填充型吸波体阻燃外壳材料的研究

针对现有吸波材料外壳阻燃性能的不足,提出以玻璃纤维为主的新型复合外壳材料,并与聚丙烯空心板制备的方体的反射损耗进行对比。研究结果表明:在保证阻燃性的情况下,在低频下使用此类复合材料整体吸波性能较聚丙烯空心板材料提升了大约5~10 dB,在高频区有所下降,下降约10 dB,具有一定的应用价值。     

Microwave Diagnostics of Dynamic Processes and Oscillations in Groups of Solar Coronal Magnetic Loops

Low-frequency (LF) modulations of the solar microwave radiation (37 GHz) recorded at the Metsähovi Radio Observatory, are analyzed. Since the intensity of solar microwave radiation, produced by the electron gyrosynchrotron mechanism, is dependent on a value of the background magnetic field [Dulk, G. A.: 1985, Ann. Rev. Astron. Astrophys. 23, 169–224], slow variations of the magnetic field associated with disturbances of the electric current in a radiating source, can modulate the intensity of the microwave radiation. The observed multi-track features of the LF spectra are interpreted as a signature of a complex multi-loop structure of the radiating source. Application of the equivalent electric circuit models of interacting loops allows to explain and reproduce the main dynamical features of the observed LF modulation dynamic spectra.     

活性碳毡对称振子阵列／树脂复合吸波材料的研究

研究了含活性碳毡对称振子阵列吸波复合材料的微波吸收特性.结果表明:含振子阵列吸波材料的吸波性能与入射电场方向、振子两臂间的电阻、振子间的距离和阵列的位置密切相关.对称振子阵列对电磁波的吸收呈各向异性,振子与入射电场平行时,吸波性能较好;随振子两臂间电阻或振子间距的增大,材料的吸波性能先提高后降低,电阻和振子间距均存在最佳值;随振子阵列和试样下表面距离的减小,材料的吸波性能提高,振子与入射电场平行时,本实验条件下可获得有效带宽13GHz,最大吸收峰值-30.3dB的反射衰减.     

在ZS195直喷式柴油机中燃用二甲基醚(DME)的实验研究

本实验使用二甲基醚-柴油二元混合燃料,在对原发动机的燃料供给系统做尽量少的改动的原则下,柴油机的排放大大降低,同时发动机仍能保持原有的动力性能。理论分析和实验证明二甲基醚是一种极有应用前景的柴油机代用燃料。      

二厘米微波衰减标准装置不确定度的验证

采用传递比较法对二厘米微波衰减标准装置不确定度进行了验证。测量标准装置的重复性以组内实验标准偏差sn(A)定量表征，测量标准装置的稳定性用组间实验标准偏差sm定量表征。     

小型微波等离子推力器研究

 介绍约100W 功率微波等离子推力器的系统结构, 谐振模式, 电磁场分布, 电磁场、等离子体和流场的耦合, 喷管中的等离子体复合流动, 真空羽流, 原理实验样机性能及应用前景。     

陶瓷材料的微波烧结机理探讨

本文根据部分陶瓷材料的微波烧结实验结果和微波加热的特点，对陶瓷材料的微观结构进行了分类，分析了电场在不同结构中的分布特点。提出了微波加热的微区温度梯度模式，以及微波连接的液相连接方式，并据之对实验结果给出了合理的分析和解释。     

The local bubble

Recently, observations with the rosat PSPC instrument and the spectrometers onboard the euve satellite have given new detailed information on the structure and physical conditions of the Local Bubble. From the early rocket experiments, and in particular from the WISCONSIN Survey, the existence of a diffuse hot gas in the vicinity of the solar system, extending out to about 100 pc, has been inferred in order to explain the emission below 0.3 keV. The higher angular resolution and sensitivity of rosat made it possible to use diffuse neutral clouds as targets for shadowing the soft X-ray background. Thus, in some directions, more than half of the flux in the 0.25 keV band appears to come from outside the Local Bubble. Further, measurements of the diffuse EUV in the LISM, show surprisingly few emission lines. These findings are in conflict with the standard LHB model, which assumes a local hot (T 10⁶ K) plasma in CIE. Model calculations, based on the non-equilibrium cooling of an expanding plasma, show a promising way of reconciling all available observations. Thus the present temperature within the LB may be as low as 4 × 10⁴ K and its number density as large as 2 × 10^–2 cm ^–3, giving a total pressure that is roughly in agreement with the Local Cloud.Abbreviations CIE collisional ionization equilibrium - ISM Interstellar Medium - LHB Local Hot Bubble - LB Local Bubble - LISM Local ISM - SB superbubble - SXR soft X-ray - SXRB SXR Background - VLISM Very Local ISM Heisenberg Fellow     

C/E复合材料声发射信号小波分析及人工神经网络模式识别

以复合材料为对象，以宽频带传感器及线阵列方式对各类模式试样采集了波形及信号参数，比较波形、信号参数、频谱及小波谱的特征，筛选出六类1300个样本，采用多分辨小波变换提取了5个特征向量，实现了特征空间的降维处理，采用B—P型反向传播神经网络构成了智能化模式分类器，研究了网络模型的学习效果和对与复合材料主要损伤机制有关的六类声发射信号的识别能力。试验结果表明，神经网络对六类信号的平均正确识别率达到90.4%。最佳识别率为97.2%。该方法成功用于90°、0°光滑和0°缺口三种试样的破坏过程分析，获得了满意的效果。     

微波测量技术在表面粗糙度测量中的应用

根据电磁波在金属表面反射的理论,提出了利用微波测量技术测量表面粗糙度的新方法。利用微波技术理论分析了测量原理,给出了测试装置图,介绍了系统的工作原理,最后,给出了实验结果和误差分析。这种方法具有非接触测量的优点。