Document ID: AN-5G-TIMING-011
Revision: 1.0
Target Audience: RF Engineers, 5G Base Station Designers, Timing & Synchronization Specialists
1. Introduction
5G New Radio (NR) networks impose the most demanding timing specifications in the history of commercial wireless communications. From the sub-500-nanosecond phase alignment required for massive MIMO beamforming to the ±50 ppb frequency accuracy mandated for macro cell synchronization, every stage of the base station clock chain must be engineered with precision as the primary objective.
This application note provides a complete technical guide to 5G base station clock chain design, starting from the oscillator selection decision and working through phase noise budgeting, jitter analysis, holdover planning, and practical PCB implementation. Whether you are designing a cost-optimized small cell or a high-performance macro base station, this guide gives you the quantitative framework to make engineering trade-offs with confidence.
2. 5G Timing Requirements Overview
Understanding the 3GPP specifications is the foundation of any clock chain design. Timing errors manifest as degraded signal quality, reduced cell coverage, inter-cell interference, and ultimately dropped connections.
2.1 Frequency Accuracy Requirements
All 5G NR base stations must maintain carrier frequency accuracy within tight tolerances relative to the network reference:
| Base Station Class | 3GPP Frequency Accuracy | Typical Application |
|---|---|---|
| Macro Cell (FR1) | ±50 ppb | Outdoor macro eNB/gNB, tower-mounted radios |
| Micro / Pico Cell | ±100 ppb | Dense urban small cells, indoor enterprise |
| Small Cell (FR1) | ±100 ppb (or ±250 ppb for some Class B) | Indoor/outdoor small cells, neutral host |
| mmWave (FR2) Macro | ±50 ppb | 28 GHz, 39 GHz macro deployments |
| mmWave Small Cell | ±100 ppb | FR2 small cells |
The ±50 ppb macro cell requirement translates to a frequency error of no more than 50 Hz at a 1 GHz carrier frequency. This is equivalent to a 5-second Allan deviation of better than 5×10⁻⁸—a specification that immediately rules out free-running TCXOs and even many un Disciplined OCXOs without external correction.
2.2 Time and Phase Alignment Requirements
Beyond frequency accuracy, 5G NR defines strict time synchronization requirements that directly impact hardware architecture:
| Requirement | Specification | Standard / Feature |
|---|---|---|
| Time Division Duplex (TDD) alignment | ±1.5 µs between cells | 3GPP TS 36.133, eICIC/FeICIC |
| Enhanced Inter-Cell Interference Coordination | ±260 ns for eICIC | 3GPP Release 10+ |
| Coordinated Multipoint (CoMP) — ideal backhaul | ±130 ns | 3GPP Release 11+ |
| 5G NR TDD — intra-band contiguous CA | ±65 ns between component carriers | 3GPP TS 38.133 |
| URLLC (Ultra-Reliable Low Latency) | ±65 ns or tighter | 3GPP URLLC deployment profile |
These sub-microsecond requirements are what distinguish 5G timing from previous cellular generations. In LTE, the ±1.5 µs TDD requirement was the primary constraint. In 5G NR, CoMP and carrier aggregation push the requirement down by an order of magnitude.
3. Clock Chain Architecture
A typical 5G base station clock chain consists of five functional stages, each contributing noise and complexity. Understanding what each stage does—and how it degrades the signal—is essential to allocating your phase noise and jitter budget correctly.
3.1 Typical Clock Chain Topology
1PPS + 10 MHz
OCXO / TCXO / Rb
Fanout / Level Shift
DPLL / ADPLL
CPRI/eCPRI/ETH
DAC / LO / PA
3.2 Stage-by-Stage Analysis
Stage 1: Reference Input (GNSS / Sync Port)
The synchronization input—typically a GNSS receiver disciplining an OCXO or a network timing input (IEEE 1588 PTP, SyncE)—provides the long-term frequency accuracy reference. The quality of this reference determines the ultimate stability of the system. GNSS timing receivers typically deliver ±20–50 ns accuracy relative to UTC under nominal conditions, but this degrades during outages.
