On m-ovoids of finite classical polar spaces with an irreducible transitive automorphism group

In this paper, we classify the m-ovoids of finite classical polar spaces that admit a transitive automorphism group acting irreducibly on the ambient vector space. In particular, we obtain several new infinite families of transitive m-ovoids.

Air-Stable Dy(III)-Macrocycle Enantiomers:From Chiral to Polar Space Group

Magnetoelectric(ME)multiferroic materials have unique advantages in low-power and high-density information storage,because they can simultaneously display ferroelectricity and ferromagnetism.However,research on how to construct air-stable highperformance ME single-molecule magnets(SMMs)is nonexistent.Herein,by introducing homochirality while reducing molecular symmetry,two doubledecker Dy(III)enantiomers adopting the polar space group P2_(1) and exhibiting excellent thermal stability were obtained.They displayed zero field SMM behavior with an anisotropy barrier(Ueff)of ca.100 cm^(−1).This work establishes a rational chemical design strategy for crystallizing SMMs in polar space groups and elucidates the direction for future research,that is,engineering small-size high-performance SMMs.

基于KA-SRCN-pSTAP的低空风切变风速估计方法

针对由于独立同分布(IID)样本严重不足,导致极化空时自适应(pSTAP)处理性能下降,进而导致低空风切变风速估计不准确的问题,本文提出了一种基于知识辅助的稀疏表示杂波零陷极化空时自适应(KA-SRCN-pSTAP)的低空风切变风速估计方法。该方法首先利用杂波脊的先验知识辅助构造极化空时稀疏字典,然后利用极化空时稀疏字典,通过SRCN算法挑选原子并对到杂波线性子空间补空间上的投影矩阵进行估计,从而得到pSTAP权矢量,最后构造pSTAP滤波器对地杂波进行抑制,准确估计低空风切变风速。该方法仅使用少量IID样本,将SRCN算法与极化-空时域相结合,完成对风切变风速的有效估计。仿真实验结果证明该方法可以有效实现少样本情况下的风速准确估计。

交替极化阵列对消盲区分析与验证

当干扰信号的空域和极化域特征与目标信号相似时,采用空极化域联合抗干扰技术在消除干扰的同时也会抑制目标信号,导致干扰对消后信干噪比(signal to interference plus noise ratio,SINR)低于雷达系统需求,从而形成干扰对消盲区。针对这一现象,通过在空域、极化域与空极化域分别建立交替极化阵列对消盲区模型,推导了对消盲区位置和大小的数学表达式,从而给出了交替极化阵列对消盲区的数学表征方法。进而分析了交替极化阵列对消盲区的分布规律与影响因素,研究发现阵元间距能够显著影响交替极化阵列对消盲区的分布,在相同条件下交替极化阵列对消盲区大于共点极化阵列对消盲区,结果表明交替极化阵列虽然通过减少天线数目降低了设备成本,但增大了阵列的对消盲区。然后,对消盲区模型进行了数值仿真,仿真结果验证了理论分析。最后,利用信道模拟器搭建了实验平台,信道模拟实验测得的对消盲区与理论值基本一致,再次证明了分析结论的有效性。

突发事件下的封闭空间情绪传播模型研究

为避免突发事件中复杂情绪在封闭空间内无序发酵引发衍生灾害,探索封闭空间的情绪传播规律,基于情绪自发传播模型SISa,考虑封闭空间个体情绪的差异性、群体极化现象、特殊情绪交互方式以及危急情景下的动态感染率,分别改进主体情绪状态、情绪转移路径、交互模式与感染率,提出1种适用于封闭空间的情绪传播模型SE 4Sa,并以武汉地铁2号线为例完成数值仿真与敏感性分析。研究结果表明:情绪自发转移过程对限制负面情绪累积起到关键作用,且情绪极化现象使系统危险性大幅增长;缩减个体情绪感知域使系统稳定时间缩短90.6%、高唤醒负面情绪占比下降27.4%;突发事件下的动态感染率更符合封闭空间情绪传播特性。研究结果可为突发事件下封闭空间的群体行为和群体情绪规律研究提供理论支持。

