激光测月

用激光测月资料检测板块运动初探

Preliminary Approach to the Plate Motion by Means of LLR Data

在将大气波前倾斜量的实时补偿引入激光测月过程中的理论基础上本论文的目的是研究从低对比度扩展源实时探测与计算大气波前倾斜量的方法。

The goal of this thesis is to study the best algorithm for computing the atmospheric Tip-Tilt real time from low contrast and extended source based on the theory that introduces the real-time compensation for atmospheric Tip-Tilt in LLR .

月球天平动模型对激光测月解算UT0的影响

Influence of the lunar libration models on uto determination from lunar laser ranging

固体潮与海潮对激光测月距的影响

Influence of earth tide and M2 wave of ocean tide on lunar laser ranging

我国进行激光测月的研究

Research on the lunar laser ranging for China

激光测月资料分析中的广义相对论效应

Relativistic effects in lunar laser ranging data analyses

用激光测月法测定地球自转参数的精度估计

Estimates of the internal precision of earth rotation parameters determined by lunar laser ranging

激光测月距中月潮的影响

Influence of lunar tide on LLR

1.56米天体测量望远镜主要用以测定暗弱恒星的三角视差。今后也拟以此望远镜作为激光测月的接收望远镜。

We have designed an astrometric telescope , 1.66 meter in diameter , for determining the trigonometric parallaxes of faint stars .

在现有技术条件下，本文对影响激光测月回波光子数的因素逐一进行分析讨论，提出应该把激光束截面能量分布和大气湍流效应包括进去。

All factors that affect the returned photon numbers of the LLR are analyzed and discussed at current technique condition , and therefore it is proposed to consider the atmospheric turbulence effects and the energy distribution of the laser beam on the LLR .

并讨论了在目前的天体测量新技术如甚长基线干涉仪（VLBI）、激光测卫（SLR）、激光测月（LLR）已成功地用于天文地球动力学的情况下，GPS发展的可能前景。

Under the recent situation that new astronomical technigues , for example , Very Long Baseline Interferometry ( VLBI ), Satellite Laser Ranging ( SLR ) and Lunar Laser Ranging ( LLR ), are successfully applied to astro-geodynamics , the possible trends of GPS are discussed .

涉及到在激光测月中对受大气湍流而畸变的激光束进行补偿，本文抓住重点，通过分析看出对大气倾斜量的实时补偿是提高激光测月回波光子数的重要因素。

For the distorted laser beam compensation on the LLR due to the atmospheric turbulence , It is found that the real-time compensation of the wavefront tilt is an important factor for increasing the returned photon numbers of the LLR .