collisionless plasma

基本解釋

The process of magnetic reconnection in the collisionless plasma and distributions of particles in different positions are studied based on two-dimensional particle simulation.
利用二維全粒子模擬方法研究了無(wú)碰撞等離子體中的磁場(chǎng)重聯(lián)過(guò)程，得到了不同區(qū)域的離子和電子速度分布。
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.
太陽(yáng)風(fēng)的漲落在磁層頂激發(fā)壓縮阿爾文波，并在磁尾的無(wú)碰撞等離子體中傳播。