星际云

网络释义：interstellar cloud; interstellar clouds; Nebula

网络释义

1.interstellar cloud射线(galactic cosmic rays)和星际云(interstellar clouds)的侵袭[02]。激波边界 (termination shock)[注：太阳风层(heliosphere)...

3.Nebula 云沃 yuwo 星际云 Nebula 【首选方案】多榕 Doright ...

1.And that our entire solar system appears to be moving into a dangerous interstellar energy cloud.而且我们的整个太阳系似乎正在进入一个危险的星际云能源。

2.This interstellar cloud is a wispy band of charged particles through which our solar system is slowly moving through.这星际云是通过它，我们的太阳系正慢慢移动的带电粒子的束状带。

3.As we have discussed in the last chapter, the density of a nebula is very low. And it contains mostly hydrogen.如上一章所述，这些星际云密度很低，成分主要是氢。

4.Barnard's markings are dark nebulae , interstellar clouds of obscuring gas and dust.巴纳德的标记黑暗星云，星际云掩盖气体和尘埃。

5.the magnetic lines of force are in effect glued to the interstellar gas , and they follow the clouds in their capricious motions.磁力线实际上是紧附在星际气体上，并跟随星际云一道作着变化莫测的运动。

6.Figure 2. 1 illustrates the departures of chemical composition from solar values for five different clouds projected against bright stars.图2.1揭示出五个不同的投影在亮星背景上的星际云的化学组成对太阳值的偏差。

7.Our Sun may exit the Local Interstellar Cloud, also called the Local Fluff, during the next 10, 000 years.我们的太阳可能在1万年内会脱离本地星际云，亦称本地纤流。

8.The slight change in density will trigger the contraction of the cloud by its own gravity. A sphere known as星际云中轻微的密度变化，皆会引致星云产生重力收缩，最后形成一个称为

9.Catastrophic ozone loss during passage of the Solar system through an interstellar cloud经由星际云太阳系统通道期间不幸臭氧损失