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近年来,低轨道LowEarthOrbit,LEO)卫星通信网络以全球覆盖、低传输时延、低功耗链路、较强的抗毁性等特点而受到广泛关注,是未来全球移动通信系统的重要组成部分。移动性管理是构建LEO卫星通信网络的关键技术,为推动移动性管理问题的研究,文章从LEO卫星通信网络的结构和特点入手,阐述了LEO卫星通信网络中移动性管理的分类,并分析了其相比地面移动无线网络的特殊性。从链路层、网络层、传输层三个协议层次综述了近年来LEO卫星通信网络移动性管理研究的国内外现状,重点介绍了移动IPv6(MobileIPv6,MIPv6)和无缝IP分集通用移动性结构(SeamlessIP-diversitybasedGeneralizedMobilityArchitecture,SIGMA)在LEO卫星通信网络中的应用。最后,指出了移动性管理的发展趋势。 相似文献
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Victor U.J. Nwankwo Sandip K. Chakrabarti 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(7):1880-1889
We study the effects of space weather on the ionosphere and low Earth orbit (LEO) satellites’ orbital trajectory in equatorial, low- and mid-latitude (EQL, LLT and MLT) regions during (and around) the notable storms of October/November, 2003. We briefly review space weather effects on the thermosphere and ionosphere to demonstrate that such effects are also latitude-dependent and well established. Following the review we simulate the trend in variation of satellite’s orbital radius (r), mean height (h) and orbit decay rate (ODR) during 15 October–14 November 2003 in EQL, LLT and MLT. Nominal atmospheric drag on LEO satellite is usually enhanced by space weather or solar-induced variations in thermospheric temperature and density profile. To separate nominal orbit decay from solar-induced accelerated orbit decay, we compute and ODR in three regimes viz. (i) excluding solar indices (or effect), where and (ii) with mean value of solar indices for the interval, where and and (iii) with actual daily values of solar indices for the interval ( and ODR). For a typical LEO satellite at h?=?450?km, we show that the total decay in r during the period is about 4.20?km, 3.90?km and 3.20?km in EQL, LLT and MLT respectively; the respective nominal decay () is 0.40?km, 0.34?km and 0.22?km, while solar-induced orbital decay () is about 3.80?km, 3.55?km and 2.95?km. h also varied in like manner. The respective nominal is about 13.5?m/day, 11.2?m/day and 7.2?m/day, while solar-induced is about 124.3?m/day, 116.9?m/day and 97.3?m/day. We also show that severe geomagnetic storms can increase ODR by up to 117% (from daily mean value). However, the extent of space weather effects on LEO Satellite’s trajectory significantly depends on the ballistic co-efficient and orbit of the satellite, and phase of solar cycles, intensity and duration of driving (or influencing) solar event. 相似文献
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针对传统分布式路由算法应用于大型低轨星座时拥塞控制能力有限的问题,提出了基于局部洪泛优化的分布式路由算法。该算法通过局部洪泛的机制收集星间链路的拥塞信息,以应对局部通信需求密集所导致的常见拥塞现象;通过局部路径优化,以较低运行开销实现了流量疏导和网络负载均衡。并且该算法可适用于多层低轨卫星网络结构,不会产生路由环路,对卫星随机故障具有宽适应性。仿真实验表明:该算法在通信需求分布不均的高网络负载情况下能降低2%~10%的丢包率,并对网络随机故障具有鲁棒的表现。 相似文献
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适于低轨卫星IP网络的单核共享树组播算法(英文) 总被引:1,自引:0,他引:1
为了解决低轨卫星IP网络中现有典型源组播算法的信道资源浪费问题,本文提出了一套单核共享树组播算法,即核心群合并共享树(CCST)和加权核心群合并共享树(w-CCST)算法。CCST 算法包括动态近似中心(DAC)选核方法和核心群合并组播路径构建方法。DAC方法专为周期、规律运动的低轨卫星网络提出,不需要复杂的星上计算。在核心群合并方法中,以核节点作为初始核心群,通过核心群和剩余组成员的最短路径方法逐步扩展直至整棵组播树构建完成,从而使得组播树的树代价最小,大大提高了网络的带宽利用率和组播传输效率。w-CCST 算法中所提出的加权因子可以调整树代价和端到端传播时延之间的折衷程度,因此,可以通过调整加权因子来适度增大树代价、降低端到端传播时延以支持某些端到端时延要求苛刻的实时组播业务。最后,与低轨卫星 IP 网络中典型算法进行了性能比较,仿真结果说明,CCST 算法的平均树代价比其它算法显著降低,w-CCST 算法的平均端到端传播时延小于 CCST 算法。 相似文献
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Cheng Lianzhen Zhang Jun Liu Kai 《中国航空学报》2007,20(4):353-361
