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Home > english-chinese > "视差法" in Chinese

Chinese translation for "视差法"

parallax method

Related Translations:
长期视差:  secular parallax
地心视差:  diurnal parallaxgeocentric parallax
视差动:  parallactic motion
垂直视差:  elevation parallaxvertical parallax
月亮视差:  lunar parallax
相对视差:  relative parallax
远近视差:  near and far visual differenceperceptive parallaxperspective parallax
折射视差:  parallactic refraction
反视差:  [物理学] anti-parallax◇反视差镜 antiparallax mirror
纵视差:  vertical parallax
Example Sentences:
1.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。
2.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。
3.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。
4.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。
5.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。
6.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。
Similar Words:
"视差导线" Chinese translation, "视差的" Chinese translation, "视差动" Chinese translation, "视差读数" Chinese translation, "视差读数误差" Chinese translation, "视差法测距" Chinese translation, "视差方程" Chinese translation, "视差方向修正量计算器" Chinese translation, "视差改正量" Chinese translation, "视差杆" Chinese translation