In this review the recent progresses in researches of Solar flare build-up through the interaction of coronal loops are discussed.
本文讨论近年来在通过冕环相互作用而形成太阳耀斑的研究上所取得的进展。
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.
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。
In this paper, whether the steady high-speed siphon flow exists in coronal magnetic loops is discussed.
本文讨论了日冕磁环中是否存在定常的高速虹吸流动的问题。
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