航空公司资本结构实证研究

借鉴西方资本结构理论成果，采用定量分析方法，通过实证研究对航空公司资本结构的影响因素进行了系统分析论证，并在此基础上，研究了资本结构的决策方法。     

液体压力激波发生器激励电源设计及研究

以复合式隔离的双端正激功率变换电路为基础研制了激波发生器激励电源,分析了电路的主要工作原理,并用 Pspice 进行了仿真分析,最后实验结果表明本方案的正确性与可行性,对压电陶瓷的激励效果好,电源效率较高。     

彩电消磁器PTCR耐电性能与显微结构

本文利用扫描电镜、透射电镜和俄歇能谱实验技术,对彩电消磁器半导化钛酸钡陶瓷显微结构进行了分析研究,证实该陶瓷显微结构中存在玻璃态第二相,玻璃相物质对PTC材料耐电性能有显著影响。工艺过程的改善可减少第二相含量,使耐电性能提高40％。本文还就PTC材料超薄片制备技术作了详细介绍。     

二阶非线性方程零解的全局稳定性

在不同于文（１，２，３，４，５）的条件下，得到了二阶非线性方程ｄｘ／ｄｔ＝ｆ１（ｘ）＋ｇ１（ｘ）ｙ，ｄｙ／ｄｔ＝ｆ２（ｘ）＋ｇ２（ｘ）ｙ，（其中，ｆｉ（ｘ），ｇｉ（ｘ）连续，且ｆｉ（０）＝０，ｉ＝１，２）零解的全局渐近稳定的充分条件，并把这一结果推广更广泛的二阶非线性方程ｄｘ／ｄｔ＝ｆ１（ｘ）＋ｈ１（ｘ）ｇ１（ｙ），ｄｙ／ｄｔ＝ｆ２（ｘ）＋ｈ２（ｘ）ｇ２（ｙ）（其中，ｆｉ（ｘ）ｈｉ（ｘ），ｇｉ（ｙ     

人体肢体多台测力天平的研制

为满足高速风洞人椅组合模型肢体测力试验的需要 ,研究在多种防护措施下 ,飞行员上肢、下肢、前臂、上臂、小腿和大腿所受气动载荷的情况 ,研制了两台 (Φ8,Φ1 0 )六分量和两台 (Φ1 0 ,Φ1 4)五分量特种内式应变天平 ,以测量肢体各段的气动载荷。为高速飞行弹射救生××标准的制定及航空弹射救生防护方法研究提供试验依据     

Three-dimensional global simulation of multiple ICMEs’ interaction and propagation from the Sun to the heliosphere following the 25–28 October 2003 solar events

This study performs simulations of interplanetary coronal mass ejection (ICME) propagation in a realistic three-dimensional (3D) solar wind structure from the Sun to the Earth by using the newly developed hybrid code, HAFv.2+3DMHD. This model combines two simulation codes, Hakamada–Akasofu–Fry code version 2 (HAFv.2) and a fully 3D, time-dependent MHD simulation code. The solar wind structure is simulated out to 0.08 AU (18 Rs) from source surface maps using the HAFv.2 code. The outputs at 0.08 AU are then used to provide inputs for the lower boundary, at that location, of the 3D MHD code to calculate solar wind and its evolution to 1 AU and beyond. A dynamic disturbance, mimicking a particular flare’s energy output, is delivered to this non-uniform structure to model the evolution and interplanetary propagation of ICMEs (including their shocks). We then show the interaction between two ICMEs and the dynamic process during the overtaking of one shock by the other. The results show that both CMEs and heliosphere current sheet/plasma sheet were deformed by interacting with each other.     

基于弹载捷联惯性导航系统精确导航的双欧拉全姿态方法

垂直发射的地空导弹在大机动飞行时,其四元数法姿态角输出存在奇异性。为解决该问题,提出了正、反欧拉角微分方程切换的双欧拉全姿态解算方法。对正、反欧拉角微分方程进行了详细推导,论述了正、反欧拉角微分方程精华区与奇异区的倒置关系。在此基础上,建立了正、反欧拉角的转换公式。根据正欧拉角的俯仰角对正、反欧拉角无缝切换,有效解决了俯仰角在±90°附近时姿态奇异性问题。仿真和半物理试验的结果表明:双欧拉全姿态算法解算的实际姿态与理论姿态保持一致,在奇异点附近的姿态角仍能正常输出,未出现突变现象,该方法得出的导航精度比四元数法得出的导航精度提高了9.81%。     

Results from the study of an M7.6 flare and its associated CME

An M7.6 flare was well observed on October 24, 2003 in active region 10486 by a few instruments and satellites, including GOES, TRACE, SOHO, RHESSI and NoRH. Multi-wavelength study shows that this flare underwent two episodes. During the first episode, only a looptop source of <40 keV was observed in reconstructed RHESSI images, which showed shrinkage with a velocity of 12–14 km s⁻¹ in a period of about 12 min. During the second process, in addition to the looptop source, two footpoint sources were observed in energy channel of as high as ∼200 keV. One of them showed fast propagation along one of the two TRACE 1600 Å flare ribbons and the 195 Å loop footpoints, which could be explained by successive magnetic reconnection. The associated CME showed a mass pickup process with decreasing center-of-mass velocity. The decrease of the CME kinetic energy and the increase of its potential energy lead to an almost constant total energy during the CME propagation. Our results reveal that the flare and its associated CME have comparable energy content, and the flare is of non-thermal property.     

一类非线性边值问题正解的存在性研究

为讨论一类非线性二阶两点边值问题正解的存在性,利用上下解方法,构造相应锥映射,给出非线性变号的二阶两点边值问题正解存在性的判定方法;对已发表文献中相应的结果进行推广,从而获得该类边值问题存在正解的重要结论。     

On the early phase of relativistic solar particle events: Are there signatures of acceleration mechanism?

Many physical processes precede and accompany the solar energetic particles (SEP) occurrence on the Earth’s orbit. Explosive energy release on the Sun gives rise to a flare and a coronal mass ejection (CME). X-ray and gamma emissions are believed to be connected with flares. Radio emission is signature of disturbances traveling through the corona and interplanetary space. Particles can gain energy both in the flare and the accompanying wave processes. The beginning of the SEP events has the advantage of being the phase most close to the time of acceleration. Influence of interplanetary transport is minimal in the case of first arriving relativistic solar protons recorded by ground based neutron monitors in so called ground-level enhancements (GLE). The early phase of the SEP events attracts attention of many scientists searching for the understanding of particle acceleration. However, they come to the opposite conclusions. While some authors find arguments for coronal mass ejections as a sole accelerator of SEPs, others prove a flare to be the SEP origin. Here, the circumstances of SEP generation for several GLEs of the 23rd solar cycle are considered. Timing of X-ray, CME, and radio emissions shows a great variety from event to event. However, the time of particle ejection from the Sun is closer to maximum of X-ray emission than to any other phenomena considered. No correlation is found between the particle fluxes and the CME characteristics.