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Bridge circuit
Bridge circuit
from Wikipedia

A bridge circuit is a topology of electrical circuitry in which two circuit branches (usually in parallel with each other) are "bridged" by a third branch connected between the first two branches at some intermediate point along them. The bridge was originally developed for laboratory measurement purposes and one of the intermediate bridging points is often adjustable when so used. Bridge circuits now find many applications, both linear and non-linear, including in instrumentation, filtering and power conversion.[1][2]

The best-known bridge circuit, the Wheatstone bridge, was invented by Samuel Hunter Christie and popularized by Charles Wheatstone, and is used for measuring resistance. It is constructed from four resistors, two of known values R1 and R3 (see diagram), one whose resistance is to be determined Rx, and one which is variable and calibrated R2. Two opposite vertices are connected to a source of electric current, such as a battery, and a galvanometer is connected across the other two vertices. The variable resistor is adjusted until the galvanometer reads zero. It is then known that the ratio between the variable resistor and its neighbour R1 is equal to the ratio between the unknown resistor and its neighbour R3, which enables the value of the unknown resistor to be calculated.

The Wheatstone bridge has also been generalised to measure impedance in AC circuits, and to measure resistance, inductance, capacitance, and dissipation factor separately. Variants are known as the Wien bridge, Maxwell bridge, and Heaviside bridge (used to measure the effect of mutual inductance).[3] All are based on the same principle, which is to compare the output of two potential dividers sharing a common source.

In power supply design, a bridge circuit or bridge rectifier is an arrangement of diodes or similar devices used to rectify an electric current, i.e. to convert it from an unknown or alternating polarity to a direct current of known polarity.

In some motor controllers, an H-bridge is used to control the direction the motor turns.

Bridge current equation

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bridge network current flow
Analysis of bridge current

From the figure to the right, the bridge current is represented as I5

Per Thévenin's theorem, finding the Thévenin equivalent circuit which is connected to the bridge load R5 and using the arbitrary current flow I5, we have:

Thevenin Source (Vth) is given by the formula:

and the Thevenin resistance (Rth):

Therefore, the current flow (I5) through the bridge is given by Ohm's law:

and the voltage (V5) across the load (R5) is given by the voltage divider formula:

See also

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References

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
A bridge circuit is an electrical arrangement consisting of two parallel branches connected by a bridging network, typically used to measure unknown electrical parameters such as resistance, , or by achieving a balance condition that nullifies the output voltage. This configuration, analogous to a mechanical balance scale, compares the outputs of two voltage dividers sharing a common excitation source, enabling precise differential measurements with minimal interference from supply variations or nonlinearities. The most foundational form, the , was first demonstrated by Hunter Christie in 1833 for DC resistance measurement and later popularized by in 1843, who adapted it for practical use in determining unknown resistances through ratio comparisons of four arms. Balance occurs when the ratio of resistances in one branch equals that in the other (e.g., R1/R2=R3/RxR_1 / R_2 = R_3 / R_x), yielding zero differential voltage across the detector, independent of the excitation voltage. This null-balance principle provides high accuracy, often up to ±0.05% with sensitive detectors, making it essential for calibration labs and instrumentation. Beyond resistance, bridge circuits extend to AC applications, including the for capacitance-inductance measurements (developed by Max Wien in 1891) and the for , each tailored to specific impedance parameters. They are integral in transducers like strain gauges (pioneered by in 1856) for sensing physical quantities such as , , and force, where small resistance changes produce measurable imbalances amplified for output. Additionally, bridge topologies underpin oscillators, such as the invented by William R. Hewlett in 1939, and switching circuits for across DC to GHz frequencies. Modern implementations often incorporate instrumentation amplifiers with high common-mode rejection (e.g., 120 dB) to enhance sensitivity and noise immunity in industrial and precision applications.

