非均匀磁化等离子体层的电磁特性分析

基于分层传播原理提出了一种计算电磁波在非均匀磁化等离子体层中反射率和吸收率的模型,并数值分析了等离子体密度与碰撞频率,以及背景磁场强度对电磁波的反射和吸收特性的影响.研究表明:该法所得结果与文献的传播矩阵(SMM)法一致.数值分析发现:低密度高碰撞频率等离子体可减少等离子体层对入射波的功率反射;高密度高碰撞频率等离子体可改善其对入射波的功率反射宽频带吸收特性;背景磁场强度可明显改变等离子共振吸收频段.     

复杂姿态下基于空时码的测控方法

为了提高复杂姿态条件下飞行器测控通信的可靠性，将LDPC（Low Density Parity Check，低密度奇偶校验）码和空时码级联，并采用2×1天线系统，建立了系统模型，阐述了信道参数估计方法，在此基础上提出了基于信道参数估计的空时软译码算法，使得空时译码器输出软信息给LDPC译码器，能充分利用LDPC的编码增益。仿真结果表明，不采用空时码时在π相位差附近出现很高的误码，导致通信中断；采用空时码能够保证在任何相位差的条件下误码率在一定的范围内，实现不间断测控。     

丁腈橡胶增韧酚醛树脂基变密度烧蚀防热复合材料研究

采用丁腈增韧酚醛树脂作为变密度烧蚀材料基体，通过化学发泡法来降低材料的密度，并通过调节发泡剂用量实现对材料密度的设计，制备了变密度烧蚀材料并进行了性能测试。实验结果表明：变密度烧蚀材料的力学性能随密度的升高而提高，隔热性能随密度的降低而提高；采用变密度烧蚀材料可使材料的烧蚀热效率提高12％左右。     

A Review of Density Holes Upstream of Earth's Bow Shock

Larmor size transient structures with density depletions as large as 99% of ambient solar wind density levels occur commonly upstream of Earth＇s collisionless bow shock. These ＂density holes＂ have a me...     

FREJA卫星观测到的低混杂小尖峰和密度空穴的关系

从FREJA卫星近期观测发现，地球低极尖区等离子体密度的衰减有多种可能的机制，不同机制所形成的密度空穴都可能捕获低混杂频率附近的湍动波，进而使原有的密度空穴加深．由于同时检测到静电和电磁的低混杂小尖峰，故提出电磁低混杂湍动的电场分量被密度空穴所捕获．     

气体密度超声检测法的研究

介绍了一种利用超声技术在线快速测量气体密度的方法。其原理是测出气体介质的压力和声速后,再根据由热力学和弹性介质力学建立起来的压力、声速和密度之间的关系算出密度。所有监控、测量和数据处理均由微机完成。还给出了在几种不同介质中的试验结果,并对结果进行了半定量的误差分析。与理论分析相比,有较好的一致性。超声检测法是一种在线检测气体密度的新方法。     

C172飞机发动机贫富油使用浅析

自从C172飞机用于我院飞行训练以来，由于对贫富油调节的方法错误而出现了几起严重的空中发动机抖动事件，危及了飞行安全。本文从使用的角度分析了飞行的几个阶段：地面运行、起飞爬升、巡航下降及着陆关车贫富油调节的方法。     

Dependence of density and burning rate of composite solid propellant on mixer size

This paper examines the effect of mixer size on the density of the propellant and it also explores the role of the propellant density with regards to burning rate and burn rate pressure index. Propellant samples were prepared in the four different size (15, 70, 200 and 1000 g) mixers with identical input of ingredients to examine the effect of mixer size on density and burning rate of the composite solid propellant. It was noticed that density and burning rate of the propellant changes significantly with change in the mixer size from 15 g to 1000 g. This is because for the smaller mixers the surface area to volume ratio is large and the actual percentage of aluminum and ammonium perchlorate (especially coarse) that goes into the propellant reduces. High burning rate with decrease in mixer size is also accompanied with increase in burn rate pressure index. The composition analysis was also carried out and it is noticed that the actual percentage of the ingredients is different from the intended percentage of the ingredients and percentage change is more when the mixer size decreases.     

Electron coronal density irregularity\overline {n^2 } /(\bar n)^2 from measurements of K-coronal and lyman lines brightnesses

We propose a technique to derive the coronal density irregularity factor , wheren is the electron density. The absolute photometric comparison between the intensity of UV lines and the white-light K-coronal polarized brightness (pB) provides an unique constraint on the inhomogeneity of the corona. The ratio of the measured H I Lyman (Ly-) line intensity to the resonant-scattering dominated H I Lyman (Ly-) intensity can be used to extract the collisonal component of the Ly-. This component yields an estimate of . The quantity is then obtained from white-light K-coronal measurements. The use of lines of the same atomic species minimizes the effects due to outflow velocities (i.e., Doppler dimming), and reduces the errors introduced by the uncertainties in the ionization balance, the atomic parameters, and the solar abundances. The UVCS/SOHO unique capability of performing cotemporal and cospatial measurements of the Ly- and Ly- lines, and ofpB makes this instrument ideal for implementing this technique.     

IRI 2001/90 TEC predictions over a low latitude station

Total electron content (TEC) over Tucumán (26.9°S, 294.6°W) measured with Faraday technique during the high solar activity year 1982, is used to check IRI 2001 TEC predictions at the southern crest of the equatorial anomaly region. Comparisons with IRI 90 are also made. The results show that in general IRI overestimates TEC values around the daily minimum and underestimates it the remaining hours. Better predictions are obtained using ground ionosonde measurements as input coefficients in the IRI model. The results suggest that for hours of maximum TEC values the electron density profile is broader than that assumed by the model. The main reason for the disagreement would be the IRI shape of the electron density profile.