
Keywords: low noise amplifiers, straingauge, bipolar, CMOS, JFET, noise density


Choosing a LowNoise Amplifier

Abstract: This article examines key parameters that contribute to amplifier noise. It explains how amplifier design, specifically the choice of bipolar, JFETinput, or CMOSinput design, affects noise. The note also explains how to select a lownoise amplifier for lowfrequency analog applications such as buffering data converters, amplifying straingauge signals, and preamplifying microphone outputs. The CMOSinput based amplifier, MAX4475, illustrates the benefits of using this newer amplifier design for many lower frequency analog applications.
A discussion of lownoise amplifiers usually implies RF/wireless applications. But noise is also a critical consideration for lower frequency analog applications like buffering data converters, amplifying straingauge signals, and preamplifying microphone outputs. To select an appropriate amplifier, an engineer must first understand the noise parameters for a particular application and then determine whether an amplifier is indeed lownoise. Additionally, it is imperative that the designer understand how the type of IC—bipolar, JFETinput, or CMOSinput—affects noise parameters.
Noise Parameters
Although many parameters specify an amplifier's noise performance, the two most important factors are voltage noise and current noise. Voltage noise is the voltage fluctuations at the input of an otherwise noisefree amplifier with shorted inputs. Current noise is the current fluctuations at the input of an otherwise noisefree amplifier with open inputs.
The typical figure of merit for amplifier noise is noise density, also called spot noise. Voltagenoise density is specified in nV/
, while currentnoise density is usually shown in units of pA/
. These values are provided in all lownoise amplifier data sheets, and are usually specified at two frequencies: at less than 200Hz for the flickernoise component, and at 1kHz for the flatband component. For simplicity, these measurements are referred to the amplifier inputs to remove the need to account for the amplifier's gain.
Figure 1 shows a typical curve for voltagenoise density vs. frequency. The noise curve is dependent on two main noise components: flicker noise and shot noise. Flicker noise, the random noise intrinsic to all linear devices, is known as 1/f noise. Its amplitude is inversely proportional to frequency. Flicker noise is usually the dominant noise source at frequencies less than 200Hz, as shown in Figure 1. The 1/f corner frequency is the frequency above which the noise amplitude is approximately flat and independent of frequency. Shot noise, the white noise caused by current fluctuations across a forwardbiased pnjunction, is present in this frequency range. Note that the 1/f corner frequency for the voltage noise may be different from the 1/f corner frequency for the current noise.
Figure 1. A typical curve for voltagenoise density vs. frequency is dependent on two main noise components: flicker noise and shot noise. Flicker noise, or 1/f noise, is inversely proportional to frequency and is usually the dominant noise source at frequencies less than 200Hz.
An amplifier circuit's total noise depends on the amplifier itself, external circuit impedance, gain, circuit bandwidth, and ambient temperature. The thermal noise from the circuit's external resistors is also part of the total noise calculation.
Figure 2 shows an example of an amplifier and its associated noise components.
Figure 2. The amplifier circuit's source impedance determines the primary noise term. As source impedance increases, current noise dominates.
Calculating Total Noise
The standard expression for an op amp's total inputreferred noise at a given frequency is:
where:
R
_{n} = Inverting input effective series resistance
R
_{p} = Noninverting input effective series resistance
e
_{n} = Input voltagenoise density at the frequency of interest
i
_{n} = Input currentnoise density at the frequency of interest
T = Ambient temperature in Kelvin (°K)
k = 1.38 x 10
^{23} J/°K (Boltzman's constant).
Equation 1 is the noise at a given frequency as a function of bandwidth. To calculate the total noise, multiply et, which is in nV/
, by the square root of the bandwidth of interest. For example, if the amplifier circuit's bandwidth ranges from 100Hz to 1kHz, the following expression gives the total noise over the bandwidth:
The above example shows how to calculate the total noise when the voltage noise and current noise do not vary over the bandwidth. (This usually occurs when the lower end of the amplifier circuit's bandwidth is above the op amp's 1/f frequency for both the voltage and the current noise.) If the voltage noise and current noise do vary over the bandwidth, then the totalnoise calculation is more involved.
