Design and validation of a high-efficiency RF amplifier for acousto-optic spectrometers.

Applied optics Pub Date : 2026-10-10 Epub Date: 2026-09-22 DOI:10.1364/AO.610160
Pallab Kr Gogoi, Mehmet Şevket Uludağ, Jurgen Vanhamel, Jérôme Loicq
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Abstract

This work presents the design and experimental validation of a space-oriented engineering model of a high-efficiency radio-frequency power amplifier (RFPA) for driving acousto-optic tunable filters (AOTFs) in spaceborne spectroscopy and remote sensing payloads. The proposed RFPA represents the first step toward the development of a flight-capable architecture specifically designed to satisfy the stringent power, thermal, mass, and volume constraints of spacecraft while maintaining high radio-frequency (RF) performance. It employs a compact, small-form-factor architecture operating over the 100-150 MHz frequency range and provides continuous output power tunability to accommodate varying mission requirements without compromising RF spectral purity. Experimental characterization demonstrates a sustained power-added efficiency (PAE) exceeding 65% across the operating band, with continuous output power tunability. The amplifier also achieves harmonic suppression of better than -30 dBc, ensuring compliance with spectral purity requirements for sensitive spaceborne instrumentation.

声光光谱仪用高效射频放大器的设计与验证。
本文提出了一种面向空间的高效射频功率放大器(RFPA)工程模型的设计和实验验证,该模型用于驱动星载光谱和遥感有效载荷中的声光可调谐滤波器(AOTFs)。拟议的RFPA代表了开发飞行能力架构的第一步,该架构专门设计用于满足航天器严格的功率、热、质量和体积限制,同时保持高射频(RF)性能。它采用紧凑的小尺寸架构,工作在100-150 MHz频率范围内,并提供连续输出功率可调性,以适应不同的任务要求,而不影响RF频谱纯度。实验表征表明,在整个工作频段内,持续的功率附加效率(PAE)超过65%,并且具有连续的输出功率可调性。该放大器还实现了优于-30 dBc的谐波抑制,确保符合敏感星载仪器的频谱纯度要求。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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