Stage 2: Reference Oscillator — The Core of the Chain
The local oscillator is the single most important component in the clock chain. It sets the floor for phase noise, Allan deviation, and holdover performance. The three mainstream choices for 5G base stations are:
- TCXO (Temperature-Compensated Crystal Oscillator): Best suited for cost-sensitive small cells where holdover duration is short and frequency accuracy is provided by the network (PTP, SyncE). Typical frequency stability: ±0.5 ppm to ±2.5 ppm over operating temperature.
- OCXO (Oven-Controlled Crystal Oscillator): The standard choice for macro base stations. Maintains ±5 ppb to ±50 ppb with excellent short-term stability. Requires warm-up time (30–60 seconds) and consumes more power (1–4 W).
- Rubidium Oscillator: Provides sub-ppb frequency stability and multi-hour holdover capability. Used in carrier-grade macro cells where extended GNSS outage tolerance is required. Higher cost and power consumption than OCXO.
Stage 3: Clock Buffer / Fanout
The clock buffer distributes the reference signal to multiple destinations—DPLL inputs, SERDES PHYs, radio unit converters—without degrading the signal integrity. Key specifications:
- Output-to-output skew: Must be <50 ps for clock domains that require tight alignment
- Additive phase noise: Low-skew buffers add typically <-120 dBc/Hz at 10 kHz offset
- Propagation delay: Matters for systems with multiple clock domains
Stage 4: Digital PLL (DPLL / ADPLL)
The DPLL cleans up any residual jitter from the reference and oscillator, generating multiple output frequencies while tracking the reference input. For 5G base stations, the DPLL must meet the 3GPP TSOC (Time and Frequency Stability Output Clock) requirements, which specify maximum Time Interval Error (TIE) and Maximum Time Interval Error (MTIE) masks. The DPLL's noise contribution should be at least 10 dB below the oscillator's phase noise floor in the integration band of interest.
Stage 5: SERDES and Radio Unit
The backhaul and fronthaul interfaces (CPRI, eCPRI, 10GbE, 25GbE) and the radio unit converters (DAC/ADC sampling clocks, local oscillator synthesis PLLs) all place jitter requirements on the clock chain. For example, a 10GBASE-KR Ethernet link operating at 10.3125 Gbps requires RMS jitter well below 1 ps to achieve acceptable bit error rates at the target signal-to-noise ratio.
4. TCXO vs OCXO Selection Decision Tree
Selecting the wrong oscillator type is one of the most expensive mistakes in base station design—either you over-spend with an OCXO in a cost-sensitive small cell, or you find yourself failing 3GPP compliance tests six months before product launch. This decision tree walks you through the trade-offs systematically.
Review 3GPP requirements in Section 2 to determine your ±50 ppb (macro) or ±100 ppb (small cell) frequency accuracy requirement.
Path A — Small Cell / Cost-Sensitive Design
If your design falls into the small cell category, the oscillator choice is typically driven by cost and power budgets. However, "small cell" does not mean "no timing requirements." Even small cells must meet 3GPP ±100 ppb for frequency and maintain TDD slot alignment.
For small cells disciplined by IEEE 1588 PTP or SyncE, the TCXO does not need to hold frequency accuracy on its own—it only needs to provide short-term stability between PTP correction cycles. Focus on:
- Frequency stability over temperature: ±0.5 ppm or better across –40°C to +85°C
- Aging: ±1 ppm/year or better (PTP will correct long-term drift)
- Phase noise: –80 dBc/Hz at 1 kHz offset, –100 dBc/Hz at 10 kHz offset for a 10 MHz reference
- Voltage control (VC-TCXO): Required if the DPLL needs to steer the oscillator
- G-Sensitivity: <0.5 ppb/g if the unit will be deployed on street furniture with vibration
Path B — Macro Cell with Holdover Requirement
Macro cells on tower rooftops or outdoor cabinets typically have clear GNSS sky visibility. Indoor macro cells, building-mounted units, or urban canyon deployments may have intermittent GNSS reception.
Path B1 — Disciplined OCXO (Reliable GNSS)
When GNSS is reliably available, pair a GPSDO (GNSS Disciplined Oscillator) module with a quality OCXO. The GPSDO steers the OCXO via its control voltage, achieving both excellent long-term accuracy (from GNSS) and superior short-term stability (from the OCXO). This is the most common architecture for outdoor macro cells.