Introduction

Definition and Basic Concept

A bridge circuit is a fundamental electrical configuration designed for precise measurement of unknown electrical parameters, such as resistance in (DC) applications or impedance in (AC) setups, by employing a null detection method. This method involves comparing two circuit branches until equilibrium is reached, where the detector indicates zero output, enabling high-accuracy determinations without direct against absolute standards. Bridge circuits function as versatile tools in instrumentation, applicable to sensing physical quantities like strain or through associated transducers. In its basic form, a bridge circuit comprises four arms—typically labeled as resistors R1, R2, R3, and the unknown Rx—connected in a -shaped . An excitation is applied across one diagonal of the diamond (between the junctions of R1-Rx and R2-R3), while a detector, such as a for DC or a sensitive for AC, is placed across the opposite diagonal (between the junctions of R1-R2 and Rx-R3). This arrangement creates two parallel networks, with the output derived from the potential difference between the midpoints, allowing for the isolation and quantification of the unknown component when balance is achieved. The primary purpose of a bridge circuit is to measure unknown electrical components with exceptional precision by adjusting the circuit until the detector registers zero current or voltage, signifying balanced conditions across the arms. This null-balance approach minimizes errors from source variations and detector sensitivities, achieving accuracies on the order of 0.1% or better in well-designed setups. Over time, bridge circuits have evolved from traditional analog null methods relying on manual adjustments to modern digital variants that integrate analog-to-digital converters, microprocessors, and amplifiers for automated balancing and improved stability in complex measurement environments.

Historical Development

The Wheatstone bridge, a foundational bridge circuit, was originally invented by British scientist Samuel Hunter Christie in 1833 as a method for measuring unknown electrical resistances through a balanced network of resistors. Christie described the configuration in a paper presented to the Royal Society, though it received limited attention initially. In 1843, , a professor at , independently refined and popularized the design, demonstrating its practical utility in a lecture that led to widespread adoption; the circuit became eponymously known as the despite Christie's prior invention. During the 19th-century Industrial Revolution, bridge circuits like the Wheatstone found early applications in precision electrical measurements and telegraphy systems, enabling accurate assessment of wire resistances over long distances to improve signal transmission reliability. A key milestone came in 1861 when William Thomson (Lord Kelvin) developed the Kelvin double bridge, an extension designed specifically for measuring very low resistances by compensating for lead wire effects, which was essential for applications in electrical engineering and metrology. The transition to alternating current (AC) bridges began in the late 19th century, with James Clerk Maxwell introducing an inductance-capacitance bridge in 1873 to measure unknown inductances using AC signals, marking an important evolution for handling reactive components. In 1891, Max Wien devised the Wien bridge, adapted for precise frequency measurements in AC circuits, further expanding bridge techniques to audio and impedance analysis. Post-World War II advancements in the mid-20th century integrated bridge circuits with emerging electronics, particularly through amplifiers in the 1960s, which amplified small differential signals from unbalanced bridges for enhanced sensitivity in sensors and transducers. By the 1970s, the development of digital and bridges, featuring LED readouts and computerized balancing, revolutionized accuracy and speed, replacing manual null detection in laboratory and industrial settings. These innovations, driven by and technologies, solidified bridge circuits as core elements in modern .

Principles of Operation

Balanced and Unbalanced Conditions

In a bridge circuit, the balanced condition is achieved when the potential difference across the detector is zero, indicating that the of impedances in the opposing arms satisfies Z1/Z2=Z3/Z4Z_1 / Z_2 = Z_3 / Z_4. This equality ensures that the voltage dividers formed by the arms produce identical potentials at the detector points, regardless of the excitation source . Under unbalanced conditions, any mismatch in the arm impedances results in a non-zero voltage or current through the detector, with the magnitude proportional to the deviation in the unknown component's value. This output signal reflects the imbalance and serves as the basis for measuring changes in the circuit parameters. The provides a classic illustration of these states in DC applications. Achieving and maintaining balance can be influenced by several factors, including variations that alter component resistances—such as a 0.385% per °C change in wiring—leading to offset errors. Component tolerances introduce initial mismatches, potentially causing up to ±10% full-scale zero balance errors. In AC bridges, the excitation affects balance by modifying the reactive components of impedances, necessitating adjustments for magnitude and phase alignment. The null method exploits the balanced condition by iteratively adjusting one arm until the detector reading reaches zero, providing a precise independent of the excitation voltage level and minimizing errors from source fluctuations.

