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231.
232.
Chi-Ming Lee Chung-Yen Kuo Jian Sun Tzu-Pang Tseng Kwo-Hwa Chen Wen-Hau Lan C.K. Shum Tarig Ali Kuo-En Ching Philip Chu Yuanyuan Jia 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(3):1280-1288
Global sea level rise due to an increasingly warmer climate has begun to induce hazards, adversely affecting the lives and properties of people residing in low-lying coastal regions and islands. Therefore, it is important to monitor and understand variations in coastal sea level covering offshore regions. Signal-to-noise ratio (SNR) data of Global Navigation Satellite System (GNSS) have been successfully used to robustly derive sea level heights (SLHs). In Taiwan, there are a number of continuously operating GNSS stations, not originally installed for sea level monitoring. They were established in harbors or near coastal regions for monitoring land motion. This study utilizes existing SNR data from three GNSS stations (Kaohsiung, Suao, and TaiCOAST) in Taiwan to compute SLHs with two methods, namely, Lomb–Scargle Periodogram (LSP)-only, and LSP aided with tidal harmonic analysis developed in this study. The results of both methods are compared with co-located or nearby tide gauge records. Due to the poor quality of SNR data, the worst accuracy of SLHs derived from traditional LSP-only method exceeds 1?m at the TaiCOAST station. With our procedure, the standard deviations (STDs) of difference between GNSS-derived SLHs and tide gauge records in Kaohsiung and Suao stations decreased to 10?cm and the results show excellent agreement with tide gauge derived relative sea level records, with STD of differences of 7?cm and correlation coefficient of 0.96. In addition, the absolute GNSS-R sea level trend in Kaohsiung during 2006–2011 agrees well with that derived from satellite altimetry. We conclude that the coastal GNSS stations in Taiwan have the potential of monitoring absolute coastal sea level change accurately when our proposed methodology is used. 相似文献
233.
Paul O’Brien 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The ASTROSAT satellite is an Indian National Space Observatory under development in India. Due for launch in 2010, ASTROSAT will carry a complement of five scientific instruments enabling simultaneous observations from the optical through to the hard X-ray energy band. This capability will enable broad-band spectroscopy and high time-resolution monitoring of both galactic and extra-galactic targets, such as X-ray binaries and AGN. One of the instruments is being built in collaboration with the Canadian Space Agency and another in collaboration with the University of Leicester. ASTROSAT also carries a scanning sky monitor to observe the variable X-ray sky. After an initial period of science verification and guaranteed time, a certain fraction of ASTROSAT observing time will also be made available to the community via a call for proposals. Here I summarise the instrument complement and principle scientific objectives of the mission. 相似文献
234.
Tommaso Pino Christian Circi Giovanni Vulpetti 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(11):3675-3690
A good model of solar-radiation pressure induced thrust is one of the key points in sailcraft trajectory design. The sail membrane’s local topographic deformations, i.e. wrinkles and creases, are among the main aspects that such a model should include. We have analyzed the influence of wrinkles/creases, as a whole, by measuring the related deformations on small samples of sail membrane, 2.5?μm thick, consisting of CP1 and physical-vapor-deposition Aluminum. Experimental outcomes from our laboratory facility have been processed, statistically investigated, and inserted into the lightness vector formalism. We have used such formalism for accurate sailcraft trajectory computation via a non-ideal reflection sail thrust model. Finally, we computed the deviations of wrinkled-sail sailcraft final orbital states with respect to the no-wrinkle sail final orbital ones for a circular to circular 2D inward transfer. The radii of the orbits are 1?AU and the semi-major axis of Mercury, respectively. It appears that sail wrinkles and creases are no longer negligible in the sailcraft trajectory design. 相似文献
235.
介绍了微分法分析计算定位误差的原理和适用范围,通过生产实例分析,证明了该方法在解决多误差因素定位误差分析与计算中的简便与快捷,从而有效简化了复杂定位方案定位误差的分析与计算,提高了夹具的设计效率。 相似文献
236.
