First a Gauss sphere is defined for the modeling of the scene, which is divided into patches uniformly.
此算法将一单位球定义为高斯球，并按一定的规则对其进行层次分割。
Using the Gauss-Bonnet theorem, Stephen Hawking proved that the topology of the event horizon of a (four dimensional) black hole is a 2-sphere.
使用高斯-博内定理， 史蒂芬· 霍金证明一个（四维）黑洞活动视界的拓扑结构是2个球体。
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