Recommended architecture: GNSS-Disciplined Oscillators for Telecom Infrastructure (AN-005)
- Frequency stability: ±5 ppb to ±20 ppb over –40°C to +70°C (after discipline)
- Holdover (un Disciplined): ±50 ppb to ±100 ppb over 24 hours
- Phase noise at 10 MHz: –90 dBc/Hz at 1 Hz, –130 dBc/Hz at 1 kHz, –150 dBc/Hz at 10 kHz
- Allan deviation (ADEV): <1×10⁻¹² at τ=1s (tau-1)
- Warm-up time: <3 minutes to ±50 ppb at 25°C
- Control voltage range: 0 to +5 V or ±5 V, with at least ±0.5 ppm tuning range
Path B2 — OCXO with Holdover Budget Analysis
When GNSS outages are anticipated (urban canyon, indoor, antenna fault risk), you must perform a holdover budget analysis to determine whether an OCXO is sufficient or whether you need to escalate to a rubidium oscillator.
See Section 7: Holdover Analysis for the quantitative method.
Path C — Rubidium-Level Holdover
For rubidium-based solutions, BRIDZA offers the STM-Rb-N miniature rubidium oscillator, which delivers ±0.001 ppb frequency stability with holdover times measured in days rather than hours. Pair it with a GPSDO module for continuous discipline and autonomous holdover capability.
If you need better than TCXO holdover but cannot justify a rubidium oscillator, consider a disciplined TCXO (GPSDO module with a high-quality TCXO as the local oscillator). This hybrid approach delivers:
- ±0.5 ppb frequency accuracy when GNSS is available
- 1–4 hours of holdover at ±100 ppb (depending on TCXO stability)
- Significantly lower cost and power than an OCXO + GPSDO combination
- Trade-off: poorer phase noise floor than an OCXO, and limited holdover duration
Use our GNSS PTP Accuracy Estimator to model the expected performance for your specific GNSS constellation and PTP profile.
5. Phase Noise Budget Example
This section walks through a complete phase noise budget for a 5G macro base station clock chain. The goal is to ensure that the combined noise contribution of all stages stays within the limits required by the 3GPP TDD alignment specification of ±260 ns.
5.1 System Configuration
Clock chain: GNSSDO reference → OCXO → Clock Buffer → DPLL → 10 MHz Output
5.2 Phase Noise Contributions at 10 MHz
| Stage | Noise Source | Typical Contribution @ 1 kHz | @ 10 kHz | @ 100 kHz |
|---|---|---|---|---|
| 1. GNSSDO Reference | GNSS satellite + receiver noise floor | –90 dBc/Hz | –105 dBc/Hz | –120 dBc/Hz |
| 2. OCXO (e.g., ST36GAH10-5V) | Inherent crystal + PLL noise floor | –130 dBc/Hz | –145 dBc/Hz | –152 dBc/Hz |
| 3. Clock Buffer (e.g., 5P49V6965) | Additive noise, thermal noise floor | –150 dBc/Hz | –152 dBc/Hz | –155 dBc/Hz |
| 4. DPLL (e.g., TI CDCM6208) | Loop-filter noise, VCO contribution | –135 dBc/Hz (loop BW = 100 Hz) | –148 dBc/Hz | –155 dBc/Hz |
| Combined (RSS) | Dominant: GNSSDO @ low offset, OCXO @ mid | –89 dBc/Hz | –104 dBc/Hz | –120 dBc/Hz |
The combined phase noise is dominated by the GNSSDO reference at low frequency offsets (1 Hz to 1 kHz), where the DPLL loop has not yet attenuated the reference noise. Above the DPLL loop bandwidth (~100 Hz), the OCXO's inherent noise floor takes over. The clock buffer contributes negligibly across the entire offset range—this is the expected result of proper buffer selection.
5.3 Visual Budget Breakdown
| Offset Freq | GNSSDO | OCXO | DPLL |
|---|---|---|---|
| 10 Hz | –80 dBc/Hz | –110 dBc/Hz | –78 dBc/Hz (tracking) |
| 100 Hz | –100 dBc/Hz | –130 dBc/Hz | –130 dBc/Hz |
| 1 kHz | –90 dBc/Hz | –130 dBc/Hz | –148 dBc/Hz |
| 10 kHz | –105 dBc/Hz | –145 dBc/Hz | –152 dBc/Hz |
| 100 kHz | –120 dBc/Hz | –152 dBc/Hz | –155 dBc/Hz |
| 1 MHz | –140 dBc/Hz | –155 dBc/Hz | –160 dBc/Hz |
Use the Phase Noise Budget Calculator to model your specific clock chain. Input the noise contributions from each stage and compute the integrated RMS jitter across any frequency range.
