Fractal Structure of the Heliospheric Plasma Sheet at the Earth''''s Orbit

An analysis of the data from the Wind and IMP-8 spacecraft revealed that a slow solar wind, flowing in the heliospheric plasma sheet, represents a set of magnetic tubes with plasma of increased density (N > 10cm-3 at the Earth's orbit). They have a fine structure at several spatial scales (fractality), from 2°-3°(at the Earth's orbit, it is equivalent to 3.6-5.4h, or (5.4-8.0)×106km) to the minimum about 0.025°, i.e. the angular size of the nested tubes is changed nearly by two orders of magnitude. The magnetic tubes at each observed spatial scale are diamagnetic, i.e. their surface sustains a flow of diamagnetic (or drift) current that decreases the magnetic field within the tube itself and increases it outside the tube. Furthermore, the value of β= 8π[N(Te + Tp)]/B2 within the tube exceeds the value of βoutside the tube. In many cases total pressure P = N(Te + Tp) + B2/8πis almost constant within and outside the tubes at any one of the aforementioned scales.     

庄河、光明山陨石的岩石矿物学研究

庄河陨石和光明山陨石是两个降落于同一地区的Ｈ５型普通球粒陨石．根据两辉石温度计求出这两个陨石的平衡温度＜ ５００℃；根据镍纹石的带宽与组成关系，获得光明山陨石在其母体中的冷却速率约为 １０－１０℃／Ｍａ，而庄河陨石中普遍出现均一的四方镍纹石表明其冷却速率更低．光明山陨石的冲击变质特征以硅酸盐颗粒破碎为主，其冲击相为Ｓ１；庄河陨石中硅酸盐矿物具明显的波状消光，并存在细小的冲击熔融脉，其冲击相划分为Ｓ２．     

SFD方法模拟高超声速进气道中激波与边界层干扰

采用ＳＦＤ方法,在ＥＸＣＥＬ软件上利用ＮＮＤ格式数值模拟了激波与平板边界层之间的相互作用以及激波与管道壁面边界层的相互作用,即高超声速进气道隔离段内激波串流动现象。该方法的特点是简单、直观而且不用常规编程,计算结果基本反映了流场的基本结构,表明ＳＦＤ方法是一种具有潜力的计算方法。     

冲击双层壁内通道表面换热系数的研究

为了研究双层壁内通道表面换热情况和冲击距离对换热影响,对双层壁结构内通道上、下表面的换热系数进行实验测量。由获得的换热系数来分析研究双层壁内部换热。并对冲击射流的机理作了分析。研究结果表明,在双层壁结构中,在高雷诺数时,在冲击板表面上会出现两个峰值;在进气板表面上也会出现位置随冲击高度变化的一高换热区;层板内通道表面上的换热系数随冲击距离的减小而增大。     

非均匀超声来流矩形隔离段内流场实验

针对超燃冲压发动机隔离段的非均匀进口条件设计了隔离段实验风洞，通过测量隔离段壁面压力和拍摄流场纹影照片研究了矩形隔离段内激波/紊流附面层相干流场。研究发现，隔离段进口的非均匀流使隔离段流场压升特征与附面层发展规律与均匀进口的隔离段流动有显著差异。用截面当量直径取代Waltrup公式中的圆管直径可以取得较好的吻合效果。在进口马赫数小于2时，升高同样的压力，非均匀进口隔离段产生的激波串长度比Waltrup公式预测的长度要长。纹影仪观察发现隔离段内激波存在严重的振荡现象。     

