| 1. | Solar flares are perhaps the most complex phenomena observed on the sun .
太阳耀斑大概是在太阳上观测到的最复杂的现象。 |
| 2. | Detailed modelling shows that this energy is sufficient to supply the energy of flares .
详细的模型计算表明，这个能量足够供给耀斑所需的能量。 |
| 3. | Hours to days before the flare release, excess energy become stored in the magnetic field .
在耀斑释放前几小时至几天，多余的能量就在磁场中储存起来。 |
| 4. | In order for the preflare energy to be stored without premature release, the magnetic field configuration must be metastable .
为了使能量在耀斑爆发前储存起来，不致过早释放，磁场结构必须是亚稳定的。 |
| 5. | Solar flare is a violent solar activity
太阳耀斑是一种剧烈的太阳活动现象。 |
| 6. | Gps ; tec ; flare ; subionosphere point
Gps tec耀斑星下点 |
| 7. | What is a " solar flare "
什么是太阳耀斑？ |
| 8. | Solar flares are sudden and brief explosions that rip through our sun s atmosphere
耀斑是太阳大气层表面短暂的爆发现象。 |
| 9. | Origin of solar flares
太阳耀斑的由来 |
| 10. | There are tens of solar researchers who have studied the post flare loop
此外，我们还总结了前人对该耀斑后环的研究成果。 |
