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Phase Locked Loops

A phase locked loop — the PLL — is one of the most elegant and powerful circuits in all of electronics. On the surface it appears complex: a loop of interconnected blocks that seem to chase each other in circles. In reality, the PLL solves a single problem with remarkable efficiency: how do you make a variable oscillator track a precise reference signal so accurately that the output inherits the reference's stability? The answer turns out to unlock an enormous range of applications — from FM demodulation in every analog receiver built in the last 50 years, to the frequency synthesizers that give modern transceivers their exact, rock-stable channel frequencies, to the clock recovery circuits inside digital data links. If you have ever wondered how your IC-7300 can tune to exactly 14.225.000 MHz and stay there without drifting, the PLL is a large part of the answer.

What you will learn: How a phase locked loop achieves phase and frequency lock, the function of each block (phase detector, loop filter, VCO), the key parameters of lock range and loop bandwidth, and the major applications of PLLs in amateur radio equipment.

The Tuner Analogy: Chasing Phase

Imagine you are a musician trying to tune a guitar string to match a tuning fork. You strike the fork, listen to the reference pitch, then adjust the tuning peg until your string sounds the same. When the two pitches are identical, you hear no beating — the tones are in sync. If the string goes slightly sharp or flat, you correct it. The string's pitch always tries to match the fork.

A phase locked loop does exactly this, but electronically and at radio frequencies. The reference signal is the tuning fork — precise, stable, usually derived from a crystal oscillator. The voltage-controlled oscillator is the guitar string — tunable, but not inherently stable on its own. The phase detector plays the role of your ear, listening for any difference between the two. The loop filter is like the time it takes you to hear the difference and move the peg — it smooths out rapid corrections. And the feedback loop itself is what makes the whole thing work: the output is continuously fed back and compared against the reference so that any difference immediately generates a correction.

The key word is "phase," not just "frequency." When a PLL is locked, the output frequency is identical to the reference frequency. But more than that, the output phase has a fixed relationship to the reference phase. The PLL locks on phase, and equal phases imply equal frequencies. This is why a PLL output can be far more stable than the VCO alone — it borrows the precision of the crystal reference and imprints it onto the tunable oscillator.

The Four Essential PLL Blocks

Phase locked loop block diagram showing reference oscillator, phase detector, loop filter, and VCO with feedback path

The four essential blocks of a PLL: reference oscillator, phase detector, loop filter, and voltage-controlled oscillator, with the VCO output fed back to the phase detector to close the loop.

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Every PLL — whether inside an FM radio chip or a $5,000 synthesizer — contains these four essential blocks arranged in a loop.

1. Reference Oscillator

The reference oscillator provides the stable, accurate frequency that the loop will lock to. In virtually all practical PLLs, the reference is derived from a crystal oscillator. It might be a simple Pierce oscillator running at 10 MHz, or a temperature-compensated TCXO, or even a GPS-disciplined oscillator for laboratory-grade accuracy. Whatever its source, the reference must be more stable than what the VCO alone can achieve — that is the entire point. The PLL cannot generate accuracy out of nothing; it transfers the reference's accuracy to the VCO output.

In a frequency synthesizer, the reference is often divided down before reaching the phase detector. A 10 MHz crystal might be divided by 1,000 to produce a 10 kHz reference at the phase detector input, which then allows the PLL to tune in 10 kHz steps. The reference frequency at the phase detector sets the minimum tuning step size of the synthesizer.

2. Phase Detector

The phase detector (PD) — sometimes called a phase comparator — compares the phase of the reference signal with the phase of the signal fed back from the VCO output. It produces an output voltage proportional to the phase difference between the two inputs. When the loop is locked and the phase difference is constant (typically zero or a fixed offset), the phase detector output is a steady DC voltage. When there is a phase error — meaning the two inputs have different phases — the output voltage rises or falls to push the VCO back toward lock.

The phase detector is the heart of the feedback loop. It performs the comparison that drives all the corrective action. Without it, the loop is just a VCO with no reference — free-running and subject to all the drift problems covered in previous lessons.

