自增压式丁烷微推进系统建模与工作特性仿真研究

利用AMESim+AMESet建立了丁烷微推进系统一维仿真模型,该模型包含:考虑丁烷相变的自增压贮箱、稳压气容、PID控制的电加热推力器等组件.研究自增压贮箱、电磁阀、气容和推力器的静态工作特性,分析气容体积和推力器加热功率以及推力器扩张比对系统工作特性的影响,对丁烷推进系统的动态响应特性进行探讨.结果显示,自增压贮箱...     

具有气液同轴喷嘴的液体火箭发动机燃烧室压力振荡及其声学特性研究

为探究液氧/煤油液体火箭发动机气液同轴喷嘴模型燃烧室具有良好稳定性的原因,采用非稳态雷诺平均（URANS）方法数值研究了其燃烧不稳定性和声学特征。两相燃烧条件下,燃烧室压力振荡幅值约为室压的10%左右、最大不超过25%,且以纵向和横向振型为主。一周六径隔板对横向振型具有很强的抑制作用,但对纵向振型影响较小。与液-液撞击式液氧/煤油发动机模型燃烧室相比,本文研究的燃烧室中煤油液滴没有发生超临界蒸发现象,第三邓克尔数较小,诱发燃烧不稳定性的激励源较弱。进一步通过数值定容弹激发了燃烧室多模态声学特征压力振荡,并得到了其振荡特征频率、幅值和衰减率。结果表明,气喷嘴具有四分之一波长喷嘴特征,能显著减小目标振型的幅值,而集气腔对纵向振型具有很强的抑制作用,同时对其他振型也有程度不同的抑制效果。因此,较弱的燃烧不稳定性激发机制以及隔板、气喷嘴和集气腔对纵向和横向振型很强的抑制作用,使得该液氧/煤油发动机气液同轴燃烧室具有很好的稳定性。     

Rapid short-term pulse-period variations in Vela X-1 (4U 0900-40)

Results are presented of an analysis of 83 days of 2–12 keV X-ray observations of Vela X-1 (4U 0900-40) obtained during three separate pointings with the ESA COS-B satellite. The pulsation period is shown to undergo very rapid intrinsic changes, at a rate of up to during intervals of a few days. The lower values of which were previously observed over longer intervals, appear to result from an averaging-out of these rapid changes. It is argued, that the transfer of angular momentum to the neutron star by the accreting matter is very unlikely to be sufficient to explain these pulsation-period changes. An alternative explanation is suggested.     

Hard X-ray observations of Cygnus X-1 with the MISO telescope

The black hole candidate Cygnus X-1 was observed in the hard X ray - soft γ ray energy range by the MISO telescope on two different occasions: in September 1979 and May 1980. We have measured two hard X-ray states of the source: in 1979 the observed spectrum confirms the superlow state measured in the same period by the HEAO-3 satellite, while in 1980 the MISO X-ray data are consistent with the so called low state of Cygnus X-1. In both occasions, no γ -ray excess has been observed above 200 KeV.     

考虑执行机构饱和的迎角跟踪控制

设计提出了 1种针对高光谱图像分类任务的 3D-MSCNN模型。在 PCA降维的基础上,利用 3D空谱特征提取网络和 2D多尺度特征提取网络实现高光谱图像特征提取,充分发挥高光谱图像空谱信息价值,增强对不同尺度地表覆盖的表达能力。最后,利用 Softmax分类损失函数实现高光谱图像分类任务。实验结果表明,本文算法在 In. dian Pines和 Pavia University数据集上都取得了较好的分类效果。与 CD-CNN、3D-CNN、SS-Net和 HybirdSN等方法相比,本文算法能够有效提升总体精度、平均精度和 Kappa系数等客观评价指标。     

