Searcharxiv⌕ Search

arXiv subjects

Zhiqian Su

Publications and source records attributed to Zhiqian Su.

2 recordsLinked to original sources

Breakdown of Axis Separability and Structured Inversion in Finite-Domain Normalized Position Measurements: A Quadrant Photodetector Case Study

Finite-domain normalized spatial measurements combine an incident field, geometric support, local response, and channel weighting. These operations can break an otherwise separable response, so accurate single-axis calibration alone does not establish separability of a multidimensional measurement. We represent normalized readouts as channel-weight expectations under a parameter-dependent effective measure. For fixed reception and channel operators, local sensitivity is the covariance between the channel weight and the source score. This representation distinguishes axis separability, parameter mixing, and local recoverability, and applies at the appropriate detector level to continuous-electrode position-sensitive detectors, Shack--Hartmann and pyramid wavefront sensors, back-focal-plane split detection, and finite pixel arrays. A quadrant photodetector (QPD) provides an analytically tractable case. Starting from the complete two-dimensional power integrals, we identify the spatial-moment origin of its lowest-order cross term. Axis calibration and system symmetry then constrain the inverse map, giving Axis-Anchored Cross-Residual Inversion (ACRI). Numerical tests of this QPD realization support the sensitivity relations and show that the constrained cross correction substantially reduces the off-axis bias retained by single-axis inversion. The results illustrate how the general measurement representation guides inverse construction, with performance bounded by the working domain, calibration state, and preserved symmetries.

physics.optics↗

High-accuracy pointing and sub-second acquisition in a space optical communication terminal with ground-based verification method

This paper presents and implements a novel space optical communication terminal achieving high-precision open-loop pointing and sub-second acquisition. We further introduce a simple and accurate ground-based performance test method that enables end-to-end verification without the need for in-orbit experiments. To accurately measure open-loop pointing accuracy and acquisition characteristics, we formulate a comprehensive mathematical error model--covering structural misalignments, installation tolerances, and environmental effects--and estimate calibration parameters from stellar observations via a least-squares solution. Field experiments show a greater than 94% improvement in open-loop pointing accuracy, reducing the mean error from 2070.24 urad to 120.16 urad, and confirm an average acquisition time of 0.908 s with all trials completed in under 1 s. The method is generalizable to large-range, high-precision optical pointing measurements and astronomical observations.

physics.optics↗