observed ray 中文意思是什麼

observed ray 解釋
觀測方向
  • observed : 觀測的
  • ray : n 雷〈姓氏，男子名， Raymond 的昵稱〉。n 1 光線，射線，熱線；〈詩〉光輝，閃爍，曙光，一線光明。2 ...
  1. The crystalline structure changes of pp induced by pan - milling were characterized by x - ray diffraction and raman spectroscopy. xrd analyses show that when pp was co - milled with uhmwpe, crystal transformation of pp occurred, its crystallinity and crystallite size decreased, whereas, only slight reduction of crystallinity and crystallite size were observed and no crystal transformation was found when pp was co - milled with wtr chips, and amorphization of pp was strongly enhanced by co - milling pp with iron

    採用x -射線衍射研究了聚丙烯碾磨粉碎過程微觀結構變化， uhmwpe存在下pp發生晶型轉變、結晶度降低和晶粒尺寸減小；彈性材料wtr抑制pp塑性變形，碾磨導致分子堆積有序區域膨脹，晶面間距增大，結晶度下降；剛性材料金屬鐵與pp產生強烈摩擦，加快晶粒細化，晶格破裂導致非晶化。
  2. The melted tungsten carbide would react with the steel matrix on the interface and the reaction zone was observed as a result. the reacting production was examined as fe3w3c by means of x - ray diffraction and scanning electron microscopy analysis. the reaction between tungsten particle and steel matrix could improve the interfacial bonding strength remarkably

    Wc鋼復合材料的制備過程中， wc顆粒在高溫下發生了局部溶解並在wc顆粒和鋼基體界面處發生了界面反應； x射線衍射和電子衍射花樣分析表明，反應產物為高穩定性的fe _ 3w _ 3c ，界面反應有效地改善了wc顆粒與鋼基體的界面結合。
  3. In order to discuss the friction and wear mechanisms of mos2 nanoparticles, it was analyzed that the chemical status of elements existed on the rubbed surface by x - ray photoelectron spectroscope, and it was observed that the surface topography of wear zone by scanning electron microscope

    通過x射線光電子能譜儀（ xps ）分析磨痕表面元素的化學狀態，掃描電子顯微鏡（ sem ）對磨痕的表面形貌進行分析，從而總結了納米二硫化鉬在n46機械油中的摩擦磨損機理。
  4. X - ray diffraction spectrum, empa methods and several tests including mechanical properties, electrochemistry, corrosion wear, on - site plate hanging, the microstructure of steel has been observed and analyzed, performance has been studied, and corrosion - abrasion, fragility mechanism, and microalloy application in ferritic stainless steel have been explored comprehensively. the test results of electrochemistry, corrosion wear and on - site plate hanging have been analyzed. the analytical result shows that crsomo has enough corrosion resistance in phosphoric acid slurry because it has high chromium and low carbon

    通過實驗室的電化學試驗、腐蝕磨損試驗和磷肥廠的現場掛片試驗結果分析，表明： cr30mo鐵素體不銹鋼高鉻低碳的配合，保證其在磷酸料漿中具有足夠的耐蝕性： cr30mo中（ fe ， cr ） _ 23c _ 6 、 （ fe ， cr ） _ 7c _ 3 、 mo _ 2c 、等碳化物硬質點從基體的彌散沉澱析出可提高鋼的硬度和耐磨性，使得鋼在磷酸料漿中具有良好的耐磨蝕效果。
  5. The surface morphologies of thin films were observed by using scan electron microscope ( sem ) and atomic force microscope ( afm ). based on grazing incidence x - ray diffraction ( gixrd ) equipment, we find that residual stress exist in magnetron sputtering plct film, in addition, the ferroelectric properties of plct thin films were measured by radiant premier lc type multifunctional ferroelectric properties test system

    利用廣角x射線衍射技術對不同濺射工藝下plct薄膜的相結構進行了研究;採用掃描電子顯微鏡（ sem ）和原子力顯微鏡（ afm ）分別觀察了薄膜的表面形貌;利用掠入射x射線衍射（ gixrd ）測量了薄膜的殘余應力。
  6. The morphologies of powder were observed by using high - resolution transmission electron microscopy ( hrtem ) ; x - ray diffraction ( xrd ) pattern was used to analyze the phases of the powder ; energy dispersive x - ray spectroscopy ( edx ) was used to analyze the component of composite powder

    用高分辨電鏡觀察復合粉體的形貌，進行電子衍射分析；用d / 3ax3b型x射線衍射儀作復合粉體的物相分析；用pv9900型能譜儀作復合粉末的成分分析。
  7. This star emits x - ray pulses with a period of 7. 47 s. from time to time, outbursts of low energy gamma - rays are also observed. hence, observational astronomers sometimes call this type of stars " soft gamma ray repeaters "

