分析了粉粒在反应区的沉降过程,导出了沉降的最大速度及时间的公式,给出了离子在不同位置上的平均动能及粒子通量。
The behaviors of the neutrals in the sheath were analyzed and their average energies and the flow rates at different positions were also given.
测量表明,在全部损失到壁上的功率中,中性粒子通量的贡献是主要的,光辐射损失只占小部分。对光辐射中不同波长的辐射功率进行了测量。
The experiments show that main power loss to the wall is carried away by energetic neutrals while the light radiation loss is only a small portion of total power loss.
利用周期轨道理论,我们计算了在不同情况下,一个粒子在二维谐振子势中存在和不存在磁通量时的量子能级密度。
Using the periodic orbit theory, we computed the quantum level density of a particle in the two-dimensional harmonic oscillator potential with and without the magnetic flux line for different cases.
FY 1C星空间粒子成分探测器能够实现对质子能谱、电子积分通量及重离子成分的同时测量。
The space particle composition detector aboard FY-1C satellite can simultaneously detect proton spectrum, electron integrated flux and heavy ion composition.
计算了电子的密度分布,电子与中性粒子的非弹性碰撞速率,以及电子能量和电子通量分布等。
The electron density, the electron -neutral inelastic collision rates, the electron energy and the electron flux distribution are calculated.
海洋粒子动力学:下沉速度,粒度分布,通量,和微生物降解率。
Marine particle dynamics: sinking velocities, size distributions, fluxes, and microbial degradation rates.
中子通量用伴随粒子法测定,并与反冲质子望远镜相比较,两种方法在1—2%的误差范围内一致。
The associated particle method was used to determine the absolute neutron flux and compared with the recoil proton telescope. The agreement between both methods appeared to be within 1—2%.
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.
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.
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