Q-learning强化学习协同拦截制导律CSCD

为实现多枚导弹协同拦截机动目标,提升拦截效能,提出了一种Q-learning强化学习协同拦截制导律。首先,基于逃逸域覆盖理论,建立了非线性多弹协同拦截模型。其次,以视线角速率为状态,依据脱靶量构造奖励函数,通过离线训练生成强化学习智能体,并结合传统比例制导控制方法,构建基于强化学习的变导引系数制导律,实时生成实现协同拦截的制导指令。最终,通过数值仿真验证了所提算法的有效性和优越性。     

轴流压气机近失速及旋转失速全通道数值模拟

为研究轴流压气机失速起始的动态过程,对某两级低速轴流压气机的第1级进行整环全通道模拟.结果表明:在近失速点流场中存在周向大尺度的速度波动,该波动与静子叶排首先出现的周向不均匀分布的叶背附面层分离密切相关,并且随着压气机进一步节流,波动幅值逐渐增大,最终诱发转子若干通道出现严重附面层分离,堵塞流道,压气机进入旋转失速.失速团完全发展后的转动频率与试验结果吻合较好.      

一种精度可调的速度测量系统的设计与实现

根据常用的频率采集方法,结合速度矢量信号的特点,提出了将速度矢量信号转换为不同相位的频率信号以实现速度矢量采集的设计思路,通过软硬件结合的方式实现速度采集系统.为提高系统的测试性,设计了自激励测试电路.为了解决速度变化带来的采样精度低问题,设计了采样时钟自动调整机制.经测试,采集结果准确,精度可调,可满足系统要求.     

Status of MAGIC and recent results

Ground-based γ-ray astronomy is part of a new field of fundamental research of Astroparticle Physics, that recently made spectacular discoveries mostly thanks to Imaging Air Cherenkov Telescopes (IACT). The MAGIC telescope is a IACT located at La Palma, Canary Islands, Spain. Composed of two telescopes with 17 m diameter each, MAGIC is equipped with the largest optical reflectors in the world, and it has the lowest threshold energy (25 GeV). MAGIC started operations in 2004 in the single-detector configuration, and in 2009 as a stereo detector. Since then, it has discovered many new sources and classes of sources, both galactic and extragalactic. Here some highlights from the most recent results are presented.     

One dimensional blood flow in a planetocentric orbit

All life on earth is accustomed to the presence of gravity. When gravity is altered, biological processes can go awry. It is of great importance to ensure safety during a spaceflight. Long term exposure to microgravity can trigger detrimental physiological responses in the human body. Fluid redistribution coupled with fluid loss is one of the effects. In particular, in microgravity blood volume is shifted towards the thorax and head. Sympathetic nervous system-induced vasoconstriction is needed to maintain arterial pressure, while venoconstriction limits venous pooling of blood prevents further reductions in venous return of blood to the heart. In this paper, we modify an existing one dimensional blood flow model with the inclusion of the hydrostatic pressure gradient that further depends on the gravitational field modified by the oblateness and rotation of the Earth. We find that the velocity of the blood flow V_B is inversely proportional to the blood specific volume d, also proportional to the oblateness harmonic coefficient J₂, the angular velocity of the Earth ω_E, and finally proportional to an arbitrary constant c. For c = −0.39073 and ξ_H = −0.5 mmHg, all orbits result to less blood flow velocities than that calculated on the surface of the Earth. From all considered orbits, elliptical polar orbit of eccentricity e = 0.2 exhibit the largest flow velocity V_B = 1.031 m/s, followed by the orbits of inclination i = 45°and 0°. The Earth’s oblateness and its rotation contribute a 0.7% difference to the blood flow velocity.     

一种负升力超高声速临近空间突击飞行概念

提出一种飞行高度70 km以上的超高速临近空间飞行概念,旨在通过火箭发动机克服大气阻力作用,通过负升力达到"增加"地球引力常数的等效效果,实现高于地球环绕速度的突击飞行,具有速度快、航程远的特点.分析了等高度巡航过程的受力情况,对气动参数选取、能量需求等问题进行了分析,给出了这类飞行器可能运行的空间区域.分析表明,该飞行方式可以实现在40 min内全球到达.     

Interactive database of cosmic ray anisotropy (DB-A10)

The worldwide neutron monitor network is a unique tool for obtaining with high accuracy the information on density variations, energy spectrum and anisotropy of comic rays at the Earth, outside its atmosphere and magnetosphere. These hourly averaged parameters were obtained over the whole period of cosmic ray monitoring by the ground level neutron monitor network (from 1957 till present) and are collected within the MySQL database. The Internet-project has developed for free access and supplying of cosmic ray density and anisotropy data in different formats.     

Russian ground-level detectors of cosmic ray observations as a part of the world wide network: History and development

The history of creation and development of the network of cosmic ray stations in USSR-Russia goes back to the difficult years of the Second War (1944–1945). The Russian neutron monitor network continuously operates at the present time, having developed from a mechanical means of registration into a modern electronic system for the collection and processing of data with the results presented in the Internet in real time. Along with the improvement of the equipment and different methods of data processing, strong scientific groups, and even Institutes have grown up at a number of stations. They carry out scientific investigations on the basis of neutron monitor network data and provide the conditions for operative and real time exchange of data.     

Possible consequences of a disk around B0656+14 on e–e and near-1 Hz gravitational wave production

Nearby pulsars B0656+14 and Geminga were proposed in the literature as the main sources of cosmic-ray positrons observed near Earth above 10 GeV. B0656+14 has comparable distance from Earth, similar magnetic field and period of Geminga. However, observations in the R and I bands indicate the presence of a disk of approximately 10⁻⁴ M_⊙ around B0656+14. Radio and pulsed γ-ray flux observations from this pulsar are also consistent with supernova fallback material and disk entering the light cylinder and partially quenching the development of electromagnetic showers in the magnetosphere. If this is the case, B0656+14 has unlikely given any contribution to e⁺ and e⁻ observed near Earth. Absolute flux measurements and the level of anisotropy in the high energy electron and positron arrival directions above 50 GeV will help in revealing if none, one of both nearby pulsars are sources of these particles observed near Earth.