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摘要

在光传输渲染领域,有一种类型的光源在很大程度上仍未被探索,那就是由超光速粒子产生的光,这种现象通常被称为切伦科夫辐射[Č37]。通过重新利用Frank-Tamm方程[FT91]进行渲染,可以估计这些粒子的能量输出,并将其映射为光子,从而可以可视化该效应的明亮蓝光特征。本文扩展了一种随机递进光子映射器,并模拟了超光速粒子从靠近高折射率介质的源物体发射的过程。在实践中,光源被视为一种新的光源,使我们能够有效地重用现有的光子映射方法。CCS概念•计算方法→光线追踪;
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Photon Mapping Superluminal Particles
One type of light source that remains largely unexplored in the field of light transport rendering is the light generated by superluminal particles, a phenomenon more commonly known as Cherenkov radiation [Č37]. By re-purposing the Frank-Tamm equation [FT91] for rendering, the energy output of these particles can be estimated and consequently mapped to photons, making it possible to visualize the brilliant blue light characteristic of the effect. In this paper we extend a stochastic progressive photon mapper and simulate the emission of superluminal particles from a source object close to a medium with a high index of refraction. In practice, the source is treated as a new kind of light source, allowing us to efficiently reuse existing photon mapping methods. CCS Concepts • Computing methodologies → Ray tracing;
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