角秒 的英文怎麼說

中文拼音 [jiǎomiǎo]
角秒 英文
second of arc
  • 角 : 角Ⅰ名詞1 （牛、羊、 鹿等頭上長出的堅硬的東西） horn 2 （古時軍中吹的樂器） bugle; horn 3 （形狀像...
  • 秒 : 量詞2 （時間計量單位） second （=1/60 of a minute）: 60 秒為1分。 sixty seconds make a minute 這...
  1. The c arm of the system can rotate at a very high speed, up to 25 degreessec. at the same time, an automatic patient safety detector allows the use of fast rotations and angulations with enhanced patient safety through non - contact detection. the sensing system adapts to the patient s size and will automatically slow down and stop moving when a patient gets too close

    系統的c臂可作高速運轉，達到每秒25度的轉動；診斷儀同時配備新式自動安全偵測儀，能以高速運轉及多角度拍攝影像而毋須接觸病人身體，它的自動感應系統會因應病人的體形，自動調節運轉的速度，一旦太接近病人時，便會減速或自動停止，保障病人的安全。
  2. As the aqueous humor was aspirated via a 26 - gauge needle through the peripheral clear cornea, the anterior chamber only showed little shallowness and regained the original volume again within several seconds

    我們從角膜邊緣用26號針頭抽取前房液的當時，發現前房深度雖曾略減，但在抽取后幾秒內就恢復了。
  3. Micro - arcsec astrometry

    微角秒天體測量
  4. Cannibalize ( undead racial ) - regeneration increased to 35 % of a character ' s total health over 10 seconds

    食屍（不死種族） -恢復率在10秒之內增加至角色血量總合的35 %
  5. Comparatively rudimentary interferometer observations suggested that this source is about 1. 5 across.

    不很精確的射電干涉儀觀測表明，這個源的角徑約為15弧秒。
  6. Technically, instead of using the traditional " four - time imaging " technology, fuji xerox s phaser color digital printer series makes use of new " once imaging " and enables it to process files three to seven times faster than traditional printers ; the printing of the first page takes only 18 seconds. the fuji xerox color digital laser printer equals spectacular printing effects and impressive speed

    從技術的角度看，與其他應用「四次成像」技術的彩色激光印表機不同，由富士施樂全新打造的phaser系列彩色激光印表機採用創新的「一次成像」列印技術，實現卓越的彩色列印速度，較其它同類彩色印表機快三到七倍，首頁輸出時間僅為18秒。
  7. Sub - arcsec radio astronomy

    亞角秒射電天文學
  8. It is demonstrated that the solution for 141 000 order normal equations for a simulated astro - geodetic network ( 47 057 points ) and a space one ( 476 points ) iterates 4 993 times to converge to 1 10 - 18 second, taking 28 min and 47 seconds, on a pii / 233 computer, showing over 40 times more efficiency, as compared with the coefficients unadjusted

    利用模擬的天文大地網（ 47057點）和空間網（ 476點）在pii / 233微機上解算14 . 1萬階方程組共迭代4993次（收斂至1 10 - 18角秒） ，花費機時28分47秒，與未進行系數調整相比，功效提高40多倍。
  9. Astrometric limit : the maximum residual in the place of a reference star, specified in arc seconds

    天文測量誤差極限：參考星位置對應的最大誤差，用角秒表示。
  10. If the angle p is one arc second, then we define the distance d to be one

    當偏移的角度為一角秒，星體與地球的距離即為天文學上所定義的一
  11. By that time, the apparent diameter of mars will be as large as 25. 1 arc seconds. shining at - 2. 9 magnitude, it will become the brightest star in the night sky for weeks

    那時火星視直徑達25 . 1角秒，光度達- 2 . 9等，成為當時夜空中最光亮的星。
  12. Gassendi estimated mercury ' s apparent diameter to be about 20 arc seconds ? that is, about 1 / 180 of a degree ? which was in itself a considerable scientific advance

    賈山迪估計水星的視直徑大約是20角秒（約是1度的1 / 180 ） ，這本身就是一大科學進展。
  13. Unfortunately, the results from the 1761 transit were not as good as expected : the measured values of the solar parallax ranged from 8. 3 to 10. 6 arc seconds

    不幸的是， 1761年凌日得到的觀測結果並不如預期的好：測量到的太陽視差范圍是8 . 3 ~ 10 . 6角秒。
  14. The note also provided columns of residuals of around one arcsecond, which adams listed to demonstrate that his theory was accounting for uranus ' s hitherto anomalous motion

    亞當斯還列出了幾行將近一角秒的殘差，證明他的理論可以解釋天王星直到當時都無法解釋的脫序運動。
  15. To measure this angle reasonably well, gp - b needed a fantastic precision of 0. 0005 arcseconds. it s like measuring the thickness of a sheet of paper held edge - on 160 km away

    要準確量度這角度，重力探測器b要達到0 . 0005角秒的精確度，精度要求相等於要量度出160公裡外一張紙張的厚度。
  16. Nasa s chandra x - ray observatory has changed this picture ; it provides the sub - arcsecond resolution equivalent to the spatial resolution of ground - based optical telescopes

    這個天文臺具備低於一角秒的解析度，精確程度足以和地面光學望遠鏡媲美，解決了一直以來對應天體證認困難的問題。
  17. According to calculations, the twisted space - time around earth should cause the axes of the gyros to drift merely 0. 041 arcseconds over a year. an arcsecond is 1 3600th of a degree

    根據運算，地球周圍扭曲的時空只會引致回轉儀轉軸每年漂移0 . 041角秒，一角秒為1度的3600分之一，可見程度之小。
  18. By this, the error of observation will be reduced. the precision requirement of angles measurement is 0. 1 arc second. angles measurement can be substituted by translation measurement between images in detectors

    根據觀測精度的要求這一夾角的測量精度必須控制在0 . 1角秒內，夾角測量可轉化為探測器上圖像平移量測量。
  19. The magnification of any telescope can be changed very easily by changing the eyepiece. even for the largest telescopes, the magnification is seldom over 500, usually between 100 - 200. thus, large telescopes do not magnify more, they only show brighter and sharper images

    其實大望遠鏡並不是把天體放得更大，而只是提供一個較光和較清晰的影像罷了倍率是物體視大小的放大比率，例如一個原本視角直徑為1角秒的物體，若放大后的視大小為30角秒，那麼倍率便是30倍。
  20. The sub - arcsecond spatial resolution of chandra, and xmm - newton s unrivaled sensitivity open a new area for the study of nearby galaxies ; many x - ray point sources are resolved without confusion and astronomers can study their x - ray properties such as timing behaviors and spectra in details

    錢德拉射線天文臺具備低於一角秒的解析度，而xmm -牛頓衛星的靈敏度更是無出其右，二者天衣無縫的配合，為研究這些天體的射線特性，例如光度變化和光譜等，開創一個全新的領域。
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