AD797 Data Sheet
Rev. K | Page 12 of 19
NOISE AND SOURCE IMPEDANCE CONSIDERATIONS
The AD797 ultralow voltage noise of 0.9 nV/√Hz is achieved
with special input transistors running at nearly 1 mA of collector
current. Therefore, it is important to consider the total input-
referred noise (e
N
total), which includes contributions from voltage
noise (e
N
), current noise (i
N
), and resistor noise (√4 kTR
S
).
2/12
2
])(4[
S
N
S
NN
RikTRetotale (1)
where R
S
is the total input source resistance.
This equation is plotted for the AD797 in Figure 34. Because
optimum dc performance is obtained with matched source
resistances, this case is considered even though it is clear from
Equation 1 that eliminating the balancing source resistance
lowers the total noise by reducing the total R
S
by a factor of 2.
At very low source resistance (R
S
< 50 Ω), the voltage noise of the
amplifier dominates. As source resistance increases, the Johnson
noise of R
S
dominates until a higher resistance of R
S
> 2 kΩ is
achieved; the current noise component is larger than the
resistor noise.
00846-033
100
1
0.1
10
10 100 1000 10000
SOURCE RESISTANCE (Ω)
NOISE (nV/
Hz)
TOTAL NOISE
RESISTOR
NOISE
ONLY
Figure 34. Noise vs. Source Resistance
The AD797 is the optimum choice for low noise performance if
the source resistance is kept <1 kΩ. At higher values of source
resistance, optimum performance with respect to only noise is
obtained with other amplifiers from Analog Devices (Table 5).
For up to date information, see AN-940.
Table 5. Recommended Amplifiers for Different Source
Impedances
R
S
(kΩ) Recommended Amplifier
0 to <1
AD8597/AD8599, AD797, ADA4004-1/
ADA4004-2/ADA4004-4, AD8671/AD8672/
AD8674
1 to <10
AD8675/AD8676, ADA4075-2, ADA4004-1/
ADA4004-2/ADA4004-4, OP1177, OP27/OP37,
OP184
10 to <100 AD8677, OP1177, OP2177, OP4177, OP471
>100
AD8610/AD8620, AD8605/AD8606/AD8608,
ADA4627-1, OP97, AD548, AD549, AD745
LOW FREQUENCY NOISE
Analog Devices specifies low frequency noise as a peak-to-peak
quantity in a 0.1 Hz to 10 Hz bandwidth. Several techniques can
be used to make this measurement. The usual technique involves
amplifying, filtering, and measuring the amplifier noise for a
predetermined test time. The noise bandwidth of the filter is
corrected for, and the test time is carefully controlled because
the measurement time acts as an additional low frequency roll-off.
The plot in Figure 6 uses a slightly different technique: an FFT-
based instrument (Figure 35) is used to generate a 10 Hz brickwall
filter. A low frequency pole at 0.1 Hz is generated with an
external ac coupling capacitor, which is also the instrument being
dc coupled.
Several precautions are necessary to attain optimum low
frequency noise performance:
Care must be used to account for the effects of R
S
. Even
a 10 Ω resistor has 0.4 nV/√Hz of noise (an error of 9%
when root sum squared with 0.9 nV/√Hz).
The test setup must be fully warmed up to prevent e
OS
drift
from erroneously contributing to input noise.
Circuitry must be shielded from air currents. Heat flow out
of the package through its leads creates the opportunity for
a thermoelectric potential at every junction of different metals.
Selective heating and cooling of these by random air currents
appears as 1/f noise and obscures the true device noise.
The results must be interpreted using valid statistical
techniques.
7
4
6
2
3
HP 3465
DYNAMIC SIGNAL
ANALYZER
(10Hz)
1
Ω
100kΩ
*
*
V
OUT
+V
S
–V
S
1.5µF
AD797
00846-034
*USE THE POWER SUPPLY BYPASSING SHOWN IN FIGURE 36.
Figure 35. Test Setup for Measuring 0.1 Hz to 10 Hz Noise
WIDEBAND NOISE
Due to its single-stage design, the noise of the AD797 is flat
over frequencies from less than 10 Hz to beyond 1 MHz. This
is not true of most dc precision amplifiers, where second-stage
noise contributes to input-referred noise beyond the audio
frequency range. The AD797 offers new levels of performance in
wideband imaging applications. In sampled data systems, where
aliasing of out-of-band noise into the signal band is a problem,
the AD797 outperforms all previously available IC op amps.