关键词: Linearization of Wheatstone Bridge, bridge circuits, RTD, temperature detection, temperature monitoring, analog front end for temperature sensing, Precision amplifier, Precision voltage reference, MAX44267, MAX6025, industrial, medical
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How to Linearize WheatstoneBridge Circuit for Better Performance

Wheatstone bridge circuits measure an unknown electrical resistance by balancing two legs—one with the unknown component—of a bridge circuit. These longestablished circuits are among the first choices for frontend sensors. Whether the bridges are symmetric or asymmetric, balanced or unbalanced, they allow you to accurately measure an unknown impedance. Since bridge circuit are so simple yet effective, they’re very useful for monitoring temperature, mass, pressure, humidity, light, and other analog properties in industrial and medical applications.
The Wheatstone bridge has a single impedancevariable element that, when away from the balance point, is inherently nonlinear. Bridge circuits are commonly used to detect the temperature of a boiler, chamber, or a process situated hundreds of feet away from the actual circuit. Usually a sensor element, typically a resistance temperature detector (RTD), thermistor, or thermocouple, is situated in the hot/cold environment to provide information about resistance change to temperature.
In this application note we will take a look at its behavior and explain how you can linearize the bridge circuit to enhance performance. Note that when we speak generally about “bridges,” this piece is focused on circuit design for a Wheatstone bridge.
Using inexpensive, accurate discrete parts, resistancevariable Wheatstone bridge circuits perform most of the frontend tasks in a design. By incorporating an RTD element (and based on the RTD manufacturer), the bridge’s inherent resistance variations stay within the accepted linearity and tolerance limits.
RTD devices generally come with very detailed data sheets characterizing their behavior with lookup tables and even transfer function equations down to four or more orders of error compensating terms. For a highprecision system, desiginers have traditionally had to consider both the inherent nonlinearity of the RTD element and the Wheatstone bridge, and then painfully calibrate the frontend while linearizing the frontend at the microcontroller side. Linearity improves by increasing the order of the equation in the microcontroller. A typical bridge circuit (Figure 1) detects milliohms of changes in resistance (ΔR).
Figure 1. A typical bridge with nodes A and B sensing output voltage from a change in resistance (ΔR).
Assuming that R1 = R2 = R3 = R4 = R in Figure 1, the bridge is balanced with nodes A and B at a constant V/2 (volts) and with a differential voltage of 0V across V_{AB}. Should a change occur in resistance (ΔR) from R3, then the output differential voltage created is:
(Eq. 1) 
When R1 = R2 = R3 = R4 = R, the bridge is balanced.
For a single variableresistance element, for R3 = R + ΔR and R1 = R2 = R4 = R:
(Eq. 2) 
Equation 2 suggests that increasing the constant supply voltage, V, to the bridge will increase the output voltage, i.e., the swing range across the bridge. It’s important to note that this equation also suggests that having a dual supply across the fourlegged resistance arrangement could be useful not only to increase the range, but also to help maintain a 0V commonmode voltage across the AB nodes.
The voltage V_{AB} is usually amplified by using a subsequent amplifying stage via a differential amplifier. However, note that changing the commonmode voltage across V_{AB} increases error and complexity in the amplifying second stage, usually realized as a instrumentation quality differential amplifier. For this reason, it’s a good idea, and easier to manage, to have, a commonmode voltage centered around 0V.
In Figure 2, you can see the natural tendency of the bridge’s singlevariable element in the form of inherent nonlinearity in its transfer function.
Figure 2. V(AB) vs. the change in ΔR, the effect of the bridge’s nonlinearity from 800Ω of resistance change. For comparison, a trend line is included here.
In Figure 2, take a closer look at the trend line. The linearity error, or the curve’s absolute deviation from an ideal straight line, is about 0.62%. This percentage is generated by comparing the curved trend line with the line of best fit, i.e., the straight line relative to the curve. This approach quantifies the worstcase linearity error for the above curved line. In some cases, a 0.6% linear is certainly not acceptable. In this application note, we’ll examine a method to achieve better than 0.1% accuracy.
Aside from addressing the bridge’s inherent nonlinearity, you must also manage the nonlinearity of the temperature sensor element, RTD, or even thermistor as discussed previously. The instrumentation amplifier (Figure 3) has a commonmode voltage of V/2 when sensing the differential voltage across the nodes A and B. The amplifier is usually either a differential amplifier with four resistors or a threeopamp instrumentation amplifier integrated in a single package.
Figure 3. An instrumentation amplifier, connected to the original bridge circuit in Figure 1.
When a differential amplifier is used, the nodes A and B are connected to the amplifier’s input gainsetting resistors, as shown in Figure 3. The choice of the op amp and the input resistors is signficant as this path directs current away from the bridge, which impacts accuracy.
Also, the type of resistors you use affects the bridge performance. For instance, even 0.1%tolerant resistors used with the amplifier provide only 60dB of commonmode rejection.
Based on our earlier discussion, having dual supplies across the resistor bridge to increase the dynamic range seems a logical approach. It would also make sense to have the sensing nodes centered around the 0V common mode. In such a design, the transfer function from the node B will be linear with a change in resistance. Compared to the output from the circuit in Figure 1, the range of the output swing from the bridge would be doubled.
In Figure 4, we see a circuit implementation with two op amps in place of a more complex instrumentation amplifier. With this design approach, the linearized bridge output avoids the unnecessary current paths created by the differential amplifier. This presents an easier design process versus the circuit in Figure 3. However, there are positive and negative supplies to the amplifiers, providing twice the swing range. Better commonmode rejection performance is an added advantage, as the second amplifier operates comfortably around 0V.
