视差法 meaning in English
parallax method
Examples
- 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。