暗暈 的英文怎麼說

中文拼音 [ànyūn]
暗暈 英文
dark halo
  • 暗 : Ⅰ形容詞1 （光線不足; 黑暗; 暗淡） dark; dim; dull 2 （不顯露的; 秘密的） hidden; secret 3 [書面語...
  • 暈 : 暈Ⅰ形容詞（頭腦發昏） dizzy; giddy; faint Ⅱ名詞[氣象學] （日光或月光形成的光圈） halo
  1. Since the scaling relation we found is intrinsic, this application is independant of how we define haloes, when we do observation and which cosmogony we choose

    另外我們發現：暗暈匯聚因子c的增長並不是簡單地正比于宇宙膨脹因子，而與質量吸積速率反相關。
  2. Containing privet essence, along with the heat of hot spring, it features favorable effect on curing liver and kidney deficiency, lumbar debility, dizziness, tinnitus, white hair and poor vision

    溫泉水中加入女貞子藥包，結合泉水的熱力作用，對肝腎陰虛、腰膝酸軟、頭暈、耳鳴、須發早白、目暗不明有一定療效。
  3. A wide halo of pearly light can be seen around the dark moon.

    可以看到一大片珍珠似的光暈圍繞著暗弱的月球。
  4. The halo of shadow outshines the holy light

    聖光不屬於我，透著暗影光暈才是最有自信的
  5. Shadowguard : this troll priest racial spell now works with vampiric embrace, blackout, and shadow weaving

    暗影守衛：巨魔牧師的種族法術現在可以影響到吸血鬼的擁抱、暈眩和暗影交織了。
  6. The hierarchical formation of dark matter halos cannot be described using simple mathematical relationships

    黑暗物質暈的階式結構無法以簡單的數學關系描述。
  7. Our results are much helpful for us to understand the building - up mechanism of the universal density profile, galaxy formation and high redshift tully - fisher relation

    這些結果對我們解釋暗暈的普適密度輪廓，高紅移盤星系的瓜111卜f討ler關系和理解星系核球及盤的形成都有很大幫助
  8. A prior investigation of fur farms in china showed workers attempting to stun foxes and raccoon dogs by slamming them against the ground or bashing their heads with clubs

    還有些暗訪活動向人們展示中國皮毛產業工人將狐貍打暈、用棍棒擊打浣熊頭部、在地上猛摔浣熊的場面。
  9. A possible approach for search of dark material halo in galaxy

    探尋銀暈暗物質的一個可能方案
  10. We find that within a given cosmological model different schemes of galaxy formation lead to significant changes of the pvd. we propose a simple phenomological model for the formation of lyman break galaxies, determined by the formation interval parameter z and the halo mass threshold mh

    首先，我們提出了一個簡單唯象模型來聯系宇宙學n體數值模擬和lymanbreak星系，該模型由兩個參量（形成時間間隔_ z和暗暈質量下限m _ h ）唯一確定。
  11. Then, we analyse in detail the mass - accretion histories and structural properties of dark haloes in high - resolution n - body simulations

    本文利用高解析度的n體數值模擬仔細分析了暗暈的質量吸積歷史和內部結構演化歷史。
  12. We model the density distribution in individual haloes using the nfw profile. for a given halo, there is a tight correlation between its inner scale radius rs and the mass within it

    我們運用nfw輪廓來擬合暗暈的密度分佈，進而發現：內部特徵半徑r _ s和其內質量m _ s的演化非常密切地相關。
  13. With a reasonable choice for these two parameters, our model predicts an occupation number distribution of galaxies in halos which agrees very well with the predictions of semi - analytical models

    通過適當選擇這兩個參量，模型預言的暗暈中星系的分佈函數和半解析模型的結果符合得非常好。
  14. These two phases are separated at a time when the halo concentration parameter c ~ 5 and the binding energy of the halo is approximately equal to that of a singular isothermal sphere with the same circular velocity

    腸『隨時間的增長和宇宙的膨脹速率基本一致: （ 2 ）在這兩個階段的分界點處暗暈的匯聚因子。
  15. Ms, for all its main progenitors, which is the basic reason why halo structural properties are closely related to their mass - accretion histories. this correlation can be used to predict the structural properties of a dark halo at any time in its history

    我們建立了模型，利用該相關關系和暗暈質量吸積歷史來預言其內部結構的演化，該方法無論從統計上還是對單個暗暈均達到了很高的精度。
  16. Haloes in the two accretion phases show systematically different properties, for example, the circular velocity vh increases rapidly with time and approximately equals the inner circular velocity vs in the fast accretion phase, but remain almost constant and less than vs in the slow accretion phase : the inner properties of a halo, such as rs and ms increase rapidly with time in the fast accretion phase but change only slowly in the slow accretion phase : the halo concentration changes slow in the fast accretion phase, but increases rapidly with the hubble expansion in the slow accretion phase. the inner structure and potential well associated with a halo is built up mainly in the fast accretion phase, while a large amount of mass can be accreted in the slow accretion phase without changing significantly the inner properties and the potential well

    ~ 4 ，其束縛能和具有相同圓周速度的等溫球大致相等; （ s ）在這兩個階段，暗暈的行為特徵迥異（例如，圓周速度均『在快速吸積階段增長迅速且略大於內部圓周速度: 、 ，而在緩慢吸積階段基本恆定甚至降低，且小於、 、 . : 、和呱在快速吸積階段增長迅猛，而在緩慢吸積階段增長滯緩） : （ l ）一個暗暈的內部結構和引力勢阱主要是在早期的快速吸積階段成長起來的，雖然在緩慢增長階段可以吸積大量的質量（超過10倍） ，但這並不顯著地改變其內部特徵和引力勢阱
  17. The build - up of dark haloes in cdm models generally consists of an early phase of fast accretion [ where the halo mass mh increases with time much faster than the expansion rate of the universe ] and a late phase of slow accretion [ where mh increases with time approximately the same as the expansion rate ]

    我們同時發現： （ 1 ）冷暗物質模型（ cdm ）中暗暈的成長均包括一個早期的快速吸積階段[暗暈質量m _ h隨時間的增長遠快于宇宙的膨脹速率和一個晚期的緩慢吸積階段
  18. Patients will feel in a sudden sensation of movement or spinning in the cases of the genuine vertigo the pseudo vertigo will affect balance and the patient fells dizzy when standing

    真性眩暈主要以旋轉感為主，亦有傾斜感、跌倒感；而假性眩暈則有不穩定感、浮遊感、搖擺感、或起立時眼前昏暗、或平衡障礙等眩暈感。
  19. The visible parts of galaxies are believed to be enveloped in giant “ halos ” of dark matter

    我們相信，星系中可以看得見的部分，其實是籠罩在巨大的黑暗物質暈里。
  20. I ' m talking about video games ; games like counter strike, diablo, smash brothers or halo

    我說的是電子游戲，像反恐精英、暗黑破壞神、任天堂明星大亂斗、光暈。
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