Qiang Guo Volodymyr G. Galushko Andriy V. Zalizovski Sergiy B. Kashcheyev Yu Zheng 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(9):2267-2274
A modification of the Doppler Interferometry Technique is suggested to enable estimating angles of arrival of comparatively broadband HF signals scattered by random irregularities of the ionospheric plasma with the use of small-size weakly directional antennas. The technique is based on the measurements of cross-spectra phases of the probe radiation recorded at least in three spatially separated points. The developed algorithm has been used to investigate the angular and frequency-time characteristics of HF signals propagating at frequencies above the maximum usable one (MUF) for the direct radio path Moscow-Kharkiv. The received signal spectra show presence of three families of spatial components attributed, respectively, to scattering by plasma irregularities near the middle point of the radio path, ground backscatter signals and scattering of the sounding signals by the intense plasma turbulence associated with auroral activations. It has been shown that the regions responsible for the formation of the third family components are located well inside the auroral oval. The drift velocity and direction of the auroral ionosphere plasma have been determined. The obtained estimates are consistent with the classical conception of the ionospheric plasma convection at high latitudes and do not contradict the results of investigations of the auroral ionosphere dynamics using the SuperDARN network. 相似文献
237.
为解决框架类零件的高位置度孔的精密镗削加工问题,研发了ZYTC600专用镗削机床.其精度指标优于现有的通用镗床(包括进口镗床),尺寸在500mm范围内,同轴度优于2μm,垂直度优于5μm,其中的关键部件双回转轴系分度精密转台采用了一套精密调整机构,可以实现0.2s”的精密调整,通过有限元分析得到其驱动刚度可达到800N/μm,可以满足加工需求. 相似文献
238.
采用了理论设计和有限元仿真分析相结合的方法,设计了基于液体静压导轨的大行程快刀伺服系统(最大加工行程30mm,行程4mm时频响不低于50Hz).首先,设计得到了基于液体静压导轨的大行程快刀伺服系统的结构模型和相关参数;接着,利用ANSYS/FLUENT软件对液体静压导轨的变形、模态以及油膜压力分布进行仿真分析,并且将油膜刚度的理论计算值和仿真计算值进行比较,验证了导轨设计的可靠性;最后,选用能够满足要求的音圈电机、位置反馈装置以及功能强大的MPAC运动控制器等完成了控制系统的搭建. 相似文献
239.
在设计控制系统模型时,首先引入了有限差分法(FDM)离散化后的波动方程,然后基于H∞最优控制原理,检查闭环控制系统的稳定性和可探测性,对控制系统传感器和作动器的位置进行优化配置.通过计算闭环反馈系统的范数,最终得到了控制系统的最优控制算法.仿真结果表明,利用波动方程来优化控制系统传感器和作动器位置的算法是可行的,可广泛应用于飞控系统的设计中. 相似文献
240.
为更好地理解热力学排气系统(TVS)的运行机理,优化其运行参数,针对节流装置,建立了热力学模型,讨论了节流过程中状态参数的变化规律,对比了单相气体、单相液体节流的性能特性,进一步揭示了焦汤节流效应的原理,分析了不同节流背压下节流前低温工质(液氢和液氧)压力和温度对节流性能的影响,并结合TVS实际应用,阐述了节流最大制冷量的利用效果,提出了优化的TVS工作区间。研究表明:在节流过程不发生相变情况下单相气体节流制冷效应要比单相液体节流制冷效应更加显著;而在节流过程发生相变情况下液体节流至两相后,由于空化吸热导致流体温度降低,对于液氢,0.5MPa的压降可产生接近3 K的温降。对于液体节流,节流前压力对节流过程影响可忽略,〖JP2〗而节流前温度和节流背压对节流过程起主导作用;对于液氢在在轨运行工况下,考虑到节流制冷量的充分利用,同时保证换热过程体积含气率不高于90%,推荐TVS系统中节流背压范围为75~143 kPa。 相似文献