极光过程化动画及其关键帧动画优化

Tomokazu Ishikawa, Ryota Nakazato, I. Matsuda
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摘要

有许多关于视觉模拟的研究考虑了极光的特征运动。我们提出了一种以用户可视化的期望形式和期望位置生成极光动画的方法。本研究基于Kojima等人[5]提出的方法,该方法通过参数调整比较容易实现形状控制。利用这种方法,已经产生了一个由空间带电粒子流入点组成的人工二维分布极光模拟。极光的幕状运动可以通过在模拟空间内应用电磁场计算和流体计算的动力学模型来再现。我们可以看到,极光特定运动的再现取决于从各个流点流出的当前体积的初始值。通过这种方式,我们试图通过控制电流来控制想要的极光的形状。在本研究中,我们从实时捕获的极光视频中提取两帧,并通过三维再现各自的极光分布来设置极光的初始分布和目标分布。由于各自的分布特征是带电粒子在地面以上100公里处形成极光的流动极限,并且许多极光视频图像经常捕捉到地平线,因此我们将相机位置设置为原点,并计算极光最低部分的世界坐标。采用遗传算法对电流进行优化。我们将代价函数设为目标形状的电势与基于仿真结果的各流点坐标的电势之差。此外,减少了搜索参数的数量,假设流向各流点的电流分布随初始形状函数变化,将该函数展开为傅里叶级数,通过优化使一般形状控制成为可能。在未来的工作中,我们的目标是提高控制精度,并获得控制复杂形状的能力。
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Procedural Animation of Aurora and its Optimization for Keyframe Animation
There have been many studies regarding visual simulations that consider the characteristic movement of auroras. We have proposed a method of generating animation of auroras in the desired form and in the desired location visualized by the users. This study is based on the method proposed by Kojima et. al [5], in which shape control is performed comparatively easily through parameter adjustment. With this method, an artificial 2D distributed simulation of auroras, comprised of inflow points for charged particles flowing from space, has been produced. The curtain-shaped movement of auroras can be reproduced by applying a kinetic model using an electromagnetic field calculation and a fluid calculation within the simulation space. We can see that the reproduction of aurora-specific movement is dependent on the initial value of the current volume flowing from the various flow points. In this way, we attempted to control the shape of the desired aurora by controlling the current flow. In this study, we extracted two frames from the live-captured aurora video, and, set the initial distribution and target distribution of the aurora by reproducing the respective aurora distributions in 3D. As the respective distributions feature flow limits of charged particles forming an aurora 100 km above the ground, and many aurora video images often capture the horizon, we set the camera position as the point of origin and calculated the world coordinates for the lowest section of the aurora. A genetic algorithm was used to optimize the current flows. We set the cost function as the difference between the electric potential of the target shape and the electric potential based on the simulation results for the coordinates of each flow point. In addition, the number of searched parameters were reduced, assuming that the current distribution flowing to each flow point changes along with the initial shape functionally by expanding this function in a Fourier series, General shape control made possible through optimization. In the future works, we aim to increase control accuracy and gain the ability to control complex shapes.
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