军用设备电磁发射测试项RE102的实现CSCD

电磁兼容性(EMC)是指设备或系统在电磁环境中符合要求运行并不对其环境中的其它设备产生影响的电磁干扰的能力。因此,EMC包括两个方面的要求:一方面是指设备在正常运行过程中对所在环境产生的电磁干扰不能超过一定的限值,即电磁干扰度(EMI);另一方面是指设备对所在环境中存在的电磁干扰具有一定程度的抗扰度,即电磁敏感度(EMS)。本文描述符合《GJB 152A-97军用设备和分系统电磁发射和敏感度测量》要求的"RE102 10kHz^40GHz电场辐射发射"实现方法。     

Factors influencing the acoustic characteristics of the reverberation chamber

Main factors influencing the characteristics of the acoustic reverberation chamber are considered. Studies of mode density and calculation of required acoustic power are carried out from the relations of the RK-600 chamber dimensions depending on technical requirements for the ground-based experimental development of communication space vehicles (SV).     

On the motions of RHESSI flare footpoints

The footpoint motions of flare hard X-ray (HXR) sources are directly related to the reconnection scenario of a solar flare. In this work, we tried to extract the information of footpoint motions for a number of flares observed with RHESSI. We found that the RHESSI flare results of the footpoint motions strongly support the classification proposed from the observations of YOHKOH/HXT. Furthermore, it is found that a flare can consist of two types of footpoint motions. We discussed the connections of the footpoint motions with the two-dimensional reconnection models.     

Metric radio bursts and fine structures observed on 17 January, 2005

A complex radio event was observed on January 17, 2005 with the radio-spectrograph ARTEMIS-IV, operating at Thermopylae, Greece; it was associated with an X3.8 SXR flare and two fast Halo CMEs in close succession. We present dynamic spectra of this event; the high time resolution (1/100 s) of the data in the 450–270 MHz range, makes possible the detection and analysis of the fine structure which this major radio event exhibits. The fine structure was found to match, almost, the comprehensive Ondrejov Catalogue which it refers to the spectral range 0.8–2 GHz, yet seems to produce similar fine structure with the metric range.     

单层板撞击成坑声发射辨识及参数估计研究

空间碎片撞击航天器的威胁对发展在轨感知系统提出需求,为研制基于声发射技术的感知系统,有必要研究利用声发射波形分析对防护结构进行损伤模式辨识的方法。文章利用超声传感器进行了铝弹丸超高速撞击单层板的声发射信号采集实验及其数值仿真,并对波形在时域和频域内进行分析,结果表明:声发射波形的主波谷值随撞击速度增加而线性增加,直到防护结构被击穿;声发射波形中的高频分量与低频分量幅值之比存在一个区别成坑模式与击穿模式的阈值。基于上述结果提出了一种在撞击弹丸尺寸已知条件下辨识成坑模式并对其撞击速度及其弹坑尺寸进行估计的方案。     

EPT-200高频声发生器在航天器噪声 环境试验中的应用

文章针对提高目前使用的高声强混响室-2163m3混响室声场的高频性能,对两个EPT-200高频声发生器系统进行分析评估。首先采用开环噪声试验,验证其性能指标是否满足要求;然后采用闭环噪声试验,以考察2163m3混响室声场的高频性能。分析结果表明:EPT-200声发生器性能指标满足要求,并且提高了2163m3混响室的高频性能。     

ACOUSTIC PROPAGATION IN SHEARED MEAN FLOW USING COMPUTATIONAL AEROACOUSTICS

Acoustic propagation problems in the sheared mean flow are numerically investigated using different acoustic propagation equations, including linearized Euler equations （LEE） and acoustic perturbation equations （APE）. The resulted acoustic pressure is compared for the cases of uniform mean flow and sheared mean flow using both APE and LEE. Numerical results show that interactions between acoustics and mean flow should be properly considered to better understand noise propagation problems, and the suitable option of the different acous- tic equations is indicated by the present comparisons. Moreover, the ability of APE to predict acoustic propagation is validated. APE can replace LEE when the 3-D flowqnduced noise problem is solved, thus computational cost can decrease.     

The investigation of powerful solar flares characteristics by analysis of excited states of C and various neutrons capture lines

Accelerated energetic particles in solar flares produced nuclear γ-lines in interactions with ambient solar atmosphere. Analysis of intensity of ratios between various γ-lines allows us to make estimations of abundance of elements, parameters of surrounding media and other solar characteristics. In this article we discuss the flux ratio between two lines from excited states of ¹²C (f_15.11/f_4.44) and our results of preliminary calculation of intensity ratio between two neutron capture lines at ³He and ¹H (f_20.58/f_2.223). In particular we consider the opportunity to obtain n(³He)/n(¹H) ratio during solar flares and using high-energy gamma-emission studying, based on the satellite data. Possible interpretation of spectral features observed during the January 20, 2005 solar flare is discussed. Preliminary analysis of energy spectrum in the band of 2–21 MeV gives n(³He)/n(¹H) ∼ 8 × 10⁻⁴ for January 20, 2005 solar flare.     

Composite profile of the Fe Kα spectral line emitted from a binary system of supermassive black holes

We used a model of a relativistic accretion disk around a supermassive black hole (SMBH), based on ray-tracing method in the Kerr metric, to study the variations of the composite Fe Kα line emitted from two accretion disks around SMBHs in a binary system. We assumed that the orbit of such a binary is approximately Keplerian, and simulated the composite line shapes for different orbital elements, accretion disk parameters and mass ratios of the components. The obtained results show that, if observed in the spectra of some SMBH binaries during their different orbital phases, such composite Fe Kα line profiles could be used to constrain the orbits and several properties of such SMBH binaries.     

民航机场飞机排放浓度分布模型

按照国际民航组织规定的起飞着陆循环过程,简化飞机在机场起飞降落的活动路线,在原有飞机排放污染物排放指数(EI)计算的基础上,再结合飞机起飞降落过程的燃油流量(F),计算出进近、滑行、起飞、爬升四段路线的排放污染强度.基于高斯点源扩散公式,对其进行积分得线源扩散模型,再对线源扩散模型中的参数进行修正,建立了民航机场飞机排放浓度模型.