Charging and Discharging Modeling of Inertial Sensors Based on Ultraviolet Charge Management

Symmetry Pub Date : 2024-09-14 DOI:10.3390/sym16091209
Zihan Zhao, Tao Yu, Shang Wang, Huadong Li, Zhi Wang
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Abstract

Inertial sensors act as inertial references in space gravitational wave detection missions, necessitating that their internal test mass (TM) maintains minimal residual acceleration noise. High-energy particles and cosmic rays in space, along with ion pumps in ground-based torsion pendulum experiments, can cause charge accumulation on the TM surface, leading to increased residual acceleration noise. Consequently, a charge management system was introduced to control the TM’s charge. The complex light path propagation within the electrode housing (EH) makes the TM’s charging and discharging process difficult to theoretically calculate and fully simulate. To address this issue, we propose a simulation method for charging and discharging inertial sensors within ultraviolet (UV) charge management systems. This method innovatively considers the impact of photoelectron emission angle and the TM’s position offset from symmetry on performance. The method also simulates charging and discharging rates over time under conditions of symmetry and preliminarily examines factors affecting the TM’s equilibrium potential. Simulation results indicate that this method effectively models the charge management system’s operation, providing a valuable reference for system design.
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基于紫外线电荷管理的惯性传感器充放电建模
惯性传感器在空间引力波探测任务中充当惯性基准,因此其内部测试质量(TM)必须保持最小的残余加速度噪声。太空中的高能粒子和宇宙射线,以及地面扭摆实验中的离子泵,都会在 TM 表面造成电荷积累,从而导致残余加速度噪声增大。因此,我们引入了电荷管理系统来控制 TM 的电荷。电极外壳(EH)内复杂的光路传播使得 TM 的充放电过程难以理论计算和完全模拟。为了解决这个问题,我们提出了一种在紫外线(UV)充电管理系统中对惯性传感器进行充放电的模拟方法。该方法创新性地考虑了光电子发射角和 TM 位置偏离对称性对性能的影响。该方法还模拟了对称条件下随时间变化的充电和放电速率,并初步研究了影响 TM 平衡电位的因素。模拟结果表明,该方法能有效模拟充电管理系统的运行,为系统设计提供了有价值的参考。
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