Dynamical evolution of high area-to-mass ratio debris released into GPS orbits

A large set of simulations, including all the relevant perturbations, was carried out to investigate the long-term dynamical evolution of fictitious high area-to-mass ratio (A/M) objects released, with a negligible velocity variation, in each of the six orbital planes used by Global Positioning System (GPS) satellites. As with similar objects discovered in near synchronous trajectories, long lifetime orbits, with mean motions of about 2 revolutions per day, were found possible for debris characterized by extremely high area-to-mass ratios. Often the lifetime exceeds 100 years up to A/M ∼ 45 m²/kg, decreasing rapidly to a few months above such a threshold. However, the details of the evolution, which are conditioned by the complex interplay of solar radiation pressure and geopotential plus luni-solar resonances, depend on the initial conditions. Different behaviors are thus possible. In any case, objects like those discovered in synchronous orbits, with A/M as high as 20–40 m²/kg, could also survive in this orbital regime, with semi-major axes close to the semi-synchronous values, with maximum eccentricities between 0.3 and 0.7, and with significant orbit pole precessions (faster and wider for increasing values of A/M), leading to inclinations between 30° and more than 90°.     

Indicators of black-hole mass and Eddington accretion ratio from QSO X-ray and UV spectra

The evolution of luminous QSOs is linked to the evolution of massive galaxies. We know this because the relic black-holes found locally have masses dependent on the properties of the host galaxy’s bulge. An important way to explore this evolution would be to measure dependences of black-hole masses and Eddington accretion ratios over a range of redshifts, i.e., with cosmological age. For low redshift QSOs (and their lower luminosity Seyfert galaxy counterparts) it has been possible to infer black-hole masses from the luminosities and velocity dispersions of their host-galaxy bulges. These masses agree with those virial black-hole masses calculated from the Doppler widths of the broad Hβ emission lines. The latter method can then be extended to more distant and luminous QSOs, up to redshifts of 0.6 with ground-based optical observations. We discuss ways to extend these explorations to higher redshifts – up to 3 using the widths of QSOs’ broad UV emission lines, and in principle, and to redshifts near 4 from ground-based infrared observations of rest-frame Hβ at 2.5 μm. We discuss the possibility of investigating the accretion history of the higher redshift QSOs using measures of Eddington accretion ratio – the soft X-ray spectral index and the eigenvectors of Principal Components Analyses of QSOs’ UV emission-line spectra.     

区域空中交通流量控制研究

运用排队论思想，结合区域控制的特点建立了区域流量控制模型，分析了郑州区域管制中心实施流量控制的实际效果，研究结果表明，仅考虑单独区域流量控制，将使航班延误的不利影响逐级放大，理想的流量控制应该全面考虑所有受影响的区域，合理地选择控制时段和控制间隔，最大限度地利用空域资源，减少航班延误，保证空中交通的安全畅通。     

当今山区公路边坡治理新技术

本文介绍我国要对占国土面积一半以上的山区发展经济 ,就必需交通先行 ,而修建山区公路不仅工程艰巨 ,需要大量投资 ,而且由于地形、地质复杂会碰到山坡滑坍、岩石崩塌、路基沉陷变形等主要病害。边坡治理的原则 ,以较多篇幅介绍了目前治理边坡的新技术、新机具、新材料、新工艺等内容     

中国特殊经济区和海关特殊监管区的发展方向

只要符合透明度原则和非歧视原则 ,继续保留对特殊经济区的优惠政策 ,就不违背中国加入世界贸易组织《议定书》和《报告书》的有关规定 ,但应该由“地区倾斜”转向“产业倾斜” ;对保税区和出口加工区等海关特殊监管区的管理最终应该体现“境内关外”的特征 ,与国际通行规则保持一致。     

NUM-1060 Ⅱ CNC系统自动回零程序设计

本文介绍了采用NUM-1060ⅡCNC系统，在设计制造CX600数控车铣加工中心过程中，通过E变量判断回零状态，调用Part功能子程序，完成自动回零的方法。该方法切实可行，已用于生产实际。     

HSDB网络稳定性的研究

高速数据总线（ＨｉｇｈＳｐｅｅｄＤａｔａＢｕｓ，ＨＳＤＢ）是新一代航空电子系统的数据总路线，ＨＳＤＢ网络实际上是基于线性令牌总线的一个专用计算机局域网，在网络上负载较重且时间非苛刻的消息到达是一般过程的条件十分别讨论了网络的局域和全域稳定性，并导出了保证整个网络稳定的令牌握有定时器最小值，同时给出了如何根据应用去调整得到的理论值。     

一种膨胀映射的不动点定理

王尚志给出了若干种膨胀映射的概念，并证明了它们的不动点存在定理。对其中第一型膨胀映射的不动点定理做了进一步推广。     

一般高速数据总线网络的吞吐量分析

分析了一般高速数据总线网络优先权方案的特性，建立了一般ＨＳＤＢ网络多优先权的平均吞吐量模型，导出了不同优先权的平均吞吐量解析表达式，并通过软件仿真验证了由得到的解析表达式。     

载人航天器密封系统漏率设计方法

载人航天器密封舱为航天员提供在轨生活、工作的环境,对密封舱及其环控生保系统、热控制系统、推进控制系统等中各管路的密封性能有严格要求。文章提出了一种漏率设计方法,建立了相应的漏率检测系统,并依据该方法制定了密封舱体和各管路的漏率设计和指标分配的流程。本流程可用作载人航天器舱体密封系统、管路密封系统的漏率设计,对保证载人航天器在轨安全可靠运行有重要参考价值。