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Electronic filter topology
Electronic filter topology
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Electronic filter topology defines electronic filter circuits without taking note of the values of the components used but only the manner in which those components are connected.

Filter design characterises filter circuits primarily by their transfer function rather than their topology. Transfer functions may be linear or nonlinear. Common types of linear filter transfer function are; high-pass, low-pass, bandpass, band-reject or notch and all-pass. Once the transfer function for a filter is chosen, the particular topology to implement such a prototype filter can be selected so that, for example, one might choose to design a Butterworth filter using the Sallen–Key topology.

Filter topologies may be divided into passive and active types. Passive topologies are composed exclusively of passive components: resistors, capacitors, and inductors. Active topologies also include active components (such as transistors, op amps, and other integrated circuits) that require power. Further, topologies may be implemented either in unbalanced form or else in balanced form when employed in balanced circuits. Implementations such as electronic mixers and stereo sound may require arrays of identical circuits.

Passive topologies

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Passive filters have been long in development and use. Most are built from simple two-port networks called "sections". There is no formal definition of a section except that it must have at least one series component and one shunt component. Sections are invariably connected in a "cascade" or "daisy-chain" topology, consisting of additional copies of the same section or of completely different sections. The rules of series and parallel impedance would combine two sections consisting only of series components or shunt components into a single section.

Some passive filters, consisting of only one or two filter sections, are given special names including the L-section, T-section and Π-section, which are unbalanced filters, and the C-section, H-section and box-section, which are balanced. All are built upon a very simple "ladder" topology (see below). The chart at the bottom of the page shows these various topologies in terms of general constant k filters.

Filters designed using network synthesis usually repeat the simplest form of L-section topology though component values may change in each section. Image designed filters, on the other hand, keep the same basic component values from section to section though the topology may vary and tend to make use of more complex sections.

L-sections are never symmetrical but two L-sections back-to-back form a symmetrical topology and many other sections are symmetrical in form.

Ladder topologies

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Ladder topology, often called Cauer topology after Wilhelm Cauer (inventor of the elliptic filter), was in fact first used by George Campbell (inventor of the constant k filter). Campbell published in 1922 but had clearly been using the topology for some time before this. Cauer first picked up on ladders (published 1926) inspired by the work of Foster (1924). There are two forms of basic ladder topologies: unbalanced and balanced. Cauer topology is usually thought of as an unbalanced ladder topology.

A ladder network consists of cascaded asymmetrical L-sections (unbalanced) or C-sections (balanced). In low pass form the topology would consist of series inductors and shunt capacitors. Other bandforms would have an equally simple topology transformed from the lowpass topology. The transformed network will have shunt admittances that are dual networks of the series impedances if they were duals in the starting network - which is the case with series inductors and shunt capacitors.

Image filter sections
 
Unbalanced
L Half section T Section Π Section
Ladder network
 
Balanced
C Half-section H Section Box Section
Ladder network
X Section (mid-T-Derived) X Section (mid-Π-Derived)
N.B. Textbooks and design drawings usually show the unbalanced implementations, but in telecoms it is often required to convert the design to the balanced implementation when used with balanced lines. edit

Modified ladder topologies

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series m-derived topology

Image filter design commonly uses modifications of the basic ladder topology. These topologies, invented by Otto Zobel,[1] have the same passbands as the ladder on which they are based but their transfer functions are modified to improve some parameter such as impedance matching, stopband rejection or passband-to-stopband transition steepness. Usually the design applies some transform to a simple ladder topology: the resulting topology is ladder-like but no longer obeys the rule that shunt admittances are the dual network of series impedances: it invariably becomes more complex with higher component count. Such topologies include;

The m-type (m-derived) filter is by far the most commonly used modified image ladder topology. There are two m-type topologies for each of the basic ladder topologies; the series-derived and shunt-derived topologies. These have identical transfer functions to each other but different image impedances. Where a filter is being designed with more than one passband, the m-type topology will result in a filter where each passband has an analogous frequency-domain response. It is possible to generalise the m-type topology for filters with more than one passband using parameters m1, m2, m3 etc., which are not equal to each other resulting in general mn-type[2] filters which have bandforms that can differ in different parts of the frequency spectrum.

The mm'-type topology can be thought of as a double m-type design. Like the m-type it has the same bandform but offers further improved transfer characteristics. It is, however, a rarely used design due to increased component count and complexity as well as its normally requiring basic ladder and m-type sections in the same filter for impedance matching reasons. It is normally only found in a composite filter.

