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。
In this review the recent progresses in researches of Solar flare build-up through the interaction of coronal loops are discussed.
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.
娇小而微微泛黄的星云NGC 6729环绕在年轻变星南冕座R的周围。
The smaller yellowish nebula (NGC 6729) surrounds young variable star R Coronae Australis.
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