| 1. | The corona gains and loses energy continuously .
日冕总是不断地获得能量和损失能量。 |
| 2. | The continuum of the corona is essentially radially polarized .
日冕连续区基本上是经向偏振。 |
| 3. | Looking at small details we find that the corona has a delicate structure .
仔细研究细节后，我们发现日冕有精细结构。 |
| 4. | The final speed of the solar wind depends mainly on the maximum temperature in the solar corona .
太阳风的最终速度主要取决于日冕中的最高温度。 |
| 5. | Much of visible light reaching us from the solar corona also seems to be due to scattering by electrons .
从日冕中射来的相当大一部分可见光看来也是由电子散射产生的。 |
| 6. | Acoustic waves are a primary candidate for supplying the energy necessary to heat the solar chromosphere and corona .
声波是供给太阳色球和日冕加热所需能量的主要候选能源。 |
| 7. | One other interesting aspect of the relation of coronal holes to the solar wind follows from the appearance of coronal holes at the poles .
日冕洞与太阳风的关系的另一个有趣的方面是日冕洞在两极的形状。 |
| 8. | The excess energy goes into creating and accelerating a high-speed solar wind that emanates primarily from the regions of the holes .
多余的能量用来产生并加速高速的太阳风，而太阳风主要发端于日冕洞区域。 |
| 9. | The gas pressure eventually overcomes the force of solar gravity and the corona inevitably expands into space as the solar wind .
这里的气体压强最终会超过太阳的引力作用，使日冕终于只好以太阳风的形式向空间膨胀。 |
| 10. | Trace , transition region and coronal trace
太阳过渡区和日冕 |
