您要查找的是不是：
- The mass-loss includes the light radiation and solar wind. 太陽(yáng)質(zhì)量損失包括光子輻射和太陽(yáng)風(fēng)造成的質(zhì)量損失。
- The flaglike object on a pole is a solar wind experiment. 一根桿上的旗形物是太陽(yáng)風(fēng)儀器。
- The solar wind protons must sputter away the surface atoms of the dust. 大陽(yáng)噴射出耀眼的光芒。
- The sun blasts something called the solar wind at the earth all the time. 太陽(yáng)無(wú)時(shí)無(wú)刻向地球爆發(fā)一些所謂的太陽(yáng)風(fēng)。
- The Impact of Solar Winds on Navigation Aids. 太陽(yáng)風(fēng)對導航輔助設備的影響。
- The solar wind does not impinge directly on the earth and its atmosphere, however. 太陽(yáng)風(fēng)一直向外吹，直到碰到星際中的離子或電中性氣體。
- Astronomers have another reason for studying the solar wind besides wanting to understand its influence on the earth. 天文學(xué)家研究太陽(yáng)風(fēng)，除了希望了解太陽(yáng)風(fēng)對地球的影響外，還有一些別的動(dòng)機。
- The solar wind has its own magnetic field, which travels with the outflowing plasma into interplanetary space. 太陽(yáng)風(fēng)有它自己的磁場(chǎng)，這個(gè)磁場(chǎng)會(huì )隨著(zhù)外流的太陽(yáng)風(fēng)電漿一起流入星際空間。
- A continuous stream of charged particles, called the solar wind, impinges on the earth's magnetosphere. 稱(chēng)作太陽(yáng)風(fēng)的連續帶電子流撞擊在地球的磁層上。
- The final speed of the solar wind depends mainly on the maximum temperature in the solar corona. 太陽(yáng)風(fēng)的最終速度主要取決于日冕中的最高溫度。
- The gas pressure eventually overcomes the force of solar gravity and the corona inevitably expands into space as the solar wind. 這里的氣體壓強最終會(huì )超過(guò)太陽(yáng)的引力作用，使日冕終于只好以太陽(yáng)風(fēng)的形式向空間膨脹。
- What ACE detected was a violent gust of "solar wind", the constant flow of charged particles from the sun. ACE探測到的是一股兇猛的“太陽(yáng)風(fēng)”，即不斷從太陽(yáng)中流出的帶電粒子。
- One other interesting aspect of the relation of coronal holes to the solar wind follows from the appearance of coronal holes at the poles. 日冕洞與太陽(yáng)風(fēng)的關(guān)系的另一個(gè)有趣的方面是日冕洞在兩極的形狀。
- The solar wind grossly distorts the earth's magnetic fields, dragging it out to a long tail. 太陽(yáng)風(fēng)使地球磁場(chǎng)的形狀發(fā)生很大的變化,將它向外牽拉,扯出一條長(cháng)尾。
- As the solar wind carries ionized particles from the sun, they form a charged layer around the earth, called the ionosphere. 這個(gè)紐帶是通過(guò)地球的導電的區域來(lái)實(shí)現的，就象太陽(yáng)風(fēng)從太陽(yáng)帶來(lái)大量的電離粒子，它們形成了一個(gè)非?；钴S的層包饒在地球外面，被稱(chēng)之為電離層。
- This energy involves tons of charged particles, hurl ed our way in the so-called solar wind. 這種能量包括數以萬(wàn)計的帶電粒子，即所謂的太陽(yáng)風(fēng)襲擊我們。
- The transfer of magnetic energy from the solar wind radically alters the shape of the magnetosphere. 從太陽(yáng)風(fēng)傳來(lái)的磁場(chǎng)能量，徹底改變了磁層形狀。
- Shielded from the buffeting of the solar wind, ions quietly leak out of the atmosphere. 在那里沒(méi)有來(lái)自于太陽(yáng)風(fēng)的沖擊，離子則安靜地泄漏出大氣層。
- The magnetosphere is a bubble of magnetism that surrounds earth and protects us from solar wind. 磁氣圈是一個(gè)包裹著(zhù)地球的磁性泡泡，保護著(zhù)我們免受太陽(yáng)風(fēng)的吹襲。
- How can so much be compressed into one day? 這么多的東西怎么能壓縮在一天之內看完呢？