3. Loop Filter

The phase detector output is not a smooth DC voltage; it contains components at the reference frequency and its harmonics in addition to the error signal. The loop filter removes these AC components and passes only the slowly-varying error information to the VCO. It is essentially a low-pass filter inserted in the feedback path.

The loop filter also sets the dynamic response of the PLL — how quickly the loop responds to changes and how stable it is. A wider filter bandwidth (higher cutoff frequency) makes the loop respond faster and lock in a shorter time, but it also passes more noise through to the VCO. A narrower filter makes the loop more stable and rejects more noise, but it responds slowly to changes. Every PLL designer must balance these competing demands based on the application.

4. Voltage-Controlled Oscillator (VCO)

The VCO generates the output signal. Its frequency is controlled by the DC tuning voltage from the loop filter: when the voltage rises, the frequency rises; when the voltage falls, the frequency falls. The VCO might be an LC oscillator with a varactor diode as the tuning element (most common in RF PLLs), a relaxation oscillator, or a ring oscillator depending on frequency range and application. In a PLL synthesizer, the VCO output is what drives the transmitter or provides the local oscillator signal in a receiver.

The VCO sensitivity, given the symbol KVCO and measured in hertz per volt (Hz/V), describes how much frequency change the VCO produces for a given change in tuning voltage. A VCO with KVCO = 1 MHz/V shifts its frequency by 1 MHz for every 1 V change in tuning voltage. This parameter critically affects loop dynamics.

How the PLL Achieves Lock: Step by Step

The locking process unfolds over several distinct stages. Understanding each stage will give you a solid mental model of what the loop is actually doing.

Stage 1: Free-Running State (Unlocked)

When power is first applied, the VCO runs at its free-running frequency — wherever it happens to land based on its component values and tuning voltage. This may be very different from the reference frequency. The phase detector sees two signals at different frequencies and produces an output that alternates rapidly between high and low voltage at a rate equal to the frequency difference. This alternating output passes through the loop filter and drives the VCO tuning voltage up and down.

Stage 2: Frequency Pulling

The loop filter is a low-pass filter, so it does not pass the rapid alternating phase detector output unchanged. It averages the output over time. If the VCO is running faster than the reference, the phase detector output produces a time-averaged error voltage that pushes the VCO tuning voltage down, slowing the VCO. If the VCO is running slower, the average error pushes the tuning voltage up. The VCO frequency is being pulled toward the reference.

Stage 3: Capture

As the VCO frequency approaches the reference frequency, the rate of phase detector output variation slows. The loop filter now passes a larger fraction of the error signal. The error becomes more effective at pulling the VCO. Eventually the VCO frequency comes close enough to the reference that the two signals slip in phase only slowly. The loop "captures" — it transitions from a frequency-difference tracking state into a phase-tracking state.

Stage 4: Lock

When locked, the output frequency exactly equals the reference frequency. The phase difference between reference and feedback is constant (possibly zero, possibly a small fixed offset depending on the phase detector type). The loop filter output is a steady DC voltage — the exact voltage needed to hold the VCO at that frequency. Any perturbation — temperature change, vibration, supply voltage fluctuation — that would normally shift the VCO frequency instead creates a small phase error, which the phase detector detects, which the loop filter passes to the VCO tuning input, which corrects the frequency back. The loop continuously self-corrects.

This self-correction is the fundamental advantage of a PLL. The VCO output borrows the long-term frequency accuracy of the crystal reference while retaining the short-term tunability of an LC or free-running oscillator.

Phase Detector Types

Comparison of XOR phase detector and charge pump phase-frequency detector showing output waveforms and linear range

Two common phase detector types: the XOR (exclusive-OR) detector produces a pulse-width-modulated output proportional to phase difference over a ±90° range; the charge pump phase-frequency detector (PFD) uses UP/DOWN current pulses and can detect both phase and frequency errors over the full ±360° range.

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XOR Phase Detector

The simplest digital phase detector is an exclusive-OR (XOR) gate. It compares two digital square waves and produces an output that is high when the two inputs differ and low when they agree. If the two inputs are perfectly in phase (phase difference = 0°), the XOR output is always low. If they are 90° apart, the output is a square wave at 50% duty cycle. If they are 180° apart, the output is always high. The average DC value of the XOR output is proportional to phase difference over the range from 0° to 180°.

