銀河宇宙線 的英文怎麼說

中文拼音 [yínhéyǔzhòuxiàn]
銀河宇宙線 英文
galactic cosmic rays
  • 銀 : Ⅰ名詞1 （金屬元素） silver （ag） 2 （姓氏） a surname Ⅱ形容詞1 （跟貨幣有關的） relating to curr...
  • 河 : 1 （天然的和人工的大水道） river 2 （指銀河系） the milky way system; the galaxy 3 （特指黃河） t...
  • 宇 : 名詞1. （房檐） eaves2. （房屋） house 3. （上下四方, 所有的空間; 世界） space; universe; world 4. （姓氏） a surname
  • 宙 : 名詞（指古往今來的時間） time （conceived as past, present and future）
  • 線 : 名詞1 （用絲、棉、金屬等製成的細長的東西） thread; string; wire 2 [數學] （一個點任意移動所構成的...
  • 銀河 : the milky way
  • 宇宙 : [天文學] universe; cosmos
  1. Washington ( reuters ) - a new space telescope that looks at the cosmos with infrared detectors has lifted the dust veils from newborn stars and a bumptious comet, and revealed the detail in the spiral arms of a neighboring galaxy

    華盛頓（路透社） - - -一種能通過紅外線觀測宇宙的新型太空望遠鏡已經揭開了覆蓋在一些新誕生的恆星和一顆（ ）彗星上的宇宙塵面紗，向我們顯示了一個鄰近銀河系的旋臂的詳細情況。
  2. Because catastrophic space weather events occur in general very suddenly, such as geomagnetic storms with sudden commencements. forbush decrease ( fds ) in ocrs intensity is also a kind of sudden event. the properties of these sudden events " are very evident

    山ttsh下降也是全球范圍內銀河宇宙線強度的突然下降，這是cme到達地球后對全球臺站記錄的宇宙線強度造成突然的影響，這些突發事件其突發特徵非常明顯。
  3. The rate of single event upset ( seu ) for space - based missions has been predicted by means of ground - based particle accelerator test and simulation calculation based on models of space radiation environment and the interaction of ions with the microelectronic device

    我們採用的方法是用地面重離子加速器模擬實驗和計算機模擬空間輻射環境進行單粒子翻轉率預估計算。引發單粒子翻轉的空間高能帶電粒子環境包括銀河宇宙線，太陽宇宙線和地球輻射帶中的高能質子及重離子。
  4. From time to time, the sun produces bursts of energetic ions and electrons ; furthermore, charged particles are a major component of the galactic cosmic radiation that constantly bombards our solar system

    太陽有時會爆發高能的離子與電子；再者，以帶電粒子為主成份的銀河宇宙射線，也會頻頻轟擊我們的太陽系。
  5. The results show that there are really obvious scintillation in gcrs intensity at the periods of 10 - 60 minutes as expected by many scientists, such as dorman, et al. then we analyzed the data observed at beijing snm between two solar cycles " transitional phases by using wavelet method

    我們還計算了幾個磁暴前銀河宇宙線強度的短周期的變化特徵，計算結果顯示，磁暴前銀河宇宙線強度在10 ? 60分鐘范圍內出現明顯的閃爍，這是磁暴前銀河宇宙線強度變化的的一種先兆特徵。
  6. Because ocrs " speed is very high, so they reach the earth ' s surface much earlier than the cmes

    銀河宇宙線穿過行星際空間到達地面時，它已經打上了「行星際環境的烙印」 。
  7. We also made a statistical study on precursors appeared in gcrs before major and large geomagnetic storms only by using the two cusp stations " nm data obtained at mcmurdo and thule

    對大磁暴前銀河宇宙線強度的變化和各向異性進行的統計分析分析表明，銀河宇宙線強度在磁暴前是有先兆的。
  8. The ocrs intensity with the periods of 32 - 64 hours increased remarkably for those events that ocrs intensity decreased before the geomagnetic storms, while the intensity of ocrs with the periods shorter than 24 - hour are not obvious

    對于磁暴前銀河宇宙線強度減弱的事件，如1982年7月事件，周期為32 ? ? 64小時的信號幅度有較明顯的增強，而周期低於24小時的信號變化非常不明顯。
  9. We still analyzed the time - frequency variation properties of the data before several selected geomagnetic storms. the result shows that the gcrs " intensity with period of 16 - 32 hours increased remarkably for those events that ocrs intensity increased before the geomagnetic storms

    對于磁暴前銀河宇宙線強度增強的事件，銀河宇宙線周期為16 ? ? 32小時的信號都有較明顯的增強，部分事件銀河宇宙線周期為兒個小時的信號也明顯提高（如1991年的事件） 。
  10. The cmes traveling in the interplanetary space may also affect the ocrs intensity suddenly, such as the cme in jan. 1997. comparison with the fds, the ocrs sudden variation degree is less remarkable and often is very weak, so it is usually not easy to find such kind of variation. by using wavelet method, for the first time we

    當cme在行星際空間傳播，還未到達地球時，在某一時刻cme有可能對地面某個、幾個臺站、或全球宇宙線強度造成突然的影響，從而使銀河宇宙線的強度發生突然的變化，但這種突變特徵往往是不明顯的，甚至根本看不出來，這時必須通過分析才能看出來。
  11. 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

    當行星際空間有cme朝向地球運動時，一部分銀河宇宙線在穿過行星際空間時要穿過cme或遇到cme而折射到達地面，銀河宇宙線的速度很高，它們比cme要提前到達地面。
  12. This paper analyzed the data obtained at mcmurdo and thule neutron monitor ( nm ) stations and at guangzhou muon monitor station during the cme event in march 1991. the results show that in this event when the cme structure passed the earth, it was shifted to the earth ' s southern hemisphere and the strongest magnetic structure associated with the cme passing the earth at about 2000ut, march 24. 1991

    我們利用mcmurdo和thule兩個臺站的銀河宇宙線強度的觀測數據和廣州多方向介子探測器記錄的宇宙線強度的數據分析了1991年3月cme的特徵，注意到cme是一定程度地偏向地球的南半球，並給出了cme中最強的磁場結構到達磁層的時間為1991年3月24日2000ut左右，這是過去沒有注意到的一個特徵。
  13. The results can show when the 24 - hour period of the gcrs disappeared and when they emerged again. we also analyzed the 27 - day periodicity of the gcrs " intensity

    分析結果可以看出銀河宇宙線強度的24小時周期和27天的周期何時消失，何時又重新出現。
  14. Though many results have been obtained so far, it is still in the research stage and far from being used in practical predictions

    磁暴前銀河宇宙線強度的譜分析主要還是採用最大熵方法和fourier方法，盡管得到不少結果，但離實際應用還是有一定的距離。
  15. It is the very reason that many scientists try to make the prediction of geomagnetic storms by analyzing gcrs variation properties before the commencement of a geomagnetic storm

    正是由於這個特性，國際上很多科學家試圖利用磁暴前銀河宇宙線強度變化的先兆特徵來進行地磁暴預報。
  16. This great debate was finally settled a few years ago by the almost simultaneous gamma - ray and optical observations of a few gamma - ray bursts. these observational data ruled out the galactic origin hypothesis and led to the definitive conclusion that gamma - ray bursts are coming from cosmological distances

    憑著差不多是同步的多波段觀測所得的數據，天文學家終能排除銀河系內發生的假說，確定伽瑪射線源於宇宙極深之處。
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