
FAST RISE
position
and
connect
external
equipment
to
the FASTRISE
OUTPUTS
connector(s)
. Set
the PERIOD
controls
for
the period or
frequency
desired.
The
output
amplitude
can be adjusted by
the
PULSE
AMPLIUTDE
control.
These signals are
usually
used
to
adjust
high-
frequency
compensation
networks
in
oscilloscope
amplifier
circuits. The
adjustments
are
made
for
optimum
response
(minimum
aberrations). The risetime and
amplitude
specifications
for
the FAST RISE
outputs
apply
only
when
they
are
terminated
into
a
500
load. Larger
amplitudes
(greater than 1 V peak-to-peak) can be ob-
tained from these
output
connectors
under
unterminated
conditions,
but
the
risetime
specification
is
no
longer
applicable.
GENERAL
INFORMATION
Risetime Considerations
The
PG
506 can
be
used
in
conjunction
with
an
oscilloscope
to
determine
the risetime of a device under
test. Risetime is
normally
measured (unless otherwise
specified) between the
10%
and
90%
amplitude
levels on
2-6
the
leading
edge of a waveform.
The
risetime
of
a
displayed waveform is
illustrated
in
Fig. 2-4.
Before
measuring
the risetime
of
a device
under
test,
the
combined
risetime
of
the
PG
506
output
signal and
the
oscilloscope
vertical
amplifier
system must
be
known.
Refer
to
Fig. 2-4
for
the
percentage
error
to
be
expected
when
the
two
devices are cascaded. Sweep
timing
ac-
curacy
should
be verified
before
any
risetime measure-
ments are made.
Inaccuracies
in
the sweep
timing
and
display
reading
errors
must
be added
algebraically
to
the
percentage
error
obtained
from
computations
related
to
Fig. 2-4.
The
graph
for
Fig. 2-4 can
be
used
as
a
guideline
for
the
following
general
conclusions.
1.
Oscilloscopes
should
have a vertical system
risetime
about
one-seventh of
the
fastest signal applied
to
keep system errors
to
a
minimum.
2.
Conversely, if
the
signal risetime
is
at
least seven
times faster
than
the
risetime of the
oscilloscope
vertical
system, the displayed (observed) waveform
will
have a
risetime
that
is very close
to
the
risetime of the vertical
system.
3.
The
displayed
risetime
as
observed on any os-
cilloscope
can never
be
faster
than
the
risetime of
the
slowest device in the system.
Risetime of a displayed waveform is related
to
total
system
bandwidth
. A system
with
limited
high-frequency
response
will
produce
a displayed risetime that is
slower
than expected. If a
fast-step
signal
produces
a crt
display
with
little
or
no overshoot
or
ringing,
the
product
of
oscilloscope
risetime and
oscilloscope
bandwidth
should
result in a
factor
whose
value lies between 0.329 and 0.350.
The
followi
ng steps
describe
the
procedure
to
follow
in
determining
the
risetime of a device
under
test.
1.
Connect
the
appropriate
output
signal
from
the
PG
506
to
the
oscilloscope
vertical
input
with
ashort
500
coaxial cable terminated
into
a 50 0 load.
2. Set the
oscilloscope
controls
to
display
the
leading
edge
of
the waveform. Risetime measurements
should
be
made over
the
largest part of the
graticule
area possible.
When
the
fastest sweep rate is relatively
slow
compared
with
the
vertical system risetime
(or
the
scale is small),
measurements become
confined
to
small
sections
of
the
graticule, and
the
probability
of
display
reading
errors
becomes
greater
.
@