Optimal Compensation and Implementation for Adaptive Optics Systems     

Douglas P. Looze  Markus Kasper  Stefan Hippler  Orhan Beker  Robert Weiss 《Experimental Astronomy》2003,15(2):67-88

This paper develops a compensation algorithm based on Linear–Quadratic–Gaussian (LQG) control system design whose parameters are determined (in part) by a model of the atmosphere. The model for the atmosphere is based on the open-loop statistics of the atmosphere as observed by the wavefront sensor, and is identified from these using an auto-regressive, moving average (ARMA) model. The (LQG) control design is compared with an existing compensation algorithm for a simulation developed at ESO that represents the operation of MACAO adaptive optics system on the 8.2 m telescopes at Paranal, Chile. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

Notes on Hori Method for Canonical Systems     

Sandro Da Silva Fernandes 《Celestial Mechanics and Dynamical Astronomy》2003,85(1):67-78

In this paper a slightly different approach is proposed for the process of determining the functions S _m and H _m ^* of the algorithm of the canonical version of Hori method. This process will be referred to as integration theory of the mth order equation of the method. It will be shown that the ordinary differential equation with an auxiliary parameter t ^* as independent variable, introduced through Hori auxiliary system, can be replaced by a partial differential equation in the time t. In this way, the mth order equation of the algorithm assumes a form very similar to the one of other perturbation methods. In virtue of this new approach of the integration theory for Hori method, Lagrange's variational equations introduced by Sessin are revised. As an example, the Duffing equation is solved through this new approach.  相似文献   

The planets capture model of V838 Monocerotis: conclusions for the penetration depth of the planet(s)     

Alon Retter  Bing Zhang  Lionel Siess  Amir Levinson 《Monthly notices of the Royal Astronomical Society》2006,370(3):1573-1580

V838 Mon is the prototype of a new class of objects. Understanding the nature of its multistage outburst and similar systems is challenging. So far, several scenarios have been invoked to explain this group of stars. In this work, the planets-swallowing model for V838 Mon is further investigated, taking into account the findings that the progenitor is most likely a massive B-type star. We find that the super-Eddington luminosity during the eruption can explain the fast rising times of the three peaks in the optical light curve. We used two different methods to estimate the location where the planets were consumed. There is a nice agreement between the values obtained from the luminosities of the peaks and from their rising time-scale. We estimate that the planets were stopped at a typical distance of one solar radius from the centre of the host giant star. The planets-devouring model seems to give a satisfying explanation to the differences in the luminosities and rising times of the three peaks in the optical light curve of V838 Mon. The peaks may be explained by the consumption of three planets or alternatively by three steps in the terminal falling process of a single planet. We argue that only the binary merger and the planets-swallowing models are consistent with the observations of the new type of stars defined by V838 Mon.  相似文献   

Water transport from the North-east Irish Sea to western Scottish coastal waters: Further observations from time-trend matching of Sellafield radiocaesium     

W.A. McKay  M.S. Baxter 《Estuarine, Coastal and Shelf Science》1985,21(4):471-480

Radiocaesium isotopes, discharged into the North-east Irish Sea from the Sellafield (formerly Windscale) nuclear fuel reprocessing plant in Cumbria, have been employed as flow monitors to update and extend the record of coastal water movement from the Irish Sea to the Clyde Sea area and, further north, to Loch Etive. The temporal trends in radiocaesium levels have been used to determine the extent of water mixing en route and to define mean advection rates. Flow conditions from the Irish Sea have changed considerably since the mid-1970s, the residence time of northern Irish Sea waters being ～12 months during 1978–1980 inclusive. Average transport times of four and six months are estimated for the Sellafield to Clyde and Sellafield to Etive transects respectively. Sellafield ¹³⁷Cs levels in seawater were diluted by factors of 27 and 50 respectively during current movement to the Clyde and Etive areas. The decrease in salinity-corrected ¹³⁷Cs concentrations between the Clyde and Etive suggests that dilution by Atlantic water occurs, the latter mainly entering the Firth of Lorne from the west. The majority (～94%) of the radiocaesium supply to Loch Etive enters the Firth of Lorne via the portion of the coastal current circulating west of Islay, only ～6% arriving via the Sound of Jura.  相似文献   

Beam Mode Expansion of Corrugated Conical Horns with Phase Correcting Lens: Application to Radioastronomy Receivers     

E. García  L. De Haro  C. O'Sullivan  G. Cahill  J. A. López Fernández  F. Tercero  B. Galocha  J. L. Besada 《Experimental Astronomy》2003,15(3):173-193

A classical radioastronomy receiver is fed with a corrugated horn and an independent lens, both placed in a cryostat to lower the noise temperature. The beam is focused and directed using a combination of elliptical and plane mirrors. This paper proposes modifying the initial feeding system by placing the lens onto the horn aperture, thereby allowing a size reduction of the horn and lens, and a simplification of their mechanical design. The profiled lens is shaped to correct the phase error on the horn aperture. A quasi-optical model of the horn-plus-lens system has been developed using a Beam Mode Expansion (BME). Results using both a hyperbolic-planar lens and a spherical-elliptical lens, as well as results obtained by using Geometrical Optics (GO) with a Kirchoff–Huygens integration to get the far-field pattern, have been compared with measurements. As a direct application, a full focusing system for the new 40-m radiotelescope at the “Centro Astronómico de Yebes” is presented for the 22, 30 and 45 GHz bands. This paper has developed a QO model for a corrugated conical horn with a phase-correcting lens. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