The XOR detector is simple and fast, but it has a limitation: it only detects phase difference, not frequency difference. If the two inputs are at very different frequencies, the XOR output alternates so rapidly that the loop filter cannot distinguish it from noise. The loop struggles to acquire lock when the frequency error is large. XOR detectors are best suited to applications where the VCO starts close to the target frequency.

Phase-Frequency Detector (PFD) with Charge Pump

The phase-frequency detector is the dominant choice in modern PLLs. Instead of comparing voltages directly, it uses flip-flop logic to detect which input leads the other in phase — and when the frequencies are different, which input is running faster. It produces separate UP and DOWN outputs that control a charge pump: a current source that pumps charge into the loop filter capacitor (UP) or drains charge from it (DOWN).

When the reference frequency is higher than the VCO output frequency, UP pulses are wider than DOWN pulses, so the charge pump net current flows into the capacitor, raising the VCO tuning voltage and speeding up the VCO. When the frequencies match but the VCO phase lags slightly, short UP pulses inject a small correction. When locked perfectly, both UP and DOWN produce identical narrow pulses that cancel, and the tuning voltage holds steady.

The PFD with charge pump has a linear range of ±360° (a full cycle), compared to the XOR detector's ±90°. More importantly, it can detect and correct frequency errors — not just phase errors — so it acquires lock reliably even when the VCO starts far from the reference frequency. This is why virtually all modern synthesizer ICs use the PFD + charge pump combination.

Phase Detector Comparison

Parameter XOR Detector PFD + Charge Pump
Linear range 0° to 180° (±90° around 90° offset) ±360° (full cycle)
Detects frequency error? No Yes
Acquisition speed Slow if large frequency error Fast — pulls in from wide range
Reference spurs Moderate Low with good charge pump matching
Typical use Simple PLLs, CD4046 Virtually all modern synthesizers

The Voltage-Controlled Oscillator

The VCO in an RF PLL is usually an LC oscillator where a varactor diode serves as the tuning capacitor. As explained in earlier lessons, a varactor's junction capacitance changes with reverse bias voltage: more reverse bias means a smaller capacitor. By varying the voltage applied to the varactor, the tank circuit capacitance changes, and so does the oscillator frequency.

The VCO sensitivity KVCO (also written K0) quantifies this relationship:

VCO Frequency Equation:
fout = fcenter + KVCO × Vtune

Where fcenter is the free-running frequency at zero tuning voltage, KVCO is in Hz/V, and Vtune is the control voltage in volts.
Example: VCO tuning range calculation

A VCO used in a 40-meter transceiver has KVCO = 200 kHz/V, a center frequency of 7.100 MHz at Vtune = 5 V, and a tuning voltage range of 1 V to 9 V.

At Vtune = 1 V: f = 7.100 MHz + 200,000 × (1 − 5) = 7.100 − 0.800 = 6.300 MHz
At Vtune = 9 V: f = 7.100 MHz + 200,000 × (9 − 5) = 7.100 + 0.800 = 7.900 MHz

Total tuning range: 6.300 to 7.900 MHz — a 1.6 MHz span, comfortably covering the entire 40-meter amateur band (7.000 to 7.300 MHz) with room to spare.

A VCO with too large a KVCO is very sensitive to supply noise and thermal drift — small disturbances produce large frequency excursions. A VCO with too small a KVCO may not cover the required tuning range. Good PLL design requires matching the VCO gain to the loop requirements. When the loop is locked, the VCO tuning noise is suppressed by the loop gain, so PLLs with wider loop bandwidth can tolerate a noisier VCO.

The Loop Filter

PLL loop filter frequency response showing loop bandwidth, noise suppression above bandwidth, and reference spur rejection

The PLL loop filter acts as a low-pass filter within the feedback path. Below the loop bandwidth frequency, the VCO tracks the reference and reference phase noise appears on the output. Above loop bandwidth, VCO free-running phase noise dominates. The optimum loop bandwidth minimizes total output phase noise.