6. Jitter Calculation for SERDES
5G base station fronthaul and backhaul interfaces rely on high-speed serial links (SERDES) to transport IQ data between the DU (Distributed Unit) and RU (Radio Unit). These links operate at multi-Gbps rates and are extremely sensitive to clock jitter.
6.1 RMS Jitter from Phase Noise
RMS jitter is the integral of phase noise power across the frequency offset range that falls within the SERDES tracking bandwidth. The formula:
Jitter_RMS = sqrt( 2 × ∫[f_min to f_max] L(f) df ) [radians RMS]
Where:
L(f) = single-sideband phase noise (dBc/Hz)
f_min = integration lower bound (typically 100 Hz for SERDES)
f_max = integration upper bound (typically 10 MHz for SERDES)
Convert to seconds: Jitter(ps_RMS) = Jitter_RMS / (2π × f_carrier) × 1e12
6.2 CPRI/OBSAI Jitter Requirements
The Common Public Radio Interface (CPRI) and Open Base Station Architecture Initiative (OBSAI) standards define jitter masks for the recovered clock in fronthaul links:
| Interface | Line Rate | Max RMS Jitter | Measurement Band |
|---|---|---|---|
| CPRI Option 3 | 2.4576 Gbps | <1.5 ps RMS | 12 kHz – 20 MHz |
| CPRI Option 5 | 4.9152 Gbps | <1.0 ps RMS | 12 kHz – 20 MHz |
| CPRI Option 6 | 6.144 Gbps | <0.8 ps RMS | 12 kHz – 20 MHz |
| CPRI Option 7 | 9.8304 Gbps | <0.7 ps RMS | 12 kHz – 20 MHz |
| CPRI Option 8 | 10.1376 Gbps | <0.65 ps RMS | 12 kHz – 20 MHz |
| 10GBASE-KR | 10.3125 Gbps | <0.6 ps RMS | 1.875 MHz – 20 MHz |
Given a 10 MHz clock with combined phase noise of –89 dBc/Hz at 1 kHz, –104 dBc/Hz at 10 kHz, and –120 dBc/Hz at 100 kHz, the RMS jitter integrated from 12 kHz to 20 MHz is approximately 0.4 ps RMS—well within the CPRI Option 8 requirement of <0.65 ps.
Use the Phase Noise to Jitter Calculator to compute your specific integrated jitter value from measured phase noise data.
6.3 Jitter Transfer Through the Clock Chain
The DPLL acts as a low-pass filter for reference jitter at frequencies above its loop bandwidth. A typical DPLL with 100 Hz loop bandwidth will:
- Pass reference jitter below ~100 Hz with unity gain (phase errors propagate directly)
- Attenuate reference jitter above ~1 kHz by 20 dB/decade (40 dB/decade for 2nd-order loop)
- Generate additional in-band DPLL noise proportional to the loop bandwidth
This means the DPLL provides significant jitter cleaning for high-frequency reference noise but cannot fix slow GNSS disciplining loops that drift at 0.001 Hz or slower.
7. Holdover Analysis
Holdover is the period during which a base station must maintain synchronization after losing its primary reference (GNSS, PTP, or SyncE). The duration you must support depends on your site's MTBF for reference outages—antenna cable failures, GNSS jamming, network timing disruptions—and your SLA with the network operator.
