定性地探讨了该耀斑环内的宏观物质运动。
A qualitative approach to the macroscopic motion of matter of the flare loop is carried out.
结果还表明，耀斑环上升和重联点上升之间没有直接的联系。
Our results also indicate that there is no direct relation between the rises of soft X ray loops and the X point.
在观测上，无论在射电波段，或者X射线和光学波段的观测都提供了一些可靠的证据，说明耀斑冕环的相互作用可能导致耀斑的产生。
Observational data in the radio, X-ray and optical wavebands provide the reliable evidences that the interaction between flare coronal loops can lead to the onset of solar flares.
应用推荐