Form Invariance and Noether Symmetries of Rotational Relativistic Birkhoff Systems

Under the infinitesimal transformations of groups,a form invariance of rotational relativistic Birkhoff systems is studied and the definition and criteria are given,In view of the invariance of rotational relativistic Pfaff-Birkhoff-D‘ Alembert principle under the infinitesimal transformations of groups,the theory of Noether symmetries of rotational relativistic Birkhoff systems are constructed.The relation between the form invariance and the Noether symmetries is studied ,and the conserved quantities of rotational relativistic Birkhoff systems are obtained.     

多维重Brown运动图集和像集的精确Hausdorff测度

设{W(t):t∈R},{B(t):t∈R }是两相互独立取值于R且W(0)= B(0)=0的标准Brown运动, {Y(t)=W(B(t)),t∈R }为R上的重Brown运动,X1(t),…,Xd(t)是Y(t)的d个独立复制．我们将探讨d维重Brown运动X(t)=(X1(t),…,Xd(t))的像集和图集的精确Hausdorff测度．更确切地,得到了X的像集X(Q)={X(t):t∈Q}和图集GrX(Q)={(t,X(t)):t∈Q}的精确Hausdorff测度,其中Q为(0,∞)上的Borel集．     

旋转圆环上的珠子动力学

对于放置在旋转圆环凹槽上的珠子,当圆环旋转时,珠子将产生一系列运动行为。可以将珠子视为刚体,研究珠子的动力学,考虑滚动摩擦和黏滞阻力两种形式的阻力,用分析力学方法推导其运动方程,并讨论相关动力学变量,包括平衡点超临界分叉、小振动周期等条件,通过实验模型进行逐一验证。并对特殊条件下进行的受迫振动进行了理论和实验研究。     

旋转导向钻井工具姿态测量陀螺仪故障估计与处理方法

针对旋转导向钻井工具姿态测量系统陀螺仪故障问题,提出一种陀螺仪加性故障估计与处理方法.首先将陀螺仪故障增广为状态变量,融合加速度计测量信息建立非线性测量模型;然后针对由于模型线性化、陀螺仪漂移、钻井过程的高温、高压、强振动等因素导致卡尔曼滤波算法估计精度变差的问题,将测量误差等效为幅值有界但分布未知的误差,提出了一种自...     

温度变化导致航天相机光学系统像面位移的研究

温度变化导致的像面位移会影响航天相机光学系统的成像质量。根据高斯光学理论,推导出了温度变化时的相机光学系统的像面位移公式,确定了温度敏感性最低的主、次反射镜的材料及与之相匹配的镜筒材料。最后计算和比较了在不同温度变化时的光学系统的传递函数。     

旋转液体特性实验测量重力加速度不确定度研究

重力加速度测量实验是大学生物理实验必修课实验内容之一,在实验过程中由于仪器使用不当或操作不正确,在计算结果时存在不同的偏差。不确定度是衡量测量精度的重要指标,本文计算了三种不同情况测量重力加速度时的不确定度,主要考虑了激光照射透明挡板的角度r、激光垂直入射点的偏差Δx和激光垂直入射方向的偏差β对重力加速度的不确定度。通过计算,当透明挡板向上/下偏移的角度为5°时,不确定度为1.496 3 m/s~2;当激光向左/右偏移5 mm时,不确定度为1.0044 m/s~2;当激光向左和向右偏移的角度为5°时,不确定度分别为1.551 5 m/s~2和1.250 8 m/s~2。本文可为减小旋转液体测量重力加速度误差提供理论依据。     

综合微光测试系统的总体设计

描述一种微光像增强器综合测试系统的总体设计。设计采用了组合结构，使系统只用单一的光源就可以测试微光像增强器九项光量子类和几何类的参数，具有以往几台常规测试仪器功能的总和。系统对各参数测量的不确定度２～４％。     

一般旋转壳在轴对称变形下的复变量方程

本文在Love-Kirchhoff的假定下,求得了一般旋转壳在轴对称变形下的复变量方程.当旋转壳是圆截面环壳时,这些方程简化为F.T?lke(1938)[3],R.A.Clark(1950)和B.B.Новожилов(1951)[3]的方程.当平均半径R比环截面半径a大得很多时,求得了细环壳的复变量方程,当这个细环壳的截面是圆形时,简化作为作者(1979)[6]的圆截面的细环壳复变量方程,我们列出了椭圆截面的细环壳复变量方程.当椭圆截面近似于圆截面时,该方程在形式上和圆细环壳方程基本相同.     

The effect of toroidal field on the rotating magnetic field current drive in rotamak plasmas

A rotamak is one kind of compact spherically shaped magnetic-confinement device. In a rotamak the plasma current is driven by means of rotating magnetic field （RMF）. The driven current can reverse the original equilibrium field and generate a field-reversed-configuration. In a conventional rotamak, a toroidal field （TF） is not necessary for the RMF to drive plasma current, but it was found that the present of an additional TF can influence the RMF current drive. In this paper the effect of TF on the RMF current drive in a rotamak are investigated in some detail. The experimental results show that addition of TF increases the RMF driven current greatly and enhances the RMF penetration dramatically. Without TF, the RMF can only penetrate into plasma in the edge region. When a TF is added, the RMF can reach almost the whole plasma region. This is an optimal strength of toroidal magnetic field for getting maximum plasma current when Bv and radio frequency generator power are fixed. Besides driving current, the RMF generates high harmonic fields in rotamak plasma. The effect of TF on the harmonic field spectra are also reported.[第一段]     

Rotational Deformation of Neutron Stars

The rotational deformations of two kinds of neutron stars are calculated by using Hartle‘s slow-rotation formulism. The results show that only the faster rotating neutron star gives an obvious deformation. For the slow rotating neutron star with a period larger than hundreds of millisecond, the rotating deformation is very weak.