望遠分光鏡 的英文怎麼說

中文拼音 [wàngyuǎnfēnguāngjìng]
望遠分光鏡 英文
telespectroscope
  • 望 : Ⅰ動詞1 （向遠處看） look over; gaze into the distance; look far into the distance 2 （探望） visi...
  • 遠 : Ⅰ形容詞1 （空間或時間的距離長） far; distant; remote 2 （血統關系疏遠） distant in relationship 3...
  • 分 : 分Ⅰ名詞1. （成分） component 2. （職責和權利的限度） what is within one's duty or rights Ⅱ同 「份」Ⅲ動詞[書面語] （料想） judge
  • 光 : Ⅰ名詞1 （照耀在物體上、使人能看見物體的一種物質） light; ray 2 （景物） scenery 3 （光彩; 榮譽） ...
  • 鏡 : Ⅰ名詞1 （鏡子） looking glass; mirror 2 （幫助視力或做光學實驗的器具） lens; glass 3 （姓氏） a s...
  • 望遠 : telescope objective
  1. So combine the item of “ space targets surveillance photoelectricity telescopes arrays system ”, this thesis does research in developing space targets visualization system. the main achievement in this thesis can be summarized as follows : 1. expatiate e the basic theory of satellite track dynamic, analyse the orbit characteristic of two - body problem and launch window, subastral point calculation, visibility and coverage analysis, two - line element sets

    本文結合「空間目標監視光電望遠鏡陣系統」課題，進行了空間目標可視化系統的設計和研究，主要作了以下幾方面的工作: 1 、闡述了衛星軌道動力學的基本原理，分析了二體軌道特性和發射窗口的基本特性，星下點軌跡計算、可見性和覆蓋分析和兩行根數。
  2. He identified some objects in the subaru deep field that were redder than the usual eros. the subaru deep field was taken in 1999 with the subaru telescope while aiming at a small patch of the sky in coma berenices and exposing for 1. 33 hours. having a 8. 2 metre mammoth mirror, the subaru telescope is located on the summit of the 4, 200 m mauna kea observatory in hawaii

    他從昴星望遠鏡於1999年對著后發座一小片星空曝光長達79分鐘所拍攝的星野照片subaru deep field或簡稱sdf中，找出四個比ero更紅的天體昴星望遠鏡口徑為8 . 2米，是日本最大的望遠鏡，位於夏威夷4 ， 200米高山上的莫納克亞天文臺內。
  3. To improve the method of adjusting the spectrometer

    分光計望遠鏡的分步快速調整
  4. Sst, spectroscopic survey telescope

    分光巡天望遠鏡
  5. The grism spectra, taken with hubble and analysed with software developed at the space telescope - european coordinating facility in munich, germany - can be obtained for objects that are significantly fainter than can be studied spectroscopically with any other current telescope

    「哈勃」所使用的棱柵以及由位於慕尼黑的空間望遠鏡歐洲合作機構開發的軟體，能夠獲取比其他現有望遠鏡上分光鏡能研究的暗得多的目標。
  6. To make full use of the karst formation in guizhou province of china, a large spherical radio telescope array of the arecibo telescope was proposed in china in 1995. therefore, a completely new design project that integrating mechatronics and optics technologies with several large span cables is proposed to drive the feed - supporting system to realize the high precision positioning. for the high requirement of trajectory tracking of the feed - supporting system with large span cables, the feasibility of stewart platform served as a fine - tuning platform and the accomplishment of the high precision tracking are considered in details in this paper

    本文依託新一代大射電望遠機電光一體化創新設計方案，針對饋源指向跟蹤系統高精度軌跡跟蹤要求，以精調stewart平臺為研究對象，進行了6自曲度並聯機器人的運動學優化設計、動力學分析與奇異性分析，設計了強魯棒性自抗擾控制器實現高精度軌跡跟蹤控制；提出了新一代大射電望遠鏡饋源指向跟蹤系統軌跡跟蹤獨立控制策略、軌跡規劃策略和控制模型； 50米縮比模型實驗驗證了軌跡跟蹤控制策略與方法的工程有效姓和可行性。
  7. The optimization theory, optimum dispersion value, dispersion direction and the factors affecting on the imaging quality of planar image in wavelength multiplexing optical fiber image transmission system was deeply and th eoretically analyzed as the emphases in this article, and at the same time through the development of true optical fiber image transmission system ( optical fiber periscope ), the studying of making the image quality optimization of optical fiber image transmission system being useable and been used in engineering was completed

