Abstract

The beam formation can be treated as the diffraction pattern. A 1-D light detection and ranging beam steering could be derived through a phase shifter array using Rayleigh–Sommerfeld Diffraction, which is then utilized to demonstrate grating lobe-free beam steering from the optical phase array emitter with half-wavelength pitches. The half-wavelength pitch cannot demonstrate beam formation without any evanescent coupling blocking between emitters. Here, two index-mismatched silicon wires in the emitter array are proposed by the optical phase compensation through waveguide width adjustment, to avoid the complex and addressable thermal control on the phase shifters. Moreover, the same output optical waveguide mode needs to be further considered to demonstrate the grating lobe-free beam steering. In order to get the adiabatic connection between two different pitches between the phase shifter and emitter, an optical path equalization will also be applied.

Highlights

  • Phase arrays have existed for more than a century

  • The optical phase array (OPA) shows no inertia phenomena, reaches large steering angles at high speed, and has the potential to be integrated into a small foot print

  • The OPA was first developed on the silicon wire-based waveguide array through the optical splitter, phase manipulation, and emitter [1,2]

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Summary

Introduction

Phase arrays have existed for more than a century. Their application in radar in the RF field plays an important role in beam forming and steering. The OPA was first developed on the silicon wire-based waveguide array through the optical splitter, phase manipulation, and emitter [1,2]. In order to get an identical phase shift on each stage of N emitters through log N voltages, the phase difference from the index-mismatched waveguides needs to be matched. The traditional method of calculating beam steering is phase array theory. The finite difference time domain (FDTD) is used to calculate the intensity distribution of a single antenna and followed by the phase array theory. We can quickly obtain the beam steering result through phase manipulation This beam formation can be from a uniformly/non-uniformly spaced optical phased array through RSD formula under different pitches. The RSD-based genetic algorithm can even be utilized to experimentally facilitate phase distribution

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