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HYB-KA-001

HYB-KA-001

HYB-KA-001

Ka-Band 90° Hybrid Coupler

Ka-Band 90° Hybrid Coupler

HYB-KA-001 is a custom Ka-band 90 degree hybrid coupler covering 26.2 to 26.8 GHz at 0.3 dB insertion loss with better than 20 dB isolation, on a WR-34 waveguide interface. It supports power splitting and combining, balanced amplifier architectures, antenna feed networks and beamforming. The design is based on hardware built for NASA's Solar Dynamics Observatory, whose Ka-band downlink has operated continuously since 2010.

HYB-KA-001 is a custom Ka-band 90 degree hybrid coupler covering 26.2 to 26.8 GHz at 0.3 dB insertion loss with better than 20 dB isolation, on a WR-34 waveguide interface. It supports power splitting and combining, balanced amplifier architectures, antenna feed networks and beamforming. The design is based on hardware built for NASA's Solar Dynamics Observatory, whose Ka-band downlink has operated continuously since 2010.

PRODUCT OVERVIEW

A 90 degree hybrid splits a signal into two equal parts in phase quadrature, or combines two into one, which makes it the building block for balanced amplifier pairs, circular polarization feed networks and beamforming architectures where relative phase governs the design. Holding 3 dB coupling with better than 20 dB isolation and 0.3 dB insertion loss across 600 MHz at 26 GHz is a machining and characterisation problem as much as an electrical one. VSWR holds below 1.5:1 on a WR-34 waveguide interface. The design lineage runs to NASA's Solar Dynamics Observatory, a long-duration on-orbit record for a component of this type. Qualification follows NASA GEVS Table 2.4-3 with 14.1 GRMS overall random vibration, minimum resonant frequency verification, and 0.25 g low-level sine sweeps before and after vibration. Thermal cycling is to mission requirements. S-parameter testing runs from 1 to 40 GHz, with workmanship inspection and acceptance testing before shipment. Custom hybrid couplers from L-band through Ka-band in 90 or 180 degree configurations, coaxial or waveguide, are developed to mission-specific requirements.

A 90 degree hybrid splits a signal into two equal parts in phase quadrature, or combines two into one, which makes it the building block for balanced amplifier pairs, circular polarization feed networks and beamforming architectures where relative phase governs the design. Holding 3 dB coupling with better than 20 dB isolation and 0.3 dB insertion loss across 600 MHz at 26 GHz is a machining and characterisation problem as much as an electrical one. VSWR holds below 1.5:1 on a WR-34 waveguide interface. The design lineage runs to NASA's Solar Dynamics Observatory, a long-duration on-orbit record for a component of this type. Qualification follows NASA GEVS Table 2.4-3 with 14.1 GRMS overall random vibration, minimum resonant frequency verification, and 0.25 g low-level sine sweeps before and after vibration. Thermal cycling is to mission requirements. S-parameter testing runs from 1 to 40 GHz, with workmanship inspection and acceptance testing before shipment. Custom hybrid couplers from L-band through Ka-band in 90 or 180 degree configurations, coaxial or waveguide, are developed to mission-specific requirements.

TECHNICAL SPECIFICATIONS

RF PERFORMANCE

FREQUENCY RANGE

26.2-26.8 GHz

INSERTION LOSS

0.3 dB

ISOLATION

>20 dB

INTEGRATION & QUALIFICATION

APPLICATION

Power splitting/combining; balanced amplifier and beamforming networks

RF CONNECTOR

WR-34 waveguide interface

HUMIDITY

VIBRATION

Typical: 14.1 GRMS random (NASA GEVS Table 2.4-3); 0.25 g low-level sine sweep before/after

SHOCK