Based on Equation 1 and Figure 2, it is easy to see the impact of the circuit's source impedance on the noise contributions. Voltage noise is the primary noise contributor in low sourceimpedance systems. As the equivalent source impedance increases, resistor noise becomes the dominant term, eventually making the amplifier's voltagenoise contribution negligible. As the source impedance increases further, current noise dominates.
The Effect of Amplifier Design on Noise Performance
Noise performance is a function of the amplifier design. The three common designs for lownoise amplifiers are bipolar, JFETinput, and CMOSinput. While each design can provide lownoise performance, their performances are not equal.
Bipolar Amplifiers
Bipolar amplifiers have traditionally been the most common lownoise amplifiers. Lownoise bipolar amplifiers such as the MAX410 offer very lowinput voltagenoise density (1.8nV/
) with a relatively highinput currentnoise density (1.2pA/
). Unitygain bandwidths are typically less than 30MHz for these amplifiers.
To ensure low voltage noise from a bipolar op amp, IC designers set up high collector currents in the input stage. This is because voltage noise is inversely proportional to the square root of the inputstage collector current. Opamp current noise is, however, proportional to the square root of the inputstage collector current. Therefore, the external feedback and source resistance must be minimized to achieve good noise performance. Note that the inputbias current is proportional to the inputstage collector current. It may thus be necessary to minimize the source resistance to minimize the offset voltage from bias current.
A bipolar amplifier's voltage noise usually dominates when its equivalent source resistance is less than 200Ω. Large inputbias current, coupled with relatively large current noise, make bipolar amplifiers best suited for only low sourceimpedance applications.
JFETInput Amplifiers
The best JFETinput lownoise amplifiers feature ultralow inputcurrentnoise density (0.5fA/
), but a higher input voltagenoise density (greater than 10nV/
) compared to bipolar designs. JFET designs allow singlesupply operation. Input bias currents of 1pA make JFET amps useful for applications with highimpedance sources. However, JFETbased designs are not the board designer's first choice for low sourceimpedance applications, due to their larger voltage noise.
CMOSInput Amplifiers
Newer lownoise amplifier designs with a CMOS input stage offer voltagenoise performance that is comparable to bipolar designs. CMOSinput amplifiers also meet or exceed the currentnoise performance of the best JFETinput designs. The
MAX4475, for example, has lowinput voltagenoise density (4.5nV/
), lowinput currentnoise density (0.5fA/
), and ultralow distortion (0.0002% THD+N) while operated from a single supply. These features make CMOSinput amplifiers an excellent choice for applications that require low distortion and low noise, such as audio preamplifiers. Additionally, the CMOS input stage allows for very low inputbias currents, low offset voltages, and very high input impedances, making these devices well suited for signal conditioning highimpedance sources, such as the photodiode preamplifier circuit shown in
Figure 3. An output buffer for a 16bit DAC output is shown in
Figure 4.
Figure 3. Lownoise amplifiers with a CMOS input stage have very lowinput bias currents and offset voltages coupled with very high input impedances. These devices are well suited for signal conditioning highimpedance sources, such as a photodiode preamplifier.
Figure 4. Lownoise performance and lowinput bias currents make CMOSinput amplifiers an ideal choice to buffer a 16bit DAC output.
Conclusion
No single amplifier is always the best choice for all applications.
Table 1 summarizes typical noise parameters for the three common amplifier designs.
Table 1. Typical Noise Specifications for Amplifier Designs
INPUT STAGE 
VOLTAGE NOISE 
CURRENT NOISE 
INPUT BIAS CURRENT 
OVERALL PERFORMANCE 
Bipolar¹ 
1.8nV/ 
1.2pA/ 
80nA 
Good 
JFET 
>10nV/ 
0.5fA/ 
>1pA 
Better 
CMOS^{2} 
4.5nV/ 
0.5fA/ 
1pA 
Best 
1. Data from the MAX410.
2. Data from the MAX4475.
Considering all sources of noise, the latest amplifiers with a CMOSinput stage, such as the MAX4475, offer the best compromise of noise performance for lower frequency analog applications and for almost any frontend application, especially highsourceimpedance, wide bandwidth circuits.
A similar version of this article appeared in the August 2004 edition of
Electronic Products.
© Nov 04, 2005, Maxim Integrated Products, Inc.

The content on this webpage is protected by copyright laws of the United States and of foreign countries. For requests to copy this content, contact us.
APP 3642: Nov 04, 2005
APPLICATION NOTE 3642,
AN3642,
AN 3642,
APP3642,
Appnote3642,
Appnote 3642
