HP 8340B Manual page 336

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The
YIG sphere magnetic
field
is
proportional to the current through the
SYTM
coil
(with
a
sensitivity
of approximately
15
mA/GHz),
which
is
generated from the
PRETUNE
signal
from the A54 YO pretune
assembly, and the latched band information
from the A27 level control assembly.
To
track the
correct
YO frequency harmonic,
the
SYTM
driver has circuitry that adds corrections to the
SYTM
tuning
current that accounts for the
effects of the nonlinear tuning curve, hysteresis, and magnetic delay.
Nonlinear Tuning Curve Compensation. The A28 SYTM
driver
has
three breakpoint adjustments to
correct for the nonlinearities
in
the
SYTM
tuning
curve (one fixed;
two adjustable)
Magnetic Delay Compensation. The SYTM
magnet does not respond fast enough to track the
cor¬
rect frequency when the current drive
is
changed
rapidly. This
causes
an increasingly
severe delay
problem as the instrument sweep rate
is
increased. To compensate for the slow SYTM response,
the
delay compensation current, which
is
a
function of sweep rate and
change
in
frequency from the
start
of sweep, adds
to the
SYTM
tuning current.
A24 Attenuator Driver/SRD
Bias
Assembly
The A24 assembly
controls three
SYTM
functions:
Step recovery
diode bias
PIN switch driver
YIG sphere temperature control
Step Recovery Diode Bias.
In
band
1,
the SRD (step recovery diode)
is
forward biased
with
a
nega¬
tive voltage.
The SYTM
conversion
efficiency
in
the higher bands
is
related
to
the
SRD DC bias
voltage. Proper
SRD
biasing
is
also necessary to
avoid squegging.
NOTE;
Squegging
is
an undesired oscillation
in
the A13
switched YIG-tuned multiplier.
Symptoms
of
squegging are
power
reversal
(RF power
decreases as selected power
is
increased), power loss at
specific frequencies, and spurious signals
on the
RF output.
To maintain optimum
SRD
bias
for the higher bands, the bias voltage
is
generated as
a
function of
both frequency and
power
level.
The
SRD
bias voltage variation with frequency
is
derived from
1.4V/
GHz
(from the A28 assembly), which
is
proportional to the
YO frequency.
The SRD
bias
is
adjusted for
power
level correction with the
SRD
bias control
from the A26
linear modulator
assembly (a
voltage
corresponding to the modulator voltage).
Pin
Switch.
In
low
band, the low band
RF
input
passes unattenuated through the
SYTM,
and the
YIG
sphere
is
tuned by the A28 assembly to
a
fixed non-interfering frequency.
In
the high bands, the
SYTM
driver provides
a
tuning current, as described previously, while the
SYTM
low band RF input port
is
grounded to keep
it
from interfering with the desired high band RF output. The process
of selectively
grounding the low band RF signal
is
facilitated
by
the PIN
diode switch
In
the
SYTM. The
PIN diode
switch
driver
is
located on the
A24 attenuator driver/SRD bias assembly.
YIG Sphere Temperature Control. Because
the
SYTM passband
drifts
if
the
temperature
varies, the
YIG sphere temperature
is
held
constant with heater resistors and
a
thermistor (located on the
SYTM
substrate), and the heater
drive circuitry (located on the
A24 attenuator
driver/SRD
bias assembly).
SYTM Peaking
SYTM
peaking tunes the
SYTM
such that the RF signal (YO frequency or multiple of
the
YO
frequency)
is in
the center of
the
SYTM
1
dB
passband, ensuring that maximum RF power
is
available.
To manually access the peaking
routine (stored
in
ROM), press [PEAK].
To
remotely access the
peaking routine, use
"RP1"
(to turn peaking on) and "RPO" (to turn peaking
off).
When
you
access
the
peaking
routine this way,
it
executes
only
if
the instrument
is in
CW
or manual mode, and the RF
is
on.
HP 8340B/41B
RF
Section
Theory
of Operation
H-9

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