Sensitivity and Detection Methods

Sensitivity in bridge circuits is defined as the of the change in detector output (such as voltage or current) to a small change in the unknown component value, often normalized to the excitation voltage, with this reaching its maximum near the balanced condition where arm resistances are equal. This measure quantifies the circuit's ability to detect minute imbalances, typically expressed in mV/V, with values ranging from 1 mV/V to 10 mV/V in standard configurations. Traditional detection methods rely on null indicators to identify balance. For DC bridges, a galvanometer serves as the detector, measuring the small current flowing through the unbalanced bridge arms with high precision, enabling detection of zero current to confirm balance. In setups requiring voltage measurement, a voltmeter is employed across the detector points, though its input impedance must be high to avoid loading the circuit. Modern detection techniques enhance sensitivity through amplification and noise rejection. Operational amplifiers (op-amps), often configured as instrumentation amplifiers, provide high gain for amplifying the low-level unbalanced output voltage, achieving resolutions suitable for precision applications. In noisy environments, particularly with AC excitation, lock-in amplifiers employ phase-sensitive detection to isolate the bridge signal from noise, improving the by orders of magnitude. Several factors influence the overall sensitivity of bridge circuits. The ratios of the arm resistances play a critical role, as equal arm values near balance maximize the output response to perturbations in the unknown component. Source impedance affects performance by introducing bias currents that can unbalance the bridge or cause voltage drops, necessitating low-impedance sources for optimal results. Bridge resolution, determined by the minimum detectable imbalance, can reach 0.1% accuracy in precision setups through careful component selection and amplification. Despite these capabilities, limitations arise from practical implementations. Detector loading effects, such as those from finite op-amp , can alter the bridge balance and reduce measured sensitivity by introducing errors up to several percent. Additionally, stray capacitances in wiring or components couple noise and cause frequency-dependent imbalances, particularly in high-resolution AC bridges, requiring shielding and guarding techniques to mitigate.

Types of Bridge Circuits

DC Bridge Circuits

DC bridge circuits employ direct current (DC) excitation to measure resistances by arranging four resistors in a diamond-shaped network, with balance achieved when the voltage across the bridge's detector arm is zero, indicating equal potential division in the opposing branches. This configuration, often powered by a stable DC voltage source, relies on the null method where adjustments to one or more arms nullify the detector current, allowing precise resistance determination without direct current measurement through the unknown resistor. These circuits are particularly suitable for purely resistive networks, as DC excitation avoids phase shifts that arise from reactive elements like inductors or capacitors, ensuring accurate steady-state measurements focused solely on ohmic values. Common configurations feature series-parallel arm setups, exemplified by the , which enables straightforward DC balance for comparing resistances in the range of 5 Ω to 10 MΩ with accuracies exceeding 0.01%. Advantages of DC bridge circuits include their simplicity in and operation, utilizing basic components without the need for frequency-specific equipment, resulting in low cost and high stability for steady-state applications such as instrumentation where temperature compensation and signal augmentation enhance reliability. However, limitations arise when measuring components with or , as these introduce transient errors that prevent true DC balance, and in low-value resistance measurements, contact and lead resistances can significantly distort results unless mitigated by four-terminal techniques like the Kelvin configuration. A representative example is the use of DC bridges for basic resistance comparison in sensor applications, such as monitoring static strains via resistive elements, where the absence of frequency dependence ensures consistent performance independent of excitation variations.

AC Bridge Circuits

AC bridge circuits employ alternating current excitation, typically from sinusoidal voltage sources, to measure complex impedances involving resistance (R), inductance (L), and capacitance (C). This approach extends the utility of bridge configurations beyond purely resistive elements by accounting for both real and imaginary components of impedance, enabling precise determination of reactive parameters in components like inductors and capacitors. The balance condition in AC bridges requires that both the magnitude and phase of the voltages across the detector be nulled simultaneously, expressed in phasor form as Z1Z2=Z3Z4\frac{Z_1}{Z_2} = \frac{Z_3}{Z_4}, where Z1,Z2,Z3,Z4Z_1, Z_2, Z_3, Z_4 represent the complex impedances of the four arms. This equality ensures zero current through the detector, analogous to the resistive in DC bridges but incorporating phase alignment for reactive elements. Key advantages of AC bridges include their versatility in handling non-resistive components, allowing measurement of L and C alongside R, and the ability to tune the excitation for enhanced selectivity in distinguishing between similar impedances. Frequency adjustment can isolate specific reactive behaviors, improving accuracy in applications like component . Additionally, the bridge balance is independent of the source voltage magnitude, facilitating high-precision measurements with stable sinusoidal drives. Despite these benefits, AC bridges face challenges such as the skin effect, which increases effective resistance in inductors at higher frequencies by concentrating current near conductor surfaces, and dielectric losses in capacitors that introduce phase errors due to energy dissipation in insulating materials. Parasitic capacitances and inductances from wiring and environment can also disrupt balance, necessitating shielded enclosures and careful grounding techniques like the Wagner ground to minimize these effects. Typical operating frequencies for AC bridges range from the audio spectrum, often around 1 kHz for general-purpose measurements where detector sensitivity is optimal with or simple null indicators, to several MHz for high-frequency component testing using click-based detection or advanced . This tunability supports applications from low-speed setups to rapid, precise evaluations of RF elements.

