Determination of K,Ar, Cl,S, Si and Al flare abundances from RESIK soft X-ray spectra

The RESIK is a high sensitivity, uncollimated bent crystal spectrometer which successfully operated aboard Russian CORONAS-F solar mission between 2001 and 2003. It measured for the first time in a systematic way solar soft X-ray spectra in the four wavelength channels from 3.3 Å to 6.1 Å. This range includes characteristic strong lines of H- and He-like ions of K, Ar, Cl, Si, S and Al in the respective spectral channels. A distinguishing feature of RESIK is its possibility of making reliable measurements of the continuum radiation in flares. Interpretation of line and the continuum intensities observed in vicinity of respective strong lines provides diagnostics of plasma temperature and absolute abundances of K, Ar, Cl, S, Si and Al in several flares. We analyzed the observed intensities of spectral lines and the nearby continuum using the CHIANTI v5.2 atomic data package. A specific, so-called “locally isothermal” approach has been used in this respect allowing us to make not only flare-averaged abundance estimates, but also to look into a possible variability of plasma composition during the course of flares.     

涡轮叶片前缘气膜冷却换热实验

针对某型涡轮叶片放大模型的前缘冷却结构气膜冷却效果开展了细致的实验研究,利用红外热像仪测量了叶片表面的温度场分布,分析了前缘的气膜孔倾角、吹风比、主流雷诺数等参数对绝热冷却效率和压力损失的影响.实验中前缘的3排气膜孔倾角变化范围是35°~90°,主流雷诺数变化范围是76112~142624,吹风比变化范围是0.44~2.64.结果表明:气膜孔倾角越小,前缘驻点附近的气膜覆盖效果越好;气膜孔倾角为45°的叶片压力损失系数最小,气膜孔倾角为75°的叶片压力损失系数最大;主流雷诺数增大,绝热冷却效率下降,压力损失系数增加;吹风比增大到1.32时,绝热冷却效率达到最大,吹风比再增大绝热冷却效率反而下降.      

大型反射面天线温度分布规律及变形影响分析

针对高频段大型反射面天线对电性能的高要求,必须降低太阳热辐射对天线的影响。先计算一天中太阳入射角度的变化规律,再基于I\|DEAS软件仿真,得到一天中各时刻天线反射面上的温度、热应力场、热变形分布,然后针对阴影对天线结构的重要影响,以“分点分段”的形式给出不同时刻温度在反射面上的分布及其影响程度和规律,为工程人员进行天线的温度补偿和结构优化提供了依据。     

中等后掠机翼平面参数设计与实验研究

采用Euler数值计算方法,对60多种中等后掠角及展弦比的切尖菱形机翼、双三角机翼纵向气动力特性进行了计算、分析和比较,从中筛选出16种切尖菱形机翼、14种双三角机翼进行了全机高速风洞实验研究,给出了机翼的展弦比、前缘后掠角、根梢比(后缘前掠角)及几何扭转变化对全机升力、阻力及俯仰力矩的影响曲线和数据分析,在此基础上提出了用于定量估算两类机翼纵向气动力特性的关系式及修正因子。本文研究结果为建立战斗机机翼气动力设计数据库及飞机气动布局设计提供了实用的数据和设计参考。     

星载辐射计扫描镜太阳辐射热-结构建模与仿真

三轴稳定卫星平台搭载的光学有效载荷都存在午夜太阳辐射干扰问题,由此产生的热变形效应对光学系统的成像品质影响显著。采用复杂外热流近似建模技术,以及多软件耦合有限元仿真方法,以FY-4卫星的扫描辐射计为应用背景,研究了昼夜太阳辐射对星载辐射计扫描镜产生的热效应,并对不同热设计条件下的工况进行了对比分析。分析结果显示：扫描镜侧面及背面的热控涂层选取对其热变形有重要影响,但是仅仅通过热设计解决温度波动和热变形的矛盾是不够的,需要通过改进扫描镜的材料和优化光机结构加以改善。     

Solar X-ray Monitor (XSM) on-board Chandrayaan-2 orbiter

The remote X-ray fluorescence spectroscopy is a powerful technique to investigate the elemental abundances in the atmosphere-less planetary bodies. The experiment involves measuring spectra of fluorescent X-rays from lunar surface using a low energy X-ray detector onboard an orbiting satellite. Since the flux of fluorescent X-ray lines critically depend on the flux and spectrum of the incident solar X-rays, it is essential to have simultaneous and accurate measurement of X-ray from both Moon and Sun. In the context of Moon, this technique has been employed since early days of space exploration to determine elemental composition of lunar surface. However, so far it has not been possible to exploit it to its full potential due to various reasons. Therefore it is planned to continue the remote X-ray fluorescence spectroscopy experiment on-board Chandrayaan-2 which includes both lunar X-ray observations and solar X-ray observations as two separate payloads. The lunar X-ray observations will be carried out by Chandra Large Area Soft x-ray Spectrometer (CLASS) experiment; whereas the solar X-ray observations will be carried out by a separate payload, Solar X-ray Monitor (XSM). Here we present the overall design of the XSM instrument, the present development status as well as preliminary results of the laboratory model testing. XSM instrument will have two packages namely – XSM sensor package and XSM electronics package. XSM will accurately measure spectrum of Solar X-rays in the energy range of 1–15 keV with energy resolution ∼200 eV @ 5.9 keV. This will be achieved by using state-of-the-art Silicon Drift Detector (SDD), which has a unique capability of maintaining high energy resolution at very high incident count rate expected from Solar X-rays. XSM onboard Chandrayaan-2 will be the first experiment to use such detector for Solar X-ray monitoring.     

一种快速自适应角度-多普勒补偿算法

自适应角度-多普勒补偿(Adaptive Angle Doppler Compensation,A2DC)算法可在惯导参数未知的情况下解决非正侧视阵列中由杂波距离相关性引起的非均匀问题,但该算法运算量大、工程实现困难.本文首先对A2 DC算法的基本工作原理进行了深入的分析,在此基础上,针对算法运算量大的缺点,将分块处理...     

1998年5月日冕三维结构的数值模拟

采用三维理想磙流体力学（MHD）模式,内边界条件把二维投影特征线边界方法推广应用到三维计算,有效地稳定了数值计算并保证稳态解的自洽性;初始猜解磁场由1935卡林顿周光球磁场观测数据得到,这样计算得到的1998年5月份期间日冕三维结构比较符合实际,计算结果表明：（1）计算得到的源表面非径向磁场量值在磁中性线附近不超过2μT,表明源表面磁场基本径向。（2）模拟得到的源表面径向磁场量值除了在磁中性线附近的区域外变化不大,这和观测一致。（3）由源表面磁场按平方反比的规律计算出1AU处磁场量值更接近观测值。（4）计算得到的日冕结构和观测定性一致,三维数值模拟结果表明,日冕的三维大尺度背景结构主要是由磁场决定的,在闭磁场处或者电流片附近,太阳风的密度高,速度低;在开场区,太阳风的密度低,速度高。     

塞式喷管主喷管角度特性

首先建立了塞式喷管角度特性的研究模型，并运用简化的塞锥设计方法设计塞锥型面，在此基础上，通过连续改变主喷管倾角来研究主喷管倾角对塞式喷管的推力性能的影响，并确定在给定设计条件下的主喷管最佳倾角，还分析研究了底部高度，内膨胀比，总膨胀比，总压和飞行高度与主喷管最佳倾角的关系以及变化规律，针对特定的塞式喷管实验发动机，进行了初步的变角度实验，并与计算结果进行比较和分析。