Terahertz and Emerging Frequencies Additional THz Topics Informational

How do I design a frequency extender module for extending VNA measurements above 110 GHz?

Designing a frequency extender module for extending VNA measurements above 110 GHz converts the VNA's microwave test signal (typically 10-20 GHz) to the target mmW or THz frequency band using frequency multiplication and harmonic mixing, enabling S-parameter measurements at frequencies far beyond the VNA's native range. The frequency extender architecture consists of: a transmit path (the VNA's source signal at frequency f_LO (approximately 10-20 GHz) is multiplied by a factor N (typically 6, 12, 18, or 24) using a Schottky diode multiplier chain to generate the test signal at N x f_LO; for a WR-3.4 (220-330 GHz) extender: 18× multiplication from a 12-18 GHz source), a receive path (the reflected or transmitted signal from the DUT returns to the extender and is downconverted to an IF signal by mixing with a harmonic of the LO signal; a subharmonic mixer uses the LO at f_LO and mixes with the RF signal at approximately N x f_LO, producing an IF at a few MHz that is sent back to the VNA for magnitude and phase measurement), and the waveguide test ports (the extender module has a waveguide port (WR-X flange) that connects to the DUT; the waveguide size determines the frequency band). The design challenges are: generating sufficient signal power (each multiplication stage has conversion loss of 8-15 dB; for 18× multiplication through three 6× stages: total conversion loss approximately 30-45 dB; the output power at 300 GHz is typically 0.1-1 mW), achieving adequate dynamic range (the system dynamic range must be sufficient to measure both the DUT's insertion loss and return loss; typical extender dynamic range: 50-90 dB depending on the frequency; this is reduced from the VNA's native dynamic range (120+ dB) due to the multiplication loss and mixer noise figure), and calibration (the extender introduces its own systematic errors (source match, load match, directivity) that must be removed through VNA calibration; calibration at mmW/THz frequencies uses: waveguide calibration standards (short, offset short, load, thru), TRL (Thru-Reflect-Line) calibration, or on-substrate calibration for on-wafer measurements).
Category: Terahertz and Emerging Frequencies
Updated: April 2026
Product Tie-In: THz Components, Detectors

THz Frequency Extender Design

Frequency extender modules are the enabling technology for characterizing mmW and THz components. Without extenders, S-parameter measurements above 110 GHz would require dedicated THz VNAs (which are extremely expensive and limited in availability).

  • Performance verification: confirm specifications against the application requirements before finalizing the design
  • Environmental factors: temperature range, humidity, and vibration affect long-term reliability and parameter drift
  • Cost vs. performance: evaluate whether the application demands premium components or standard commercial grades
  • Interface compatibility: verify impedance, connector type, and mechanical form factor match the system architecture
  • Margin allocation: include sufficient design margin to account for manufacturing tolerances and aging effects
Common Questions

Frequently Asked Questions

How do I calibrate at these frequencies?

Calibration removes the systematic errors of the VNA, cables, and extender modules. At mmW/THz frequencies: use waveguide calibration standards (a set of precision waveguide shorts, offset shorts, loads, and thru connections). TRL (Thru-Reflect-Line) calibration is preferred because: the Line standard can be made with high precision (it is simply a section of waveguide), the Reflect standard is a flat short (trivial to make), and TRL does not require a broadband matched load (which is difficult to make at THz). Calibration uncertainty: ±0.5 dB for S21, ±2-3 dB for S11 at frequencies up to 500 GHz.

What dynamic range can I achieve?

The dynamic range depends on: the output power (0.1-1 mW at 200-300 GHz, decreasing to 1-100 uW at 500-1100 GHz), the mixer conversion loss (15-30 dB), the IF bandwidth (narrower BW = better dynamic range), and the IF amplifier noise figure. Typical dynamic range: WR-3.4 (220-330 GHz): 70-90 dB. WR-1.5 (500-750 GHz): 50-70 dB. WR-1.0 (750-1100 GHz): 40-60 dB. For comparison: a standard microwave VNA achieves 120+ dB dynamic range.

Can I do on-wafer measurements?

Yes. On-wafer probing at mmW/THz frequencies uses waveguide-to-coplanar waveguide (CPW) probe tips. Probe manufacturers (GGB Industries, FormFactor/Cascade) offer probes rated to WR-3.4 (330 GHz) and beyond. The probe station must: be vibration-isolated, have sub-micrometer positioning resolution, and accommodate the waveguide extender modules close to the wafer surface. On-wafer calibration uses TRL or LRRM standards fabricated on a reference substrate provided by the probe manufacturer.

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