English translation for "视差法"
|
- parallax method
Related Translations:
地心视差: diurnal parallaxgeocentric parallax 垂直视差: elevation parallaxvertical 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
- 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" English translation, "视差的" English translation, "视差动" English translation, "视差读数" English translation, "视差读数误差" English translation, "视差法测距" English translation, "视差方程" English translation, "视差方向修正量计算器" English translation, "视差改正量" English translation, "视差杆" English translation
|
|
|