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161.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(5):1402-1413
The present paper reports coordinated ionospheric irregularity measurements at optical as well as GPS wavelengths. Optical measurements were obtained from Tiny Ionospheric Photometer (TIP) sensors installed onboard the Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) satellites. GPS radio signals were obtained from a dual frequency GPS receiver operational at Calcutta (22.58°N, 88.38°E geographic; geomagnetic dip: 32.96°; 13.00°N, 161.63°E geomagnetic) under the SCIntillation Network Decision Aid (SCINDA) program. Calcutta is located near the northern crest of Equatorial Ionization Anomaly (EIA) in the Indian longitude sector. The observations were conducted during the unusually low and prolonged solar minima period of 2008–2010. During this period, four cases of post-sunset GPS scintillation were observed from Calcutta. Among those cases, simultaneous fluctuations in GPS Carrier-to-Noise ratios (C/No) and measured radiances from TIP over a common ionospheric volume were observed only on February 2, 2008 and September 25, 2008. Fluctuations observed in measured radiances (maximum 0.95 Rayleigh) from TIP due to ionospheric irregularities were found to correspond well with C/N0 fluctuations on the GPS links observed from Calcutta, such effects being noted even during late evening hours of 21:00–22:00 LT from locations around 40° magnetic dip. These measurements indicate the existence of electron density irregularities of scale sizes varying over several decades from 135.6 nm to 300–400 m well beyond the northern crest of the EIA in the Indian longitude sector during late evening hours even in the unusually low solar activity conditions. 相似文献
162.
Kai Matsuka Aaron O. Feldman Elena S. Lupu Soon-Jo Chung Fred Y. Hadaegh 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(11):3527-3545
For spacecraft swarms, the multi-agent localization algorithm must scale well with the number of spacecraft and adapt to time-varying communication and relative sensing networks. In this paper, we present a decentralized, scalable algorithm for swarm localization, called the Decentralized Pose Estimation (DPE) algorithm. The DPE considers both communication and relative sensing graphs and defines an observable local formation. Each spacecraft jointly localizes its local subset of spacecraft using direct and communicated measurements. Since the algorithm is local, the algorithm complexity does not grow with the number of spacecraft in the swarm. As part of the DPE, we present the Swarm Reference Frame Estimation (SRFE) algorithm, a distributed consensus algorithm to co-estimate a common Local-Vertical, Local-Horizontal (LVLH) frame. The DPE combined with the SRFE provides a scalable, fully-decentralized navigation solution that can be used for swarm control and motion planning. Numerical simulations and experiments using Caltech’s robotic spacecraft simulators are presented to validate the effectiveness and scalability of the DPE algorithm. 相似文献
163.
Fengsi Wei Xueshang Feng Xu Ya Quanlin Fan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,36(12):2363-2367
A so-called “ISF” prediction method for geomagnetic disturbances caused by solar wind storms blowing to the Earth is suggested. The method is based on a combined approach of solar activity, interplanetary scintillation (I) and geomagnetic disturbance observations during the period 1966–1982 together with the dynamics of solar wind storm propagation (S) and fuzzy mathematics (F). It has been used for prediction tests for 37 geomagnetic disturbance events during the descending solar activity phase 1984–1985, and was presented in 33rd COSPAR conference. Here, it has been improved by consideration of the three dimensional propagation characteristics of each event, the search for the best radio source and the influence of the southward components of interplanetary magnetic fields on the geomagnetic disturbances. It is used for prediction tests for 24 larger geomagnetic disturbance events that produced space anomalies during the period 1980–1999. The main results are: (1) for the onset time of the geomagnetic disturbance, the relative error between the observation, Tobs, and the prediction, Tpred, ΔTpred/Tobs 10% for 45.8% of all events, 30% for 78.3% and >30% for only 21.7%; (2) for the magnetic disturbance magnitude, the relative error between the observation, ∑Kp,obs, and the prediction, ∑Kp,pred, Δ∑Kp,pred/∑Kp,obs 10% for 41.6% of all events, 30% for 79% and 45% for 100%. This shows that the prediction method described here has encouraging prospects for improving predictions of large geomagnetic disturbances in space weather events. 相似文献
164.
简要介绍了利用通信和广播电视卫星对地面干扰辐射源进行定位的必要性和基本工作原理、技术难点及解决方法,以及提高定位精度的主要技术途径。 相似文献
165.
166.
为了解决大规模车队同时利用短消息业务和通用分组无线业务与多个监控中心进行通信的问题,研究了基于上述两种通道的车辆监控通信模型,详细设计了其中的通信服务器的功能和结构,使其能够支持各监控中心自由选择监控车辆、信息广播、特殊信息优先等服务.为了提高服务器的运行效率,在数据结构中充分采用了以空间换时间的方法,自行设计了监控接口协议,实现时采用了多线程、消息通信和组件技术.系统完成后大量的现场实验结果表明了服务器的高效性和稳定性. 相似文献
167.
168.
过冷大水滴规章提高了飞机在结冰条件下飞行的安全等级,将会对结冰探测系统的设计产生一定影响。本文概述了附录0过冷大水滴结冰条件,并对附录O第1部分大气结冰条件进行了浅析;分析了FAR25.1420过冷大水滴结冰条件对结冰探测系统设计的影响,并提出符合相关要求的结冰探测方式;指出了对于目前申请在结冰条件下飞行的合格审定的最大起飞重量小于60000磅或具有可逆飞行控制系统的飞机,按照FAR25.1420(a)(1)的要求进行审定是一个较为合适的选择。此外,还给出了一种符合FAR25.1420要求的结冰探测系统方案。 相似文献
169.
非线性分析是药柱结构分析中的难点,针对其对结构分析的影响,基于不可压缩材料的粘弹性本构关系,应用完全拉格朗日(T.L)法的虚功方程,综合考虑药柱的近似不可压缩性和几何非线性,推导了三维粘弹性几何非线性有限元增量方程,编写了有限元程序对星型药柱在受压力载荷以及固化降温载荷作用下的结构进行了分析,并与线性计算的结果进行了对比,结果表明,在大载荷作用下,非线性对药柱结构分析的影响比较显著,计算时考虑非线性的影响是必要的。 相似文献
170.
雷达遥感卫星作为一种重要的民用空间基础设施,能够实现全天时、全天候的高分辨对地观测,对推动科学进步、促进经济发展和维护国家安全具有重大战略意义。但随着全域无线电业务的快速增长,频率共享导致的兼容冲突日益加剧,衍生出的射频干扰已成为困扰定量化精确遥感探测性能的共性难题。本文系统地梳理了典型波段的对地观测业务频率分配现状,介绍了射频干扰的定义和影响机理,提出了模型数据混合驱动的干扰抑制新思路,并对面临的机遇与挑战进行了归纳总结,为新一代雷达遥感卫星的频率优化设计提供知识依据,进而保障其在复杂电磁环境的对地观测效能。 相似文献