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.     

MAP-CA在视频压缩中的应用

信息时代的重要特征是信息的数字化,但数字化的视频数据量是非常巨大的。为了使数字化的视频信号更有效地传输,对其进行压缩势在必行。应用MAP-CA这个DSP芯片可以对视频图像进行MPEG-4标准的压缩,压缩比可以达到1000:1。在公用电话线上就可以连续传输视频,并能保持图像的质量,最高图像清晰度为768×576,可以达到接近DVD的画面效果。     

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。     

Collaborative image compression and classification with multi-task learning for visual Internet of Things

Widespread deployment of the Internet of Things(Io T) has changed the way that network services are developed, deployed, and operated. Most onboard advanced Io T devices are equipped with visual sensors that form the so-called visual Io T. Typically, the sender would compress images, and then through the communication network, the receiver would decode images, and then analyze the images for applications. However, image compression and semantic inference are generally conducted separately, and t...     

非线性规划的SUMT混合法及其应用

本文提出了非线性规划的内点法与外点法相结合的一种新方法－ＳＵＭＴ混合法,它既兼备内,外点法的功能,又克服了各自单一方法中的缺点。另外,本文还给出无约束问题两种解法的比较及证明,并应用上述方法,利用计算机对精密齿轮按最小转动惯量进行最优设计,取得了令人满意的成果。     

方位维逆合成孔径雷达(ISAR)运动补偿成象中的预加处理

在方位维逆合成孔径雷达（ISAR）运动补偿成象中,为了获得方位维的高分辨力,需要处理的数据量很大。预加处理首先对原始数据进行频移和滤波,然后由滤波后的数据进行抽取,从而大大压缩了所需处理的数据,减小了运动补偿和成象的计算量,提高了成象处理速度。电磁仿真数据和外场实测数据的处理结果验证了预加处理的有效性。     

视频图像压缩技术的研究与应用

视频图像压缩技术是多媒体系统不可回避的关键技术。文章对ＱＩＦ制式标准的视频图像,以Ｐ×６４标准为核心进行了解码与压缩技术的研究。分析了变换编码、运动补偿、量化和变字长嫡编码对压缩效率与图像质量的影响,并对实时传输的视频图像进行了计算机解码分析。恢复的图像表明：解码是成功的,画面清晰,效果显著。在４８６微机上软件处理时间为平均为３ｓ／帧,进一步的硬件处理将有可能为实际使用。     

Al－Al_3Ni自生复合材料的高周疲劳损伤断裂机制及其应力比的影响

实验观察和研究了Ａｌ－Ａｌ３Ｎｉ自生复合材料的高周疲劳损伤断裂行为以及应力比Ｒ的影响,结果显示在Ｒ＝－１疲劳过程中孔洞沿界面区基体的优先萌生、联接和扩展是其损伤断裂的主要机制;并且发现Ｒ对疲劳寿命及断裂过程有明显影响,当Ｒ＝０时滑移带裂纹生长相对容易,寿命减小,而Ｒ＝∞时,裂纹集中在类似于压缩变形的宏观形变带内发展,寿命很长     

以太阳为射电源直接测量天线G／T

介绍以太阳为射电源,直接测量扩充后中国陆地卫星地面接收站,３个数据通道天线的Ｇ／Ｔ性能．对固定通道,测量了Ｌａｎｄｓａｔ—５下行频率的Ｇ／Ｔ～α（天线俯仰角）性能曲线;对可变通道,在α＝５°、３０°时,测量了Ｌａｎｄｓａｔ—６、ＪＥＲＳ—１、ＥＲＳ—１、ＳＰＯＴ卫星、ＺＹ—１卫星下行频率的Ｇ／Ｔ性能,以及可变通道的Ｇ／Ｔ～ｆ性能曲线,最后进行了误差分析．