7.1 The Holdover Equation
The timing error accumulated during a holdover interval is directly proportional to the oscillator's frequency offset and the duration of the outage:
Time Error (ns) = Frequency Offset (ppb) × Holdover Duration (seconds)
Rearranged for holdover duration:
Holdover Duration (s) = Time Error Budget (ns) / Frequency Offset (ppb)
For 3GPP ±260 ns requirement with OCXO (±10 ppb drift):
Holdover Duration = 260 ns / 10 ppb = 26,000 seconds = 7.2 hours
For TCXO (±500 ppb drift):
Holdover Duration = 260 ns / 500 ppb = 0.52 seconds
The calculation above reveals why TCXOs alone cannot support the ±260 ns eICIC requirement during GNSS outages. A typical TCXO with ±0.5 ppm (±500 ppb) drift will accumulate the 260 ns error budget in just 0.52 seconds. For any practical outage scenario, an OCXO or rubidium oscillator is mandatory. A TCXO can only be used in small cells where:
- The timing reference is network-based (PTP/SyncE) with sub-second re-convergence
- The ±260 ns eICIC requirement does not apply (e.g., isolated cell, no neighboring cells)
- The holdover duration is effectively zero because the backup reference (PTP grandmaster) is always available
7.2 Holdover Time Table by Oscillator Type
| Oscillator | Typical Freq. Drift | Time Error @ 1 sec | Time Error @ 1 min | Time Error @ 1 hour | Time Error @ 8 hours | Time Error @ 24 hours | Max Holdover @ 260 ns |
|---|---|---|---|---|---|---|---|
| Standard TCXO | ±500 ppb | ±0.5 ns | ±30 ns | ±1,800 ns | ±14,400 ns | ±43,200 ns | 0.52 seconds |
| High-Stability TCXO | ±100 ppb | ±0.1 ns | ±6 ns | ±360 ns | ±2,880 ns | ±8,640 ns | 2.6 seconds |
| OCXO (standard) | ±10 ppb | ±0.01 ns | ±0.6 ns | ±36 ns | ±288 ns | ±864 ns | 26 seconds |
| OCXO (high-stability) | ±2 ppb | ±0.002 ns | ±0.12 ns | ±7.2 ns | ±57.6 ns | ±172.8 ns | 130 seconds |
| Rubidium (Rb) | ±0.001 ppb | ±0.000001 ns | ±0.00006 ns | ±0.0036 ns | ±0.0288 ns | ±0.0864 ns | 260,000 seconds (~3 days) |
The "Max Holdover @ 260 ns" column shows how long each oscillator type can maintain the 3GPP ±260 ns eICIC timing budget without external discipline. Only rubidium oscillators provide full-day holdover capability. High-stability OCXOs (~±2 ppb) can provide about 2 minutes of holdover—useful for bridging brief GNSS interruptions but insufficient for extended outages. This is why carrier-grade macro cells use rubidium oscillators or implement automatic failover to PTP grandmaster redundancy.
7.3 Allan Deviation and Holdover
Allan deviation (ADEV) is the preferred metric for characterizing oscillator stability over the holdover interval. Unlike variance-based metrics, ADEV does not diverge for non-stationary noise processes (random walk frequency modulation) that dominate at long averaging times.
For holdover analysis, focus on the ADEV at τ = 1,000 s to τ = 10,000 s (corresponding to 17-minute to 3-hour outages). Typical values:
- TCXO: 10⁻⁸ to 10⁻⁹ (τ=10,000 s) — insufficient for holdover
- OCXO: 10⁻¹⁰ to 10⁻¹¹ (τ=10,000 s) — useful for short outages
- Rubidium: 10⁻¹¹ to 10⁻¹² (τ=10,000 s) — multi-hour holdover capable
Use the Allan Deviation Calculator to compute ADEV from frequency stability measurements and estimate holdover error.
8. Practical Design Tips
A well-specified clock chain can still fail if the PCB implementation does not control noise coupling and thermal effects. These practical guidelines address the most common clock chain design errors in base station hardware.
8.1 PCB Layout for Clock Signals
- Use a dedicated clock plane: Route the reference clock (10 MHz, 122.88 MHz) on an isolated microstrip or stripline with a solid reference plane beneath it. Avoid crossing other signal planes—every via is a potential impedance discontinuity and radiation source.
- Maintain 50 Ω characteristic impedance: Use controlled-impedance traces (±10% tolerance) for all clock lines. For 122.88 MHz clocks driving multiple loads, use daisy-chain or star topology based on your buffer's drive strength.
- Keep clock traces short: Minimize trace length to reduce susceptibility to electromagnetic interference. For differential clock pairs (LVDS, LVPECL, CML), maintain strict pair length matching (<5 mil difference for critical paths).