Bridged-T topologies

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Typical bridged-T Zobel network equaliser used to correct high end roll-off

Zobel constant resistance filters[3] use a topology that is somewhat different from other filter types, distinguished by having a constant input resistance at all frequencies and in that they use resistive components in the design of their sections. The higher component and section count of these designs usually limits their use to equalisation applications. Topologies usually associated with constant resistance filters are the bridged-T and its variants, all described in the Zobel network article;

  • Bridged-T topology
  • Balanced bridged-T topology
  • Open-circuit L-section topology
  • Short-circuit L-section topology
  • Balanced open-circuit C-section topology
  • Balanced short-circuit C-section topology

The bridged-T topology is also used in sections intended to produce a signal delay but in this case no resistive components are used in the design.

Lattice topology

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Lattice topology X-section phase correction filter

Both the T-section (from ladder topology) and the bridge-T (from Zobel topology) can be transformed into a lattice topology filter section but in both cases this results in high component count and complexity. The most common application of lattice filters (X-sections) is in all-pass filters used for phase equalisation.[4]

Although T and bridged-T sections can always be transformed into X-sections the reverse is not always possible because of the possibility of negative values of inductance and capacitance arising in the transform.

Lattice topology is identical to the more familiar bridge topology, the difference being merely the drawn representation on the page rather than any real difference in topology, circuitry or function.

Active topologies

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Elementary feedback topology

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The elementary feedback topology is based on the simple inverting amplifier configuration. The transfer function is:

An elementary filter topology introduces a capacitor into the feedback path of an op-amp to achieve an unbalanced active implementation of a low-pass transfer function

Multiple feedback topology

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Multiple feedback topology circuit.

Multiple feedback topology is an electronic filter topology which is used to implement an electronic filter by adding two poles to the transfer function. A diagram of the circuit topology for a second order low pass filter is shown in the figure on the right.

The transfer function of the multiple feedback topology circuit, like all second-order linear filters, is:

.

In an MF filter,

is the quality factor.
is the DC voltage gain
is the corner frequency

For finding suitable component values to achieve the desired filter properties, a similar approach can be followed as in the Design choices section of the alternative Sallen–Key topology.

Biquad filter topology

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For the digital implementation of a biquad filter, see Digital biquad filter.

A biquad filter is a type of linear filter that implements a transfer function that is the ratio of two quadratic functions. The name biquad is short for biquadratic. Any second-order filter topology can be referred to as a biquad, such as the MFB or Sallen-Key.[5][6] However, there is also a specific "biquad" topology. It is also sometimes called the 'ring of 3' circuit.[citation needed]

Biquad filters are typically active and implemented with a single-amplifier biquad (SAB) or two-integrator-loop topology.

  • The SAB topology uses feedback to generate complex poles and possibly complex zeros. In particular, the feedback moves the real poles of an RC circuit in order to generate the proper filter characteristics.
  • The two-integrator-loop topology is derived from rearranging a biquadratic transfer function. The rearrangement will equate one signal with the sum of another signal, its integral, and the integral's integral. In other words, the rearrangement reveals a state variable filter structure. By using different states as outputs, any kind of second-order filter can be implemented.

The SAB topology is sensitive to component choice and can be more difficult to adjust. Hence, usually the term biquad refers to the two-integrator-loop state variable filter topology.

Tow-Thomas filter

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Figure 1. The common Tow-Thomas biquad filter topology.

For example, the basic configuration in Figure 1 can be used as either a low-pass or bandpass filter depending on where the output signal is taken from.

The second-order low-pass transfer function is given by

where low-pass gain . The second-order bandpass transfer function is given by

.

with bandpass gain . In both cases, the

  • Natural frequency is .
  • Quality factor is .

The bandwidth is approximated by , and Q is sometimes expressed as a damping constant . If a noninverting low-pass filter is required, the output can be taken at the output of the second operational amplifier, after the order of the second integrator and the inverter has been switched. If a noninverting bandpass filter is required, the order of the second integrator and the inverter can be switched, and the output taken at the output of the inverter's operational amplifier.

Akerberg-Mossberg filter

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Figure 2. The Akerberg-Mossberg biquad filter topology.

Figure 2 shows a variant of the Tow-Thomas topology, known as Akerberg-Mossberg topology, that uses an actively compensated Miller integrator, which improves filter performance.

