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ADA4938-2_15 Datasheet, PDF (20/28 Pages) Analog Devices – Ultralow Distortion Differential ADC Driver
ADA4938-1/ADA4938-2
Similar to the case of a conventional op amp, the output noise
voltage densities can be estimated by multiplying the input-
referred terms at +IN and −IN by the appropriate output factor,
where:
GN
=
(β1
2
+
β2 )
is
the
circuit
noise
gain.
β1
=
RG1
RF1 + RG1
and
β2
=
RG2
RF2 + RG2
are the feedback factors.
When RF1/RG1 = RF2/RG2, β1 = β2 = β, and the noise gain
becomes
GN
=
1
β
=1+
RF
RG
Note that the output noise from VOCM goes to zero in this case.
The total differential output noise density, vnOD, is the root-sum-
square of the individual output noise terms.
8
∑ vnOD =
vn2Oi
i =1
THE IMPACT OF MISMATCHES IN THE FEEDBACK
NETWORKS
As previously mentioned, even if the external feedback networks
(RF/RG) are mismatched, the internal common-mode feedback
loop still forces the outputs to remain balanced. The amplitudes
of the signals at each output remain equal and 180° out of phase.
The input-to-output, differential mode gain varies proportionately
to the feedback mismatch, but the output balance is unaffected.
As well as causing a noise contribution from VOCM, ratio matching
errors in the external resistors result in a degradation of the
ability of the circuit to reject input common-mode signals, much
the same as for a four-resistor difference amplifier made from a
conventional op amp.
In addition, if the dc levels of the input and output common-
mode voltages are different, matching errors result in a small
differential-mode output offset voltage. When G = +1, with a
ground referenced input signal and the output common-mode
level set to 2.5 V, an output offset of as much as 25 mV (1% of
the difference in common-mode levels) can result if 1% tolerance
resistors are used. Resistors of 1% tolerance result in a worst-case
input CMRR of about 40 dB, a worst-case differential-mode
output offset of 25 mV due to 2.5 V level-shift, and no significant
degradation in output balance error.
CALCULATING THE INPUT IMPEDANCE OF AN
APPLICATION CIRCUIT
The effective input impedance of a circuit depends on whether
the amplifier is being driven by a single-ended or differential
signal source. For balanced differential input signals, as shown
in Figure 59, the input impedance (RIN, dm) between the inputs
(+DIN and −DIN) is simply RIN, dm = 2 × RG.
RF
+DIN
–DIN
ADA4938
+VS
RG
+IN
VOCM
RG
–IN
RF
VOUT, dm
Figure 59. ADA4938 Configured for Balanced (Differential) Inputs
For an unbalanced, single-ended input signal (see Figure 60),
the input impedance is
( ) RIN, cm
=
⎜⎛
⎜
⎜
⎜⎝
1
−
2×
RG
RF
RG +
RF
⎟⎞
⎟
⎟
⎟⎠
RF
+VS
RS
RG
RT
VOCM ADA4938
VOUT, dm
RG
RS
RT
RF
Figure 60. ADA4938-x Configured for Unbalanced (Single-Ended) Input
The input impedance of the circuit is effectively higher than it
would be for a conventional op amp connected as an inverter
because a fraction of the differential output voltage appears at
the inputs as a common-mode signal, partially bootstrapping
the voltage across the Input Gain Resistor RG.
INPUT COMMON-MODE VOLTAGE RANGE IN
SINGLE-SUPPLY APPLICATIONS
The ADA4938 is optimized for level-shifting, ground-referenced
input signals. As such, the center of the input common-mode
range is shifted approximately 1 V down from midsupply. The
input common-mode range at the summing nodes of the amplifier
is from 0.3 V above −VS to 1.6 V below +VS. To avoid clipping at
the outputs, the voltage swing at the +IN and −IN terminals must
be confined to these ranges.
Rev. A | Page 20 of 28