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The loop filter is usually a passive RC network (one or two poles) or an active filter built around an op-amp. Its two main functions are: remove the reference frequency ripple from the phase detector output, and set the loop's dynamic response.

Simple Passive RC Filter

The simplest loop filter is a single resistor and capacitor forming a first-order RC low-pass filter. The resistor is in series between the phase detector output and the capacitor, and the capacitor connects to ground. The loop filter capacitor is charged and discharged by the charge pump current, and the voltage across it drives the VCO. The RC time constant τ = R × C sets the loop bandwidth approximately as floop ≈ 1/(2πτ).

Second-Order Loop Filter

A single-pole filter gives a loop that can become unstable because the loop itself contributes phase shift. Most practical PLLs use a second-order loop filter — a capacitor in parallel with a series resistor-capacitor combination — which provides a "zero" (a frequency where phase shift is reduced) that stabilizes the loop. The addition of a second capacitor after the series RC provides extra attenuation of reference spurs without sacrificing stability.

Loop Bandwidth: The Critical Trade-Off

The loop bandwidth is the most important parameter of loop filter design. Inside the loop bandwidth, the VCO is phase-locked to the reference — it tracks the reference signal's phase noise and suppresses the VCO's own phase noise. Outside the loop bandwidth, the loop cannot follow fast perturbations, and the VCO's free-running phase noise appears on the output.

If the reference crystal has low phase noise (which crystals typically do) and the VCO has high phase noise (which free-running LC oscillators typically do), you want a wide loop bandwidth — let the reference suppress as much VCO noise as possible. But a wide loop bandwidth also passes reference frequency spurs to the output, creating unwanted sidebands. In a receiver, strong spurs create phantom signals on nearby frequencies. In a transmitter, spurs violate spectral purity requirements.

The optimum loop bandwidth sits at the crossover point where the reference phase noise equals the VCO phase noise — which typically falls somewhere between 1 kHz and 100 kHz depending on the oscillator types involved. This is a key design parameter that requires both analysis and empirical testing in practice.

PLL Parameters: Lock Range, Capture Range, Loop Bandwidth

Three frequency ranges describe a PLL's ability to lock and remain locked.

Parameter Definition Physical Meaning
Hold range (lock range) Frequency range over which an already-locked PLL will remain locked Largest reference frequency offset the VCO can still follow without losing lock. Set primarily by VCO tuning range and DC loop gain.
Capture range (pull-in range) Frequency range over which an unlocked PLL will achieve lock Narrower than hold range — requires the loop filter to pass enough energy to pull the VCO in from a standing start. Set by loop bandwidth.
Loop bandwidth 3 dB frequency of the closed-loop transfer function Determines speed of response, noise rejection, and reference spur suppression. Narrower = slower but quieter; wider = faster but noisier.

In general, hold range > capture range > loop bandwidth. A PLL can remain locked through a larger disturbance than it can acquire lock from a standing start. When designing a synthesizer, you ensure the capture range covers the full tuning range of the VCO so the loop can always acquire lock when frequency is changed.

Lock Time

Lock time is how long the PLL takes to settle to a new frequency after the reference or divider ratio changes. It is approximately 1/(loop bandwidth). A 10 kHz loop bandwidth gives a lock time of roughly 100 µs. A 100 kHz loop bandwidth gives 10 µs. In a transceiver that needs to hop frequencies, faster lock time allows quicker channel switching. Lock time and phase noise are again in direct conflict: wider bandwidth for faster lock time brings more noise.

Adding a Frequency Divider: Multiply the Reference

The simple four-block PLL described above locks the VCO output to exactly the same frequency as the reference. That is useful for locking an oscillator to a crystal standard, but it does not allow you to generate different output frequencies. The breakthrough comes from inserting a programmable frequency divider (divide-by-N counter) in the feedback path between the VCO output and the phase detector input.

PLL with Divide-by-N:
When the loop is locked, the signal at the phase detector's feedback input equals the reference frequency.
Signal at PD feedback input = fVCO / N = fref

Therefore: fVCO = N × fref

By programming N, you select the output frequency in steps of fref.

