CYGNI

Power Device Parasitics Analyser

Equipment

Cosmic’s Cygni measures the full set of small-signal parasitics of a power semiconductor – Ciss, Coss, Crss, Cgs and gate resistance – from
100kHz to 5MHz with programmable drain bias to 3kV in a single device insertion. It uses the same measurement core as Cosmic’s M2 and VIP
Ultra production platforms, to seamlessly move between characterisation testing and production screening.

Reasons Why

Complete parasitic set

Ciss, Coss, Crss, Cgs and Rg in one insertion, without re-cabling and under one calibration

Relevant frequency range

Programmable from 100kHz to 5MHz, including the primary 1MHz datasheet correlation point

Bias and precision

Drain bias to 3kV, gate bias to ±30V, bridge-null Rg measurement and software-selectable 4-terminal Kelvin sensing.

Production-ready speed

Under 30ms in high-speed mode, with measurement time reported alongside every reading

Bench-to-line correlation

The same measurement core as Cosmic's M2 and VIP Ultra, with LXI-compatible LAN, SCPI and an embedded web interface

Product Presentation

Power-semiconductor datasheets specify a set of small-signal parasitics – input, output and reverse-transfer capacitance, gate-source capacitance, and gate resistance. Verifying them on a general-purpose LCR meter means four-terminal configurations, four re-cablings and four separate fixture corrections, and the results will still not match the production tester used to screen the parts in volume.

Cygni closes that gap. It is a digital auto-balancing bridge requiring only one calibration cycle that measures the whole parasitic set in a single device insertion, from 100kHz to 5MHz, with a programmable drain bias to 3kV to allow capacitance to be characterised over the DUT’s full voltage range. Because the reading is taken at the bridge null, the phase resolution that gate-resistance extraction depends on is physically available – a matter of measurement architecture, yielding more sensitive measurements.

For production installations, measurements run in under 30ms in high-speed mode and the instrument is built for a minimal handler footprint with a height of just 60mm and the option of soft-dock or hard-dock DUT connection.

Control is via Cosmic’s Linux-based System Software which automates the whole production test cell, whether that be wafer sorting, KGD or packaged device testing. For characterisation use, the interface is LXI-compatible LAN with SCPI commands, or through a comprehensive stand-alone embedded web interface that needs no software installed.

FEATURES

CYGNI

Consumption
≤60W (typ. 30W); 90 – 264V AC, 47 – 63Hz
Quality Assurance
Traceable verification report: 48 reference devices across 6 frequencies
built-in self-test
Temperature Control
Internal thermal and supply monitoring with protective shutdown
no DUT temperature forcing

Dimensions

D⨯W⨯H
330 mm ⨯ 407 mm ⨯ 60mm
Weight
6.5kg

Absolute maximum voltage

Withstand voltage
Programmable drain bias to 3kV

Misc.

Gate Resistance
Measured for Cg >= 1nF
±(1% + 0.05Ω) in high-repeatability mode
Parasitic Stray Inductance
Fixture residuals characterised and corrected by the calibration module
4-terminal Kelvin sensing removes the fixture's resistive contribution

Additional instruments

High-speed digitizer
Coherent digital acquisition of both bridge nodes with live waveform display (Characterisation mode)

Analog/Power

Drain High Voltage Power Supply
Programmable to 3kV
Gate Voltage Power Supply
Programmable, ±30V

DC Measure

Accuracy
Forcing accuracy at the DUT: Gate ±3mV; Drain ±(0.5V + 0.1% of setting).
Read-back accuracy: typ. ±5mV (Gate), typ. ±1% (Drain)
Resolution
Gate:1.2mV, Drain: 100mV

DC Source

Voltage
Drain: 3kV programmable
Gate: ±30V programmable

Measurements instruments

Digitizer
Coherent digital acquisition of both bridge nodes, with live waveform display
LCR meters
Digital auto-balancing bridge, 100kHz to 5MHz

Scalability

Number of instrumentation slots
n/a
Number of test sites
1 site
two devices tested sequentially via an internal switch matrix

System

Minimum Requirements
Stand-alone: web browser and Ethernet connection (no software to install); SCPI over LAN for remote control.
Production test cell: Cosmic HPT Linux system software (version to be confirmed by Cosmic)
Certifications
SEMI S2/S8 compliant
CE / UKCA - pending

More info

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