| 1. | The rest escapes as sound waves, mechanical vibrations that heat the chromosphere, the middle layer of the sun's atmosphere .
其余部分则以声波即机械振动的形式散逸，它们加热了太阳大气的中间一层，即色球层。 |
| 2. | There is no sharp break between the photosphere and the outer atmosphere of the sun on one side and the solar interior on the other .
无论在光球与它上面的太阳大气之间，或是在光球层与它下面的太阳本体之间，都没有明显的突变。 |
| 3. | It is a very thin layer 500km thick in the atmosphere of the sun
，这是太阳大气中非常薄的一层，厚度只有500公里。 |
| 4. | Is the outermost layer of the sun . similar to the chromosphere , usually it is only visible during total solar eclipse
是太阳大气的最外层，和色球层相类，亦是通常只能在日全食时才看得见。 |
| 5. | 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里的热气有一些基本认识。 |
| 6. | When you graduate from the academy , you will understand how the human body has adapted to ensure you can cope with elements such as gravity , the sun , the atmosphere , temperature extremes and processing the activities around you
当你从学院毕业时，便会明白人体是怎样应付地球各种环境元素如地心吸力太阳大气极端温度和处理你身边的活动。 |
| 7. | Investigators concluded decades ago that the generation of a voltage driving a simple , single current could not heat the solar atmosphere quickly enough or produce a flux of accelerated particles that is sufficient to make a flare
研究人员数十年前的结论认为，单单由电压驱动电流，无法很快加热太阳大气，或产生足以形成日焰的加速粒子流量。 |
| 8. | Based on the direct and scattering irradiance spectra measurements of ultraviolet waveband arrived at beijing ground surface by the sun - atmosphere ultraviolet spectrum radiometer ( sauvs ) , a method for retrieving the atmospheric aerosols optical depth ( aod ) is given in this paper
摘要利用太阳大气紫外光谱辐射计( sauvs ) ，测量到达北京地表的太阳直接和散射紫外光谱辐射，给出反演大气气溶胶光学厚度的一种方法。 |