双层壳型涡轮叶片中冲击旋流换热增益效果试验

以双层壳型涡轮叶片内冷通道中旋流换热特性为研究对象,采用热膜法,对双层壳型冷却结构中的狭小受限通道中,旋流作用下换热特性的变化规律开展了细致的试验研究。重点分析了冷却空气的旋流作用对换热的强化增益效果。试验中通过改变冲击Re数(10 000～20 000),冲击间距和冲击孔直径之比H/D(0.35～1.7)等参数,研究了其对旋流的形成及内表面局部换热系数的影响规律。研究发现:由于双层壳型叶片内冷通道的空间受限,冷却空气在通道内形成了旋流结构,该旋流结构显著影响了内表面的局部换热系数并可以有效提高换热效果。研究结果表明:内表面局部换热系数对冲击间距和冲击孔直径之比H/D最为敏感,对于不同冲击Re数,存在一个最佳的H/D使得旋流换热增益效果达到最大(Re=10 000时,最佳H/D为0.95;Re=15 000,20 000,最佳H/D=0.63)。     

基于激波控制的流体推力矢量喷管试验

以二元收扩喷管为对象,开展了基于二次流喷射的流体推力矢量技术研究。基于试验研究,得到了不同喷管落压比、不同的二次流总压比和不同的二次流喷射角度多种工况下的喷管上下壁面中心线压力分布规律以及喷管壁面油流分布图。通过对不同工况下参数变化规律分析,给出了基于二次流喷射的流体推力矢量喷管的主次流气动参数及几何参数对流体推力矢量喷管流场结构和性能影响的关联关系。从试验和分析结果可以看出,喷管落压比、二次流总压比和二次流喷射角度等喷管的主次流气动几何参数对基于流体推力矢量喷管参数变化有明显的影响。     

洛仑兹力控制高超声速进气道边界层分离的数值模拟

采用空间HUE格式、时间LU-SGS推进、sst-kw湍流模型、多块结构网格程序,对磁流体动力学(Magnetohydrodynamic:MHD)控制高超声速二维进气道边界层分离进行了数值研究.研究发现,不施加控制时,数值模拟得到的壁面静压和实验结果符合良好,进气道喉道处分离区占据喉道高度的1/3左右.通过施加MHD控制,消除了进气道内部的边界层分离,总压恢复系数从0.502提高到0.56,喉道处流场畸变系数减小了18.6%.     

A swept fin-induced flow field with different height mounting gaps

In order to apply the air fin successfully and ensure the maneuverability of hypersonic vehicle, a key problem to be studied urgently is the heat flux brought by the fin mounting gap. The appearance of mounting gap and fin shaft can induce many complex flow structures which need more attentions to be investigated. Under Ma 6, Nano-tracer-based Planar Laser Scattering (NPLS) and Temperature Sensitive Paints (TSP) were applied to visualize and measure transient flow structures and heat flux distribution of a swept fin-induced flow field with different height mounting gaps. Complementarily, Reynolds-averaged N-S equations were solved with k-ω SST turbulent model. The heat flux distribution results of numerical simulation and TSP observed the change of high heat flux region with different mounting gap, both in position and magnitude. The streamlines based on Computational Fluid Dynamics (CFD) and flow visualization results obtained by NPLS revealed the cause of high heat flux region. The high heat flux region in this flow field is mainly related to the reattachment of vortex and flow stagnation. The increase of gap height can lead to stronger gap overflow and shaft-induced horseshoe vortex, which are source of the high heat flux around the fin. The case with the highest mounting gap (4 mm) en-counters the most severe aerodynamic heating, both on the surface of fin and plate. Thus, under the premise of ensuring the flexibility of the fin, the gap should be set as small as possible.     

Cosmic ray acceleration by supernova shocks

We analyse the results of recent measurements of nonthermal emission from individual supernova remnants (SNRs) and their correspondence to the nonlinear kinetic theory of cosmic ray (CR) acceleration in SNRs. It is shown that the theory fits these data in a satisfactory way and provides the strong evidences for the efficient CR production in SNRs accompanied by significant magnetic field amplification. Magnetic field amplification leads to considerable increase of CR maximum energy so that the spectrum of CRs accelerated in SNRs is consistent with the requirements for the formation of Galactic CR spectrum up to the energy ∼10¹⁷ eV.