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