- Isolate clock domains: Place the reference oscillator, buffer, and DPLL in a designated clock management zone on the PCB. Use ground slots or keep-out areas to prevent digital switching noise from coupling into the clock path.
8.2 Power Supply Noise
- Dedicated LDO for the oscillator: Never share the oscillator supply rail with digital loads. Use a low-noise LDO (output noise <10 µV RMS, PSRR >60 dB at 10 kHz) to power the OCXO/TCXO. Switching regulators—even those with post-LDO filtering—can introduce spurious signals into the clock path.
- Filter the DPLL supply: DPLL devices are sensitive to supply noise on their reference and VCO supply pins. Add an LC filter ( ferrite bead + capacitor) between the LDO and the DPLL analog supply pins.
- Spreading clock buffer load: Clock buffers driving multiple output stages (SERDES PLLs, DAC clocks, radio unit PLLs) should be powered from a separate supply domain from the loads to prevent load current transients from feeding back into the clock distribution network.
8.3 Thermal Management
- OCXO temperature gradient: OCXOs are sensitive to thermal shock and temperature gradients across the crystal assembly. Place the OCXO away from heat-generating components (power amplifiers, LDOs, FPGAs). Maintain at least 15 mm clearance and ensure forced-air cooling does not create turbulence directly over the oscillator.
- Temperature compensation: If using TCXOs, account for self-heating (typically 2–5°C above ambient under normal operation). The oscillator's frequency vs. temperature curve is usually characterized over the external operating temperature range—internal self-heating can shift the effective operating point.
- Thermal simulation: Run a thermal simulation of the clock zone to identify hot spots. TCXOs and OCXOs specified for –40°C to +85°C operation may exhibit degraded stability if the local temperature exceeds the rated maximum.
8.4 Bypass Capacitor Selection
- Oscillator VCC bypass: Place a 10 µF tantalum or ceramic capacitor (X5R/X7R) as close as possible to the oscillator's VCC pin, followed by a 100 nF ceramic in parallel, followed by a 1 nF ceramic for high-frequency decoupling. The small capacitor (1 nF) handles the sub-nanosecond switching currents.
- DPLL bypass: DPLL devices require careful power supply decoupling per the manufacturer's recommended layout. Typically: 100 nF per power pin, with a 4.7 µF bulk capacitor on the analog supply rail. Follow the datasheet layout religiously—the wrong capacitor ESR can cause loop instability.
- ☐ Oscillator selected matches holdover and phase noise requirements (Section 4)
- ☐ Phase noise budget allocated across all stages (Section 5)
- ☐ SERDES jitter requirement verified for fronthaul interface (Section 6)
- ☐ Holdover duration calculated for worst-case drift scenario (Section 7)
- ☐ Clock traces routed on controlled-impedance dedicated layer
- ☐ Oscillator on dedicated low-noise LDO supply
- ☐ Thermal analysis confirms oscillator stays within rated temperature range
- ☐ Bypass capacitors placed within 3 mm of oscillator and DPLL pins
- ☐ DPLL loop filter components selected per manufacturer simulation tool
9. Component Selection Guide
The following table provides typical specifications for oscillators suitable for 5G base station applications. BRIDZA stocks components across all three categories to support every point in the selection decision tree.
