某些NTO盐的热分解特性及在固体推进剂中催化特性的相关性研究

采用高压差示扫描量热仪,研究了几种ＮＴＯ（３－硝基－１,２,４－三唑－５－酮）盐在不同压力下的热分解特性,同时测定了以ＮＴＯ盐为催化剂的固体推进剂的燃速特性。结果认为,这些ＮＴＯ盐的热分解特性与催化特性间存在某种联系,热分解行为压力不敏感的ＮＴＯ盐,可能会是较好的燃速催化剂。因此热分解行为可作催化能力的判据之一。     

数字电子气动式座舱压力控制系统模型及性能分析

在分析数字电子气动式座舱压力控制系统结构的基础上,建立了座舱及控制系统中执行机构各部件的数学模型.分析系统的传递函数得到了系统稳定所需的PID控制参数取值范围,通过对系统动态性能的仿真进一步确定PID各参数的关系.结果表明:为了满足数字电子气动式座舱压力变化速率和稳定性的要求,PID参数需满足一定的关系:在一定范围内,控制器的比例参数应大于微分参数,而微分参数应大于积分参数.     

Properties of Sharp and Large Changes in the Solar Wind Ion Flux (Density)

The results of a detailed study of large (by 20% and more) and sharp (faster than ten minutes) changes of the ion flux in the solar wind are presented. The data are provided by regular measurements onboard the INTERBALL-1 satellite in the period 1996–1999. Using statistical analysis, we obtained the distribution of these changes in their absolute and relative strength. It is shown that, for a considerable proportion of the events, such sharp and large changes of the ion flux (density) take place under conditions of fairly constant values of the solar wind velocity and of both the magnitude and components of the interplanetary magnetic field.     

Orientation of Middle-Scale Structures in the Solar Wind Plasma

An estimation of the value and orientation of the inclination of middle-scale structures in the solar wind plasma is obtained on the basis of time lags of simultaneous correlated measurements on three spacecraft: INTERBALL-1, IMP-8, and WIND. It is shown that middle-scale plasma structures, in the majority of cases, are not perpendicular to the Sun–Earth line, but inclined to it (presumably, in the ecliptic plane), on average, at an angle of approximately 63° (or 27° to the Y _SE axis). However, this inclination is significantly less than the inclination of the Parker spiral for the interplanetary magnetic field (45° at the Earth's orbit).