Diagram from the article.
This schematic of the receiver plane illustrates the definition of the laser deflection angle and the laser transverse displacement. The ideal laser beam should be parallel to the z-axis and pass through the intersection point of the x- and y-axis. However, when the real laser beam passes through the space plasma, it generates a deflection of the laser direction (red dashed line) and a displacement of the beam center (red cross). This can introduce pointing accuracy noise in the gravitational wave detection. Credit: Zhou et al. [2026], Figure 2
Editors’ Highlights are summaries of recent papers by AGU’s journal editors.
Source: Space Weather

TianQin is a geocentric space-borne gravitational wave detector, which is proposed to detect the gravitational wave by measuring tiny displacements using inter-satellite laser interferometry. However, the space surrounding the orbit and laser links of TianQin is not a vacuum—but filled with plasma, which can bend the laser links and induce pointing accuracy noise in the gravitational wave detection.

Based on a global magnetohydrodynamic model, Zhou et al. [2026] use a ray-tracing method to obtain the laser deflection caused by laser propagation through plasma, and to evaluate the pointing accuracy noise.  The result shows that the laser deflection effect caused by large-scale space plasma distribution under quiet to moderate space weather conditions does not represent a fundamental risk to the TianQin mission. However, during severe space weather events, the laser propagation effect could become a considerable noise in the gravitational wave detection.

This work establishes a connection between space weather and gravitational wave detection. Furthermore, this work raises awareness of the impact of space weather on other high-precision electromagnetic wave measurements in space.

Citation: Zhou, S. W, Su, W., Zhou, S. Y., Li, C. F., & Zhang, J. X. (2026). The pointing error due to laser propagation in space plasma for TianQin gravitational wave detection. Space Weather, 24, e2025SW004784. https://doi.org/10.1029/2025SW004784

—Jiuhou Lei, Editor, Space Weather

Text © 2026. The authors. CC BY-NC-ND 3.0
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