Plasma noise in TianQin time delay interferometry

Abstract

TianQin is a proposed geocentric space-based gravitational wave observatory mission, which requires time-delay interferometry (TDI) to cancel laser frequency noise. With high demands for precision, solar-wind plasma environment at $\sim 10^5$ km above the Earth may constitute a non-negligible noise source to laser interferometric measurements between satellites, as charged particles perturb the refractivity along light paths. In this paper, we first assess the plasma noises along single links from space-weather models and numerical orbits, and analyze the time and frequency domain characteristics. Particularly, to capture the plasma noise in the entire measurement band of $10^{-4}-1$ Hz, we have performed additional space-weather magnetohydrodynamic simulations in finer spatial and temporal resolutions and utilized Kolmogorov spectra in high-frequency data generation. Then we evaluate the residual plasma noises of the first- and second-generation TDI combinations. Both analytical and numerical estimations have shown that under normal solar conditions the plasma noise after TDI is less than the secondary noise requirement. Moreover, TDI is shown to exhibit moderate suppression on the plasma noise below $\sim 10^{-2}$ Hz due to noise correlation between different arms, when compared with the secondary noise before and after TDI.

arXiv comment12 pages, 15 figures, accepted by Phys. Rev. D

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Cited by in corpus (4)

• Evaluating residual acceleration noise for TianQin gravitational waves observatory with an empirical magnetic field model
• Doppler effect in TianQin time-delay interferometry
• The Pointing Error Due To Laser Propagation in Space Plasma for TianQin Gravitational Wave Detection
• Modeling coupled constellation dynamics for TianQin under self-gravity