| 1. | The remnant nebular gas pervades the interplanetary space .
星云的残余气体充斥星际空间。 |
| 2. | Comprehensive studies on magnetic clouds in interplanetary space and their associated events
行星际磁云及其相关事件的综合研究 |
| 3. | The solar wind has its own magnetic field , which travels with the outflowing plasma into interplanetary space
太阳风有它自己的磁场，这个磁场会随著外流的太阳风电浆一起流入星际空间。 |
| 4. | The field that space environment contain is high - layer atmosphere , ionosphere , magnetic layer , interplanetary space and even sun
涵盖的区域包括地球高层大气、电离层、磁层、行星际空间直至太阳。 |
| 5. | A very small fraction of the sun ' s light and heat is emitted in such directions that after passing unhindered through interplanetary space , it hits the earth
只有很小一部分太阳的光和热由此方向释放出来，并且未被阻挡，穿越星空，来到地球。 |
| 6. | We are investigating the possibility of a commercial venture , where a solar sail would conduct station - keeping at points in interplanetary space that are useful for monitoring in the solar system
我们研究了一种商业风险的可行性，就是太阳帆能定点保持在太阳系内的某处，这对监测太阳系很有用。 |
| 7. | Such experiments , which would put the biological materials within simulated meteoritic materials and expose them to the environment of interplanetary space , could be conducted on the surface of the moon
这类实验要将生物体置入仿造的陨石物质内，并且暴露于行星际空间的环境，月球表面可充当试验场。 |
| 8. | When structures of cmes are traveling in the interplanetary space and towards to the earth , some galactic cosmic ray ( ocr ) may penetrate through the structures or be refracted by them before reaching the earth ' s surface
当行星际空间有cme朝向地球运动时，一部分银河宇宙线在穿过行星际空间时要穿过cme或遇到cme而折射到达地面，银河宇宙线的速度很高，它们比cme要提前到达地面。 |
| 9. | Solar wind flows out from the corona the sun s outer atmosphere into interplanetary space at speed of between 300 and 900 km per second . it causes fluctuation to the earth s magnetic field , which we call magnetic storm . such event will cause deflection of compass needles
而太阳风则以每秒300至900千米的速度由日冕太阳外大气层向外抛射，进入行星际空间，对地球磁场造成扰动而产生磁暴，导致指南针指针偏移，严重的话更会导致电力受阻和电话线路中断。 |
| 10. | More and more researches have shown that most of the intense geomagnetic storms are caused by fast coronal mass ejections in interplanetary space ( icmes ) . though the ace satellite can provide solar wind data in almost real time for prediction of geomagnetic storms , the time interval is too short ( shorter than 30 - min ) for effective predictions of major geomagnetic storms
位于拉格朗日点的ace卫星可以提供近实时的太阳风数据，但依据ace卫星太阳风数据进行地磁暴预报，时间的提前量非常有限，对于大地磁暴，这个时间提前量往往不超过30分钟，这样的时间提前量对于实际应用来说，是不能令人满意的。 |
