视差法的英文

• parallax method

• "视差"英文翻译    optical parallax; parallax e ...
• "法"英文翻译    law
• "视差法测距" 英文翻译 :    subtense method distance measurement
• "无视差法" 英文翻译 :    method of no-parallax
• "遮盖视差法" 英文翻译 :    screen parallax methods
• "横基尺视差法" 英文翻译 :    subtense method with horizontal staff
• "竖基尺视差法" 英文翻译 :    subtense method with vertical staff
• "时间基线视差法" 英文翻译 :    time－baseline parrallax method
• "差法" 英文翻译 :    lsd
• "视差" 英文翻译 :    [物理学] optical parallax; parallax error; parallax◇视差角 parallactic angle
• "倍差法" 英文翻译 :    difference-in-difference
• "变差法" 英文翻译 :    method of variable differences
• "动差法" 英文翻译 :    method of moments
• "方差法" 英文翻译 :    variance method
• "积差法" 英文翻译 :    product moment method
• "离差法" 英文翻译 :    departure method; deviation method
• "零差法" 英文翻译 :    zero balancing
• "落差法" 英文翻译 :    fall method
• "浓差法" 英文翻译 :    concentration difference method
• "平差法" 英文翻译 :    adjustment method; compensation method; consummation of errors; method of adjustment
• "时差法" 英文翻译 :    tofd
• "示差法" 英文翻译 :    differential method
• "试差法" 英文翻译 :    trial and error method; try and error method
• "外差法" 英文翻译 :    heterodyne method; heterodyne-beat method; process heterodyning; process of heterodyning
• "微差法" 英文翻译 :    differential process

• Although mercury has 13 or 14 transits every century , it was not a suitable candidate for either halley ' s parallax method or the variations devised by later astronomers
  水星虽然每百年会发生13 ~ 14次的凌日，但却不适用于哈雷的视差法或后来天文学家的其他改良方法。
• This is a simple method to measure the distances between us and nearby stars . however , we cannot measure many stars by this method because the angle is very small . for larger distances , we have to use other methods of measurement
  视差法是量度天体距离最简单的办法，但这个方法只适用于小部分的天体上，由于绝大部分天体距离地球实在太远，视差所造成的角度偏移根本小得难以量度。
• We analysis the factor has effect on the precision of locating in parallax . on basis of that , we present method to correct the parameters in parallax and to realize parallax by rolling the workpiece instead of moving workpiece
  为此，本课题首先通过射线数字成像来实现视差法，并且详细分析了视差法中影响定位精度的各个因素，找出了误差的来源及各种误差对定位精度的影响程度。
• To measure the distance of heavenly objects close to us , we can use a method called " parallax " , a simple visual phenomenon that was well understood by ancient greek more than two thousand years ago and was then used to estimate the earth s radius
  要量度邻近天体的距离，我们可采用视差法parallax 。古希腊天文学家在二千多年前已提出视差法的基本原理，并藉此测定地球的半径。
• The methods of location defects include : density method , stereo - scope observing , industrial ct and parallax . compared with other methods , parallax is widely applied for its convenience and strong applicability . parallax is also limited under some circumstances because of the low precision
  缺陷定位的方法主要有黑度法、体视法、工业ct及视差法等，其中视差法相对于其它几种方法，以其操作简便、适用范围广而得到了普遍应用。
• We have to use some other methods to measure the luminosity or equivalently the absolute magnitude of the cepheid variable . since we can readily measure the apparent magnitude of a cepheid variable , to measure the luminosity means measuring the distance . we use some distance measurement methods , for example , parallax , to determine the relation
  要弄清这个关系，我们要知道不同造父变星的光度和光变周期数据，量度光变周期当然不是问题，但要得知一颗恒星的光度，我们首先要得知它的距离，这时便须借助好像视差法等其他量度天体距离的方法。