塵埃微粒 的英文怎麼說

中文拼音 [chénāiwéi]
塵埃微粒 英文
dirt particle
  • : 名詞1. (塵土) dust; dirt 2. (塵世) this world 3. [書面語] (蹤跡) trace; tracks 4. (姓氏) a surname
  • : Ⅰ名 (小圓珠形或小碎塊形物) small particles; grain; granule; pellet Ⅱ量詞(用於粒狀物)
  • 塵埃 : dirt; dust
  1. Edge of the granule image by video is the key of its image partition, the article tries to carry through a deeper research on image partition at the same time. granule is made up of savageness mater and industry material ( including of rock, sand, earth, atomy, steel, china, concrete, ink powder, magnetism powder, light fine and tiny powder used silicon, cell etc. )

    是構成天然物質和工業材料(巖石、礦石、沙子、泥土、、鋼鐵、陶瓷、水泥、墨粉、磁粉、光纖和料封裝材用高純硅粉、細胞等)的基本單元,顆尺寸(度)是顆的首要特徵和粉體材料的第一指標。
  2. Macrophages phagocytize foreign materials such as dust and carbon particles in the lung, as well as vital dye particles.

    巨噬細胞吞噬異物,如肺內的及碳,同樣還有活體染料的
  3. In many stellar disks, observers also have found the spectral signature of silicate emission, indicating that small dust grains on the disk surface have been strongly heated by the stellar radiation

    天文學家也發現了許多恆星氣盤具有矽的發射光譜,表示盤面上的已被恆星輻射強烈加熱。
  4. Dust tails are created when small particles from a comet are swept backward by the sun ' s radiation pressure

    來自彗星的子被太陽輻射壓向後推斥,形成尾。
  5. On this scale the moon would be scarcely more than a dust speck about 1cm from the sand grain.

    照這樣的比例尺度,月球將是僅離小沙一厘米遠的一顆塵埃微粒
  6. For a warm dusty plasma with variable dust charge, the modulational instability of the dust - acoustic waves can be described by the nonlinear schrodinger equation ( iut 4 - auxx + b | u | 2u = 0 ). it shows that the dust - acoustic wave is modulational stable in this dusty plasma. only the dark soliton exists in warm dusty plasma with variable dust charge

    通過約化攝動法,得到了描述塵埃微粒電荷可變的熱等離子體中聲波的非線性薛定諤方程( iu _ t + u _ ( xx ) + | u | ~ 2u = 0 ) ,不論是單離子溫度情形,還是兩離子溫度情形,塵埃微粒電荷可變的熱等離子體中的聲波是調制穩定的,僅存在暗孤子(包絡穴)
  7. The spitzer telescope shows microscopic dust particles ( colored red ) that have been heated by the supernova shock wave

    斯必澤望遠鏡的數據展現了超新星激波加熱過的(以紅色表示) 。
  8. Two years before, on january 2, 2004, stardust flew through the hail of rocks and dust that make up comet wild 2 ' s coma, collecting invaluable samples of cometary particles that will help scientists decipher the history of our solar system

    在兩年前, 2004年1月2日, 「星」飛越了由冰、石塊和構成的「懷爾特2 」彗星的彗發,收集無價的彗星樣本,這些樣品將幫助科學家解讀太陽系的歷史。
  9. As we know from how these rings scatter light, the particles are fine dust, typically microns in size, comparable to the size of smoke particles

    我們知道光如何由這一類行星環散射出來,由此可以推論,環內子是很小的,只有米大小,與一般煙差不多。
  10. For the following training tutorial, we have used tracks of extraterrestrial particles that were captured in the odce collector on the russian space station mir, and tracks of submicron dust particles shot into aerogel at 20 km / sec using a van der graaf dust accelerator in heidelberg, germany

    在隨后的培訓指南里,我們使用的軌跡是俄羅斯和平號空間站上的odce收集器捕獲的地外軌跡,和一些使用德國海德堡「范德夫岡」加速器以20千米/秒的速度射入氣凝膠的亞的軌跡。
  11. Standard practice for continuous sizing and counting of airborne particles in dust - controlled areas and clean rooms using instruments capable of detecting single sub - micrometre and larger particles

    使用能檢測單個亞測計及較大子的儀器在控制區域及無菌區中連續測定空氣中懸浮子的大小及計數
  12. But the stardust return capsule carried with it something else, even rarer and no less precious : tiny particles of interstellar dust that originate in distant stars, lightyears away

    然而星號的返回艙還攜帶有其他的東西,更為稀少的珍寶:源於遙遠恆星的星際塵埃微粒
  13. The numbers and amplitudes of both transimtted and reflected solitons from an incident soliton are given analytically for this case. if the interface of two kinds of dust grains is continuous, neglecting the reflection, the nonlinear dust - acoustic wave can be described by a kdv - type equation in the lowest order. the amplitudes, propagating velocities of these quasi - solitons for this case are also given analytically

    無論是分界面不連續變化還是連續變化,對于小的、但有限振幅的長波振動,電勢孤子從質量小的等離子體穿過分界面進入質量大的等離子體,電勢孤子的振幅將增大,速度將變快,反之,電勢孤子從由質量大的塵埃微粒組成的等離子體穿過分界面進入由質量小的塵埃微粒組成的等離子體,電勢孤子的振幅將減小,速度將減緩。
  14. This particle is so big that you can easily see it at the end of its track ; it is larger than we expect to see in the stardust interstellar dust collector

    這個相當的大,你能在它軌跡的末端清楚地看到它;它比我們期望在星際收集器中看到的要大得多。
  15. Q. why can ' t a computer program find the particles

    問:為什麼計算機程序不能發現塵埃微粒
  16. In the same way, under stable and dry conditions, dust particles suspended in the air are not easily dispersed, resulting in haze

    同樣,在大氣穩定而又乾燥的情況下,近地面的懸浮塵埃微粒不容易擴散,形成煙霞。
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