利用U—1000型激光拉曼探针测定流体包裹体气体成分的研究

本文利用U－1000型激光拉曼探针成功地测量出单个流体包裹体中H2S、CH4、CO2气体成分，并讨论了包裹体中这些气体的拉曼谱峰位移与包裹体内压的关系，分析了影响激光拉曼探针定量测定包裹体气相成分的取面积和拉曼定量因子因素。     

A laser-photolysis fragment-fluorescence (LPFF) method for the detection of gaseous nitric acid in ambient air

The development and first tests of a novel method for the direct, sensitive, selective, and fast detection of gaseous nitric acid in air are described. The detection method is based on the laser-photolysis fragment-fluorescence (LPFF) method using 193 nm (ArF) laser light. The photolysis process yielding OH fluorescence has been thoroughly investigated. Up to now, the method has been found to be practically free of interferences. The mixing ratio for nitric acid is measured on-line with a detection limit of about 0.1 ppbv for an accumulation time of the signal of 10–15 min. A number of tests and field measurements were performed to demonstrate the feasibility and limits of the described detection method.     

HP—3808A测距仪测距精度分析

本文采用数理统计方法,详细分析了HP—3808A激光测距仪近几年来积累的测量数据,求得仪器平均测距相对精度为1:70万。并且讨论了进一步提高测距精度的技术措施。     

北京正负电子对撞机直线加速器安装的精密测量

本文介绍为北京正负电子对撞机安装直线加速器所进行的波带板激光准直测量,以及为对测量结果校核所进行的尼龙线准直测量和精密水准测量。并论述了各种准直测量的精度。     

激光束光学系统的变焦理论

从高斯光束经过光学系统的传输与变换规律出发，借助于高斯括号的性质，研究了激光束光学系统的变焦特性，导出了机械补偿式激光束变焦系统的变焦方程及补偿点位置方程，并给出了计算实例。     

The lunar barometric tide in New Zealand

The lunar barometric tide has been determined with reasonable accuracy, on an annual and seasonal basis, at five stations on the mainland of New Zealand and at three of the outlying islands. The determinations show that in the New Zealand region the lunar tide has a larger amplitude and smaller phase than might have been expected from previously available southern-hemisphere results. In general, the seasonal variation of phase in the New Zealand region conforms to the currently recognised global pattern, with the J-season phase greater than that of the D-season. Similarly, the amplitude variation tends to support the suggestion that, south of latitude 30°S, the D-season amplitude is greater than that of the J-season. Approximate tests are introduced and used to assess the statistical significance of some of the apparent differences in amplitude and phase made evident by the analysis. These assessments indicate that although many of the apparent differences may be attributed to sampling fluctuations, the main regional anomalies in amplitude and phase are likely to be real. It is suggested that these anomalies may indicate a significant regional input of tidal energy to the atmosphere (at the lower boundary) from the Pacific oceanic tide.     

Unified Approach to Photon-Counting Microlaser Rangers, Transponders, and Altimeters

Unlike current manned systems, NASA's next generation SLR2000 Satellite Laser Ranging (SLR) station is fully autonomous, eye-safe, relatively compact and inexpensive, and, during daytime tracking, operates at signal-to-noise ratios several orders of magnitude below unity. Tiny, passivelyQ-switched microlasers generate ultra-short pulses with output energies on the order of 100 J at few kHz rates to achieve mm-levelranging precision to satellite altitudesof 20,000 km. Special ranging receivers, combined with Poisson statistical analysis of the received photon distribution, enable the system to rapidly and reliably identify and extract the single photon laser echoes from the solar background. The enhanced rate of return, combined with a uniform signal strength, can actually drive down both systematic and random range errors. The new SLR2000 technology has already spawned exciting new applications. Compact microlaser altimeters, capable of mapping the surface of a planet or other celestial body at multikilohertz rates, is one such application, and a high altitude, airborne version is currently being developed under NASA's Instrument Incubator Program. Interplanetary microlaser transponders would be capable of performing decimeter ranging or subnanosecond time transfer to spacecraft throughout the inner Solar System, resulting in improved knowledge of planetary motions and librations and enhanced General Relativity experiments.