Ultralow THD: < 0.01% @ G = 100 Over the Full Audio
Band
Wide Bandwidth: 1 MHz @ G = 100
High Slew Rate: 17 V/ms typ
Unity Gain Stable
True Differential Inputs
Subaudio 1/f Noise Corner
8-Pin Mini-DIP with Only One External Component
Required
Very Low Cost
Extended Temperature Range: –408C to +858C
APPLICATIONS
Audio Mix Consoles
Intercom/Paging Systems
Two-Way Radio
Sonar
Digital Audio Systems
Hz or 1.5 dB
Audio Preamplifier
SSM2017
FUNCTIONAL BLOCK DIAGRAM
V–
+IN
RG
RG
2
–IN
1
5kΩ
5kΩ
X1
PIN CONNECTIONS
Epoxy Mini-DIP (P Suffix)
X1
5kΩ
5kΩ
SSM2017
5kΩ
5kΩ
REFERENCE
V+
OUT
V–
GENERAL DESCRIPTION
The SSM2017 is a latest generation audio preamplifier, combining SSM preamplifier design expertise with advanced processing. The result is excellent audio performance from a selfcontained 8-pin mini-DIP device, requiring only one external
gain set resistor or potentiometer. The SSM2017 is further enhanced by its unity gain stability.
Key specifications include ultralow noise (1.5 dB noise figure)
and THD (<0.01% at G = 100), complemented by wide bandwidth and high slew rate.
Applications for this low cost device include microphone preamplifiers and bus summing amplifiers in professional and consumer audio equipment, sonar, and other applications requiring
a low noise instrumentation amplifier with high gain capability.
16-Pin Wide Body SOL (S Suffix)
16
NC
15
RG
14
NC
13
V+
NC
12
OUT
11
REFERENCE
10
NC
9
2
RG
NC
1
NC
–IN
+IN
NC
V–
NC
1
2
3
SSM2017
4
TOP VIEW
TOP VIEW
(Not to Scale)
5
(Not to Scale)
6
7
8
NC = NO CONNECT
REV. C
Information furnished by Analog Devices is believed to be accurate and
reliable. However, no responsibility is assumed by Analog Devices for its
use, nor for any infringements of patents or other rights of third parties
which may result from its use. No license is granted by implication or
otherwise under any patent or patent rights of Analog Devices.
*θJA is specified for worst case mounting conditions, i.e., θJA is specified for device
in socket for cerdip and plastic DIP; θJA is specified for device soldered to printed
circuit board for SOL package.
JA
= 134; θJC = 12 . . . . . . °C/W
JA
= 96; θJC = 37 . . . . . . . . . . °C/W
JA
= 92; θJC = 27 . . . . . . . . . . . . . °C/W
Figure 2. Typical THD+ Noise * at G = 2, 10, 100, 1000;
= 10 V rms, VS = ±18 V, RL = 5 kΩ; TA = +25°C
V
O
ORDERING GUIDE
ModelRange*DescriptionOption
SSM2017P–40°C to +85°C8-Pin Plastic DIPN-8
SSM2017S–40°C to +85°C16-Lead SOLR-16
SSM2017S-REEL–40°C to +85°C16-Lead SOLR-16
*XIND = –40°C to +85°C.
TemperaturePackagePackage
CAUTION
ESD (electrostatic discharge) sensitive device. Electrostatic charges as high as 4000 V readily
accumulate on the human body and test equipment and can discharge without detection.
Although the SSM2017 features proprietary ESD protection circuitry, permanent damage may
occur on devices subjected to high energy electrostatic discharges. Therefore, proper ESD
precautions are recommended to avoid performance degradation or loss of functionality.
REV. C
–3–
SSM2017
Figure 3. Voltage Noise Density vs.
Frequency
Figure 6. Maximum Output Swing
vs. Frequency
Figure 4. RTI Voltage Noise Density
vs. Gain
Figure 7. Maximum Output Voltage
vs. Load Resistance
Figure 5. Output Impedance vs.
Frequency
Figure 8. Input Voltage Range vs.
Supply Voltage
Figure 9. Output Voltage Range vs.
Supply Voltage
Figure 10. CMRR vs. Frequency
–4–
Figure 11. +PSRR vs. Frequency
REV. C
SSM2017
Figure 12. –PSRR vs. Frequency
Figure 15. V
vs. Temperature
OOS
Figure 13. V
Figure 16. V
vs. Temperature
IOS
vs. Supply Voltage
OOS
Figure 14. V
vs. Supply Voltage
IOS
Figure 17. IB vs. Temperature
Figure 18. IB vs. Supply Voltage
REV. C
Figure 19. ISY vs. Temperature
–5–
Figure 20. ISY vs. Supply Voltage
SSM2017
G =
(+In) – (In)
V
OUT
=
10kV
+1
R
G
Basic Circuit Connections
GAIN
The SSM2017 only requires a single external resistor to set the
voltage gain. The voltage gain, G, is:
10kΩ
G =
+1
R
G
and
10kΩ
RG =
G–1
For convenience, Table I lists various values of RG for common
gain levels.
Table I. Values of RG for Various Gain Levels
A
V
dBR
G
10NC
3.2104.7k
10201.1k
31.330330
10040100
3145032
10006010
The voltage gain can range from 1 to 3500. A gain set resistor is
not required for unity gain applications. Metal-film or wirewound resistors are recommended for best results.