空间天文紫外偏振探测技术研究进展

新型空间天文探测技术在科学进步和国家发展方面起着至关重要的作用。其高精度的观测提供了独特的机遇,深化了人们对宇宙的理解,同时推动了天体物理学和宇宙学的前沿研究。这些探测不仅为理论模型的验证与发展提供了不可或缺的数据,还在基础物理学领域催生了新理论。在国家层面,拥有先进的空间天文探测技术不仅凸显了国家在科研领域的实力,同时为培养高水平的科研人才提供了重要平台,有助于国家在全球科研舞台上赢得竞争优势。因此,对新型空间天文探测技术的研究和发展显得十分紧迫。天文紫外偏振作为一种创新的空间天文探测手段,相较于传统探测手段,紫外偏振测量技术能够提供多维度的观测数据,进而实现全方位的宇宙感知能力,具备巨大地应用潜力。鉴于目前尚未有关于空间天文紫外偏振探测的系统性综述报告和文章,因此,文中从紫外偏振科学研究的角度出发,总结已有的紫外偏振载荷,挖掘这一领域技术发展的思路和途径,最后对该技术未来发展方向进行展望与总结,为我国在该领域的未来研究提供有益参考。

TG-2伽玛暴偏振探测仪POLAR

伽玛暴偏振的测量对喷流机制的确定有着至关重要的作用。伽玛暴偏振探测仪POLAR是中欧合作的、专门用于探测伽玛暴偏振的探测仪器,POLAR通过康普顿散射的原理实现对伽玛暴偏振度高灵敏度的测量。介绍了POLAR的整体方案和载荷研制情况,通过蒙卡模拟和地面实验对仪器性能进行验证,结果表明POLAR具有符合设计要求的偏振测量能力。

基于空时极化处理的机载雷达非平稳杂波抑制方法

针对传统方位-多普勒域空时自适应处理(STAP)方法无法区分不同模糊距离单元的杂波,难以有效抑制近程非平稳杂波的问题,提出了基于空时极化处理的机载雷达非平稳杂波抑制方法.该方法在俯仰-方位-多普勒3D-STAP方法的基础上引入回波的极化维信息,然后对回波信号进行极化-俯仰-方位-多普勒四维联合空时极化自适应处理.仿真结果表明,相对于传统方位-多普勒域STAP方法和俯仰-方位-多普勒3D-STAP方法,本文所提方法可更有效地实现对非平稳杂波的抑制.

浅谈极区空间物理学的科学革命

极区空间物理学重要的研究方向之一是剖析南北两极的热层、电离层和磁层的耦合问题。本文简明扼要地描述了极区空间物理学的一场革命——即理论框架的革新。这场科学革命是用磁流体力学理论取代电机工程理论,目前进行得比较缓慢,但将在今后的30~50年彻底改变人们对于热层-电离层-磁层的认知。

铜电解电效影响因素及控制措施

铜电解过程中,电流效率是极为重要的经济技术指标。随着国家绿色发展政策的实施,工业用电电价逐渐上升,铜电解过程电流效率的控制就显得尤为重要。本文分析总结了影响铜电解电流效率的各因素,针对其中极间距、槽电压等重要影响因素,提出了铜电解电效控制措施方法,可以有效提高和稳定电流效率,对降低铜电解生产成本有参考价值。

高压电缆在电压极性反转过程中的空间电荷行为研究

为探明同轴结构交联聚乙烯(XLPE)电缆绝缘在外施电压极性反转过程中的空间电荷注入、迁移、抽出等动态演变规律,分析外施电压极性反转过程中空间电荷导致的反转“滞后效应”,并探究温度梯度协同作用的影响规律,对XLPE电缆进行了不同电场强度、温度梯度场下,外施电压快速极性反转过程中的空间电荷研究,并基于异极性电荷注入、迁移理论,对极性反转过程中电缆绝缘空间电荷的演变规律进行分析。研究结果表明:XLPE电缆在外施电压快速反转过程中,由于电缆绝缘内部残余电荷的影响,电缆两侧电极电荷峰表现出不平衡的反转特性,导致电缆外半导电层电极的电荷峰出现了明显的反转“滞后效应”。

