TL;DR
This paper reviews the current state of LISA technology and instrumentation, detailing the measurement principles, mission architecture, and key payload components essential for gravitational wave detection.
Contribution
It provides a comprehensive overview of the technological components and requirements for the LISA mission, highlighting recent advancements and design considerations.
Findings
Detailed description of the interferometric measurement system
Analysis of disturbance reduction system components
Summary of subsystem requirements for sensitivity
Abstract
This article reviews the present status of the technology and instrumentation for the joint ESA/NASA gravitational wave detector LISA. It briefly describes the measurement principle and the mission architecture including the resulting sensitivity before focussing on a description of the main payload items, such as the interferomtric measurement system, comprising the optical system with the optical bench and the telescope, the laser system, and the phase measurement system; and the disturbance reduction system with the inertial sensor, the charge control system, and the micropropulsion system. The article touches upon the requirements for the different subsystems that need to be fulfilled to obtain the overall sensitivity.
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