The total gain accuracy of the SSM2017 is determined by the
tolerance of the external gain set resistor, R
, combined with the
G
gain equation accuracy of the SSM2017. Total gain drift combines the mismatch of the external gain set resistor drift with
that of the internal resistors (20 ppm/°C typ).
Bandwidth of the SSM2017 is relatively independent of gain as
shown in Figure 21. For a voltage gain of 1000, the SSM2017
has a small-signal bandwidth of 200 kHz. At unity gain, the
bandwidth of the SSM2017 exceeds 4 MHz.
Figure 21. Bandwidth of the SSM2017 for Various Values
of Gain
NOISE PERFORMANCE
The SSM2017 is a very low noise audio preamplifier exhibiting
a typical voltage noise density of only 1 nV/√
Hz at 1 kHz. The
exceptionally low noise characteristics of the SSM2017 are in
part achieved by operating the input transistors at high collector
currents since the voltage noise is inversely proportional to the
square root of the collector current. Current noise, however, is
directly proportional to the square root of the collector current.
As a result, the outstanding voltage noise performance of the
SSM2017 is obtained at the expense of current noise performance. At low preamplifier gains, the effect of the SSM2017’s
voltage and current noise is insignificant.
The total noise of an audio preamplifier channel can be calculate by:
En =
2
e
n
+(inRS)2+e
2
t
where:
= total input referred noise
E
n
= amplifier voltage noise
e
n
= amplifier current noise
i
n
= source resistance
R
S
= source resistance thermal noise.
e
t
For a microphone preamplifier, using a typical microphone impedance of 150 Ω the total input referred noise is:
e
= 1 nV/√Hz @ 1 kHz, SSM2017 e
n
in = 2 pA/√Hz @ 1 kHz, SSM2017 i
n
n
RS = 150 Ω, microphone source impedance
= 1.6 nV/√Hz @ 1 kHz, microphone thermal noise
e
t
=
√
(1 nV√Hz)2 + 2 (pA/√Hz× 150 Ω)2 + (1.6 nV/√Hz)
E
n
2
= 1.93 nV/√Hz @ 1 kHz.
This total noise is extremely low and makes the SSM2017
virtually transparent to the user.
–6–
REV. C
SSM2017
INPUTS
The SSM2017 has protection diodes across the base emitter
junctions of the input transistors. These prevent accidental avalanche breakdown, which could seriously degrade noise performance. Additional clamp diodes are also provided to prevent the
inputs from being forced too far beyond the supplies.
a. Single Ended
b. Pseudo Differential
Although the SSM2017’s inputs are fully floating, care must be
exercised to ensure that both inputs have a dc bias connection
capable of maintaining them within the input common-mode
range. The usual method of achieving this is to ground one side
of the transducer as in Figure 22a, but an alternative way is to
float the transducer and use two resistors to set the bias point as
in Figure 22b. The value of these resistors can be up to 10 kΩ,
but they should be kept as small as possible to limit commonmode pickup. Noise contribution by resistors themselves is negligible since it is attenuated by the transducer’s impedance. Balanced transducers give the best noise immunity and interface
directly as in Figure 22c.
REFERENCE TERMINAL
The output signal is specified with respect to the reference terminal, which is normally connected to analog ground. The reference may also be used for offset correction or level shifting. A
reference source resistance will reduce the common-mode rejection by the ratio of 5 kΩ/R
. If the reference source resis-
REF
tance is 1 Ω, then the CMR will be reduced to 74 dB (5 kΩ/1 Ω
= 74 dB).
COMMON-MODE REJECTION
Ideally, a microphone preamplifier responds only to the difference between the two input signals and rejects common-mode
voltages and noise. In practice, there is a small change in output
voltage when both inputs experience the same common-mode
voltage change; the ratio of these voltages is called the commonmode gain. Common-mode rejection (CMR) is the logarithm of
the ratio of differential-mode gain to common-mode gain,
expressed in dB.
c. True Differential
Figure 22. Three Ways of Interfacing Transducers for High
Noise Immunity
Figure 23. SSM2017 in Phantom Powered Microphone Circuit
PHANTOM POWERING
A typical phantom microphone powering circuit is shown in
Figure 23. Z
through Z4 provide transient overvoltage protec-
1
tion for the SSM2017 whenever microphones are plugged in or
unplugged.
REV. C
–7–
SSM2017
BUS SUMMING AMPLIFIER
In addition to is use as a microphone preamplifier, the SSM2017
can be used as a very low noise summing amplifier. Such a circuit is particularly useful when many medium impedance outputs are summed together to produce a high effective noise gain.
The principle of the summing amplifier is to ground the SSM2017
inputs. Under these conditions, Pins 1 and 8 are ac virtual
grounds sitting about 0.55 V below ground.
To remove the 0.55 V offset, the circuit of Figure 24 is
recommended.
A
forms a “servo” amplifier feeding the SSM2017’s inputs.
2
This places Pins l and 8 at a true dc virtual ground. R4 in conjunction with C2 remove the voltage noise of A
about any operational amplifier will work well here since it is removed from the signal path. If the dc offset at Pins l and 8 is not
too critical, then the servo loop can be replaced by the diode biasing scheme of Figure 24. If ac coupling is used throughout,
then Pins 2 and 3 may be directly grounded.
, and in fact just
2
OUTLINE DIMENSIONS
Dimensions shown in inches and (mm).
C1534–24–4/91
Figure 24. Bus Summing Amplifier
8-Pin Plastic DIP (P) Package
8-Pin Hermetic DIP (Z) Package
16-Pin SOIC (S) Package
–8–
PRINTED IN U.S.A.
REV. C
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