coronal heating meaning in Chinese

日冕加热

As one of the major problems in solar - terrestrial physics , coronal heating has kept to attract physicists " attention for a few decades
近半个多世纪以来，日冕加热问题一直都是日地物理学界关注研究的难题。
In this thesis , we investigate the role of alfven wave in the coronal heating process . all the work consists of two main parts
我们从两个方面对这个问题进行了探讨：第一个方面主要地研究了加热日冕的alfven波源。
Then , torsional alfven waves propagate upwards along the coronal loop and the carried wave energy can make a play in coronal heating
当被激发的扭转alfven波沿着磁通管向上传播到达日冕，其携带的能量就可以加热日冕。
And consequently , the phase modulation dissipation arises from the strong phase mixing between the waves inside and outside the modulation layer , and the pump wave is strongly damped near the resonant layer of coronal loop . after above analytical theories , we combine the two part of work into an integrated model of coronal heating
由于位于共振层附近的相调层非常薄，那么，对应的位于这个薄层之内的pump波就会和在这个薄层之外传播的pump波有强烈的相混作用，从而对共振层附近的pump波有很强的阻尼作用。