Phase synchronisation system receiver module for the Mid-Frequency Square Kilometre Array

TL;DR

This paper introduces a phase-locked receiver module for the SKA telescope that achieves ultra-low jitter and wide tuning range, addressing phase noise suppression in fiber-linked radio astronomy signals.

Contribution

The paper presents a novel RM architecture that meets stringent jitter, tuning, and size requirements for the SKA, with potential applicability to ngVLA.

Findings

Achieves less than 100 fs output jitter.

Provides 4 MHz tuning range at 3.96 GHz.

Predicts 30 fs jitter through analytical modeling.

Abstract

Next generation radio telescopes, such as the Square Kilometre Array (SKA) and Next Generation Very Large Array (ngVLA), require precise microwave frequency reference signals to be transmitted over fiber links to each dish to coherently sample astronomical signals. Such telescopes employ phase stabilization systems to suppress the phase noise imparted on the reference signals by environmental perturbations on the links; however, the stabilization systems are bandwidth limited by the round-trip time of light travelling on the fiber links. A phase-locked Receiver Module (RM) is employed on each dish to suppress residual phase noise outside of the round-trip bandwidth. The SKA RM must deliver a 3.96 GHz output signal with 4 MHz of tuning range and less than 100 fs of timing jitter. We present an RM architecture to meet both requirements. Analytical modelling of the RM predicts 30 fs of output jitter when the reference signal is integrated between 1 Hz and 2.8 GHz. The proposed RM was conceived with best practice electromagnetic compatibility in mind, and to meet size, weight and power requirements for the SKA dish indexer. As the ngVLA reference design also incorporates a round-trip phase stabilization system, this RM may be applicable to future ngVLA design.