Inverse Square Law, Light反平方定律,光
As one of the fields which obey the general inverse square law, the light from a point source can be put in the form 作为遵循一般反平方定律的场之一,点光源发出的光可以表示为
![]() where E is called illuminance and I is called pointance. 其中 E 称为光照度,I 称为点照度。
The source is described by a general "source strength" S because there are many ways to characterize a light source - by power in watts, power in the visible range, power factored by the eye's sensitivity, etc. For any such description of the source, if you have determined the amount of light per unit area reaching 1 meter, then it will be one fourth as much at 2 meters. 光源由一般的“源强度”S来描述,因为有多种方式可以表征光源——以瓦特功率、可见光范围内的功率、考虑人眼灵敏度后的功率等。对于任何这样的光源描述,如果你已经确定了每单位面积到达1米处的光量,那么在2米处就会减少到四分之一。
The fact that light from a point source obeys the inverse square law is used to advantage in measuring astronomical distances. If you have a source of known intrinsic brightness, then it can be used to measure its distance from the Earth by the "standard candle" approach. 光从点光源遵循平方反比定律的特性被用来测量天体距离。如果你有一个已知的固有亮度的光源,就可以通过‘标准烛光’方法来测量它与地球的距离。
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Index Photometry concepts Vision concepts 索引 光度学概念 视觉概念 | |||||
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