1) beam coordinate
天线波束坐标系
1.
This paper introduces antenna beam stabilization which is based on tri-axis stabilization platform of azimuth-elevation-polarization,presents a new concept of antenna beam coordinate,and antenna beam stabilization isolation equations are deduced,for overcoming disturbance of vehicle\'s angle movement,and simulated based on the model.
本文基于方位—俯仰—极化三轴稳定平台的天线波束稳定方案,提出了天线波束坐标系的概念,推导出天线波束稳定隔离方程,以克服载体角运动对天线波束的干扰,并基于此模型进行了仿真,结论对实现天线波束稳定具有一定的理论意义。
2) antenna beam coordinates system
波束坐标系
1.
According to the gyro self-stabilization method and the concept of the defined antenna beam coordinates system,the influences on pointing and polarization of the beam caused by the carrier\'s attitude variation are analyzed,and the stabilization isolation equations are deduced,so the stabilization of the beam\'s pointing and polarization are realized.
文中结合陀螺自稳定方法和定义的天线波束坐标系,分析了载体运动对波束指向和极化的影响,推导出了稳定隔离方程,实现了波束指向和极化的稳定。
3) antenna array coordinate
天线阵面坐标系
1.
By use of the sinusoidal spatial transform, the method transfers the nonlinearly variational characteristics on monopulse angle sensitive function versus scan angle in antenna array coordinate to a simple linearly shift one in sinusoidal space.
该方法利用正弦空间变换 ,将单脉冲角敏函数在天线阵面坐标系中随扫描角的非线性变化特征转变为正弦空间中简单平移的线性变化特征 ,使得二维相扫测角系统在装订角敏函数时 ,方位和仰角仅需各装订一条曲线 ,不仅节约了大量存储空间 ,而且消除了分区装订和波控机量化引入的误差 ,极大地提高了雷达跟踪精度。
5) celestial coordinate system
天球坐标系
1.
The celestial coordinate system is a coordinate system for mapping position in the sky which based on the rotation and revolution around the Sun of the planets.
行星的自转和绕太阳公转是建立天球坐标系的事实依据。
2.
In this article,“celestial coordinate system”, the difficult point in the teaching of the Conspectus of the Earth, is analysed and studied and three key points are proposed: finding the joint point, establishing an coordinate system mode that can be accepted easily and giving out the basic dots & great circle system very distinctly.
本文主要对《地球概论》中的教学难点“天球坐标系” ,结合教学实践与有关教材进行深入的分析和研究 ,提出突破这一教学难点的 3个关键 :找准衔接点 ;建立易于掌握的坐标系模式 ;清楚地给出基本点和大圆的系统。
6) astronomical coordinate system
天文坐标系
补充资料:甚大天线阵
甚大天线阵 Very-Large Array 世界上最大的综合孔径射电望远镜。简称甚大阵,常用VLA表示。1981年建成于美国新墨西哥州圣阿古斯丁平原,属美国国立射电天文台。它由27面直径25米的抛物面天线组成,Y型排列,每臂长21千米。有3种组合模式,最长基线为36千米。可在6个波段工作,并可作圆偏振(左旋和右旋)和线偏振测量。在厘米波段,最高空间分辨率达角秒量级,与地面光学望远镜的分辨率相当;灵敏度比世界上其他射电望远镜高一个量级;成像时间8~10小时。根据观测要求,可分别作连续谱、射电谱线和甚长基线干涉测量的观测研究工作。 |
说明:补充资料仅用于学习参考,请勿用于其它任何用途。
参考词条