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Satellite Laser Ranging 卫星激光测距
Pub Date : 1900-01-01 DOI: 10.1887/0750306076/b1388v3c48
R. Wood, G. Appleby
Satellite laser ranging (SLR) began as a concept in 1962 when Plotkin [1] of the Goddard Space Flight Center (GSFC) in Maryland, USA first proposed the development of accurate laser ranging to retro-reflectors on orbiting spacecraft in order to improve geodetic information. At that time optical and radar tracking of satellites was being used to yield tracking station coordinates at a level of accuracy of only about 100 m. The interesting geophysical processes that deform the solid Earth, such as Earth tides and plate tectonic motions, were understood at that time to be affecting station coordinates at the level of only a few centimetres over timescales varying from sub-daily to several years. It was clear that in order to challenge the theoretical work the measurement techniques would have to reach a level of accuracy of a few centimetres and the observations would need to be carried out over many years. The first SLR observations, of the Beacon Explorer-B spacecraft, in 1964 achieved metre-level precision in range, and showed that the technique was viable and potentially capable of reaching the required centimetric precision. These experiments prompted NASA to place retro-reflectors on the GEOS I and II spacecraft and on the Moon, and to begin the development of more SLR stations. In 1975 France launched the first geodetic satellite STARLETTE into a relatively low 950 km orbit, and this was followed in 1976 when NASA launched its laser geodynamic satellite LAGEOS into a near circular, near polar orbit at a height of 6000 km. Both these satellites are inert, dense spheres, uniformly encrusted with retro-reflecting corner-cubes specifically designed to reflect laser light back to the emitting tracking station. STARLETTE has a diameter of 24 cm, LAGEOS a diameter of 60 cm. In 1979 NASA created the Crustal Dynamics Project (CDP) with the aim of ‘developing laser ranging and very long baseline interferometry (VLBI) systems to obtain relative positions with ±2 cm accuracy, to define directions with respect to the inertial reference with a 0.001 arcsecond accuracy to monitor relative rates of motion of different parts of the Earth’s crust well enough to infer irregularities in plate tectonic motions, and to monitor the wobbles and rotational variations to infer their excitations and dampings, as well as to determine accurately the orbits of the distant satellites (higher than 6000 km altitude)’ [2]. This project formalized and consolidated the cooperative efforts between scientists and engineers, which were already underway in several countries, and other independent groups worldwide began to design and build their own SLR systems. During the 1970s the accuracy of the best systems was at the decimetre level, limited mainly by the relatively long laser pulse-lengths that were in routine use at the time. For a typical pulse-length of some 30 cm, a large uncertainty exists in the measurement because it is impossible to relate the detected photons to their
卫星激光测距(SLR)的概念始于1962年,当时美国马里兰州戈达德太空飞行中心(GSFC)的Plotkin[1]首次提出了对在轨航天器上的后向反射器进行精确激光测距,以改善大地测量信息。当时正在利用卫星的光学和雷达跟踪来获得精度仅为100米左右的跟踪站坐标。使固体地球变形的有趣的地球物理过程,如地球潮汐和板块构造运动,在当时被理解为在从次日到几年不等的时间尺度上仅在几厘米的水平上影响台站坐标。很明显,为了挑战理论工作,测量技术必须达到几厘米的精度,而观测需要进行多年。1964年,信标探索者- b宇宙飞船的第一次单反观测在距离上达到了米级的精度,这表明该技术是可行的,并且有可能达到所需的厘米精度。这些实验促使美国宇航局在地球观测系统1号和2号航天器以及月球上安装了反光板,并开始开发更多的单反站。1975年,法国将第一颗大地测量卫星STARLETTE发射到相对较低的950公里轨道上,随后在1976年,美国国家航空航天局(NASA)将其激光地球动力学卫星LAGEOS发射到6000公里高度的近圆形近极轨道上。这两颗卫星都是惰性的、致密的球体,均匀地覆盖着反向反射的角立方,专门用于将激光反射回发射跟踪站。STARLETTE直径24厘米,LAGEOS直径60厘米。1979年,美国宇航局创建了地壳动力学项目(CDP),其目的是“发展激光测距和超长基线干涉测量(VLBI)系统,以±2厘米的精度获得相对位置,以0.001弧秒的精度定义相对惯性参考的方向,以监测地壳不同部分的相对运动速率,足以推断板块构造运动的不规则性。”并监测摆动和旋转变化,以推断它们的激励和阻尼,以及准确确定远距离卫星(海拔高于6000公里)的轨道[2]。这个项目正式巩固了科学家和工程师之间的合作努力,这种努力已经在几个国家进行,世界各地的其他独立团体也开始设计和建造自己的单反系统。在20世纪70年代,最好的系统的精度在分米水平,主要受到当时常规使用的相对较长的激光脉冲长度的限制。对于约30厘米的典型脉冲长度,测量中存在很大的不确定性,因为不可能将检测到的光子与其在脉冲中的位置联系起来。然而,激光和电子技术的进步仍在继续
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引用次数: 0
Laser Micromachining 激光微加工
Pub Date : 1900-01-01 DOI: 10.1201/9781315310855-5
B. Neuenschwander
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引用次数: 0
Laser Printing 激光打印
Pub Date : 1900-01-01 DOI: 10.1201/9781315310855-7
Z. Vangelatos, C. Grigoropoulos
Dot Matrix • An impact printer that transfers characters by striking a pattern (from a matrix) through an inked ribbon and onto paper. • The most common number of pins on a dot matrix printer is 9, 18, or 24. • The speed of dot matrix printers is measured in characters per second (CPS). Common speeds for a dot matrix printer are 32 to 72 CPS. • Dot matrix printers can use either a friction feed or a tractor feed system to move paper through the printing assembly. • Because dot matrix printers strike the image onto paper, it is a good printer to use when carbon-copy documents are being printed.
一种冲击式打印机,通过带墨的色带将图案(从矩阵中)打到纸上,从而将字符转移到纸上。•点阵打印机上最常见的引脚数是9,18或24。•点阵打印机的速度是以每秒字符数(CPS)来衡量的。点阵式打印机的常见速度为32至72 CPS。•点阵式打印机可以使用摩擦送纸或牵引送纸系统来移动纸张通过打印组件。•由于点阵打印机将图像打印到纸上,因此在打印复写文件时使用它是一种很好的打印机。
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引用次数: 2
Rapid Manufacturing 快速制造
Pub Date : 1900-01-01 DOI: 10.1201/9781315310855-6
G. Lewis
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引用次数: 72
Therapeutic Applications: Dermatology—Selective Photothermolysis 治疗应用:皮肤选择性光热溶解
Pub Date : 1900-01-01 DOI: 10.1887/0750306076/b1388v3c26
S. Lanigan
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引用次数: 0
Laser Stabilization for Precision Measurements 激光稳定精密测量
Pub Date : 1900-01-01 DOI: 10.1201/9781003130123-7
G. Barwood, P. Gill
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引用次数: 0
Therapeutic Applications: Lasers in Vascular Surgery 治疗应用:激光在血管手术中的应用
Pub Date : 1900-01-01 DOI: 10.1887/0750306076/b1388v3c27
M. Pai
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引用次数: 0
Attosecond Metrology 阿托秒计量
Pub Date : 1900-01-01 DOI: 10.1201/b21828-21
P. Agostini, Andrew J Piper, L. DiMauro
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引用次数: 0
Beam Propagation 光束传播
Pub Date : 1900-01-01 DOI: 10.1201/b21828-32
B. A. Ward
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引用次数: 0
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Handbook of Laser Technology and Applications
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