Sallen–Key topology

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Figure 1: The generic Sallen–Key filter topology

The Sallen-Key design is a non-inverting second-order filter with the option of high Q and passband gain.

See also

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Notes

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References

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Electronic filter topology refers to the specific circuit configurations and arrangements of components used to implement electronic filters, which are networks designed to process electrical signals by selectively attenuating or passing certain frequency bands while altering the amplitude and phase of others. These topologies enable the realization of various filter types, including low-pass, high-pass, band-pass, and band-reject (notch) filters, each characterized by key parameters such as cutoff frequency (where the response drops by 3 dB), quality factor (Q) for selectivity and peaking, and order (number of poles determining roll-off rate, typically -6 dB/octave per pole). Electronic filters can be broadly classified into passive and active topologies. Passive filters rely solely on resistors (), capacitors (), and inductors (L) to form networks like , L-section, T-section, or π-section configurations, which provide frequency-dependent impedance without amplification but suffer from loading effects and limited selectivity at low frequencies due to bulky inductors. In contrast, active filters incorporate operational amplifiers (op-amps) alongside and components to achieve gain, sharper , and tunability without inductors, making them suitable for integrated circuits and frequencies from 1 Hz to 1 MHz. Among the most prominent active filter topologies are the Sallen-Key and Multiple Feedback (MFB) designs, both typically used for second-order sections that can be cascaded for higher-order filters. The Sallen-Key topology, valued for its simplicity and low component sensitivity, employs a unity-gain or non-inverting op-amp configuration and is commonly applied to low-pass and high-pass filters with moderate values (under 3), offering high design accuracy through adjustable gain. The MFB topology, on the other hand, uses an inverting op-amp as an for higher (up to 20) and gain, providing independent control over frequency, , and gain, though it exhibits greater sensitivity to component tolerances and is ideal for band-pass or narrowband applications. Other notable topologies include state-variable filters for versatile parameter adjustment and discrete or cavity structures in RF/ contexts for high-power handling. Filter performance is further defined by response types, such as Butterworth (maximally flat passband), Chebyshev (sharper transition with ripple), Bessel (linear phase for minimal distortion), and Elliptic (steepest roll-off with ripple in both bands), each influencing trade-offs in insertion loss, return loss, and bandwidth (from <0.5% to over 100%). These topologies must account for practical limitations like op-amp bandwidth, component parasitics, and power handling (e.g., up to kilowatts in cavity filters), ensuring stability and minimal distortion. In applications ranging from audio processing and anti-aliasing in analog-to-digital converters to RF signal separation in communications systems and noise rejection in power electronics, electronic filter topologies enable precise signal conditioning while balancing size, cost, and performance.

Overview

Definition and scope

Electronic filter topology refers to the specific interconnection pattern of passive and active components—such as resistors, capacitors, inductors, and operational amplifiers—in an analog circuit to realize a desired frequency response. This configuration dictates how the circuit selectively attenuates or amplifies signals across different frequencies, independent of the exact component values used. By defining the structural layout, topology enables the synthesis of filters that shape the amplitude and phase of input signals for applications in communications, audio processing, and instrumentation. The scope of electronic filter topology primarily encompasses linear time-invariant (LTI) analog filters, where component parameters remain constant and responses are proportional to inputs, thereby excluding nonlinear elements like diodes, though it also includes discrete-time implementations such as switched-capacitor filters. These LTI filters form the foundation for predictable signal manipulation in continuous-time domains. Historically, filter topologies emerged in the early 20th century amid efforts to improve long-distance telephony; George A. Campbell, an AT&T engineer, developed the electric wave filter around 1915—patented in 1917—to equalize telephone lines by compensating for frequency-dependent attenuation, extending on his 1899 loading coil innovations that mitigated signal loss in transmission lines. Key types of frequency-selective filters are distinguished by their ideal magnitude responses, which describe the theoretical gain as a function of frequency. A maintains unity gain for frequencies below a cutoff point while ideally dropping to zero above it, preserving baseband signals like audio. Conversely, a attenuates low frequencies and passes higher ones, useful for removing DC offsets. transmit a narrow frequency band with unity gain while rejecting others, ideal for channel selection; do the opposite, suppressing specific interference bands. , meanwhile, pass all frequencies with equal magnitude but introduce phase shifts, aiding in delay equalization. Practical topologies approximate these brick-wall ideals with gradual roll-offs. Topology selection profoundly impacts filter performance, particularly in sensitivity to manufacturing tolerances—where variations in component values alter the response—impedance matching to ensure maximal power transfer between source and load, and realizability of complex transfer functions without excessive element count or instability. Topologies with inherently low sensitivity, for example, maintain response accuracy despite ±5% component drifts, enhancing reliability in mass production. Broadly, topologies divide into passive (R, L, C only) and active (with amplification) categories, the latter offering impedance independence and gain.

