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| Main Authors: | , , , , |
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| Format: | Preprint |
| Published: |
2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2508.08950 |
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Table of Contents:
- To meet the urgent need for sub-second link establishment in inter-satellite and satellite-to-ground free space optical communication, this paper presents a periscope-type optical communication terminal and a ground-based verification scheme for its pointing accuracy and acquisition performance, thereby avoiding costly in-orbit tests. This ground-based measurement method takes the positions of stellar constellations in inertial space as its reference. By establishing a theoretical attitude determination model for the optical terminal and analyzing both structural and non-structural error sources that affect its pointing, it proposes an error-compensated, high-precision evaluation technique for open-loop pointing. Combined with laboratory component tests, it also derives a measurement method for acquisition time. Field experiments show that the mean pointing error is reduced from 2070.24 microrad to 120.16 microrad after error correction, corresponding to an improvement exceeding 94%. Acquisition tests report an average equivalent acquisition time of 0.908 s, with every run completed in under 1 s. These results demonstrate that the developed terminal achieves high-precision pointing and sub-second acquisition, and they validate the effectiveness of the proposed ground-based verification method.