激光推进辐射击穿温度特性的数值研究

在9种等离子体击穿温度下,数值模拟了二次反射式聚焦系统聚焦情况下激光推力器内流场的演化过程,得到了不同击穿温度对应的能量沉积率、推力峰值、冲量和冲量耦合系数,能量沉积率和推进性能参数在某个等离子体击穿温度值处发生突变。根据空气对激光的逆韧致吸收系数公式,计算了CO2激光辐照下不同等离子体击穿温度对应的空气辐射自由程,发现当等离子体击穿温度为14000K时,辐射自由程为1.4mm,与计算网格的典型尺寸相当,此时入射激光能量在一个网格内以一定效率被吸收,由此确定了基于逆韧致吸收的激光等离子体的击穿温度。     

基于同步双口SRAM的原子磁强计磁共振相位提取系统设计

针对原子磁强计磁共振激励信号相位提取过程中,数据量大、实时性强、同步要求高等特点,设计了一种基于同步双口SRAM的磁共振相位信息提取系统。首先利用FPGA控制高速同步采样AD进行数据转换;然后经同步双口SRAM实现数据的高速缓存和同步读写;最后由DSP经外部中断触发定时读取缓存的数据,并进行数字锁相处理,提取相位信息。实验结果表明:该系统对频率为35~350kHz之间的正弦信号相位提取稳定度达到0.006°,满足原子磁强计静态噪声小于20pT的应用要求。     

Sagnac横向剪切干涉仪设计方法的研究

详细论述了实体Sagnac型干涉仪的工作原理和几何尺寸的优化设计方法,并对实体棱镜构成的干涉仪用展开成平板玻璃的方法来计算分束膜的投射高度,简单且快捷。结合实例给出了计算结果,并对干涉仪的加工要求与装调方法等进行了定性分析。     

Excellent electromagnetic wave absorption of MOF/SiBCN nanomaterials at high temperature

Electromagnetic wave absorbing materials at high-temperature are urgently needed for stealth aircrafts or aero-engines worked in harsh environments. In this contribution, cobalt-containing siliconboron carbonitride (MOF/SiBCN) nanomaterials were prepared by pyrolyzing metal–organic framework, i.e. cobalt 2-methylimidazole (ZIF-67), and hyperbranched polyborosilazane. The rhombic dodecahedral ZIF-67 and cobalt element promoted in situ formation of dielectric loss phases, including SiC nanocrystals, CoSi nanocrystals and turbostratic carbons. The ZIF-67/SiBCN nanomaterials showed excellent microwave absorption both at room and elevated temperature. The minimum reflection coefficient (RC_min) was −51.6 dB and effective absorption bandwidth (EAB) is 3.93 GHz at room temperature. At an elevated temperature of 600 °C, the RC_min reached −30.29 dB and EAB covered almost the whole X-band (3.95 GHz, 8.45–12.4 GHz). The ZIF-67/SiBCN nanocomposites are promising and useful platform for microwave absorbing materials at high-temperature. It may shed light on the downstream applications in designing next generation areo-engines and stealth aircrafts.     

羰基镍粉中铜、锰、钴含量的连续测试技术

建立了一种用AIR-C2H2火焰原子吸收光谱法连续测试镉镍电池羰基镍粉中铜、锰、钴含量,介绍了铜、锰、钴最佳测试条件,同时对样品硝化处理条件及在测试样品中的干扰因素进行了综合考虑。该方法具有很好的精密度和准确度,具有操作简便、时间快速、灵敏度高、重现性好、容易掌握等特点。铜、锰、钴含量的相对标准偏差均小于1.0%（n=6）。标准加入回收率均在97.0%-99.0%范围内。适用于镉镍电池羰基镍粉中含有较多共同被测离子铜、锰、钴的生产现场控制分析和样品系统分析。     

卫星表面原子氧通量和遭遇量的计算及讨论

建立了一个较为理想情况下卫星表面原子氧通量和遭遇量的计算模式。在此基础上,着重讨论了轨道高度、太阳活动、飞行攻角及轨道倾角等因素对原子氧通量和遭遇量的影响。      

差分吸收激光雷达的信号处理技术

针对差分吸收激光雷达系统 ,研究信号平均和卡尔曼滤波两种信号处理技术 ,并进行了数值仿真。通过仿真可以看出 ,采用信号平均和卡尔曼滤波技术都可以很好地估计出待测气体的浓度 -光程积 ,大大地提高测量精度 ,同时也将两者的性能进行了比较     

基于CORDIC算法的DDS在铷原子频标中的应用

铷原子频标是各种原子频标中发展最为活跃的,由于其独特的外在及内在的特点,使其在商业通信、空间导航等领域得到最为广泛的应用。铷原子频标中,通过DDS和倍频链共同生成Rb87原子跃迁所需的微波信号,其中带有任意尾数频率DDS的产生是非常重要的一个环节,而目前的DDS多采用查表法来实现,而对于高分辨力的DDS,查表法则需要相当巨大的ROM空间,以至于无法用于较高要求的设计中。简要介绍铷原子频标的基本原理的基础上,提出并且实现了一种基于CORDIC算法的DDS,本算法通过简单的加、减和移位等基本操作来实现DDS的功能,并给出实现DDS的实例。     

微波消解-FAAS法测定铜尾矿中的铜

为了提高铜尾矿中铜的测试准确性,本试验采用微波消解法制备样品试液,并将标准加入法运用于火焰原子吸收(FAAS)法中,从而有效地抑制共存物的干扰。试验先用标准曲线法初步确定铜浓度及其线性区间,然后确定加入量,实验所得标准加入校准曲线的线性相关系数为0.9 998;加标回收率为101%~103%;相对标准偏差为0.5%~2.1%。试验证明该法快速、简便、稳定可靠。     

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.