Classification of topologies

Electronic filter topologies are primarily classified into passive and active categories based on their component composition and operational principles, with switched-capacitor topologies forming a distinct class that emulates analog behavior using discrete-time processing with capacitors and switches, often in integrated circuits for low-frequency applications. Passive topologies consist solely of passive elements such as , , and , which do not require an external energy source and cannot provide gain or amplification. In contrast, active topologies incorporate active devices, typically or , to enable signal amplification, impedance transformation, and precise tuning of filter characteristics like . Secondary classifications further refine these topologies according to implementation and signal handling. Lumped-element topologies use discrete R, L, and C components where the physical dimensions are much smaller than the signal wavelength, making them suitable for lower frequencies up to the microwave range. Distributed-element topologies, however, employ continuous structures like transmission lines or waveguides to realize inductance and capacitance, which become necessary at high frequencies where lumped approximations fail due to parasitic effects. Additionally, topologies can be single-ended, referencing signals to ground, or balanced/differential, using two complementary signal paths for improved noise rejection and common-mode suppression in noisy environments. Filter topologies are also categorized by design methodologies that influence their frequency response optimization. The image parameter method designs filters by cascading sections with predefined cutoff frequencies, offering simplicity for constant-k prototypes but limited control over passband ripple. The insertion loss method, also known as network synthesis, provides greater flexibility by optimizing the overall power loss and ripple through polynomial approximations, enabling precise control over both passband and stopband characteristics. Regardless of topology, electronic filters are linear time-invariant (LTI) systems characterized by their transfer function in the Laplace domain: H(s)=Vout(s)Vin(s)=N(s)D(s)H(s) = \frac{V_\text{out}(s)}{V_\text{in}(s)} = \frac{N(s)}{D(s)} where N(s)N(s) and D(s)D(s) are polynomials in the complex variable ss, representing zeros and poles, respectively. For low-pass and high-pass filters, the order nn corresponds to the degree of the denominator polynomial, determining the roll-off steepness. Band-pass and band-stop filters typically feature second-order sections with paired poles and zeros to achieve selectivity. These classifications involve inherent trade-offs: passive topologies excel in high-power and high-frequency applications due to their robustness and lack of power dissipation in active elements, but they suffer from loading effects and fixed Q factors limited by component tolerances. Active topologies, conversely, support low-power operation and tunable Q factors through feedback, enhancing versatility at the cost of requiring stable power supplies and sensitivity to noise.

Passive topologies

Ladder topologies

Ladder topologies form a fundamental class of passive electronic filter structures, characterized by a cascaded arrangement of series and shunt elements that create a repetitive network resembling a ladder. These topologies typically alternate between series arms providing impedance ZZ and shunt arms providing admittance YY, which can be realized as basic L-sections (a single series element followed by a shunt), T-sections (series elements split around a central shunt), or Π-sections (shunt elements split around a central series). This iterative configuration enables the realization of higher-order filters by stacking multiple sections, promoting simplicity in construction and analysis for both lumped and distributed implementations. The development of ladder topologies originated with George A. Campbell's invention of the constant-k ladder filter in 1922, detailed in his seminal paper on the physical theory of electric wave-filters, which laid the groundwork for periodic network designs used in telephony and signal processing. Building on this, Wilhelm Cauer advanced the field in 1931 through his work on network synthesis, introducing methods that facilitated the insertion loss approach for designing ladder filters with prescribed frequency responses. Constant-k ladder designs maintain a constant product k=ZYk = Z \cdot Y across all sections, ensuring uniform image parameters and predictable behavior. For a prototypical low-pass LC ladder, the series arm impedance is Zseries=jωLZ_\text{series} = j \omega L and the shunt arm admittance is Yshunt=jωCY_\text{shunt} = j \omega C, yielding k=ω2LCk = -\omega^2 L C. The cutoff frequency, marking the transition from passband to stopband, is determined by ωc=1LC\omega_c = \frac{1}{\sqrt{L C}}
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