三乙胺与硝酸-27S自燃技术研究

三乙胺和硝酸-27S作为自燃推进剂可应用于火箭发动机中。对这两种自燃推进剂的燃烧性能进行了研究,应用逐步逼近法计算其热力性质,当最佳混合比为4．1,燃烧室压力为4．5MPa时,最佳海平面比冲为2786m／s。通过试验证明了三乙胺和硝酸-27S自燃技术的可行性。     

小型热真空试验设备网络化集群测控技术

随着航天器部组件试验任务的日益增多,在人员少的情况下,高效率地完成型号任务的需求十分迫切。文章介绍了小型热真空试验设备网络化集群测控的方法与技术,以某小型热真空试验设备群为例,针对其接口复杂、数据量大、地理位置分散且要求集中管理的特点,详细阐述了采用混合B/S模式与C/S模式的网络化测控技术来实现小型热真空试验设备群集群测控的功能。该技术已在小型热真空试验设备的集群控制中得到了成功的应用。     

基于Web的e—CRM系统的分析与设计

首先介绍了CRM和e-CRM的概念,进而提出了基于WEB的六层技术架构,并介绍了各个层次的功能,最后对企业实施e-CRM提出了几点建议,并对CRM发展趋势做了预测。     

新机研制争速度 当年首飞上蓝天──加速教11工艺准备工作的几项措施

论述了南飞公司为加速教11飞机的研制，对工艺准备工作所采取的几项措施，主要是：按研制顺序倒排计划；控制二装需求总量；实行阶段承包；开展平行工程；实行系统管理。     

象征型拟微分算子的L~2－有界性

证明了象征型拟微分算子的一个Ｌ２有界性定理，其中象征ａ（ｘ，ξ）关于ｘ的正则性条件被进一步减弱了。在某种意义下，该结果给出了定理Ａ与定理Ｂ之间的联系。     

不确定串联非线性系统具有L2增益的鲁棒自适应控制

研究了一类含有未知参数和干扰的串联非线性系统H∞鲁棒自适应控制问题。结合H∞控制和自适应控制，基于李亚普诺夫函数递推设计方法设计了H∞状态反馈自适应控制器，并且得出了控制器的精确解，避免了求解HJI不等式设计控制器的困难。该控制器不仅保证闭环系统ISS稳定，而且使得系统对于所有允许的参数不确定从干扰输入以可控输出的L2增益不大于给定的值。仿真结果表明了所设计的控制器的可行性和有效性。     

物体穿越斜激波干扰特性的数值研究

当物体以超声速穿越同向运动的斜激波时，它的飞行Mach数和攻角都会发生较大的变化。穿越过程中斜激波与物体脱体激波发生相互作用，形成复杂的激波干扰波系结构，基本的干扰形式为复合Mach反射结构。不同的穿越位置时，由于不同的来流条件，使物体上尾部凹坑内的流场和波系发生很大的变化，随着物体的穿越过程，当头部和凹坑下游壁面与翼面穿越激波时，阻力系数有两次剧烈的变化，法向力基本呈线性下降，压力中心先大幅度后移，物体逐渐穿过激波后又快速前移。因此穿越过程使物体加速，给物体的姿态带来很大的扰动。翼面穿过激波也造成阻力、法向力下降，压心后移。如果对有控制的飞行器，穿越激波时气动力特性和稳定性的急剧变化，将给控制系统带来很大的困难。     

车载遥测站天线标校复查中存在的问题及对策

车载遥测跟踪站天线展开后,需要进行远场标校复查。由于受标校距离、天线仰角以及周围环境等各种条件的限制,使得主天线、引导天线的光电轴匹配检查难以保证精度要求,从而影响跟踪性能。针对这些问题,本文提出在近场条件下直接悬挂信标机进行标校复查,以保证光电轴匹配精度。并针对YQ- 312 S频段遥测跟踪车载站的实际推出角度转换公式。最后给出实例     

On the correlation of the solar wind observed at the L5 point and at the Earth

The L5 point is a promising location for forecasting co-rotating high-speed streams in the solar wind arriving at the Earth. We correlated the solar wind data obtained by the Nozomi spacecraft in interplanetary space and by the Advanced Composition Explorer (ACE) at the L1 point, and found that the correlation is significantly improved from that of the 27-day recurrence of ACE data. Based on the correlation between the two spacecraft observations, we estimated the correlation of the solar wind velocity between the L5 point and at the Earth, and found that the correlation coefficient was about 0.78 in late 1999, while that of the 27-day recurrence was 0.51. Eighty-eight percent of the velocity difference falls within 100 km/s between the L5 point and the Earth. This demonstrates the potential capability of solar wind monitoring at the L5 point to forecast the geomagnetic disturbances 4.5 days in advance.     

Statistical characteristics of locally generated ESF during equinoctial months over Sanya

Understanding the local generation rate of equatorial spread-F (ESF) is important for forecasting ionospheric scintillation. Using the GPS ionospheric scintillation/TEC and VHF radar data during March-April and September-October from 2010 to 2014, the occurrence of ionospheric scintillation, TEC fast fluctuation, and backscatter plume were studied. Through analyzing the simultaneous occurrence of ionospheric scintillation, TEC fast fluctuation and backscatter plume, the local generation rate of ESF over Sanya was investigated. The results show that the monthly generation rate varies between 0% and 68%. A significant equinoctial asymmetry of local generation rate of ESF can be found in 2010, 2013 and 2014. The local generation rate of ESF increases from 2010 to 2014 during March-April, while it does not have similar trend during September-October. The plasma vertical drift influenced by solar activity has a significant impact on the monthly generation rate. The equinoctial asymmetry of plasma vertical drift may contribute a lot to the equinoctial asymmetry of the generation rate of ESF.