Model 1815 - Keithley 181 Service Manual

Digital nanovoltmeter
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THEORY
OF OPERATION
MODEL
181
rnugl~yiblo, The bootstrap
supply
is decoupled
from the input
via C414. C415, R425and
R426. Rejection
from the + 15V sups
plies is critic;iil
as well.
Therefore.
current
regulators
CR406
and CR407 are a necessity
iRp>
1M ohm) since Rs of VR403
and VR404 is approximately
100 ohms,
The key to maintaimng
low current
noise in the drain circuit
of
Cl413 IS the selection
of a low noise, high gain device for Q414
and maintaining
low emitter
and base impedances
over the
bandwidth,
R431, R432 and R433 provide
bias for Q414 and
are referer~:ed
10 _t VR for low noise contribution
Noise contribution
from the second
stage depends
upon drain
loads of Q413, gain of the lirst stage and input noise of the second
srage~ Q412 is a precisely
matched
low noise amplifier
Wan
sister piiir which
act as the second
stage for the 181 preamp,
III addilior
10 low now,
Ihls fransislor
pa~r IQ4121 is required
because
of 1,s hlgtl CMRR performance.
4.18. Linearity
and Gain
,r a diifarential
DC amplifier.
nonlinearities
irI the input stage
provide
Ihe Iirnifal,on
10 gain linearity
under
the closed
loop
condluon.
In fact,
no amount
of loop gain car cailcol
these
nonIinearities.
The input
FETS are square
law devices
which
means the output
current
varies as the square of the VGS. In
order
fo r:anr:o, this nonlinearity.
a second
FET is used as a
load 10 the Hurst FET idifierer,lIaI
pair). The degree of linearity
depends
upon the match,ng
between
the two devlces~
The lolaI amplifier
loop gain must be kept high so that closed
Ioop gain is independent
of open loop gain.
This eliminates
problems
with gain drifts
due to time/temperature
var~atlons
inside
Ihe loop. To maintain
stable closed
loop gains of 1000
i2mV
rangel.
100 IZOmV range1 and 10 (200mV
range)
apt
propriate
film or wirewound
resistors
are chosen
as feedback
elements.
Refer to Table 4~2~
TABLE
4-2
GAIN RESlSTORS
Range
Gain Resistors
Gain
Adjustment
2mv
R40S. R414. R435
1000
R40S
ZOnl"
R410, R415, R435
10"
R410
zoomv
R411, R416. R434
10
R411
Thermal
drifts
in the input amplifier
are relatively
unimporfant
since
they
are autozeroed
our.
Slowly
varying
drill
come
ponents
isuch as solder joints,
reed relay contacts)
are of little
significance.
'Therefore,
no special
lowthermal
term~naIs are
necessary
irl the feedback
,oop
However,
for
the
nanovolt
ranges
(2mV.
ZOmVl,
it
IS
necessary
Lo use wirewound
resistors
wherever
low voltage
signals are present,
This is why R435 is a wirewound
element,
whereas
R434,
R409-R416
are film
resistors.
Film resistors
display
much
higher
voltage
noise whereas
wirewounds
are
avaiInb,e
whose
noise approaches
theoretical
limifs.
R435 is
s&x&d
as 200 ohms since the Johnson
noise of this value is
negligible
compared
to amplifier
noise.
4.20. Offset
Null
4.21. NMRR
Filter
and Buffer
Additional
NMRR is provided
111 the preamp using a threepole
cascaded
filter.
As can be seen from
Figure
4~7. the three
poles are provided
by three RC networks~
Wher, FFT Q4,S turns o,. sii drw
0405. 0407 and Q4OS~ The
fliters arc mow in tile nrw11 arrd Ihe input signal is now liltered
and
amplliicd,
The
filter
settling
I~me is equal
10 200
mi,Iiseconds.
After
lhe 200 millisecond
~rlferval
the signa
integration
1s done by the A/D~ FET 0420 (now lums 011, and
FETs Q419. Q405, Q407 arid 0408 lurn off, Since 110 liller IS !n
while
the amplifier
looks at "zero,"
settling
time depends
on
amplifier
speed
and is 4 milliseconds.
The zero is lhen
Inn
tegrated
by the A/D.
The reasorl
the filter must shut off is so fhc A/D
can record
amplifier
xxo
rlghl after if records
sign;lI
By keeping
the tlrll~
delay bctween
signal anti iclo
as small as pilss~t~lo, effective
,,o,se ar,d dr,f, iire reduced
tc lI,e desired
lkwel. Co~lcurrerltly,
filtering
of ~nrxmal mode signals
IS accomplished
only whet1
needed;
wl,an
looking
at the signn,~
T11e first pole is formed
by "416,
C407 and Q4oS. The on
resistance
of Q409
rnair~lains
i:,osed
loop
gain
aI all ire
qurncies
greater
than 10 which
maintains
ampI,firr
stability~
The second
pole is formed
by C406. R406 and Q407. It is butt
fered from tile third pole by U401 5, The third pale is formed
by
R401, C403 arid Q405~ AI, 11,rw ,x>Ies ,havr Ihr same 1,mc con
slant 01 10 miI,lseconds~
U401A builcrs
Ihr: oulput
01 thn third
p0le.
Buffers
U4OlA
and
U4OlB
are boo&trapped
in a similar
fashion
to the input amplifier.
VR401 and VR402 provide
the
+6.2V
reference,
and emitter
followers
WI1
and Q402 supply
Ihe currenl
10 ,,4Ol,
R40,C
and R407D b,as Ihi! r~iemnces.
The effect
oi This boofstrap
is fo provide
higher
CMRR
10
"401,
Ihnrefore
imprrivirng
linearity.
The baotstia,,
CllClllt aoiis a pole I" 11k ir"qlicrrcy
rcsp""sa
0,
U4016.
The dominant
pole formed
by R407A.
R407R. C401
arid C402 m~intnins
stability
rif the bootsrrap
c~rcoif. Q403 and
Q404 illIi ,ciw capai:ilarK:~
FtTs
used as d,odc clamps
10 Ihii
boolslraji
c~rcuil
to preve~lf
latch
up rcsult,ng
lrom
driviing
inputs
to U4OlB
out 01 lhoir
common
mode
range
durincj
overload
4-6

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