x-ray telescope中文意思是什麼
x-ray telescope 的中文意思
【天文學】X射線望遠鏡。
x-ray telescope 例句
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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, " solarma x " e x amines 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。
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This great observatories view of the famous sombrero gala x y 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。
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Accordingly, hard x - ray modulation telescope ( h x mt ) 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。
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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
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Compared with the traditional nai scintillator probe, cd1 _ x zn x te 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。
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Of course, the ne x t 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 gala x ies space - based multi - band variable objects monitor
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This image combines data from four different observatories : the chandra x - ray observatory ( purple ) ; the gala x y evolution e x plorer 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) 。
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The space observation in soft x - ray and e x treme 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
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Beautiful hubble space telescope images are allowing astronomers to pick apart the comple x events at the hearts of gala x ies, 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。
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Nasa ' s three great observatories - - the hubble space telescope , the spitzer space telescope , and the chandra x - ray observatory - - joined forces to probe the e x panding remains of a supernovaNasa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。
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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 。
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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 62402002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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