This is the key insight behind frequency synthesis. The VCO output frequency is forced to be exactly N times the reference frequency. Change N, change the output frequency. The crystal reference never changes, so every output frequency benefits from crystal accuracy.

The minimum frequency step (channel spacing) equals the reference frequency at the phase detector. If you want 10 kHz channel spacing, you use a 10 kHz reference. If you want 1 kHz steps, you use a 1 kHz reference. Many synthesizers start with a higher-frequency crystal (say, 10 MHz) and divide it down to the desired reference frequency using a fixed prescaler.

Worked Example: 14 MHz HF PLL

Design a PLL for a 20-meter receiver local oscillator covering 14.000 to 14.350 MHz in 1 kHz steps.

Step 1: Choose reference frequency.
Channel spacing = 1 kHz → reference frequency at PD = 1 kHz.
Use a 1.000 MHz crystal oscillator divided by 1,000 using a fixed ÷1000 prescaler to generate 1 kHz reference.

Step 2: Determine N range.
fVCO = N × fref = N × 1 kHz
For 14.000 MHz: N = 14,000,000 / 1,000 = 14,000
For 14.350 MHz: N = 14,350,000 / 1,000 = 14,350
So N is a programmable integer between 14,000 and 14,350, giving 350 channels at 1 kHz spacing.

Step 3: VCO requirements.
VCO must cover 14.000 to 14.350 MHz continuously. With 8 V tuning range (1 to 9 V), KVCO needed:
KVCO = 350,000 Hz / 8 V = 43.75 kHz/V — achievable with a standard varactor-tuned LC VCO.

Step 4: Loop filter bandwidth.
For a receive LO, phase noise matters. Use loop bandwidth = 2 kHz:
— Captures the VCO from any point in range (capture range >> 350 kHz tuning span with PFD)
— Suppresses VCO noise at 2 kHz offset and above
— Reference spurs at 1 kHz offset are attenuated by the filter
— Lock time ≈ 1 / (2 kHz) = 500 µs — acceptable for HF band changing

Verification: Tune to 14.225 MHz (USB calling frequency): N = 14,225. Program N = 14,225 into the programmable divider. PLL locks to exactly 14.225 MHz. Stability is set by the 1 MHz crystal reference — typically ±2 ppm without TCXO, or ±0.5 ppm with TCXO.

PLL Applications in Ham Radio

FM Demodulation

One of the oldest and most elegant uses of a PLL is as an FM demodulator. In FM, the carrier frequency is varied (deviated) by the audio signal — higher audio peaks produce higher deviation. A PLL locked to the FM carrier tracks this deviation: as the carrier frequency rises and falls with the audio, the loop filter output voltage rises and falls to keep the VCO following the carrier. The loop filter output voltage is therefore a direct copy of the original audio modulation. This is the demodulated audio signal.

FM demodulation via PLL became practical with integrated circuit PLLs like the NE565, CA3089, and MC3357. These chips contain all four PLL blocks on a single die. The CD4046 CMOS PLL, popular in homebrew radio projects, is another well-known example. PLL-based FM demodulation replaced the discriminator and ratio detector circuits in most equipment from the late 1970s onward because the IC approach is smaller, cheaper, and requires no coil alignment.

Frequency Synthesis

The largest application of PLLs in amateur radio is frequency synthesis — generating any desired frequency from a single crystal reference. The receive VFO (local oscillator), the carrier insertion oscillator (BFO), the transmitter exciter frequency — all of these can be generated by PLLs in a modern rig. The next lesson covers frequency synthesis in detail.

Clock Recovery in Digital Modes

Digital modes such as PSK31, FT8, and WSPR use coherent demodulation that requires knowledge of the exact transmit clock frequency and phase. When receiving a digital signal, a PLL in the receiver locks to the incoming data transitions and recovers the clock embedded in the data stream. This recovered clock then gates the data slicer at exactly the right moments to correctly identify each bit. Without PLL-based clock recovery, coherent digital demodulation at low SNR would be impossible.