Dynamics of Two Planets in the 3/2 Mean-motion Resonance: Application to the Planetary System of the Pulsar PSR B1257+12     

N. Callegari Jr  S. Ferraz-Mello  T. A. Michtchenko 《Celestial Mechanics and Dynamical Astronomy》2006,94(4):381-397

This paper considers the dynamics of two planets, as the planets B and C of the pulsar PSR B1257+12, near a 3/2 mean-motion resonance. A two-degrees-of-freedom model, in the framework of the general three-body planar problem, is used and the solutions are analyzed through surfaces of section and Fourier techniques in the full phase space of the system.On the possibility of existence of a fourth planet in distant orbit, see Wolszczan et al., 2000  相似文献   

可移动中继节点在传感器网络中的节能应用     

唐帙  罗惠琼 《成都信息工程学院学报》2005,20(2):147-150

介绍了一种新颖的静态传感器网络实现方法，它利用可移动的中继节点来收集静态传感器网络的数据，有效的节约各传感器节点的能源，延长整个传感器网络的有效工作时间。也可以对该方法进行适当的改进，应用到某些实时性要求较高的场合中去。然后介绍了应用该原理实现的一个通讯协议。  相似文献   

基于加权破产博弈模型的跨境流域水资源分配研究     

李芳  吴凤平  陈柳鑫  许霞  赵越 《地理科学》2021,41(4):728-736

基于公平合理利用视角,将多准则决策模型与破产理论相结合探讨跨境水资源分配问题。通过梳理国际水法,设计了跨境流域水资源公平合理分配的指标体系,采用投影法解决这一多准则决策问题,并依此加权调整流域国用水需求。在加权调整用水需求和考虑议价能力的基础上,基于破产博弈模型探讨跨境流域水资源分配问题,以提高分配方案的公平合理性和可接受性。最后以澜沧江-湄公河流域的水资源分配为例进行研究,得到了澜沧江-湄公河旱季的水资源分配方案,并分析了需求加权调整系数对各流域国水资源分配的影响,进一步验证了分配模型的可靠性。  相似文献   

雅鲁藏布江曲水-泽当段风沙活动动力条件分析与风沙灾害防治建议   总被引：5，自引：4，他引：1  

马鹏飞  张正偲  论珠群培  高佳佳  戴睿  次旺  潘凯佳 《中国沙漠》2021,41(1):10-18

雅鲁藏布江河流宽谷区是青藏高原风沙活动最为强烈地区之一。本文选择雅鲁藏布江曲水-泽当段为研究区,分析该地区1981—2010年以来的风动力条件变化特征。结果表明：1981年以来年平均风速明显降低,月平均风速2—4月最大。受河流-山地复合系统的影响,风向复杂且具有明显的空间差异性,贡嘎以西风和东风为主,泽当包括西风、南风和东北风。日极大风速超过起沙风速的天数所占比例较大（>83%）,且自西向东逐渐增加（泽当达96%）。冬春季输沙势所占比例最大,扎囊地区年输沙势最大（77 UV）,其次为桑耶地区（37 UV）,泽当地区最小（5.4 UV）。近年来,沙尘天气有增加的趋势。风动力条件特点和该段河流宽谷区广泛分布的风沙沉积物是形成该区风沙地貌空间格局、导致沙尘天气频发的主要原因。基于该区河流-山地复合系统下风沙环境的复杂性和野外实地调查结果,提出了科学布置防沙治沙措施的建议。  相似文献   

能源地缘政治与能源权力研究   总被引：2，自引：1，他引：1  

杨宇  何则 《地理科学进展》2021,40(3):524-540

围绕油气资源的权力博弈仍然是当今世界最主要的能源权力争夺,但不同时代的能源权力的属性有所不同,能源安全与能源战略内涵也有所不同。论文在系统梳理能源地缘政治基础上,提出了能源权力的概念,并从地缘政治格局、能源安全观、能源网络和全球能源治理4个方面进行了具体阐述。研究认为：① 以能源分布、产销空间变化及其规律性总结是传统能源地缘政治研究的核心,油气资源地理分布的不平衡性是能源权力产生的最直接因素。② 从石油危机时代到未来新能源时代,能源安全观的不同是影响国际能源地缘政治权力变化的重要因素。③ 能源的商品属性和地缘属性决定了能源贸易不仅是经济行为,其空间的流动与国际政治关系密切。生产与消费的分离使得油气二次分配过程中的贸易控制和通道控制对能源权力重构产生重要影响。④ 全球能源权力巨变和复杂错综的能源权力网络将引发全球能源治理体系的新秩序。权力的主体从国家、国际组织、跨国公司转变为全球能源网络中利益共同体,能源治理的主题从一国之利益走向了全球能源权力的再分配过程。展望未来,如何在理论上建构新时代的能源权力的理论体系,深化气候变化和新能源等因素影响下的世界能源权力的演变、地理空间与权力的相互依赖关系、权力秩序的重构及其效应、全球能源治理机制及其治理模式等研究,对科学认知和研判世界能源形势与能源战略的演化具有重要的意义,也是能源地缘政治学研究的重要方向性命题。  相似文献