
In part 1 of this series, we looked at ways to simplify resistor networks by identifying series and parallel combinations of resistors. We closed with a look at a version of the Wheatstone bridge, such as the one in Figure 1. Although it has only five resistors, not one of them is in series or parallel with another, so the simple equations we used in part 1 won’t work here. There is a workaround, called a delta-to-wye conversion.[1] But that just gives you three more equations to memorize, and unless you do the conversion often (if you work with three-phase power, for example), those equations aren’t likely to become second nature, the way the series and parallel resistor equations are for most electrical engineers.

Q: Wait, what about the version of the Wheatstone bridge with a galvanometer taking the place of R5?
A: That version, shown in Figure 2, is easier to analyze. Here, R3 becomes a variable resistor RV, and R4 becomes an unknown resistor RX, whose value we are trying to find.
In the classic Wheatstone bridge application, we manually adjust RV until the galvanometer or multimeter voltage VG is 0, at which point we have what we call a balanced bridge. It consists of two simple voltage dividers, and R5 from Figure 1 is essentially infinite. R1 and RV make up the first divider, and the voltage across RV is:
R2 and RX make up the second divider, and the voltage across RX is:
Since the galvanometer reads zero, we can determine RX as follows:
Q: What’s the drawback to this balanced bridge?
A: If we are trying to measure a parameter such as strain in real time, it’s not practical to manually adjust Rv until VG is zero, then record the value of RV, and calculate RX. We could probably kludge together something based on a voltage-controlled or digitally controlled resistor to replace the manual adjustment, but Kirchhoff’s and Ohm’s laws offer a simpler way for us to derive RX from the voltages and currents in a fixed-resistor bridge.

Q: How does that work?
A: Let’s go back to our original Figure 1 bridge with five fixed resistors. In Figure 3, I’ve rearranged Figure 1 to make more room for notations showing branch (red arrows) and loop (blue arrows) currents. Kirchhoff gives us two laws that we can apply to solving such a problem. The current law states that the net sum of currents into any node is 0. In Figure 3, for example, that law implies the following:
The second law, Kirchhoff’s voltage law, states that the voltage drops around any closed loop must equal zero. For the loop on the left of Figure 3, this law results in the following equation:
For a given circuit, each law will give us multiple equations on multiple unknowns. Which law or combination of the two laws is easiest for us to use will depend on exactly what we are trying to determine. In our case, we have two goals. First, following up on our work from part 1, what is the equivalent impedance of the bridge if all resistors are fixed and we know their individual values? In other words, what is VIN/IIN? And second, of particular interest from a test-and measurement-perspective, is this question: If R1, R2, R3, and R5 are fixed and known and R4 is unknown (it might be a strain-gauge element or temperature sensor, for instance), can we calculate R4 based on the voltage VV – VX across R5? We’ll take a closer look next time.
References
[1] Delta-to-Wye Equivalent Circuits, Utah State University.
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