MASc Seminar Notice: "Millimeter-wave 39 GHz 4x4 Phased Antenna Array with Embedded Near-field Probing Antenna for Performance Enhancement"

Wednesday, March 15, 2023 4:09 pm - 4:09 pm EDT (GMT -04:00)

Name: Huixin Jin

Date: Thursday 23rd of March  2023

Time: 4:00pm to 5:00pm (EST)

Location: E5-4047

SupervisorSlim Boumaiza

Attending faculty member: Prof. Raafat Mansour

Title: Millimeter-wave 39 GHz 4x4 Phased Antenna Array with Embedded Near-field Probing Antenna for Performance Enhancement

Abstract:

Beamforming arrays are a vital technology for millimeter-wave (mm-wave) wireless communication systems. A large amount of research and an increasing number of phased array prototypes have been developed which provide high data rates and low latency. However, as sub-6 GHz bands have limited bandwidth and crowded spectrum occupation, mm-wave phased arrays are more desirable for future generation systems. Yet, there are challenges with current phased array technologies that need to be addressed by researchers. Linear power amplifier response, radio frequency front-end calibration, and affordable prototyping costs are the main challenges that must be taken into consideration when designing arrays for mm-wave systems.

This seminar presents approaches to these challenges and trade-offs and proposes an optimized design solution. A novel wideband near-field (NF) probing antenna is proposed that can be embedded in mm-wave phased arrays to provide the feedback signal path necessary for carrying out array calibration and digital pre-distortion training. Specifically, the topology and layout of the proposed NF probing antenna have been carefully devised to achieve a coupling to its surrounding antenna elements with flat magnitude and constant group delay. A proof-of-concept 4x4 linear-polarized active phased array prototype with embedded NF probing antennas is designed to operate over 37-41 GHz. Measurements confirm the negligible impact of the NF probing antennas on the antenna array's radiation pattern, and the array prototype was successfully used to train a digital pre-distortion function which enabled the effective isotropic radiated power to be increased from 32 dBm to 34.3 dBm, while maintaining an error vector magnitude below 3.5%, when the array was steered from -50 degrees to +50 degrees.