CLF-1钢X数字射线照相等效系数的确定

针对聚变堆结构材料拟采用的新材料CLF-1(low-activated ferritic/martensitic steel)钢在进行射线检测过程中没有特定标准参考的问题,采用等效法在相同透照条件开展了不同厚度CLF-1钢和Q235钢的X数字射线等效透照实验研究。基于相同成像条件下两种材料对应的X射线图像具有相同灰度即透照系数相同,通过对比拥有相同图像灰度值的两种材料的厚度,得出CLF-1钢对应于Q235钢的等效透照系数。试验设计了4~20 mm,递增0.5 mm的阶梯厚度的CLF-1钢和Q235钢在100~400 kV(递增50 kV)管电压条件下进行了透照实验,获得了对应电压下CLF-1钢相对于Q235钢的X射线透照等效系数为1.10~1.13。该研究结果对CLF-1钢在进行X射线检测时的检测技术参数的确定具有指导意义。     

平面压气机叶栅通道分离流动高精度直接数值模拟

采用高精度有限差分格式直接求解二维Navier-Stokes方程组,数值模拟V103平面压气机叶栅分离流动,数值结果表明:在瞬时流场中,吸力面后部发生流动分离,在分离区前端存在大尺度分离涡,分离涡下游是由二次涡和脱落涡交替形成的涡串,直至叶片尾缘,形成以脱落涡为主结构的尾迹;在时均流场中,吸力面后部存在短分离泡,分离区压力分布存在明显压力平台。与逆压力梯度下平板边界层分离流动相比,瞬时和时均流场结构相似;叶栅通道内无量纲涡脱落频率是前者的两倍。与文献计算结果对比表明:叶片表面压力分布除分离区外吻合很好;非定常计算所得分离区轴向长度比定常计算大41%。在分离区内三个二阶统计量均达到最大值,表明流场强非定常性集中在分离区。     

High-cadence Hα imaging of solar flares

The Hα observation is a powerful tool to study the high-energy aspect of solar flares. Spiky brightenings of flare kernels at the Hα center reflect the rapid fluctuation in particle acceleration; linear polarization of Hα emission might be evidence of accelerated protons; red-shifts of the Hα line are caused by the chromospheric evaporation. To study the spiky brightenings of flare kernels with high-cadence imaging at the Hα center, a high-speed Hα camera for the Solar Flare Telescope at Mitaka, NAOJ, had been developed and it started the regular observation in 2001 July. However, the polarimetry and the Dopplermetry are also important and they are required to be carried out in parallel with the high-cadence imaging at the Hα center. Then, we upgraded the original high-speed Hα camera to a new Hα camera system for the multi-aspect Hα observations, which performs all of the high-cadence imaging, the linear polarization measurements, and the off-band imaging for velocity measurements. The new system started the observation in 2002 July. In this paper, the multi-aspect Hα imaging system is described and sample Hα images are presented.     

萤火一号探测器有效载荷数据管理器设计

针对萤火一号探测器各有效载荷的需求设计出安全、可靠的载荷数据管理器(PDHU), 实现对其 进行数据采集、处理、存储以及供配电等; PDHU提供操作系统, 便于应用软件的 开发; 针对火星探测的实际情况, 对地通信采用无交错的RS码加卷积码的级连编码方式进行信道编码.      

Preliminary Scientific Results of Chang'E-1 Lunar Orbiter: Based on Payloads Detection Data in the First Phase

Chang'E-1 lunar Orbiter was launched by Long March 3A rocket from Xichang Satel-lite Launch Center at 18:05BT(Beijing Time) Oct.24,2007.It is the first step of its ambitious three-stage moon program,a new milestone in the Chinese space exploration history.The primary science objectives of Chang'E-1 lunar orbiter are to obtain three-Dimension(3D) stereo images of the lunar surface,to analyze the distribution and abundance of elements on the surface,to investigate the thickness of lunar soil,evaluate helium-3 resources and other characteristics,and to detect the space environment around the moon.To achieve the above four mission objectives,eight sets of scientific instruments are chosen as the payloads of the lunar orbiter,including a CCD stereo camera(CCD),a Sagnac-based interferometer spectrometer(ⅡM),a Laser Altimeter(LAM),a Microwave Radiometer(MRM),a Gamma-Ray Spectrometer(GRS),an X-ray spectrometer(XRS),a High-Energy Particle Detector(HPD),and two Solar Wind Ion Detectors(SWID).The detected data of the payloads show that all payloads work well.This paper introduces the status of payloads in the first phase and preliminary scientific results.