Comptonization of low-frequency radiation in accretion disks: Angular distribution and polarization of hard X-ray radiation

We present the results of computation for angular distribution and polarization of radiation for the set of the disk Thomson optical depth values.     

舰船燃气轮机气路测量参数的理论选择方法

针对舰船燃气轮机气路性能监测诊断的有效性要求,归纳总结了气路测量参数选择要求,提出了1套系统完整的燃气轮机气路测量参数的理论选择方法。在可测量和易测量要求及测试精度要求的初步选择基础上,依次采用影响系数、相关系数和条件数对气路测量参数的敏感性、相关性和诊断误差等进行了分析,最终从理论上选择了某舰船3轴燃气轮机气路性能监测诊断的测量参数。实例表明该理论方法具有一定的通用性和工程应用价值,对燃气轮机气路测量参数的选择有一定的指导作用。     

三旋流燃烧室点火阶段燃烧性能

为研究三旋流燃烧室的点火熄火性能,对单头部燃烧室进行了地面和高空的点、熄火试验研究,测取了负温条件下的高空点火性能,借助高速摄像法录取了地面点火过程,采用燃气分析法对地面点火燃烧效率进行了测量,获得了单头部燃烧室的点、熄火性能和点火燃烧性能参数,以及火焰传播过程。结果表明:三旋流燃烧组织方式可在宽广的主燃区气流速度范围内,具有良好的点熄火性能,地面点火边界的燃烧充分性较高,燃烧效率约为80%,负温条件增加了点火难度,与常温点火边界相比,进气压力70 kPa时的负温点火的边界变窄了188%~375%,高空贫油熄火边界与点火边界接近,所获结果可为三旋流燃烧室设计提供参考。     

Whole-process modeling of titanium disc forming for gradient distributions of temperature and deformation

Gradient distributions of temperature and deformation (GDTD) are crucial for achieving dual-performance discs of titanium alloys which is required by the service environment of aeroengine. However, heating, cooling and deforming sequence in the whole process of the titanium disc forming, which leads to difficulties for achieving GDTD due to a lot of parameters. To solve this problem, a whole-process model of the titanium disc forming for GDTD has been established. In the model, heating and cooling via heat radiation, conduction and convection, and deforming by local loading with mold chilling are all considered. Experiments on heating and cooling as well as deforming were carried out by using a furnace and the Gleeble-3500 machine. The experimental data are used to determine thermal parameters and constitutive relations of the IMI834 titanium alloy, and then to verify the reliability of the model. Then the model was used to simulate the evolution rules of temperature and deformation of the titanium disc. The results show that the heating surface, furnace temperature, billet profile and loading rate play the core role for the control of GDTD, and thus a set of parameters were determined. Therefore, this work provides a base for developing a new forming technology of the dual-performance titanium discs with the approach of local heating and local loading.     

船舶燃气轮机进气系统中过滤装置数值模型化处理方法研究

为了研究船舶燃气轮机进气系统中,过滤装置数值模型化处理方法的模拟精度及其适用性。针对一种双通道船舶燃气轮机进气系统,分别采用Fan边界和多孔介质模型方法对过滤装置（百叶窗、滤清器）的复杂结构进行处理,开展进气系统内流场特性的详细数值计算研究。结果表明：进气系统大部分总压损失源于燃烧空气滤清器产生的总压损失和竖井中的流动损失;与Fan边界相比,多孔介质模型方法能够获得更贴合实际的进气系统流场,对系统总压损失的预测更具可靠性;两种方法计算出的进气系统流动损失相差不超过10%;使用Fan边界需保证过滤装置不产生明显的整流作用,且压力损失实验数据完备,而选用多孔介质模型需要已知过滤装置阻力系数、孔隙率等物理参数。     

A Novel Magnetic Configuration for Space Radiation Active Shielding

Space radiation has been identified as the main health hazard to crews involved in manned Mars missions. Active shielding is more effective than passive shielding to the very energetic particles from cosmic rays. Particle motion in a magnetic field is studied based on the single-particle theory and Monte Carlo method. By comparing the shielding efficiency of different magnetic field configurations, a novel active magnetic shielding configuration with lower mass cost and power consumption is proposed for manned Mars missions. The new magnetic configuration can shield 92.8% of protons and 84.4% of alpha particles with E < 4 GeV·n-1, when considering the passive shielding contribution of 10.0 g·cm-2 Al Shielding, the required magnetic stiffness can be reduced from 27 Tm to 16 Tm. The detailed analysis of mass cost and power consumption shows that active shielding will be a promising means to protect crews from space radiation exposure in manned Mars missions.      

空间粒子辐射对卫星中集成芯片的影响

本文分析了在“风云一号(B)”气象卫星环境中各种粒子辐射在集成芯片临界体积中产生的能量沉积, 即LET(线性能量传输);得到了银河宇宙线1≤Z≤28、银河宇宙线异常成分(C、N、O、Ne、Ar、Fe)、内辐射带质子等产生的LET, 计算了其分别产生的单粒于事件(SEU)翻转率。      

太阳微波射电快速精细结构亚类型的观测分析

通过分析"云南天文台4波段太阳射电快速同步观测系统"1990-01-1994－01取得的103个射电爆发,发现其中29个存在不同类型的快速精细结构（FFS）.尤其是发现了几个少见的亚类FFS现象.本文仅介绍两个亚类型:窄带变周期脉动和宽带慢漂移长周期脉动.这些现象表明太阳射电FFS的多样性,它们发生在射电爆发的不同阶段（耀斑不同相）,从而说明在耀斑演化中日冕非热电子的加速或注入可能贯穿于整个耀斑发展过程.由于耀斑后相FFS的发生,可验证耀斑后相存在磁重联和似环结构（耀斑后环）的重新形成.由于不同的亚类FFS反映日冕中存奇特别的环境条件,从而推测日冕中可能存在更复杂的多重类型的磁结构.      

辐射换热系统温度场的渐近特性研究

本文讨论辐射换热系统温度场的渐近特性,该问题与具有周期热源的人造卫星热模拟试验紧密相关。本文工作使文献[1,2]阐述的行之有效的方法得到进一步完善。     

γ射线辐射对空间光学玻璃透射率的影响

利用60Co γ-射线对钡冕玻璃（BaK3）、镧冕玻璃（LaK3）、火石玻璃（F10）、镧火石玻璃（LaF3）、轻火石玻璃（QF3）和重火石玻璃（ZF4）进行辐照,研究不同辐照剂量对光学透射率的影响及这些玻璃在空间光学系统中的适应性。光学透射率测试范围为400~1 100 nm。结果表明所有玻璃在辐照后可见光透射率都下降了,而在近红外波段下降不明显（除了QF3和LaF3）。尽管F10和QF3光学透射率在辐照前相似,但是辐照后F10衰减是所有玻璃中最小的,而QF3衰减最为严重。研究发现,当达到一定辐照剂量后,玻璃材料的透射率不再继续衰减,而是趋于稳定。这些结果为空间光学系统针对辐射进行冗余设计提供了依据。