Solar atmosphere and solar activities 太阳大气(SA)和太阳活动
Temperatures in the parts of the solar atmosphere are high enough to decompose nearly all molecules into atoms. 在太阳大气(SA)层的某些部分,温度高到足以使几乎全部分子都被还原为原子。
Corona : the outer solar atmosphere, can be extended to a number of solar diameter, or even farther. 日冕:太阳大气(SA)的最外层,可以延伸到几个太阳直径,甚至更远。
Following what exactly happens during a reconnection event requires, first off, a general understanding of how invisible magnetic loops can trap hot gas in the solar atmosphere. 想了解磁力线重连事件中究竟发生了些什麽事情,必须先对看不见的磁力环圈如何捕捉太阳大气(SA)里的热气有一些基本认识。
Solar magnetic field means the magnetic field in the solar atmosphere. 太阳磁场是指分布于太阳大气(SA)中的磁场。