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961.
波束扫描合成孔径雷达是为了满足星载合成孔径雷达宽测绘的要求而提出的,本文主要研究SCANSAR成象处理。SCANSAR的工作原理、信号格式、信号结构和信号参数限制的深入分析是成象处理研究的基础,成象处理算法包括块数据成象算法和块图象拼接算法两部分,频谱分析法和时域频域混合相关法被用于块数据成象,块图象的拼接是利用时间关系剪裁块图象再顺次拼接,完整的计算机仿真验证了本文提出的SCANSAR信号格式和 相似文献
962.
虚拟制造系统中刀具磨损仿真作为物理仿真的一个模块,对加工精度和表面粗糙度等仿真模块都有影响,是影响虚拟制造系统发展的关键技术。本文综述了虚拟制造系统中刀具磨损技术的发展过程,列举出几种典型的刀具磨损计算方法,对比分析了各种方法的优缺点,提出以二维值来描述刀具磨损乃至刀具磨损的三维仿真将成为虚拟制造系统中刀具磨损预测技术新的发展方向。 相似文献
963.
964.
965.
《Space Science Reviews》2007,128(1-4):433-506
The Optical, Spectroscopic, and Infrared Remote Imaging System OSIRIS is the scientific camera system onboard the Rosetta
spacecraft (Figure 1). The advanced high performance imaging system will be pivotal for the success of the Rosetta mission.
OSIRIS will detect 67P/Churyumov-Gerasimenko from a distance of more than 106 km, characterise the comet shape and volume, its rotational state and find a suitable landing spot for Philae, the Rosetta
lander. OSIRIS will observe the nucleus, its activity and surroundings down to a scale of ~2 cm px−1. The observations will begin well before the onset of cometary activity and will extend over months until the comet reaches
perihelion. During the rendezvous episode of the Rosetta mission, OSIRIS will provide key information about the nature of
cometary nuclei and reveal the physics of cometary activity that leads to the gas and dust coma.
OSIRIS comprises a high resolution Narrow Angle Camera (NAC) unit and a Wide Angle Camera (WAC) unit accompanied by three
electronics boxes. The NAC is designed to obtain high resolution images of the surface of comet 67P/Churyumov-Gerasimenko
through 12 discrete filters over the wavelength range 250–1000 nm at an angular resolution of 18.6 μrad px−1. The WAC is optimised to provide images of the near-nucleus environment in 14 discrete filters at an angular resolution of
101 μrad px−1. The two units use identical shutter, filter wheel, front door, and detector systems. They are operated by a common Data
Processing Unit. The OSIRIS instrument has a total mass of 35 kg and is provided by institutes from six European countries. 相似文献
966.
对应用于嵌套网格技术中的Collar网格思想进行了拓宽,提出了建立结合部网格系统的思想,使得对于复杂的组合体,Collar网格的生成都非常容易,并将其与虚拟网格和其他网格相结合,在保证计算网格的生成方便快捷而且网格质量高的前提下,成功地解决了嵌套网格技术中的结合部问题。机身-边条-机翼组合体绕流计算的实例表明,将结合部网格系统应用在嵌套网格技术中能保证几何外形不发生变化,能有效地处理各种复杂组合体外形的结合部问题,对于嵌套网格的自动化生成具有一定的实际意义。 相似文献
967.
David H. Rodgers Patricia M. Beauchamp Laurence A. Soderblom Robert H. Brown Gun-Shing Chen Meemong Lee Bill R. Sandel David A. Thomas Robert T. Benoit Roger V. Yelle 《Space Science Reviews》2007,129(4):309-326
MICAS is an integrated multi-channel instrument that includes an ultraviolet imaging spectrometer (80–185 nm), two high-resolution
visible imagers (10–20 μrad/pixel, 400–900 nm), and a short-wavelength infrared imaging spectrometer (1250–2600 nm). The wavelength ranges were chosen
to maximize the science data that could be collected using existing semiconductor technologies and avoiding the need for multi-octave
spectrometers. It was flown on DS1 to validate technologies derived from the development of PICS (Planetary Imaging Camera
Spectrometer). These technologies provided a novel systems approach enabling the miniaturization and integration of four instruments
into one entity, spanning a wavelength range from the UV to IR, and from ambient to cryogenic temperatures with optical performance
at a fraction of a wavelength. The specific technologies incorporated were: a built-in fly-by sequence; lightweight and ultra-stable,
monolithic silicon-carbide construction, which enabled room-temperature alignment for cryogenic (85–140 K) performance, and
provided superb optical performance and immunity to thermal distortion; diffraction-limited, shared optics operating from
80 to 2600 nm; advanced detector technologies for the UV, visible and short-wavelength IR; high-performance thermal radiators
coupled directly to the short-wave infrared (SWIR) detector optical bench, providing an instrument with a mass less than 10
kg, instrument power less than 10 W, and total instrument cost of less than ten million dollars. The design allows the wavelength
range to be extended by at least an octave at the short wavelength end and to ∼50 microns at the long wavelength end. Testing
of the completed instrument demonstrated excellent optical performance down to 77 K, which would enable a greatly reduced
background for longer wavelength detectors. During the Deep Space 1 Mission, MICAS successfully collected images and spectra
for asteroid 9969 Braille, Mars, and comet 19/P Borrelly. The Borrelly encounter was a scientific hallmark providing the first
clear, high resolution images and excellent, short-wavelength infrared spectra of the surface of an active comet’s nucleus. 相似文献
968.
杜有威 《中国民航学院学报》2003,21(6):56-59
根据2个城市的航运时刻表,通过相应的程序计算出飞机在各机场停留的最短时间,完成每个航运时刻表最少使用的飞机架数与某架飞机完成一个飞行周期所需要的天数。给出4个例题的进一步讨论:1)当nm时的m×n阶停留时间阵;3)目标函数的极大值;4)多个城市间航空班次的最佳匹配问题。 相似文献
969.
970.
信号导向的可互换仪器驱动技术是当前自动测试领域发展的重点、热点。虚拟仪器技术、信号导向技术和组件对象模型COM技术的发展为实现硬件资源可互换性和测试程序集可移植性提供了技术支持。文中论述的基于信号的可互换仪器驱动和测试系统架构模型借助信号导向机制和COM技术优秀的封装性和独立性,利用实时引擎技术和动态链接技术将测试程序集与测试资源无关性变成了现实。逐一分析系统架构中各功能模块的工作机制及设计思路,并重点论述信号驱动器和开关信号驱动器的实现方法,为自动测试系统首次实际应用IVI信号驱动器进行了有益的实践工作。 相似文献