非机械指向空间激光通信接收系统设计与分析

采用非机械指向结构能够极大缩小空间激光通信系统尺寸与重量,由于现有器件性能局限,目前尚未见到成熟的非机械指向空间激光通信接收系统。提出基于正交液晶级联偏振光栅与四象限探测器的空间激光通信接收光学系统,利用了正交液晶级联偏振光栅体积小、口径大、偏转范围大,及四象限探测器接收角度范围大的优势,根据正交液晶级联偏振光栅与四象限探测器的理论与器件性能,设计了光学系统,分析了探测器噪声、背景噪声、系统噪声对于通信与入射角度测量的影响,计算了可实现的通信速率,给出了系统的最大响应角速度。

遥感卫星地面站天线遮挡预报模型及其应用

基于遥感卫星地面站业务运行中所遇到的实际问题和运行经验,为降低因地面站天线周边遮挡物对低轨道空间科学卫星、陆地观测卫星等极轨卫星的空间通信任务所产生的影响,以提高航天器和地面的有效通信时长和通信质量为目标,将地面站天线作为基准,对周边环境的遮挡进行建模分析.建立遮挡模型空间几何关系,模型选择推导“天线无遮挡最小仰角”的求解思路,通过模型分析和推导得到了遮挡物的实体遮挡模型公式和大型天线遮挡模型公式.通过模型验证,将模型计算结果同实际遮挡采样信息对比,结果表明遮挡模型和遮挡实际情况基本吻合,模型计算结果准确度可达到99.67%.以天线遮挡预报模型为信息支持,将天线遮挡预报封装成服务,在任务规划阶段调用天线遮挡预报的计算服务和相应任务规划策略,以实现天线遮挡预报模型在地面站运行管理资源调度中的工程应用.经试运行和应用统计结果表明,某地面站的运行管理资源调度优化率达到56.07%.

基于空间馈电的高功率波束扫描螺旋透射阵列天线设计

传统的透射式空馈阵列存在功率容量低的缺点,不能直接应用于高功率微波领域。现有的高功率空馈阵列布局不够灵活,波束扫描速度较慢,不能充分发挥空馈阵列在系统集成方面的优势。提出并设计了一种新型的采用空间馈电的螺旋辐射单元,并构建了一种透射式空馈螺旋阵列天线,通过控制单个螺旋旋转可以实现二维波束扫描,在设计上更加灵活,可根据实际应用需求调整阵列布局,符合高功率微波天线紧凑化、模块化的发展趋势。仿真设计了包含324个单元的透镜阵列,数值模拟结果表明,单元反射系数S11≤-20 dB,功率容量0.35 MW,阵列口径效率0.68,可在±45°范围内扫描,最大增益下降3 dB。

基于模式空间-极化平滑的均匀圆阵解相干算法

为实现极化敏感阵列的相干信源波达方向(direction of arrival,DOA)估计,提出了一种均匀圆阵的极化敏感阵列解相干算法。通过对均匀圆阵极化敏感阵列的输出信号作模式变换,使其阵列流形生成的虚拟均匀线阵具有与均匀线阵相似的平移不变性,继而采用平滑重构Toeplitz矩阵使其秩与信号相干性无关,实现了对相干信号的DOA估计。通过仿真实验将该算法与其他两种模式空间算法进行了对比,验证了该算法在角分辨率和目标检测概率上的优越性。该算法具有广阔的应用前景。

Progress in polar upper atmospheric physics research in China

The Chinese Antarctic Great Wall, Zhongshan, Kunlun and Arctic Yellow River stations have unique geographical locations, well suited to carry out polar upper atmospheric observations. This paper reviews the tremendous history of nearly 30 years of Chinese polar expeditions and major progress in polar upper atmospheric physics research. This includes the polar upper atmospheric physics conjugate observation system at Zhongshan Station in the Antarctic and Yellow River Station in the Arctic, and original research achievements in polar ionospheric fields, aurora and particle precipitation, the polar current system, polar plasma convection, geomagnetic pulsations and space plasma waves, inter-hemispheric comparisons of the space environment, space weather in polar regions, power spectrum of the incoherent scatter radar, ionospheric heating experiments and polar meso- spheric summer echoes, polar ionosphere-magnetosphere numerical simulation and others. Finally, prospects for Chinese polar upper atmospheric physics research are outlined.