    這顆星以7 . 47秒的周期發放著x射線脈沖，並不時發射低能量伽瑪射線，因此，觀測天文學家有時稱這類星為繼發軟伽瑪射線源。
  8. The band was previously associated with f - type color centers and v - type color centers, as analyzed in x - ray irradiated ysz sample. however, the absorption band observed in our experiments has a shift towards the longer wavelength ( red shift ) as comparing with that in the x - ray or neutron irradiated ysz spectra. this shift may mainly due to large local distortions near the f - type centers and the v - type centers and the presence of multiple color centers

    本文通過光吸收、光熒光、 tem 、 xps測試及trim96計算分別研究了不同注量xe ~ +注入ysz前後光學性能和缺陷形態變化，以及ni ~ +注入對不同摻雜單晶al _ 2o _ 3結構和光學性能的影響，得到以下結果： （ 1 ） ysz注量達到10 ~ （ 16 ） cm ~ （ - 2 ）時，開始出現由f型和v型色心重疊而產生的吸收帶，與x射線、中子輻照相比，重離子輻照產生了更為復雜的缺陷復合體而導致吸收峰紅移。
  9. Most astronomers accept the binary spin - up scenario for creating millisecond pulsars because they have observed neutron stars speeding up in x - ray binary systems, and almost all radio millisecond pulsars are observed to be in binary systems

    多數天文家接受這個假想的模式，因為他們已經在x射線雙星系統中觀測到了中子星的加速現象，而且幾乎所有的毫秒脈沖星都被發現時處于雙星系統中。
  10. The films are developed and the degree of fogging observed is a measure of the gamma-ray exposure.

    經顯影之後，可以根據觀察到的模糊發黑程度來確定r射線的照射程度。
  11. The bastille - day flare of 14 july 2000, a great solar flare with x - ray / ha importance of x5. 7 / b3, was observed around 10 : 24 ut in the noaa 9077 ar at position n22w07. in this flare, very rich interesting radio bursts and fine radio spectral structures were detected, not only in metric wave band, but also in decimetric and microwave band ( 1. 0 - 7. 6 ghz by national astronomical observatories of chinese academy of sciences - naoc )

    2000年7月14日的太陽耀斑爆發? bastille事件，備受國際太陽物理學家關注，著名的sci刊物「 solarphysics 」特出版專輯研討該事件，從光球、色球、日冕、直至日地空間的廣闊空間尺度范圍內，對該事件的觀測資料進行了分析和理論研究。
  12. Such sources are believed to be either quark stars or neutron stars, and a subclass of these are already observed by conventional means as pulsars or x - ray emitting celestial objects

    一般認為這些信號源就是夸克星或中子星，其中一些已經通過傳統的方法觀測到，稱為脈沖星。
  13. The morphology of powders is observed, with scanning electron microscopy ( sem ) and transmission electron microscopy ( tem ). x - ray diffraction ( xrd ) pattern is used to analyze the phase of the composite powders. the copper nanoparticles / paraffin thermosensitive composite materials are obtained by the compress moulding

    用掃描電鏡（ sem ）對復合顆粒的表面形貌進行觀察，分析顆粒的粒度、團聚情況等，用透射電鏡（ tem ）觀察分析了復合顆粒中銅的形貌、粒徑及復合顆粒的精細結構， x射線衍射（ xrd ）分析復合顆粒物相組成。
  14. The samples were characterized by x - ray diffraction ( xrd ), optical spectroscopy, transmission electron microscopy ( tem ) and scanning tunneling microscopy ( stm ). as a result, a self - assembled monolayer ( sam ) of msa on the surface of fee au particles was directly observed in atomic level

    在此基礎上，對金納米粒子和其自組織結晶體進行了一系列的x射線衍射儀（ xrd ） 、透射式電子顯微鏡（ tem ） 、光吸收譜和掃描隧道顯微鏡（ stm ）的檢測和分析。
  15. The centre of ngc 6240 as observed by the chandra x - ray observatory

    利用陳德拉x射線天文臺所觀測得的ngc 6240星系中心。
  16. Abstract : the microstructure of as - cast high cr injection micro - alloying martensitic cast iron and the substructure of martensite in it have been observed under sem and tem. the alloying element distribution related to phase formation, as well as the various types of branch and distortion of carbide in the martensitic cast iron have been explored by using x - ray diffraction and electron probe analysis

    文摘:應用掃描電鏡和透射電鏡研究了噴射微合金化的鑄態馬氏體高鉻鑄鐵顯微組織及馬氏體的亞結構，並藉助x射線衍射與電子探針分析探討了合金元素的分佈與相形成的關系，以及碳化物的不同形式分枝與畸變。
  17. I am not joking. the five pictures look so different because they are observed at different wavelengths, namely, in optical, ultraviolet, x - ray, far infrared and radio wave respectively

    我不是在開玩笑，這五張照片看來完全不同，是因為它們是以不同波段拍攝，分別是可見光紫外線x射線遠紅外線和無線電波。
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