计算表明 ，当电磁波的频率接近电子碰撞频率时 ，磁等离子体对电磁波的吸收达到最大值。
The results illustrate that the collisional absorption have a maximum value when the collision frequency is near the radiation frequency.
与臭氧层类似，磁层对地球生物至关重要，绝大多数来自太阳的有害射线和热等离子体都被地球磁层折射回太空，从而使我们免受伤害。
Like the ozone layer, the magnetosphere is important to life on Earth because it protects us from most of the harmful radiation and hot plasma from the Sun, deflecting it into space.
实际上我们所做的就是降低等离子体的磁引力场强度到细胞的等离子体强度。
In fact what we do, we reduce the strength of the gravitational magnetic field of the plasma to the plasma of the cell.
因此，当地球的磁引力场体在太阳的等离子体前面创造出一个壁垒，其产物就是氮。
So, when the Earth gravitational magnetic field puts a barrier in front of the floor of the plasma of the Sun, the product is nitrogen.
在杂散场测量与软件补偿实验中，发现同心圆逆磁线圈感应的杂散信号主要来自垂直场、涡流电流、等离子体电流和纵场电流的变化。
In the experiments of measurement and software compensation of diamagnetism, it is found that stray fields mainly come from the vertical field, plasma current and eddy current.
本文解出了具有固定边界的平衡等离子体磁面方程的解析解和数值解。
The analytic solutions and numerical solutions of the equations of magnetic surface with fixed-boundary conditions are solved for the equilibrium plasma.
根据MHD气球模稳定性理论，计算了负磁剪切位形中等离子体气球边缘稳定性区域。
Based on MHD ballooning mode stability theory, marginal stability regions of the plasma ballooning mode in negative magnetic shear configuration are calculated in this paper.
聚乙烯阳极外磁绝缘离子二极管阳极等离子体的形成基于阳极聚乙烯膜表面脉冲放电过程和阴极电子轰击效应。
The formation of anode plasma in external magnetic field MID is derived from the pulsed discharge and electron impact on the surface of anode polymer.
率很高，太阳风能量投入是显而易见的大振幅的等离子体波和大型磁结构的磁强计测量了整个遭遇。
The high rate of solar wind energy input was evident in the great amplitude of the plasma waves and the large magnetic structures measured by the Magnetometer throughout the encounter.
在静电磁流体方程基础上，提出了柱状放电电弧等离子体磁螺旋不稳定性的一种新的线性分析方法。
A new linear analysis for magnetic helical instabilities of arc discharges in a cylindrical plasma is developed based on a set of electrostatic magnetohydrodynamic equations.
采用PIC模拟方法对同轴混合铁磁摇摆器自由电子激光器进行了研究，分析了等离子体填充对其性能的影响。
A coaxial hybrid wiggler free-electron laser (FEL) amplifier with and without plasma filling is studied by a method of PIC simulation in this paper.
采用打靶法，数值求解了在负磁剪切托卡马克等离子体中离子温度梯度驱动的复本征模方程。
An eigenmode equation of ion temperature gradient driven instability in a tokamak plasma with negative magnetic shear is solved numerically by the shooting method.
首先是磁曲率对等离子体电阻性不稳定性的影响。
The first is that the effects of the magnetic curvature on the resistive interchange mode in tokamak plasmas.
采用电荷中和及磁中和模型，求解了束-等离子体系统的初值问题，得到了等离子体的响应函数。
The electrostatic and magnetic neutralization model has been adopted in solving the initial value problem of the beam-plasma system to obtain the plasma response functions.
现在在等离子体条件下，我们创造了一个等离子壁垒，一个磁引力场的壁垒。
Now in the plasmatic condition, we create a plasmatic barrier, gravitational magnetic field barrier against another.
通量管为太阳风等离子体向磁层输运和磁层粒子向行星际空间逃逸提供了通道。
The flux ropes offered channels for the transport of the solar wind plasma into the magnetosphere and the escape of the magnetospheric plasma into the interplanetary space.
由此我们讨论了多极场对等离子体磁阱和剪切的影响。
Furthermore, the influence of multipole 'fields on the longitudinal magnetic well and the magnetic shear is discuss.
观测表明，多数磁尾等离子体团为具有强核心场的通量绳结构。
It was demonstrated from the observations that most plasmoids in the magnetotail are the flux rope structures with a large core field.
（时间01：08？）提升不是我们在胸腺、血浆的自由等离子体中要找的。它是当我们创造与我们灵魂的物理相互作用时我们所允许的磁引力场定位。
Lift is not what we're looking for in the Free Plasma of the Thymus/Thyroid - it is the Gravitational magnetic positioning which we allow when we create the physical interaction with our soul.
太阳风的涨落在磁层顶激发压缩阿尔文波，并在磁尾的无碰撞等离子体中传播。
The fluctuations of solar wind quantities at the magnetopause excite the compressed Alfven waves, which propagate through the collisionless plasma in the tail of magnetosphere.
太阳风的涨落在磁层顶激发压缩阿尔文波，并在磁尾的无碰撞等离子体中传播。
The fluctuations of solar wind quantities at the magnetopause excite the compressed Alfven waves, which propagate through the collisionless plasma in the tail of magnetosphere.
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