导弹子母弹子弹抛撒弹道模型及数字仿真

建立了导弹子母弹抛撒弹道模型，并编制了抛撒弹道仿真程序，仿真结果与靶场试验结果一致，仿真程序也适用于所有弹道导弹子母弹撒 轴对称子弹的无控弹道仿真，可为地地导弹子母作战使用及作战效能研究提供强有力的分析工具。     

Optimization and verification of free flight separation similarity law in high-speed wind tunnel

Based on the similarity of separation time, a similarity law optimization method for high-speed weapon delivery test is derived. The typical separation state under wind load is simulated by the numerical method. The real separation data of aircraft, separation data of previous test methods, separation data of ideal wind tunnel test of previous methods, and simulation data of the proposed optimization method are obtained. A comparison of the data shows that the method proposed can improve the performance of tracking. Similarity law optimization starts with the development of motion equations and dynamic equations in the windless state to address the problems of mismatching between vertical and horizontal displacement, and to address the problems of separation trajectory distortion caused by insufficient gravity acceleration of the scaling model of existing light model. The ejection velocity of the model is taken as a factor/vector, and is adjusted reasonably to compensate the linear displacement insufficiency caused by the insufficient vertical acceleration of the light model method, so as to ensure the matching of the vertical and horizontal displacement of the projectile, and to improve the consistency between the test results of high-speed projection and the actual separation trajectory. The optimized similarity law is applicable to many existing free-throwing modes of high-speed wind tunnels. The optimized similarity law is not affected by the ejection velocity and hanging mode of the projectile. The optimized similarity law is suitable not only for the launching of the buried ammunition compartment and external stores, but also for the test design of projectile launching and gravity separation.     

一种引射增强型二次喉道新方案的数值模拟

为提高大型超声速风洞的运行经济性,设计了一种通过引射低总压冷介质提高扩压性能的新型二次喉道扩压器,其结构特征是在扩压器收敛段前方增加侧壁凹槽,在凹槽前沿位置引入低总压常温空气作为冷介质,通过引射扩散作用在扩压器壁面形成气膜,调节二次喉道实际流通直径,较大程度上增强二次喉道的静压恢复能力,同时又降低二次喉道壁面热负荷,冷却壁面。数值验证结果表明,所设计新型二次喉道方案可通过调节引射气量自适应较宽范围的运行条件,有效隔离扩压器壁面直接接触高温燃气,同时提高了扩压能力,节省后段接力引射器的主动流流量近30%,对风洞运行经济性提升十分明显。     

Investigating the Coronal Mass Ejections associated with DH type-II radio bursts and solar flares during the ascending phase of the solar cycle 24

We studied a set of 74 CMEs, with shedding the light on the halo-CMEs (HCMEs), that are associated with decametric – hectometric (DH) type-II radio bursts (1–16?MHz) and solar flares during the period 2008–2014. The events were classified into 3 groups (disk, intermediate, and limb events) based on their longitudinal distribution.We found that the events are mostly distributed around 15.32° and 15.97° at the northern and southern solar hemispheres, respectively. We found that there is a clear dependence between the longitude and the CME’s width, speed, acceleration, mass, and kinetic energy. For the CMEs’ widths, most of the events were HCMEs (～62%), while the partial HCMEs comprised ～35% and the rest of events were CMEs with widths less than 120°. For the CMEs’ speeds, masses, and kinetic energies, the mean values showed a direct proportionality with the longitude, in which the limb events had the highest speeds, the largest masses, and the highest kinetic energies. The mean peak flux of the solar flares for different longitudes was comparable, but the disk flares were more energetic. The intermediate flares were considered as gradual flares since they tended to last longer, while the limb flares were considered as impulsive flares since they tended to last shorter.A weak correlation (R?=?0.32) between the kinetic energy of the CMEs and the duration of the associated flares has been noticed, while there was a good correlation (R?=?0.76) between the kinetic energy of the CMEs and the peak flux of the associated flares. We found a fair correlation (R?=?0.58) between the kinetic energy of the CMEs and the duration of the associated DH type-II radio bursts.     

