In: Mechanical Engineering
In load measurement applications, strain gauge load cells are a popular choice. Strain gauge type load cells are cost-effective, accurate and highly configurable. This explains the underlying technology behind these versatile devices.
What is a Strain Gauge?
A strain gauge is an electrical component whose resistance changes when it undergoes a mechanical strain from an applied force.
A bonded strain gauge consists of a thin wire etched in a back-and-forth pattern onto a non-conductive substrate material with connectors at each end of the wire (Figure 1). The length of wire is the total length of all the loops; the end loops (labeled) are wider to make negligible any difference in resistance from the same length of straight wire. Additionally, note the alignment marks indicating the direction of a normal strain and an orthogonal one. These are the arrowhead marks on the top and bottom (normal strain) and sides (orthogonal).
From a circuit standpoint, the wire acts as a resistor. The resistance is a function of the elastic properties of the wire. When the wire is stretched, its length increases, its cross section decreases and therefore its resistance goes up. When the wire is compressed, the opposite occurs. An analogy of this is flexible tubing. When stretched, it lengthens and narrows in cross section which restricts the fluid flow compared to the original tube.
The ratio of the wire’s change in length divided by the wire’s original length is known as its mechanical strain. It is expressed as the equation:
where
is the conventional symbol for strain,
L is the change in length of the wire and L is the original length
of the wire.
The relationship between the change in resistance of the strain
gauge, and the strain in the etched wire due to an applied load, is
approximately linear within the elastic limit of the wire. This
relationship is expressed as a ratio known as the gauge factor (G
).
OR
This linear relationship is the key to the strain gauge’s operation. The applied load creates a strain which in turn alters the resistance. Consequently, a voltage drop through the strain gauge will change depending on whether the gauge experiences a load or not. This change in voltage due to a change in applied strain produces a corresponding change in the strain gauge load cell’s output voltage.
Unbonded strain gauges also exist but the bonded type are most common and therefore this article focuses on the latter.
Strain Gauge Load Cell Circuitry
Strain gauges have load limits. The strain on the wire cannot exceed the point where the metal will no longer return to its original length but instead permanently deforms. For most metals, this change is very small. For example, for steel the elastic limit occurs at a strain of 0.001 mm/mm.
The gauge factor tells us the resistance change in a metal is proportional to the strain. For most metals, the gauge factor is around the order of 2. This means for a strain gauge of 100 ohms unloaded, assuming the strain at the elastic limit is 0.001, the maximum change in resistance possible within the elastic limit is about 0.2 ohms.
Obviously this resistance change is very small. In fact, if a simple ohm-meter were to measure it, the change in resistance in the strain gauge would be so small that it would fall within the percent error of the meter, and therefore would be imperceptible. To accurately measure this resistance change, a strain gauge load cell employs a simple circuit known as a Wheatstone Bridge.
The Wheatstone Bridge
A Wheatstone bridge is simply two voltage dividers wired in parallel arms of a circuit with a common voltage source. Figure 2 shows a representation of this circuit.
The input voltage, Vex , is the excitation voltage. The variable resistor at represents the strain gauge. R,R1,R2,R3 have equal resistances and ^R has a value of zero under no load. Therefore when the strain gauge bears no load, the voltages at the nodes V0- and V0+ are equivalent. This means the output of the bridge circuit, which is the voltage difference across these two
es, is zero volts.
What happens when a force or load is applied and delta R is non-zero? Let’s look at the general equation for the voltage at each output node. Recall ohm’s law states that the voltage between two nodes in a series circuit is equal to the current through it multiplied by the total resistance in that path, or more commonly seen as V=IR . Rearranging, I=V/R , the current on the left half of the bridge circuit in Figure 2 is then equal to Vex/(R1+R2) . The two resistors along this path divide the excitation voltage at V0- . Substituting our expression for current in the left path for I in the ohm’s law equation, this voltage at the V0- node is:
Similarly, the voltage at the node is:
The total output voltage is simply the difference between these two:
V0=(V0+) - (VO-)
The reason this setup improves accuracy is that now the voltage
drop across the strain gauge is being compared to the voltage drop
across a similar resistance for the same excitation voltage,
instead of being compared to the much larger excitation voltage
itself. That means the change in voltage across the strain gauge
will be the same order of magnitude as the comparison voltage; any
error in output voltage will be a fraction of this. Also, any
changes in strain due to temperature or other environmental factors
will affect all of the resistors in the circuit equally. This
becomes important in mitigating the effect of these environmental
factors on the output.
The Quarter, Half, and Full-Bridge Configurations
All Wheatstone bridges have four resistive elements. However in load cell design, the number of those elements that are strain gauges vs non-variable resistors is flexible. If only one of the resistive elements in the bridge is a strain gauge, it is a quarter bridge. If two are strain gauges, it is a half bridge. And in the case where all four resistive elements are strain gauges, the Wheatstone bridge is a full bridge. See Figures 3-5 below
The pros and cons of each bridge configuration motivate the choice for a particular application. In general, fewer gauges mean cheaper construction and easier installation. However, additional gauges increase bridge output, allow for temperature compensation, and cancel unwanted strain components.
To describe an example, one must know the property of the Wheatstone Bridge that strains on adjacent positions in the bridge cancel, while strains on opposite bridge arms sum. Now let’s assume that we want to cancel a bending strain in a loaded beam and just measure any tensile strain. This can be achieved by bonding a strain gauge to both the top and the bottom (vertically aligned) of the beam in a half bridge configuration with the gauges on opposite bridge arms. The strain measured at the top gauge will have the load strain plus tensile strain due to bending; the bottom gauge will have a compressive bending component similar in magnitude but opposite to the tensile component at the top. The bridge output will be the sum of the common strain components but the opposite strains will cancel to 0V.
Likewise, strain components due to temperature add equally to all gauges in a bridge configuration; therefore, by placing a non-loaded gauge in a position adjacent to a load-bearing one, the strain components due to temperature will cancel. In addition, bonding gauges at angles to each other on a measuring device can account for additional (non-axial) strain components and determine the angle of maximum strain. This configuration of strain gauges is called a strain gauge rosette.
Conclusion
This article introduces the underlying principles of a strain gauge, the main component in Tacuna Systems’ load cell product line. Strain gauges have many advantages in load cell construction. These include low cost, high accuracy (especially due to the wide variety of bridge configurations and bonding geometries) and durability. Because they can be built into a wide array of supporting structures and can handle a broad range of loads, strain gauge type load cells are practical for many applications. They are truly versatile.
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