Reference Frequency Distribution

In a station with multiple pieces of equipment — transceiver, amplifier, SDR panadapter, computer sound card interface — it can be valuable to lock all equipment to a common 10 MHz reference. A PLL in each device locks its internal crystal to the 10 MHz reference, ensuring everything is frequency-coherent. GPS-disciplined oscillators (GPSDOs) that provide a 10 MHz output locked to GPS atomic timing are popular for this purpose among serious contesters and weak-signal operators.

Phase Noise in PLLs

A PLL does not produce a perfectly clean output signal. There are two sources of phase noise in a PLL output, and they dominate in different regions of the frequency spectrum:

Inside the loop bandwidth: The VCO is phase-locked to the reference, so the output phase noise closely follows the reference phase noise multiplied by N². When the divide ratio N is large — as it is in a high-frequency synthesizer — the reference noise is multiplied by 20 × log₁₀(N) dB. A synthesizer with N = 14,000 adds 20 × log₁₀(14,000) = 82.9 dB to the reference phase noise inside the loop bandwidth. This is why low-phase-noise references and small frequency steps are both important for clean synthesizer outputs.

Outside the loop bandwidth: The loop cannot suppress VCO noise at offsets beyond the loop bandwidth. The VCO's free-running phase noise appears directly on the output. This is why VCO quality matters — you need a high-Q tuned circuit (good inductor, stable capacitor) in the VCO to minimize its free-running phase noise.

Reference spurs: At offsets equal to the reference frequency and its harmonics, the output spectrum often shows discrete sidebands called reference spurs. These arise from charge pump leakage, substrate coupling in the IC, and other non-ideal behaviors. Reference spurs appear as discrete signals that create ghost interference in a receiver. Careful loop filter design and good PCB layout minimize them. A typical well-designed synthesizer achieves −80 to −100 dBc reference spurs. FCC Part 97 rules require amateur transmitters to have suppressed spurious emissions, so synthesizer spur performance is a real regulatory concern.

Experiment: Observing PLL Lock with a CD4046

⚖ Experiment: PLL Lock and Capture with the CD4046

This experiment builds a basic audio-frequency PLL using the CD4046 CMOS PLL IC. You will observe the VCO locking to a reference, measure the loop filter voltage during lock, and see what happens when the reference moves outside the lock range.

You will need:
  • CD4046 CMOS PLL IC (or CD74HC4046)
  • 555 timer IC (to generate reference square wave)
  • Breadboard
  • 9 V battery and snap connector
  • Resistors: 100 kΩ × 2, 10 kΩ × 2, 1 kΩ
  • Capacitors: 10 nF × 2, 100 nF, 100 µF electrolytic
  • 10 kΩ potentiometer (for reference frequency adjustment)
  • Digital multimeter
  • Oscilloscope (helpful but not required)
  • Small speaker or piezo buzzer (optional — to hear the audio)
  1. Build a 555 astable oscillator on the breadboard tunable from about 500 Hz to 5 kHz using a 10 kΩ pot, 10 kΩ fixed resistor, and 100 nF timing capacitor. This is your reference signal. Connect the output (pin 3) to a test point.
  2. Wire the CD4046 following the datasheet pinout. Pin 14 is VDD (9 V). Pin 7 is VSS (ground). Connect the reference signal to pin 14 (Phase Comparator In). Set up the VCO with R1 = 100 kΩ and R2 = 100 kΩ between pins 11 and 12 and ground, and a 10 nF VCO capacitor between pin 6 and ground. This sets the VCO free-running range roughly 100 Hz to 5 kHz.
  3. Connect a simple passive loop filter: 10 kΩ resistor from the Phase Comparator 2 output (pin 13) to a 10 nF capacitor to ground. Connect the junction of resistor and capacitor to the VCO input (pin 9).
  4. Connect the VCO output (pin 4) back to the Phase Comparator Input 2 (pin 3). This closes the loop. The VCO output is also your loop output.
  5. Power up the circuit and set the 555 potentiometer to approximately mid-range. Wait a few seconds.
  6. Measure the voltage at the loop filter output (pin 9) with your multimeter. You should see a steady DC voltage between 1 V and 8 V — this is the lock voltage holding the VCO at the reference frequency.
  7. If you have an oscilloscope, probe both the reference (555 output) and the VCO output (pin 4). When locked, they will be at the same frequency with a fixed phase relationship.
  8. Slowly turn the 555 potentiometer to change the reference frequency. Observe the loop filter voltage on the multimeter: as the reference goes up in frequency, the lock voltage rises (VCO speeds up); as it goes down, the voltage falls (VCO slows down).
  9. Turn the potentiometer rapidly to a very high or very low frequency. Observe what happens: if you move outside the lock range, the lock voltage will swing to a rail and the VCO will lose lock. The output will no longer match the reference.
What you should see:

When locked, the loop filter voltage is a stable DC value proportional to where the reference frequency sits within the VCO tuning range. As you slowly change the reference frequency, the voltage tracks it — proving the PLL is following the reference. When you force the reference outside the capture range by changing frequency too rapidly or by going too far, you will see the lock voltage rail and the output frequency decouple from the reference. Re-entering the lock range allows re-acquisition. This demonstrates both the locking mechanism and the limits of PLL capture range. The CD4046 Phase Comparator 2 (PC2, pin 13) is a PFD type — it will acquire lock more reliably from a wider frequency range than Phase Comparator 1 (PC1, pin 2), which is an XOR detector. Try comparing both outputs to observe this difference.

Frequently Asked Questions

What does "phase locked" actually mean — why phase and not frequency?

Locking on phase is more precise than locking on frequency. Two signals are at the same frequency if they complete the same number of cycles per second — but they could still be drifting apart in phase. When a PLL is truly phase-locked, the phase difference between reference and output is constant, which automatically means the frequencies are exactly equal. The phase detector gives the loop a finer measurement than a simple frequency comparator would, which is why PLLs can achieve such close tracking. Any deviation from locked phase — even a tiny one — generates an immediate correction signal.

Why does the PLL output have lower phase noise than the VCO alone?

Inside the loop bandwidth, the PLL actively corrects VCO phase noise. Any time the VCO wanders in phase, the phase detector sees the error, the loop filter passes a correction voltage, and the VCO is pulled back. Close-in VCO noise — noise within the loop bandwidth — is suppressed by the loop gain. The output phase noise in this region is dominated by the reference crystal's much lower phase noise. Outside the loop bandwidth, the loop cannot respond fast enough, and the VCO's free-running noise appears. The PLL thus transfers the crystal's excellent close-in phase noise to the VCO output, while the VCO's own noise dominates only at larger offsets where it is already low enough for most applications.

What is the difference between lock range and capture range?

Lock range (also called hold range) is how far the reference can move before an already-locked PLL loses lock — it is a measure of tracking performance. Capture range (pull-in range) is how far the reference can be from the VCO before an unlocked PLL can still acquire lock — it is a measure of acquisition performance. Lock range is always larger than capture range. Think of it like pushing a car: you need more force to get it moving from rest (capture) than to keep it rolling once it is underway (lock).

Can a PLL generate a frequency that is not an integer multiple of the reference?

Yes, using a technique called fractional-N synthesis. Instead of a fixed integer N, the divider alternates between two values — say N and N+1 — in a pattern controlled by a delta-sigma modulator. Over time, the average divide ratio is a fraction, allowing output frequencies between integer multiples of the reference. For example, alternating between N=14 and N=15 with equal time produces an average divide ratio of 14.5, giving an output of 14.5 × fref. Modern fractional-N PLLs achieve sub-hertz frequency resolution while maintaining crystal stability. Most contemporary synthesizer ICs (ADF4350, Si5351, MAX2870) use fractional-N techniques.

Why do some PLLs have a reference spur problem and others do not?

Reference spurs occur because the charge pump does not produce a perfectly clean DC output — it injects small current pulses at the reference frequency into the loop filter even when locked. Non-ideal effects like charge pump current mismatch, leakage, and delay mismatches cause small residual pulses that modulate the VCO. Better ICs minimize these imperfections, and wider loop filter bandwidth more effectively attenuates spurs at the reference frequency. In critical applications, a second-order or third-order loop filter provides extra spur attenuation, and careful PCB layout prevents substrate coupling of the reference into the VCO signal path.

Test Your Knowledge

Answer the questions below to check your understanding. Every answer can be found in the lesson above.

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