9.1 Oscillator Selection Matrix
| Parameter | TCXO (Small Cell) | OCXO (Macro Cell) | Rubidium (Carrier-Grade) |
|---|---|---|---|
| Frequency Stability | ±0.5 to ±2.5 ppm | ±5 to ±50 ppb | ±0.5 to ±5 ppb |
| Temperature Stability | ±0.5 ppm (–40 to +85°C) | ±5 ppb (–40 to +70°C) | ±0.5 ppb (–25 to +55°C) |
| Aging / Year | ±1 to ±3 ppm | ±5 to ±50 ppb | ±0.001 to ±0.01 ppb |
| Phase Noise @ 10 MHz, 1 kHz | –80 to –90 dBc/Hz | –125 to –140 dBc/Hz | –130 to –145 dBc/Hz |
| Phase Noise @ 10 MHz, 10 kHz | –100 to –110 dBc/Hz | –145 to –155 dBc/Hz | –150 to –160 dBc/Hz |
| Warm-up Time | <2 ms (instantaneous) | 30 s to 5 min | 5 to 15 min |
| Power Consumption | 1–10 mW | 1–4 W | 5–15 W |
| Typical Holdover @ ±260 ns | <1 second | 26 s to 130 s | >72 hours |
| Typical Cost | $2–$15 | $50–$400 | $500–$3,000 |
| Recommended BRIDZA Products | STC3 series TCXO | ST36GAH10-5V, ST20DH10-5V | STM-Rb-N |
9.2 Key Specifications Explained
| Specification | Why It Matters for 5G | Typical Target |
|---|---|---|
| Frequency Stability (over temp) | Determines free-running frequency accuracy without discipline | <±50 ppb for macro, <±500 ppb for small cell |
| Allan Deviation τ=1s | Characterizes short-term stability for SERDES jitter budget | <1×10⁻¹¹ for macro, <1×10⁻⁹ for small cell |
| Phase Noise @ 1 kHz offset | Dominates integrated jitter for CPRI/eCPRI interfaces | <–130 dBc/Hz for macro cell clock |
| Control Voltage Range | Required for DPLL/GPSDO discipline loop | ±5 ppm minimum tuning range |
| G-Sensitivity | Critical for street furniture and tower deployments | <0.5 ppb/g (macro), <1 ppb/g (small cell) |
| Power Supply Rejection Ratio | Prevents supply noise from modulating oscillator frequency | >60 dB PSRR at 10 kHz |
9.3 Cross-Reference: BRIDZA Products for 5G Clock Chains
| Application | Recommended Product | Key Specifications |
|---|---|---|
| 5G Small Cell (FR1) — PTP/SyncE disciplined | STC3-TC15-5V (TCXO) | ±1.5 ppm, –90 dBc/Hz @ 1 kHz, 2.8×2.8 mm |
| 5G Macro Cell — GPSDO OCXO | ST36GAH10-5V (OCXO) | ±5 ppb, –130 dBc/Hz @ 1 kHz, 36×27 mm |
| 5G Macro Cell — Low Phase Noise OCXO | ST20DH10-5V (OCXO) | ±10 ppb, –140 dBc/Hz @ 1 kHz, 20×13 mm |
| 5G Macro Cell — Ultra-Stable OCXO | ST12AER100-5V (OCXO) | ±2 ppb, –135 dBc/Hz @ 1 kHz, oven-compensated |
| Carrier-Grade Holdover — Rb oscillator | STM-Rb-N (Rubidium) | ±0.001 ppb, multi-day holdover, N-series module |
| GNSS Timing Module | STW-NTJ1 (GNSSDO) | Multi-constellation, 1PPS + 10 MHz output |
| GNSS PTP Grandmaster | STW-PTJ1-R | PTP grandmaster, GNSS timing, redundancy-ready |
| Phase Noise Measurement | STW-TFM0-017 | Satellite timing module, Allan deviation traceable |
For a complete comparison of TCXO vs OCXO characteristics including trade-offs, see our OCXO vs TCXO Comparison Guide.
10. Conclusion
5G base station clock chain design is a systems engineering challenge that spans component physics, RF system integration, and network synchronization standards. The oscillator selection—TCXO vs OCXO vs Rubidium—is the single most consequential decision in the clock chain, and it must be driven by a rigorous analysis of your holdover requirements, phase noise budget, and the 3GPP compliance specifications for your deployment scenario.
For most macro cell deployments, the answer is a disciplined OCXO: pair a high-stability OCXO with a GNSSDO module to achieve ±5 ppb frequency accuracy, sub-nanosecond holdover for brief GNSS interruptions, and excellent phase noise for CPRI/eCPRI jitter compliance. For small cells with PTP discipline, a high-quality TCXO reduces cost and power while meeting the ±100 ppb requirement. For carrier-grade applications requiring extended holdover, a rubidium oscillator is the definitive solution.
The clock chain is not a place for cost-cutting—the consequences of a failed timing architecture include 3GPP certification failures, network-level interference, and costly field replacements. Use the decision tree, phase noise budget, and holdover analysis in this application note as your quantitative framework, and engage with BRIDZA's engineering team for component recommendations and evaluation units matched to your specific requirements.
For additional technical specifications, application support, or evaluation units, contact your BRIDZA representative.