    其中，重點對波分復用光纖傳像系統二維圖像的像質優化機理、最佳色散量與最佳色散方向的選擇，以及影響系統成像效果的各種主要因素進行了深入的理論分析；並結合實際光纖望遠系統? ?光纖潛望鏡的研製，完成了光纖傳像系統像質優化的實用化、工程化實現研究。
  8. As an example, polarization changes in vector gsm beams propagating through a telescopic system have been analyzed and illustrated by numerical results. it has been found that propagation - induced polarization changes are non - uniform across the beam cross - section. for the symmetric gaussian spectrum, the effect of the bandwidth on the polarization is barely noticeable

    以望遠鏡系統為例進行的數值分析表明，多色矢量gsm光束的偏振不再是均勻偏振，對源光譜為對稱分佈高斯型的多色矢量gsm光束，譜寬對光束偏振特性的影響不明顯。
  9. 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。
  10. Most objects in the sky are very dim. telescope effectively collects more light and converges it for our viewing

    夜空中大部分天體皆十分昏暗，望遠鏡能有效收集光線，讓我們可以看見更暗的天體。
  11. However, radio telescopes do have their own shortcoming. firstly, radio astronomical images are not as fascinating as optical images. moreover, they do not work like optical telescopes which can receive all visible wavelengths and then produce monochromatic signals by means of filters

    可是，射電天文望遠鏡也有它的缺點，首先射電天文圖像並沒有光學照片那麼具美感，而且它不像光學望遠鏡般，可以把可見光全部接收，然後加上濾色片分出單色光。
  12. This system can be used for ar, bs, high reflectance mirror, edge filter, bandpass filter, window for laser, telescope film etc

    已經在多家用戶成功應用於寬帶增透膜、分光膜、激光器窗口、望遠鏡紅膜等膜系監控。
  13. The optics of most telescopes are designed to produce images rather better than the anticipated seeing disk.

    大部分望遠鏡的光學設計都能得到比預期的視影圓面要好一些的象。
  14. The simulation program has been implemented to simulate the procedure of hxmt detecting x - ray source. the simulation result has been used to analyze the overlay region in celestial sphere, the variation of photon current intensity and the variation of the angle between sun and orbit, which demonstrate the reason why to select a 550 km height and 43o inclination low earth orbit as hxmt ' s orbit

    利用模擬程序，實現了模擬一個正在預研的天文衛星? ?硬x射線調制望遠鏡hxmt觀測x射線源的過程，分析了天球覆蓋、 hxmt接收的光子流強度的變化和太陽軌道面夾角的變化，說明了選取高度為550km ，傾角43o的近地圓軌道作為hxmt的運行軌道是合理的選擇。
  15. According to earth - bound and space - bound observations, the black drop is confirmed to be a mere optical illusion caused by the earth s atmospheric turbulence and insufficient resolution of small telescopes

    根據世界各地及衛星的觀測，黑滴現象是由於地球大氣層的擾動及部分望遠鏡的解像力不足而產生的光學假象，並非由金星的大氣層造成。
  16. A speedy stepped regulation method of telescope within spectrometer

    分光計實驗中望遠鏡和載物臺調整的一種快速方法
  17. 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。
  18. Using star testing astronomical telescopes as a guide, your telescope will perform to the best of it ' s abilities and perhaps it will show images better than you would have believed possible

    使用光軸矯正已經成為使用天文望遠鏡時必備的一本指南，這樣你就能了解你的望遠鏡是否充分發揮出它的性能。
  19. Telescopes - photometric parameters for observation telescopes and telescopic sights - part 1 : determination of veiling glare

    望遠鏡.觀察望遠鏡和望遠鏡描準具的光度參數.第1部分
  20. However, it is very pale and cannot be detected by ground based telescopes

    ，但它的光環十分暗淡，地面望遠鏡根本看不到。
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