telescope mirror 中文意思是什麼

telescope mirror 解釋
望遠鏡的反射鏡
  • 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...
  • mirror : n. 1. 鏡；反射鏡。2. 反映；借鑒；榜樣。vt. 映，反射；反映。
  1. The mirror of an astronomical telescope forms at its focal point an image of a star on the axis of the mirror.

    天文望遠鏡把在鏡軸上的星體成象在焦點上。
  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. After measured the laser energy distribution of kunming slr station, the parameters of this non - gassian and non - spherical symmetric laser beam were deduced according to correlation definition. applying its laws and deduced laser beam parameters, the change of laser beam dirvergence angle was studied in detail when adjusts transmission system focus. moreover, calculation based on these measured data indicates that the laser shaded by the second mirror of telescope is amazingly up to 39. 8 %, an optical element was designed for the settlement and it worked satisfactorily when put it into practice

    之後測量了雲南天文臺激光的橫向能量分佈，根據相關定義確定了這束非高斯非球面激光的參數，應用它的傳輸變換規律和測量參數研究了調焦中激光發散角的變化，並根據測量數據計算出激光發射時副鏡擋光比例達到驚人的39 . 8 ，研製出光劈解決這一問題，取得了很好的效果。
  4. When i get into astronomy building, the astronomy equipments of inside, make me dim in vision and confused, getting into the first floor is an exhibition hall, there is various brief introduction concerning astronomy, get into second floor to have various of telescope concerning astronomy, see through a mirror etc. equipments, and the introduction of various horoscope

    11月10日10 : 57當我進入天文館，裏面的天文設備，讓我眼花繚亂，進入到第一層是一個展廳，有各種關于天文的簡介，進入到第二層有各種的關于天文的望遠鏡，透視鏡等設備，以及各種星座的介紹
  5. As long as it is smaller than your diagonal mirror, it will not affect your telescope ' s performance

    只要它比斜面鏡小一些就行，黑膠布也不會影響望遠鏡的性能。
  6. It is the first time to be brought out and designed that the solar x - euv imaging telescope integrates the grazing mirror and the normal incidence mirror. this design can fully meet the applied requirements according to simulation

    太陽x - euv成像望遠鏡在國際上首次提出並設計實現單臺設備集成掠入射望遠鏡和正入射望遠鏡系統，分析表明，該設計方式完全滿足應用要求。
  7. Point diffraction interferometer - a physical idea, is invented by smartt and strong in 1972, advanced by smartt and steel, and used to test astronomical telescope, it has simple structure and has not special demand to source. recently. with the development of fiber ' s manufacture and coupling technology. the simple modern fiber ' s center is smaller than before, this make it possible to progress fiber point diffraction interferometer ( pdi ), in addition to test convergent wavefront, it can test the reflective concave. the excellence of pdi is that it does not need standard mirror. in intereference testing, the standard mirror is the main reason which limit the improvement of precision, pdi can avoid difficulty to provide the wide future for high precision testing. pdi, which produce the standard sphere wavefront, is an instrument which realize the phase shifting with piezoelectric transducer ( pzt ), and collect the interferogram with ccd, in this paper, a adjusting methord is described, then data processing is obtained

    點衍射干涉儀這一物理思想，早在1972年smartt和strong就已發明，由smartt和steel做了進一步發展，並成功的用於檢測天文望遠鏡，它結構簡單，對光源沒有特殊要求，近年來，由於光纖製造工藝以及耦合技術的發展，單模光纖纖芯不斷縮小，為光纖點衍射干涉儀得以發展提供了前提條件，該干涉儀由激光照明，除了檢測會聚波前外，還可以用來檢測反射凹球面，進而應用到單個面形的檢測；另外，光纖點衍射干涉儀最大的優點是不需要標準鏡，在干涉檢測中，標準鏡是檢測精度受限的很大原因，光纖點衍射干涉儀能繞開這一難度，為進行高精度的光學檢測提供了廣闊的前景。
  8. Nowadays the light collected by the lens or mirror of a telescope is directed to a photographic plate rather than to the astronomer's eye.

    被望遠鏡的透鏡或反射鏡所收集的光線，如今直接射到照相底板上，而不是天文學家的眼睛里。
  9. 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。
  10. Thus, a telescope with larger collecting area, which usually means larger main mirror or lens, is more powerful. this is the main reason why we prefer large telescopes. large telescopes also improve the

    由於望遠鏡主鏡口徑越大，便意味著它的集光能力越強，即它的能力亦越強，難怪天文學家都是以大為美的傢伙。
  11. Monolithic - mirror telescope

    單鏡面望遠鏡
  12. As one of the most widely used of manufactured materials, and certainly the most versatile, it can be as imposing as a telescope mirror the width of a tennis court or as small and simple as a marble rolling across dirt

    作為一種最廣泛的使用是製造原料，並且的確十分萬能，它能夠像一個網球場寬的望遠鏡鏡片那樣壯觀，或像在地上滾的彈珠一樣小。
  13. 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 。
  14. Mmt, multiple - mirror telescope

    多鏡面望遠鏡
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