Multi-point observations and modeling of subauroral polarization streams (SAPS) and double-peak subauroral ion drifts (DSAIDs): A case study

While subauroral polarization streams (SAPS) are well recognized as representatively one of the most important features of magnetosphere-ionosphere (M-I) coupling processes in the subauroral region, the double-peak subauroral ion drifts (DSAIDs) is a newly recognized ionospheric phenomenon, categorized as a subset of subauroral ion drifts (SAIDs). In this study, we investigate both SAPS and DSAIDs that appear during the storm main phase of the 17 March 2015 event through a combination of multi-point observations and numerical simulations. We find that when SAPS/DSAIDs are observed by the DMSP spacecraft near the dusk subauroral region, strong electric fields are detected minutes later by the Van Allen Probes almost in the same conjugate region near the equatorial plane. Numerical simulations are carried out not only to reveal the global context and dynamic evolution of the SAPS in both the magnetospheric and ionospheric systems, but also to aid the understanding of the effect of conductance on the DSAIDs. Our results confirm that SAPS are indeed associated with Region 2 field-aligned currents (FACs) flowing into the low conductance region. On the other hand, the DSAIDs may be related to the double-conductance-trough in the subauroral region.     

光正交码

OCDMA技术已成功应用于无线通信领域，它具有抗干扰，提高系统容量等优点。本文对实现OCDMA技术关键的光地址码中较成熟的光正交码进行了介绍。阐述了光正交码的众多构造方法和现有的存在性结果，主要介绍了如何利用组合设计的方法构造光正交码。     

一种新Turbo码交织器的VHDL设计

介绍了Turbo码和交织技术，分析了几种常用交织算法的特点。根据组合交织器的设计思路，提出了隔行写入螺旋式交织方案。利用硬件描述语言（VHDL）编程设计了这种交织器的电路，并给出了仿真结果。     

Mercury’s Surface Composition and Character as Measured by Ground-Based Observations

Mercury’s surface is thought to be covered with highly space-weathered silicate material. The regolith is composed of material accumulated during the time of planetary formation, and subsequently from comets, meteorites, and the Sun. Ground-based observations indicate a heterogeneous surface composition with SiO₂ content ranging from 39 to 57 wt%. Visible and near-infrared spectra, multi-spectral imaging, and modeling indicate expanses of feldspathic, well-comminuted surface with some smooth regions that are likely to be magmatic in origin with many widely distributed crystalline impact ejecta rays and blocky deposits. Pyroxene spectral signatures have been recorded at four locations. Although highly space weathered, there is little evidence for the conversion of FeO to nanophase metallic iron particles (npFe⁰), or “iron blebs,” as at the Moon. Near- and mid-infrared spectroscopy indicate clino- and ortho-pyroxene are present at different locations. There is some evidence for no- or low-iron alkali basalts and feldspathoids. All evidence, including microwave studies, point to a low iron and low titanium surface. There may be a link between the surface and the exosphere that may be diagnostic of the true crustal composition of Mercury. A structural global dichotomy exists with a huge basin on the side not imaged by Mariner 10. This paper briefly describes the implications for this dichotomy on the magnetic field and the 3 : 2 spin : orbit coupling. All other points made above are detailed here with an account of the observations, the analysis of the observations, and theoretical modeling, where appropriate, that supports the stated conclusions.     

一种Turbo码短交织器的设计方法

短交织器的结构对Turbo码的性能有很大的影响,通过探讨Turbo码编码器中反馈最小多项式的周期性和序列的可整除性问题,把可整除序列变为不可整除序列交织器,从而获得高码重的码字,并给出一种基于输入信息序列周期性特性的短交织器的设计方法.仿真结果表明是一种很有效的设计方法.     

Optical and X-ray aspects of quasars

We review the present knowledge on the cosmological evolution of quasars, by discussing some of the recent results obtained from studies of optically selected objects. Despite the fast development of prism survey tecniques, the color selection still appears to be the best tecnique for constructing the complete samples which are necessary for statistical studies. It is shown, however, that even the best available complete samples of quasars selected on the basis of ultraviolet excess (z < 2.2) are not sufficient to univocally determine the “correct” evolutionary model. Moreover, some preliminary results suggest that the evolution law derived from quasars with m_B<20 and z<2.2 can not be extrapolated to fainter magnitudes and higher redshifts. On the basis of what is known today about the optical and X-ray properties of quasars, we then discuss some of teh possible results, relevant to cosmology, which can be achieved with future coordinated optical and X-ray observations of quasars.     

非连续系统控制的研究

综述Ｂａｎｇ－Ｂａｎｇ控制、变结构控制、模糊控制、ＰＷＭ及ＰＣＭ（脉冲码控制）等非连续系统控制的原理及设计方法与近期研究成果，这些控制方法简化了机械结构并可达到复杂的控制，故具有广阔的应用前景。     

反欺骗抗干扰方法中欺骗脉冲的选择研究

反欺骗抗干扰方法是通过在真实脉冲前加入欺骗脉冲,使敌方干扰机截获欺骗脉冲释放干扰,抑制干扰幅度,可以从源头上削弱干扰效果。欺骗脉冲的选择影响抑制干扰幅度的效果,因此通过分析单频、伪随机码调相和线性调频等不同调制方式的欺骗脉冲与真实脉冲的失配效果,给出欺骗脉冲选择策略。     

导航辅助下基于LAS码的天基多目标测控

中继卫星的天基测控是解决中低轨道航天器大范围、长时间、多目标测控的有效途径,但用户星到中继卫星的时延误差、多普勒频移校正误差等参数会对多目标测控带来干扰。针对该问题,首先分析了定位误差引起的时延误差、多普勒频移校正误差等因素,设计了天基多目标前向链路遥控SMA(S-band Multiple Access,S频段多址)信号形式和反向遥测链路SMA信号形式,选择与时延校正误差相匹配的LAS(Large Area Synchronous,大区域同步)码作为反向遥测信息的扩频码,建立了导航辅助的终端时延和频率预校正方案模型,可以有效消除多用户干扰。仿真表明,当Eb/N0≥10.5dB时,前向遥控信息误码率pe≤1×10~(-6),反向遥测信息误码率pe≤1×10~(-6),使用LAS码比Gold序列约有2dB性能改善,为基于我国天链卫星的中低轨道卫星稳定运行、载人航天交会对接以及后续空间站建设等任务的测控提供重要参考。     

双星定位系统入站信号在低信噪比条件下的快速捕获

从整个系统的角度出发,对各种可行的快捕方式进行了分析,建立了简明准确的数学模型。运用这些数学模型就伪随机码、高斯限带噪声和多卜勒频移对快捕性能的影响进行了计算机模拟分析,得出了一些定量和定性的结论。并指出SAW 匹配滤波器是一种最佳的选择。此外,还对RDSS 标准入站信号的伪码同步图案进行了理论分析,并构想了一种可能的捕获方式。