Figure 4. In this circuit, two op amps replace the complex instrumentation amplifier (Figure 3)
From Figure 4, node A sees GND as it is the summing node of amplifier 1. Thus, a constant current of is forced through the R1R3 branch, producing an equal and opposite voltage on the other side of the bridge with V. When the single variableresistance R3 changes (from R3 to R ±ΔR), then Ix (the change in current due to change in the resistance) flowing through this resistance produces a voltage V ±ΔV. A factor of this ΔV is manifested across node B by the balancing of the resistance bridge (for a balanced bridge, of course), as the current forced through resistor branch R2R4 is equal to (V+  (V + ΔV))/(R3 + R4). Since node B is centered at 0V common mode, the voltage produced across node B is going to be gained by a noninverting amplifier. Furthermore, filtering can be done on this gain stage to optimize the bandwidth in order to produce an acceptable noise level for the application.
At balance, when R1 = R2 = R3 = R4 = R, the voltage at nodes A and B is:
When a single variableresistive element (R3) changes by ΔR (R3 + ΔR):
1 × x(R3 + ΔR) = (V) + (1 × x(ΔR))
Since node A is at ground, the voltage at node B is:
We know that term is = 0. Hence the voltage at node B is
And in a balanced bridge:
The same equation can be written as:
When using a balanced bridge with ratio , and we know that ΔV = Ix × ΔR and , then the equation becomes:
(Eq. 3) 
And simplistically putting R1 = R2 = R3 = R4 = R, then:
At the output of the noninverting op amp, the equation then is:
(Eq. 4) 
This suggests that the output from the second op amp is inverting in nature.
Figure 5 shows the transfer function and its nonlinearity from the Figure 4 implementation.
Figure 5. Bridge output vs. change in resistance. Data are based on the design in Figure 4.
In Figure 5, the linearity error, the absolute deviation from an ideal straight line, is less than 0.02%. When there’s improvement in absolute nonlinearity, there will also be improvement in the fullscale error (relative error).
Since there aren’t interacting resistive branches, you don’t have to apply precision matching of resistors. Rx and Rg variation will only yield a gain error, which can be calibrated at the same as the RTD device.
Based on the above data, it appears that this approach can be viable for 12, 14, 16, and even 18bit applications. It’s a simple design and requires very little calibration by the microcontroller. As noted earlier, this circuit is well established and has been widely used in the field for many years.
A dualsupply voltage for the frontend is needed to implement the circuit in Figure 4. This negative supply also requires additional board space and components; however, this may not be a viable option if this is the only place in the entire system where the negative supply is needed. A highprecision bridge sensor also needs lowoffset voltage, lowoffset drift, and lownoise performance.
Consider this scenario: a single power supply for the amplifier used in Figure 4. As an example, let’s take a look at Maxim’s MAX44267, which operates from a single supply and can output bipolar voltages. Unlike other singlesupply amplifiers requiring headroom above ground, the MAX44267 provides a truezero output, which makes it ideal for bridge sensors (Figure 6). The MAX44267 integrates chargepump circuitry that generates the negative voltage rail in conjunction with external capacitors. The amplifier can then operate from a single +4.5V to +15V power supply, while remaining as effective as a normal dualrail ±4.5V to ±15V amplifier.
Figure 6. . From a single supply, the MAX44267 precision, lownoise, lowdrift, dual op amp provides a truezero output.
In the Figure 6 circuit, you can implement the MAX44267 with a single supply voltage (positive supply, V_{CC}). The integrated negative V_{SS} generator or charge pump generates a negative supply voltage. One of the advantages of this architecture is that it eliminates the need for negative supply regulators while also reducing board layout space and cost.
Figure 7 includes the MAX6070_A25 voltage reference to generate a 2.5V_{OUT} reference. A dual op amp (again, the MAX44267) is used with the resistance bridge where R1 = R3 = 1kΩ and R2 = R4 = 10kΩ. . To reduce the amount of current flowing through the bridge along with the power dissipation, an additional 1.8kΩ is used in series. At a balanced condition, the V(+) node becomes onethird the voltage reference’s output. This is followed with secondstage amplification with a gain of 11 at the OUTA node.
Figure 7. The MAX44267 op amp operates from a single supply.
In our examination, R3 was replaced by a Fluke^{®} RTD calibrator, which served as the temperaturedependent resistance element (as PT1000) to evaluate a temperaturedependent change from 50°C to +155°C. For the given temperature change using a PT1000, the change in resistance (±R) is about 800Ω and an equivalent range of 325mV is effected (see Equation 4). Amplifier 2, since it boasts an internal negative supply, can accommodate this swing (242mV to 83mV) at its input below ground, while providing an output gain of 11.
FIn the second stage of Figure 7, a SallenKey filter filters the input signal to the required bandwidth (in this instance, 50Hz). Without calibration or trim, we’re able to achieve fullscale error accuracy within ±0.05% is obtained from the bridge output at node B. This approach renders the transfer function of the bridge circuit linear. Using the MAX44267 results in improved frontend circuit performance.
Figure 8. The transfer curve shows the absolute voltage output vs. temperature for the Figure 7 circuit.
Figure 9. Error % vs. full scale for the circuit in Figure 7.
Figure 10. Output noise density vs. frequency for the circuit in Figure 7.
Figure 11. Peaktopeak voltage noise from 0.1Hz to 10Hz for the circuit in Figure 7.
A similar version of this application note appeared in Electronics 360 on June 23, 2015.
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© Sep 02, 2016, Maxim Integrated Products, Inc. 
APP 6144: Sep 02, 2016
应用笔记6144, AN6144, AN 6144, APP6144, Appnote6144, Appnote 6144 