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For the laser ablation propulsion in space, the rule of the pulse energy from ground-based lasers is studied, in which both the complex beam propagation effects in the turbulent atmosphere of a real-world scenario and the momentum coupling of laser-matter interaction in space are considered. The analytical propagation formulae of laser beams in the turbulent atmosphere along a slant path are derived, and the fitting formula of optimized pulse width is obtained. In particular, the analytical rule of the pulse energy from ground-based lasers to reach the threshold and optimal momentum coupling of laser-matter interaction is derived. It is necessary to increase the laser altitude in order to reach the threshold momentum coupling of laser-matter interaction in space. Furthermore, by ground-based lasers, the several nanoseconds pulse width at the target (e.g., around 1 ns) may be suitable for the laser ablation propulsion, and the removal of the centimeter-scale space debris is much more suitable than the meter-scale one.
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http://dx.doi.org/10.1364/OE.554720 | DOI Listing |
Sensors (Basel)
July 2025
Xi'an Institute of Optics and Precision Mechanics, Chinese Academy of Sciences, Xi'an 710119, China.
To enable accurate evaluation of satellite laser communication terminals under solar outage interference, this paper presents the design and implementation of a solar radiation simulation system targeting the 1540-1560 nm communication band. The system reconstructs co-propagating interference conditions through standardized and continuously tunable output, based on high irradiance and spectral uniformity. A compound beam homogenization structure-combining a multimode fiber and an apodizator-achieves 85.
View Article and Find Full Text PDFFor the laser ablation propulsion in space, the rule of the pulse energy from ground-based lasers is studied, in which both the complex beam propagation effects in the turbulent atmosphere of a real-world scenario and the momentum coupling of laser-matter interaction in space are considered. The analytical propagation formulae of laser beams in the turbulent atmosphere along a slant path are derived, and the fitting formula of optimized pulse width is obtained. In particular, the analytical rule of the pulse energy from ground-based lasers to reach the threshold and optimal momentum coupling of laser-matter interaction is derived.
View Article and Find Full Text PDFLow and dense cloud cover is often encountered in daily observing experiments with lidar. In such scenarios, the laser cannot penetrate the clouds and it is not possible to use the clean atmosphere to initially calibrate the calibration heights required for the actual inversion, which can pose a significant challenge to the inversion of aerosols under clouds. This paper proposes an iterative proximal calibration algorithm based on slope method and Fernald's backward integral equation, combined with the inherent observational mode characteristics of the micro infrared lidar (mIRLidar).
View Article and Find Full Text PDFOpt Express
June 2025
For ground-based segmented telescopes, the active control system primarily adjusts three out-of-plane DOFs: tip, tilt, and piston. In contrast, in-plane DOFs rely on high-precision mechanical alignment. A systematic analysis of the effects of in-plane motion on the optical performance of ring segmented mirror systems is presented, and an analytical relationship between in-plane motion and the higher-order residual aberrations after tilt compensation is derived.
View Article and Find Full Text PDFPhys Rev Lett
May 2025
University of Hamburg, Institute for Experimental Physics, Luruper Chaussee 149, 22761 Hamburg, Germany.
A major limitation of laser interferometers using continuous wave lasers are parasitic light fields, such as ghost beams, scattered or stray light, that can cause nonlinear noise. This is especially relevant for laser interferometric ground-based gravitational wave detectors. Increasing their sensitivity, particularly at frequencies below 10 Hz, is threatened by the influence of parasitic photons.
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