Specific Bridge Configurations

Wheatstone Bridge

The Wheatstone bridge is a fundamental configuration in DC bridge circuits, specifically designed for precise measurement of medium-range electrical resistances. It consists of four resistors arranged in a diamond-shaped network, forming two parallel voltage dividers. The resistors are typically labeled as R1 and R2 in one arm, connected in series, and R3 and Rx (the unknown resistance) in the other arm, also in series. A DC voltage source, such as a battery, is applied across the top and bottom nodes (the junction between R1 and R3, and the junction between R2 and Rx), providing excitation to the circuit. A sensitive null detector, traditionally a galvanometer but often a high-impedance voltmeter in modern setups, is connected across the left and right nodes (the junction between R1 and R2, and the junction between R3 and Rx) to measure any differential voltage. The bridge operates on the principle of null balance, where the circuit is balanced when the indicates zero current or voltage, meaning the voltage drops across the two dividers are equal. This occurs when the ratio of the resistors satisfies the condition: R1R2=R3Rx\frac{R_1}{R_2} = \frac{R_3}{R_x} Solving for the unknown resistance gives Rx=R3R2R1R_x = R_3 \cdot \frac{R_2}{R_1}. In practice, R1 and R2 are fixed known resistors forming a ratio arm (often R1 = R2 for simplicity, making the ratio 1:1), while R3 is a variable , such as a decade box, adjusted during measurement. To measure Rx, the operator applies the excitation voltage, monitors the , and incrementally adjusts R3 until null deflection is achieved, at which point Rx is calculated directly from the known values without needing to measure currents or voltages during the balanced state. This null method provides high precision because it relies on the sensitivity of the detector rather than absolute measurements. The accuracy of the Wheatstone bridge can reach up to 0.01% when using precision decade resistance boxes for R1, R2, and R3, with tolerances better than 0.01% and stable temperature coefficients. However, several error sources can limit performance, including lead resistance, which adds unintended resistance in series with Rx and introduces systematic errors, particularly for values below 1 Ω where lead drops can exceed 0.1% of the total. Other errors arise from thermal effects on resistors, loading if not high-impedance, and at connections, though these are minimized by using four-wire techniques or guarding in advanced setups. Although the bridge is named after Sir , who popularized it through a public demonstration and paper in 1843, the original circuit was invented by Hunter Christie in 1833 as a method for measuring unknown resistances by balancing currents in a network of wires. Wheatstone acknowledged Christie's priority in his work, but the name persisted due to Wheatstone's improvements, such as incorporating a rheostat for finer adjustments.

Kelvin Double Bridge

The Kelvin double bridge is an advanced configuration of the bridge circuit specifically engineered for accurate of very low resistances, typically in the range below 1 , where conventional methods like the suffer from significant errors due to lead and contact resistances. This setup employs a approach for both the unknown resistance and the standard, ensuring that the potential leads carry negligible current and thus isolating the from extraneous resistances. In terms of configuration, the Kelvin double bridge features two interconnected Wheatstone bridges: a primary bridge with ratio arms R1R_1 and R2R_2, and an auxiliary bridge with smaller ratio arms r1r_1 and r2r_2, linked by a low-impedance network (often denoted as rlr_l) that connects the midpoints. The unknown low resistance RxR_x and a standard RsR_s (or R3R_3 in some notations) are each connected via separate pairs of current-carrying and voltage-sensing terminals, totaling eight terminals overall to prevent lead resistance interference. A or null detector is placed across the bridge junction to indicate balance. The balance condition for the Kelvin double bridge is achieved when the galvanometer current is zero, leading to the equation: Rx=R3R1R2+corrections for lead resistances r1,r2R_x = \frac{R_3}{R_1} R_2 + \text{corrections for lead resistances } r_1, r_2 where the corrections account for unequal ratios between the main and auxiliary arms, typically expressed as small terms involving rlr_l (the linking resistance) to adjust for any residual lead effects; in the ideal case where r1r2=R1R2\frac{r_1}{r_2} = \frac{R_1}{R_2}, the lead resistances are fully eliminated, simplifying to Rx=R3R1R2R_x = \frac{R_3}{R_1} R_2. This condition ensures high precision, with accuracies often reaching ±0.05% for resistances down to 0.00001 ohms. The measurement procedure requires two sequential balance adjustments to null the detector. First, the auxiliary bridge is balanced by varying r1r_1 and r2r_2 to match the ratio of the main arms R1R_1 and R2R_2, minimizing the impact of lead resistances r1r_1 and r2r_2. Second, the main bridge is balanced by adjusting R2R_2 or R3R_3 until the galvanometer shows no deflection, at which point RxR_x is directly computed from the known arm values. A stable DC current source is used throughout to maintain consistent voltage drops. In applications, the Kelvin double bridge is widely employed in and laboratories for verifying shunt resistors used in precision ammeters and standard low-value resistors essential for electrical standards. Its ability to handle resistances as low as milliohms with minimal error makes it indispensable for high-impact tasks like calibrating current shunts in national measurement institutes.