Strong geomagnetic activity forecast by neural networks under dominant southern orientation of the interplanetary magnetic field

The paper deals with the relation of the southern orientation of the north–south component _Bz$B_z$ of the interplanetary magnetic field to geomagnetic activity (GA) and subsequently a method is suggested of using the found facts to forecast potentially dangerous high GA. We have found that on a day with very high GA hourly averages of _Bz$B_z$ with a negative sign occur at least 16 times in typical cases. Since it is very difficult to estimate the orientation of _Bz$B_z$ in the immediate vicinity of the Earth one day or even a few days in advance, we have suggested using a neural-network model, which assumes the worse of the possibilities to forecast the danger of high GA – the dominant southern orientation of the interplanetary magnetic field. The input quantities of the proposed model were information about X-ray flares, type II and IV radio bursts as well as information about coronal mass ejections (CME). In comparing the GA forecasts with observations, we obtain values of the Hanssen–Kuiper skill score ranging from 0.463 to 0.727, which are usual values for similar forecasts of space weather. The proposed model provides forecasts of potentially dangerous high geomagnetic activity should the interplanetary CME (ICME), the originator of geomagnetic storms, hit the Earth under the most unfavorable configuration of cosmic magnetic fields. We cannot know in advance whether the unfavorable configuration is going to occur or not; we just know that it will occur with the probability of 31%.     

弹射动力系统燃气发生器流热固耦合数值研究

为了判断弹射动力系统燃气发生器工作的安全性,需要预示工作过程中燃气发生器壳体的力学响应。基于软件CFX和ANSYS,建立了燃气发生器复合结构流热固耦合仿真模型。对燃气发生器内流场和结构温度场进行流热耦合计算,并将壳体温度场计算结果与试验数据进行对比,再将算得的燃气压强分布与结构温度场分布导入ANSYS以计算结构的力学响应。计算结果表明,燃气发生器工作过程中,直筒段最高温度点位于直筒段与后封头连接的绝热层缝隙处,后封头最高温度点位于后封头与喉衬配合部位的上游端。结构最高温度值仅354K,说明热防护良好;直筒段和后封头壳体主体区域应力安全系数>3,满足设计要求,而在法兰附近圆角过渡处外壁存在应力集中,最大应力处安全系数降为1.13,燃气发生器壳体仍处于安全状态,但存在安全裕度显著降低的风险。     

Debris swarms seen by SMEI

The large 3° × 60° fields-of-view of the Solar Mass Ejection Imager (SMEI) instruments are oriented on the stabilized Coriolis satellite to image most of the sky each Sun-synchronous orbit. Besides observing coronal mass ejections, the SMEI mission objective, SMEI also has detected a plethora of Earth-orbiting satellites (resident space objects or RSOs) brighter than ∼8th magnitude at a rate of about 1 per minute. Occasionally, SMEI sees an RSO swarm: a sudden onset of a large number of RSOs, many more than the nominal rate, upto dozens detected in a 4-s frame. These swarms usually last for a few minutes. A sample of six such RSO ensembles is analyzed in this paper in which the distance and the direction of the velocity vector for individual objects are estimated. We present the observational evidence indicating that the swarms must be near-field objects traveling in orbits near that of Coriolis, and that the relatively speeds between the objects and Coriolis are low. Further, analyses indicate that the RSOs are quite close (<20 m) and are generally moving radially away from the satellite. The predicted encounter geometries for Coriolis passing through or near a small debris cloud is, generally, quite inconsistent with the observations. The most likely explanation consistent with the observations is that SMEI is seeing debris being ejected from the Coriolis spacecraft itself. An analysis of distance and brightness for a subset of the RSOs indicates that the median diameter of the debris particles is ∼80 μm.     

支板火箭引射冲压发动机引射模态燃烧流动 (Ⅱ )二次燃烧及构型的影响

对比研究了两种构型的支板火箭引射冲压发动机引射模态的瞬时掺混燃烧(SMC)三维掺混和反应流场，详细分析了静态海平面零马赫数情况下燃烧及构型对引射流场的影响，发现几何构型和二次燃烧的综合影响决定了引射掺混后流体的速度、总温、总压及引射流量，从而也主要确定了发动机的性能，其中构型因素主要决定了掺混的质量，从而决定了低速模态的性能。     

RBCC引射模态气流抵抗反压能力受掺混程度影响研究

为了获得气流的掺混效果与引射过程总体性能的关系,研究了轴对称引射流场中圆形和环形喷管的掺混程度及其对引射比和气流抵抗反压能力的影响。以一次流动量覆盖整个横截面位置为分界截面,将引射流场中的掺混分为上游掺混和下游掺混两个过程。研究表明,气流的引射效果以及抵抗反压能力几乎不受下游掺混过程掺混程度影响,而是由分界截面的掺混程度决定。上游掺混过程决定了分界截面的掺混程度,对引射过程的引射比以及抵抗反压能力有明显影响,分界截面位置的掺混程度越高,被引射的二次流流量越大,抵抗反压能力越弱。对于RBCC发动机引射模态,引射比和抵抗反压能力指标相互矛盾,不应以引射比为唯一目标。