Stochastic acceleration of charged particle in nonlinear wave field

Possibility of stochastic acceleration of charged particle by nonlinear waves is investigated. Spatially regular (SR) and spatiotemporal chaotic (STC) wave solutions evolving from saddle steady wave are tested as the fields. In the non-steady SR field the particle is finally trapped by the wave and averagely gains its group velocity, while in the STC field the particle motion displays trapped-free phases with its averaged velocity larger or smaller than the group velocity depending on the charge sign. A simplified model is established to investigate the acceleration mechanism. By analogy with motor protein, it is found that the virtual pattern of saddle steady wave plays a role of asymmetric potential, which and the nonlinear varying perturbation wave are the two sufficient ingredients for the acceleration in our case. This revised version was published online in August 2006 with corrections to the Cover Date.     

计算谐振机翼气动力的激波膨胀波级数展开法

本文根据激波-膨胀波理论,忽略了反射波对翼面压强分布的影响,把斜激波之后和通过一族主特征线的压强展成级数,给出了沉浮和俯仰谐振翼型表面压强分布的近似解析解。然后应用片条理论导得三维机翼振动导数的闭式解。文中给出三角形机翼俯仰导数的几个实例,数值结果与现有其它方法的结果有很好的一致性。     

彗星环境中尘埃等离子体的电荷涨落和静电波动

本文分析了尘埃等离子体中尘埃颗粒的带电过程，给出了一套自洽的工流体方程组．运用这组方程研究了尘埃电荷的起伏涨落，得到了非磁化均匀尘埃等离子体中静电波动的色散关系．针对彗星空间环境中尘埃等离子体的特点，讨论了尘埃电荷的涨落对各种静电波动的影响．     

缝隙漏波波导天线及其RCS

介绍了非谐振缝隙组成的漏波波导行波天线，它是在短形波导宽面切铣间距密集的横向短槽构成的线阵；以该线阵为单元设计并研究了驻波平面阵列及其后向ＲＣＳ；给出Ｋｕ波段的天线例子，实验测试结果表明，本天线具有良好的辐射方向图、增益、输入驻波比（ＶＳＷＲ）、带宽和ＲＣＳ特性。     

收缩段出口型式对水槽流场品质的影响

研究了收缩段出口顶壁型式对表面波的影响，得到了最佳的出口设计，并分析了满流和明流情况下，流场速度，湍流等澡程的发展变化。     

逆压梯度湍流边界层中的相干结构

利用流动稳定性理论中一般共振三波的概念对4种定常逆压梯度以及两种变逆压梯度湍流边界层的相干结构进行研究.其中2种变逆压梯度分别为压力梯度由小变大和由大变小,变化的终了具有相同的压力梯度.通过计算得出逆压梯度能够激励相干结构的生成和发展,而且逆压梯度越大作用越强.在变压力梯度流动中,压力梯度由大变小的情况对相干结构的激励最强.此外,逆压梯度使相干结构的流向尺度变小,而展向间距基本在100个粘性长度左右,这些变化趋势与实验以及直接数值模拟结果一致.     

低温下三组元固体推进剂燃烧波阵面变化规律实验研究

深入了解高能固体推进剂在低温条件下燃烧性能,获得燃烧波阵面变化规律,对评估推进剂在低温条件下的适应性能力具有重要指导意义。本文设计了燃烧波狭缝观测实验装置,采用高速摄影观测技术,对三组元HTPB固体推进剂在常温和低温条件下的燃烧过程进行了观测,获得了燃烧过程中波阵面的图像。结果表明,相比于在常温条件下,固体推进剂在低温条件下出现了燃烧波不稳定的情况。根据燃烧波图像计算出了推进剂的燃速,并与靶线法燃速测量结果进行比较。结果表明,两种方法测量的结果差异较小,推进剂在低温条件下的燃烧速度明显低于在常温条件下,常温条件的燃速在1.717～2.127mm/s,低温条件下的燃速在1.252～1.583mm/s。     

一维非定常流的气体格子模型

本文研究气体格子模型的一维流动。阐述一般的简单气体格子族。利用2-速度系数模型研究了激波的形成、反射以及相互干扰。计入了不同的初始条件和边界条件。一维气体格子模型考虑了可压缩性和二维、三维模型的基本特性。     

超声电喷推进微细驻波形成及影响因素分析

对超声电喷推进微细驻波进行了研究,试验观测了微细驻波形成形态,并在不同频率下对比分析了微细驻波波长的理论值和试验值;同时分析了不同推进剂条件下,振动频率对微细驻波波长和形成驻波所需振幅的影响规律。结果表明：不同频率下,形成微细驻波波长的理论值和试验值具有较好的一致性;微细驻波的波长和振幅随着振动频率的增大而减小,同时推进剂的粘度越大,形成微细驻波所需的振幅也越大。     

An investigation of the solar cycle impact on the lower thermosphere O(S) nightglow emission as observed by WINDII/UARS

The yearly variation of the integrated emission rate of the O(¹S) nightglow in the lower thermosphere is studied and the solar cycle impact is examined from the observations of the Wind Imaging Interferometer (WINDII) operated on the Upper Atmosphere Research Satellite (UARS). More than 300,000 volume emission rate profiles of the O(¹S) nightglow observed by WINDII for 40°S–40°N latitudes during November 1991–August 1997 over half of a solar cycle are utilized. These profiles are vertically integrated for the altitude range of 80–100 km and the equivalent column integrated emission rates are then zonally averaged for bins with 10° latitude and 3 month intervals. It is found that for each latitude the O(¹S) nightglow emission rate appears to increase with increasing solar F10.7 cm flux, following a linear relationship. This characterizes the solar cycle impact on the O(¹S) nightglow, while the solar influence is modulated by a seasonal variation. Based on these variations, an empirical formula is derived for predicting the three-month averages of the O(¹S) nightglow integrated emission rate. The standard error of the estimated values from the formula is smaller than 30 Rayleigh.