Maxwell Bridge

The is an AC bridge circuit designed for the precise measurement of unknown and its associated series resistance, particularly suitable for medium-Q inductors. It consists of three resistors and one arranged in a configuration that compensates for the inductive reactance without requiring a . Specifically, the unknown LxL_x in series with resistance RxR_x forms one arm of the bridge, while the adjacent arm contains R2R_2, the opposite arm has R3R_3, and the remaining arm features the C4C_4 in parallel with R4R_4. This setup allows for balance by adjusting the and one , leveraging the phase opposition between the inductive and capacitive arms to achieve null detection. At balance, the bridge satisfies the condition where the product of opposite arm impedances are equal, resulting in magnitude-only equations independent of and ω\omega. The is given by Lx=R2R3C4L_x = R_2 R_3 C_4 and the series resistance by Rx=R2R3R4.R_x = \frac{R_2 R_3}{R_4}. The phase balance occurs automatically due to the capacitive arm counteracting the inductive phase shift, eliminating the need for frequency-specific adjustments. This configuration ensures that both magnitude and phase conditions are met simultaneously through simple variation of C4C_4 and R4R_4. Key advantages of the Maxwell bridge include its simplicity in adjustment using a readily available , which avoids the complexities and cost of variable inductors, and its independence from source frequency, making it robust against variations in the AC supply. It is particularly effective for inductors with quality factors QQ between 1 and 10, where Q=ωLx/RxQ = \omega L_x / R_x, as the balance equations remain stable without residual inductance errors from mutual coupling. However, it is less suitable for very low-Q or high-Q coils due to sensitivity limitations in those ranges. The bridge typically operates in the audio frequency range of 1 to 10 kHz, ideal for measuring medium s from millihenries to henries with high accuracy, as higher frequencies can introduce parasitic effects while lower ones reduce sensitivity. A variation known as the inductance comparison bridge adapts the Maxwell configuration for comparing an unknown to a standard one, often used in calibrations involving mutual effects by incorporating a reference in place of the capacitive arm to directly ratio s while minimizing lead and ground errors.

Wien Bridge

The is an AC bridge circuit invented by Max Wien in 1891 and originally developed for precision measurement of , particularly in the context of dielectric testing to determine and conductance for calculating loss angles in materials like electric cables. This configuration extends the principle to handle frequency-dependent impedances, enabling accurate assessment of capacitive components under sinusoidal excitation. The circuit features a series RC arm (typically resistor R1R_1 in series with known capacitor C1C_1) and an adjacent parallel RC arm (resistor R2R_2 in parallel with unknown capacitor CxC_x), completed by two ratio arms consisting of resistors R3R_3 and R4R_4. At balance, the voltage across the detector is zero, allowing the unknown capacitance CxC_x or the operating frequency to be determined by adjusting the bridge elements while applying an AC source. The balance conditions derive from equating the impedances of opposing arms, yielding two independent equations: one for the resistive components and one for the reactive components. For capacitance measurement, the unknown CxC_x satisfies Cx=C1R3R4C_x = C_1 \cdot \frac{R_3}{R_4}, assuming specific in the RC arms. Alternatively, for frequency determination with known components, the balance occurs at f=12πR1R2C1Cxf = \frac{1}{2\pi \sqrt{R_1 R_2 C_1 C_x}}
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