A statistical study of CME-associated flare during the solar cycle 24

We investigate on the relationship between flares and coronal mass ejections (CMEs) in which a flare started before and after the CME events which differ in their physical properties, indicating potentially different initiation mechanisms. The physical properties of two types flare-correlated CME remain an interesting and important question in space weather. We study the relationship between flares and CMEs using a different approach requiring both temporal and spatial constraints during the period from December 1, 2008 to April 30, 2017 in which the CMEs data were acquired by SOHO/LASCO (Solar and Heliospheric Observatory/Large Angle Spectrometric Coronagraph) over the solar cycle 24. The soft X-ray flare flux data, such as flare class, location, onset time and integrated flux, are collected from Geostationary Environmental satellite (GOES) and XRT Flare catalogs. We selected 307 CMEs-flares pairs applying simultaneously temporal and spatial constraints in all events for the distinguish between two associated CME-flare types. We study the correlated properties of coincident flares and CMEs during this period, specifically separating the sample into two types: flares that precede a CME and flares that follow a CME. We found an opposite correlation relationship between the acceleration and velocity of CMEs in the After- and Before-CMEs events. We found a log-log relation between the width and mass of CMEs in the two associated types. The CMEs and flares properties show that there were significant differences in all physical parameters such as (mass, angular width, kinetic energy, speed and acceleration) between two flare-associated CME types.     

考虑模态质量耦合的随机振动准静态载荷计算

针对目前模态质量参与法没有考虑模态质量耦合影响而导致模态密集时随机振动准静态载荷计算出现较大误差，从多自由度振动方程出发，利用模态理论和随机谱理论，分析推导出包含模态质量耦合作用的完全模态质量参与法，分析了耦合项的影响规律。此改进的模态质量参与法可用于计算包括密集模态在内的随机振动准静态载荷，并针对模态频率比大于0.95的密集模态给出简化计算公式。以一个算例验证了密集模态的准静态加速度载荷计算。     

单喷管火箭自由喷流噪声数值模拟

利用非定常燃气流场数值模拟方法，研究超声速喷流核心区及其外围亚声速区燃气流动态分布和流动特性，在此基础上利用欧拉方程条件的伽辽金有限元方法以及FWH方法，实现并完成喷流噪声传播特性、辐射特性数值模拟。喷流噪声数值模拟结果显示：燃气流推进初期，强喷流噪声区域紧随燃气流前锋；燃气流场相对稳定后，强喷流噪声区域主要位于燃气流等能区末稍，一些小尺度试验的燃气流激波系附近也存在较强喷流噪声。这些强喷流噪声主要由燃气流前锋带动的大涡动态卷吸、燃气流强湍流脉动以及激波扰动引起。受数值模拟网格分辨率影响，当前仅能保持中低频段声压级数值模拟结果与实测结果总体接近。     

高速飞行器变质心控制技术综述

基于变质心附加惯量消旋、质量矩姿控、操稳性能调控三种控制模式对变质心控制的基本原理进行了阐述.详细分析了变质心高速飞行器所面临的动力学建模、制导控制、执行机构设计研制和系统仿真评估四方面的关键控制问题.最后,对变质心高速飞行器发展趋势和未来主要研究方向进行了展望.     

CMEs and active regions on the sun

The relationship between active regions (ARs) and coronal mass ejections (CMEs) is studied. For this purpose a statistical analysis of 694 CMEs associated with ARs was carried out. We considered the relationship between properties of the CMEs and ARs characterized using the McIntosh classification. We demonstrated that CMEs are likely to be launched from ARs in the mature phase of their evolution when they have complex magnetic field. The fastest and halo CMEs can be ejected only from the most complex ARs (when an AR is a bipolar group of spots with large asymmetric penumbras around the main spot with many smaller spots in the group). We also showed that the wider events have a tendency to originate from uncomplicated magnetic structures. This tendency was used for estimation of the real angular widths of the halo CMEs. The probability of launching of fast CMEs increases together with increase of the complexity and size of ARs. The widest, but slow, CMEs originate from the simplest magnetic structure which are still able to produce CMEs. Our results could be useful for forecasting of space weather.     

Phobos-Grunt: Russian sample return mission

As an important milestone in the exploration of Mars and small bodies, a new generation space vehicle “Phobos-Grunt” is planned to be launched by the Russian Aviation and Space Agency. The project is optimized around a Phobos sample return mission and follow up missions targeted to study some main asteroid belt bodies, NEOs and short period comets. The principal constraint is use of the “Soyuz-Fregat” rather than the “Proton” launcher to accomplish these challenging goals. The vehicle design incorporates innovative SEP technology involving electrojet engines that allowed us to increase significantly the mission's energetic capabilities, as well as highly autonomous on-board systems. Basic criteria underlining the “Phobos-Grunt” mission scenario, scientific objectives and rationale including Mars observations during the vehicle's insertion into Mars orbit and Phobos approach maneuvers, are discussed and an opportunity for international cooperation is suggested.     

Numerical investigation on jet interaction with a compression ramp

A numerical investigation on jet interaction in supersonic laminar flow with a compres- sion ramp is performed utilizing the AUSMDV scheme and a parallel solver. Several parameters dominating the interference flowfield are studied after defining the relative increment of normal force and the jet amplification factor as the evaluation criterion of jet control performance. The computational results show that most features of the interaction flowfield between the transverse jet and the ramp are similar to those between a jet and a flat plate, except that the flow structures are more complicated and the low-pressure region behind the jet is less extensive. The relative force increment and the jet amplification factor both increase with the distance between the jet and the ramp shortening till quintuple jet diameters. Inconspicuous difference is observed between the jet-before-ramp and jet-on-ramp cases. The variation of the injection angle changes the extent of the separation region, the plateau pressure, and the peak pressure near the jet. In the present computational conditions, 120 is indicated relatively optimal among all the injection angles studied. For cold gas simulations, although little influence of the jet temperature on the pressure distribution near the jet is observed under the computation model and the flow parameters studied, reducing jet temperature somehow benefits the improvement of the normal force and the jet efficiency. When the pressure ratio of jet to freestream is fixed, the relative force increment varies little when increasing the freestream Mach number, while the jet amplification factor increases.     

纳米胶体射流抛光技术综述

纳米胶体射流抛光技术是一种超光滑表面加工方法,加工范围广,具有广泛的应用前景。本文回顾了纳米胶体射流抛光技术的提出以及目前的研究现状,最后对其今后的发展进行了简单展望。     

有效载荷基频降低对火箭动特性的影响

为了分析有效载荷基频降低对火箭动特性的影响规律,采用纵横扭一体化梁模型与耦合质量方法模拟箭体承力结构与液体推进剂,使用NASTRAN中的RBE2单元模拟芯级与助推器连接接头.通过修改有效载荷有限元模型以得到不同的有效载荷基频,选取飞行过程中的四个典型秒状态,计算三种不同有效载荷基频下全箭的前九阶固有振动频率.结果表明：纵横扭一体化梁模型在进行全箭动特性分析时模型简单,结果满足要求,可用于设计初期的模态分析;同时,分析得到基频降低对全箭动特性的影响规律,给卫星设计人员提供了相关依据.     

基于A*算法的质量特性测试流程规划

航天器质量特性集成测试内容复杂且相互依赖,为了减少反复,提高效率,文章对测试流程进行了规划。首先对测试路网进行建模,继而采用A＊算法搜索最佳路径,最后得到目标测试流程。开销计算表明,与目前使用的典型流程相比,目标流程更优化。