x-ray telescope 中文意思是什麼

x-ray telescope 解釋
【天文學】X射線望遠鏡。

  • x : X2＝ （羅馬數字）10 XX ＝ 20 IX ＝ 9 XV ＝ 15 XL ＝ 40 LX ＝ 60 XC ＝ 90 DXL ＝ 540 MX ＝ 1010 ＝...
  • 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 ...
  • telescope : n 1 望遠鏡。2 【天文學】遠鏡座。vi 嵌進，套疊；（列車等）相碰撞而嵌在一起。 The two cars collided...
  1. From the x - ray eyes of the trace satellite to the projected images on the floor of the solar telescope observatory at kitt peak in arizona, " solarmax " examines man s changing perception of the sun throughout time

    本片帶你從追號星的x -光眼，到利用位於亞里桑那州基特峰天文臺上的太陽望遠鏡觀看太陽，藉此探索人類從古至今對太陽觀點的改變。
  2. This great observatories view of the famous sombrero galaxy was made using nasa ' s chandra x - ray observatory, hubble space telescope and spitzer space telescope

    這張著名草帽星系的照片是nasa的錢德拉x射線天文臺、哈勃太空望遠鏡與斯必澤太空望遠鏡大這3架大天文臺所見的圖景。
  3. Accordingly, hard x - ray modulation telescope ( hxmt ) is a significant implement that will accelerate human ' s knowledge about the thermal radiation process of high - energy celestial bodies

    硬x射線調制望遠鏡hxmt正是推進人類對天體高能輻射過程的認識重要工具。
  4. The main research contents of the technical design include : analyzing the necessary parts of the solar x - euv telescope and the method of imaging x and euv ray ; developing the optic, electronic and mechanical design of this instrument ; computing solar x - euv imaging telescope ' s response to different temperature plasma, analyzing combination application of telescope filters for reconstructing the plasma paramaters and apprasing the telescope ' s response to the solar activities

    技術設計的主要內容包括：分析瞭望遠鏡的系統組成及成像方式選擇；完成太陽x - euv成像望遠鏡光學、電子學、機械等方面的技術設計：計算分析了太陽x - euv成像望遠鏡對不同溫度的等離子體響應、反演高低溫等離子體參數的最佳過濾片組合利用及望遠鏡對不同太陽活動現象的響應。
  5. Compared with the traditional nai scintillator probe, cd1 _ xznxte probe has higher detecting efficiency and power resolution, and can be widely used in fields such as security monitor, industrial flaw detection, medical diagnosis, celestial body x ray telescope and so on

    與傳統的碘化鈉閃爍體探頭相比， cdznte探頭具有很高的探測效率和能量解析度，可廣泛用於安檢、工業探傷、醫學診斷、天體x射線望遠鏡等方面。
  6. Of course, the next big step for chinese space astronomy would be to deploy a satellite dedicated only for astronomical research. there are currently a few projects in the planning stage, including a hard x - ray all - sky survey satellite the hard x - ray modulation telescope mission, and a " microsatellite " weight less than 100 kg mission to study long - term variability of stars and galaxies space - based multi - band variable objects monitor

    當然，下一步首先應是發射專門用作天文研究的衛星，目前有幾個計劃正處于策劃階段，包括建造一枚作硬x射線巡天觀測的衛星硬x射線調制望遠鏡， hxmt和一枚微型衛星重量不逾100公斤，來研究恆星和星系的長期變化空間變源監視器， svom 。
  7. This image combines data from four different observatories : the chandra x - ray observatory ( purple ) ; the galaxy evolution explorer satellite ( ultraviolet / blue ) ; the hubble space telescope ( visible / green ) ; the spitzer space telescope ( infrared / red )

    這張照片是使用4架軌道天文臺的數據合成的：錢德拉x射線天文臺（紫） 、星系演化探測器（紫外波段，藍色） 、哈勃太空望遠鏡（可見光波段，綠色）以及斯必澤太空望遠鏡（紅外波段，紅色） 。
  8. The space observation in soft x - ray and extreme ultraviolet ( euv ) region is an important portion of the space astronomy and an effective solar observation method developed increasingly. in this thesis we designed a euv multi spectrum space solar telescope ( eut ) based on the requirement of high angular resolution and wide field of view for solar observations ; investigated the transmission performance of eut ; invented a method of eut pointing calibration on the space orbit and solved the high precision pointing calibration problems ; constructed a prototype of 17. 1nm telescope, tested the possibility of eut design, and developed some cutting - edge techniques

    本文根據空間平臺上高解析度對日觀測的需要，設計出一種可以在四個極紫外波段對日同時成像多光譜太陽望遠鏡（ eut ） ；研究了極紫外（ euv ）波段太陽望遠鏡光學傳輸特性；提出了真空紫外波段在軌指向的標定方法，解決了高精度指向標定問題；研製出一臺17 . 1nm望遠鏡的地面樣機，驗證eut設計的可行性，攻克了部分關鍵的技術難關；為進一步的研究工作奠定了基礎。
  9. Beautiful hubble space telescope images are allowing astronomers to pick apart the complex events at the hearts of galaxies, the chandra x - ray observatory is peering into places hidden to hubble, and theorists are trying to make sense of it all

    藉由哈伯太空望遠鏡所攝得的清晰影像，天文學家得以發掘出那些暗藏在星系中心的復雜事件；錢卓x射線太空望遠鏡正窺視著哈伯所無法探知的區域，而理論學家也正試著弄懂它們。
  10. Nasa ' s three great observatories - - the hubble space telescope, the spitzer space telescope, and the chandra x - ray observatory - - joined forces to probe the expanding remains of a supernova

    Nasa的三架大天文臺，也就是哈勃太空望遠鏡、斯必澤太空望遠鏡以及錢德拉x射線天文臺聯合起來，探測著膨脹的超新星遺跡。
  11. In this paper, we mainly discuss multilayer mirrors for x - ray solar telescope operating at 17. 1nm wavelength. the diameter of primary mirror for telescope is 130 millimeters and secondary mirror is 66mm. especially, we will engage in controllation of uniformity of period thickness

    本文主要針對工作波長為17 . 1nm的x射線空間望遠鏡中的主鏡與次鏡的膜厚分佈均勻性進行控制，其中主鏡直徑為130mm ，曲率半徑為7 . 5m 。
  12. In 2002, based on the observation results from the chandra x - ray observatory and the hubble space telescope, astronomers employed computer to simulate the merging process of two supermassive black holes at the centre of ngc 6240

    2002年，天文學家結合了陳德拉x射線天文臺和哈勃太空望遠鏡的觀測結果，用電腦模擬出星系ngc 6240核心兩個超級黑洞融合的過程。
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