空气动压探头的动态响应研究

本文采用动力类比法对用于核爆炸测量的空气动压探头的动态响应进行了理论分析,并对探头的三个压力量程计算了总压边和静压边进气管道中的阻尼孔直径和动压波形的上升时间。分析计算表明,在探头的三个系统中,电学系统对动态响应的影响可忽略不计;力学系统的影响也是较小的;对动态响应起主要作用的是声学系统(即管道空腔系统)。在直径为130mm 激波管中进行了全尺寸探头的动态响应实验。实验表明,阻尼孔直径和波形上升时间的实验值与计算值符合较好。此探头曾多次用于我国大气层核试验测试中。从核爆炸和激波管实验中测得的空气动压波形可看出,它们的前沿都是很好的,这反映出此探头具有良好的动态响应特性。     

Optical/X-ray correlations as a signature of jet-disc coupling in the accreting black hole XTE J1118+480

We interpret the rapid correlated UV/optical/X-ray variability of XTE J1118+480 as a signature of the coupling between the X-ray corona and a jet emitting synchrotron radiation in the optical band. We propose a scenario in which the jet and the X-ray corona are fed by the same energy reservoir where large amounts of accretion power are stored before being channelled into either the jet or the high energy radiation. This time-dependent model reproduces the main features of the rapid multi-wavelength variability of XTE J1118+480. A strong requirement of the model is that the total jet power should be at least a few times larger than the observed X-ray luminosity, implying a radiative efficiency for the jet _j  3 × 10⁻³. This would be consistent with the overall low radiative efficiency of the source. We present independent arguments showing that the jet probably dominates the energetic output of all accreting black holes in the low-hard state.     

Time dependent accretion onto a black hole in a disk plus corona system

Hard X-ray lightcurves exhibit delays of 1 s with respect to the soft X-ray lightcurves when the microquasar GRS 1915+105 is in the state of frequent, regular outbursts. Such outbursts are supposed to be driven by the radiation pressure instability of the inner disk parts. The hard X-ray delays are then caused by the time needed for the adjustment of the corona to changing conditions in the underlying disk. We support this claim by the computation of the time evolution of the disk, including a non-stationary evaporation of the disk and mass exchange with the corona.     

Determination of temperature maps of EUV coronal hole jets

Coronal hole jets are fast ejections of plasma occurring within coronal holes, observed at Extreme-UltraViolet (EUV) and X-ray wavelengths. Recent observations of jets by the STEREO and Hinode missions show that they are transient phenomena which occur at much higher rates than large-scale impulsive phenomena like flares and Coronal Mass Ejections (CMEs). In this paper we describe some typical characteristics of coronal jets observed by the SECCHI instruments of STEREO spacecraft. We show an example of 3D reconstruction of the helical structure for a south pole jet, and present how the angular distribution of the jet position angles changes from the Extreme-UltraViolet-Imager (EUVI) field of view to the CORonagraph1 (COR1) (height ∼2.0 R_⊙ heliocentric distance) field of view. Then we discuss a preliminary temperature determination for the jet plasma by using the filter ratio method at 171 and 195 Å and applying a technique for subtracting the EUV background radiation. The results show that jets are characterized by electron temperatures ranging between 0.8 and 1.3 MK. We present the thermal structure of the jet as temperature maps and we describe its thermal evolution.     

Neutrino flares from black hole coronae

We present a model for neutrino flares in accreting black holes based on the injection of a non-thermal population of relativistic particles in a magnetized corona. The most important products of hadronic and photohadronic interactions at high energies are pions. Charged pions decay into muons and neutrinos; muons also decay yielding neutrinos. Taking into account these effects, coupled transport equations are solved for all species of particles and the neutrino production is estimated for the case of accreting galactic black holes.     

航天产品深孔加工技术综述

在航空航天制造业中，深孔加工技术是一项仍在发展的综合技术。深孔加工是处于封闭或半封闭状态下进行的，加工难度主要体现在精加工工序上。深孔加工分为内排屑和外排屑两大类，不同的工艺选用不同的排屑方式。本文作者对难切削材料、深孔精密加工，加工实时监测进行了介绍，探讨了该领域的研究动向。     

高精度喷嘴环斜锥孔加工专用铰刀的研究与应用

通过对某型号发动机喷嘴环斜锥孔加工铰刀的工艺研究与试验,确定了该刀具的基体材料、涂层材料(TiN)、涂层工艺(PVD)及设计参数,实现了该零件的批次性加工的实际状态与设计要求相一致的目标。进一步探寻了不锈钢斜锥孔高精度加工的特殊规律。     

三维孔的数控检测及数学处理

本文叙述了任意孔的数控检测方法及相应的数学处理，解决了任意孔的数控检测问题。     

唇口斜切修型对S形进气道RCS影响

采用基于迭代物理光学法与等效边缘电磁流法的雷达散射截面计算程序,分析了水平、垂直两种极化方式下唇口斜切修型对菱形进口S形进气道边缘绕射场及腔体内部散射场的影响。计算结果表明：在水平、垂直两种极化方式下,斜切修型可有效降低边缘绕射场的雷达散射截面,但随斜切角度的增大,其减小幅度降低;正负斜切角度对应的绕射场雷达散射截面分布关于0°探测角对称;斜切修型对腔体内部散射场的影响较小。     

飞机铆接件隐藏缺陷的远场涡流检测探头优化与试验

远场涡流检测技术因检测深度深和检测结果可靠性高等诸多优点适合飞机多层金属铆接构件的快速检测。针对飞机铆接件铆钉孔沿边隐藏裂纹的原位检测，建立了多层金属铆接构件隐藏缺陷平面远场涡流检测有限元模型，对激励线圈内径、磁路结构以及屏蔽阻尼进行了仿真优化，研制了激励线圈和检测线圈均带组合屏蔽结构的传感器，采用激励-检测线圈环绕铆钉旋转扫描的方式，研究多层金属铆接构件铆钉孔沿边隐藏裂纹信号特征。仿真与试验结果表明：罐形磁芯聚磁效果是柱形磁芯的1.85倍，采用铝+铜组合屏蔽罩能够将远场区提前10 mm，检测线圈位于缺陷正上方时，检测信号的幅值和相位存在极大值，且极大值随着缺陷埋深的增加逐渐下降，研究成果可望用于指导飞机多层金属铆接构件的工程检测实践。