将此图像复制到现有图像中后,通过使用一条简单的指定为从图像的中心(所有分区半径相交的位置)开始的填充命令,径向分区半径将被渲染成白色。
After copying this onto the existing image, the radial divisor arms are colored white with a simple fill command specified to begin at the center of the image, where all of the divisor arms meet.
举例来说当我们讨论径向概率分布时,距离原子核最可能的半径是,比s轨道半径,更近的可以离原子核有多近。
For example, when we're talking about radial probability distributions, the most probable radius is closer into the nucleus than it is for the s orbital.
基于径向半径偶次幂级数的相对畸变表达式在相机校准中被广泛地采用。
The expression of relative distortion based on even-power series of a radial radius is commonly used in camera calibration.
We can graph out what this is where we're graphing the radial probability density as a function of the radius.
我们可以,画出它来,这是径向概率密度,作为半径的一个函数图。
So what we're graphing here is the radius as a function of radial probability.
我们要画的是径向概率,作为半径的函数分布。
We'll start with talking about the shape, just like we did with the s orbitals, and then move on to those radial probability distributions and compare the radial probability at different radius for p orbital versus an s orbital.
想我们对待s轨道那样,我们先讨论p轨道的形状,然后是径向概率密度分布,并且把s轨道和p轨道在,不同半径处的径向概率做一个比较。
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