A new core-based shared tree algorithm, viz core-cluster combination-based shared tree (CCST) algorithm and the weighted version (i.e. w-CCST algorithm) are proposed in order to resolve the channel resources waste problem in typical source-based multicast routing algorithms in low earth orbit (LEO) satellite IP networks. The CCST algorithm includes the dynamic approximate center (DAC) core selection method and the core-cluster combination multicast route construction scheme. Without complicated onboard computation, the DAC method is uniquely developed for highly dynamic networks of periodical and regular movement. The core-cluster combination method takes core node as the initial core-cluster, and expands it stepwise to construct an entire multicast tree at the lowest tree cost by a shortest path scheme between the newly-generated core-cluster and surplus group members, which results in great bandwidth utilization. Moreover, the w-CCST algorithm is able to strike a balance between performance of tree cost and that of end-to-end propagation delay by adjusting the weighted factor to meet strict end-to-end delay requirements of some real-time multicast services at the expense of a slight increase in tree cost. Finally, performance comparison is conducted between the proposed algorithms and typical algorithms in LEO satellite IP networks. Simulation results show that the CCST algorithm significantly decreases the average tree cost against to the others, and also the average end-to-end propagation delay ofw-CCST algorithm is lower than that of the CCST algorithm. 相似文献
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Galileo系统在空间飞行器定位中的应用 总被引:5,自引:0,他引:5
欧洲的Galileo系统将在2008年建成,届时它将与美国的GPS系统相互补充。在对Galileo系统导航星座轨道和信号结构分析的基础上,结合各种不同轨道高度的空间飞行器用户的动态特点,推导了用户卫星接收天线的可见可用性模型,建立了基于Galileo坐标系统(ITRF-96)的高动态定位算法模型,针对实际航天工程任务的LEO和GEO卫星进行了定位仿真,为Galileo系统在空间领域的实际应用打下了基础。 相似文献
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D. Kuang S. DesaiA. Sibthorpe X. Pi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
We present a method to estimate the total neutral atmospheric density from precise orbit determination of Low Earth Orbit (LEO) satellites. We derive the total atmospheric density by determining the drag force acting on the LEOs through centimeter-level reduced-dynamic precise orbit determination (POD) using onboard Global Positioning System (GPS) tracking data. The precision of the estimated drag accelerations is assessed using various metrics, including differences between estimated along-track accelerations from consecutive 30-h POD solutions which overlap by 6 h, comparison of the resulting accelerations with accelerometer measurements, and comparison against an existing atmospheric density model, DTM-2000. We apply the method to GPS tracking data from CHAMP, GRACE, SAC-C, Jason-2, TerraSAR-X and COSMIC satellites, spanning 12 years (2001–2012) and covering orbital heights from 400 km to 1300 km. Errors in the estimates, including those introduced by deficiencies in other modeled forces (such as solar radiation pressure and Earth radiation pressure), are evaluated and the signal and noise levels for each satellite are analyzed. The estimated density data from CHAMP, GRACE, SAC-C and TerraSAR-X are identified as having high signal and low noise levels. These data all have high correlations with anominal atmospheric density model and show common features in relative residuals with respect to the nominal model in related parameter space. On the contrary, the estimated density data from COSMIC and Jason-2 show errors larger than the actual signal at corresponding altitudes thus having little practical value for this study. The results demonstrate that this method is applicable to data from a variety of missions and can provide useful total neutral density measurements for atmospheric study up to altitude as high as 715 km, with precision and resolution between those derived from traditional special orbital perturbation analysis and those obtained from onboard accelerometers. 相似文献