SCATTERING OF CIRCULAR CAVITY IN RIGHT-ANGLE PLANAR SPACE TO STEADY SH-WAVE

Complex function method and multi-polar coordinate transformation technology are used here to study scattering of circular cavity in right-angle planar space to SH-wave with out-of-plane loading on the horizontal straight boundary. At first, Green function of right-angle planar space which has no circular cavity is constructed; then the scattering solution which satisfies the free stress conditions of the two right-angle boundaries with the circular cavity existing in the space is formulated. Therefore, the total displacement field can be constructed using overlapping principle. An infinite algebraic equations of unknown coefficients existing in the scattering solution field can be gained using multi-polar coordinate and the free stress condition at the boundary of the circular cavity. It can be solved by using limit items in the infinite series which can give a high computation precision. An example is given to illustrate the variations of the tangential stress at the boundary of the circular cavity due to different dimensionless wave numbers, the location of the circular cavity, the loading center and the distributing range of the out-of-plane loading. The results show the efficiency and effectiveness of the mothod introduced here.

A novel x-ray circularly polarized ranging method

Range measurement has found multiple applications in deep space missions. With more and further deep space ex- ploration activities happening now and in the future, the requirement for range measurement has risen. In view of the future ranging requirement, a novel x-ray polarized ranging method based on the circular polarization modulation is proposed, termed as x-ray circularly polarized ranging （XCPolR）. XCPolR utilizes the circular polarization modulation to process x-ray signals and the ranging information is conveyed by the circular polarization states. As the circular polarization states present good stability in space propagation and x-ray detectors have light weight and low power consumption, XCPolR shows great potential in the long-distance range measurement and provides an option for future deep space ranging. In this paper, we present a detailed illustration of XCPolR. Firstly, the structure of the polarized ranging system is described and the signal models in the ranging process are established mathematically. Then, the main factors that affect the ranging accuracy, including the Doppler effect, the differential demodulation, and the correlation error, are analyzed theoretically. Finally, numerical simulation is carded out to evaluate the performance of XCPolR.

Einstein’s General Relativity and Pure Gravity in a Cosserat and De Sitter-Witten Spacetime Setting as the Explanation of Dark Energy and Cosmic Accelerated Expansion

Ordinary energy and dark energy density are determined using a Cosserat-Cartan and killing-Yano reinterpretation of Einstein’s special and general relativity. Thus starting from a maximally symmetric space with 528 killing vector fields corresponding to Witten’s five Branes model in eleven dimensional M-theory we reason that 504 of the 528 are essentially the components of the relevant killing-Yano tensor. In turn this tensor is related to hidden symmetries and torsional coupled stresses of the Cosserat micro-polar space as well as the Einstein-Cartan connection. Proceeding in this way the dark energy density is found to be that of Einstein’s maximal energy mc2 where m is the mass and c is the speed of light multiplied with a Lorentz factor equal to the ratio of the 504 killing-Yano tensor and the 528 states maximally symmetric space. Thus we have E (dark) = mc2 (504/528) = mc2 (21/22) which is about 95.5% of the total maximal energy density in astounding agreement with COBE, WMAP and Planck cosmological measurements as well as the type 1a supernova analysis. Finally theory and results are validated via a related theory based on the degrees of freedom of pure gravity, the theory of nonlocal elasticity as well as ‘t Hooft-Veltman renormalization method.

Recent progress in Chinese polar upper-atmospheric physics research: review of research advances supported by the Chinese Arctic and Antarctic expeditions

It has been more than 30 years since the first Chinese Antarctic Expedition took place. Polar upper atmospheric observations started at this time. First began at Great Wall Station and then at Zhongshan Station in Antarctica, and later in the Arctic at Yellow River Station, Kjell Henriksen Observatory on Svalbard, and at the China-Iceland Joint Aurora Observatory in Iceland. In this paper, we reviewed the advances in polar upper atmosphere physics （UAP） based on the Chinese national Arctic and Antarctic research over the last five years. These included newly deployed observatories and research instruments in the Arctic and Antarctic; and new research findings, from grotmd-based observations, about polar ionosphere dynamics, aurora and particle precipitation, polar plasma convection, geomagnetic pulsations and space plasma waves, space weather in the polar regions, simulations of the polar ionosphere-magnetosphere. In conclusion, suggestions were made for future polar upper atmosphere physics research in China.