相关实验视频
Updated: Jul 29, 2025

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Visualization of High Speed Liquid Jet Impaction on a Moving Surface
Published on: April 17, 2015
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从冲击加速接口喷射出的螺旋环的和
Michael J Wadas1, Loc H Khieu1, Griffin S Cearley1
1University of Michigan, Ann Arbor, Michigan 48109, USA.
Physical review letters
|May 27, 2023
概括
冲击加速的流动会产生环,从天体物理学到聚变能量都可以观察到. 这项研究将环理论扩展到复杂的多流体场景,解释观察到的流动模式.
科学领域:
- 流体动力学 流体动力学
- 天体物理学 天体物理学
- 在惯性封闭的核聚变中.
背景情况:
- 环结构在各种科学领域的冲击加速流中被观察到.
- 了解这些现象对于从推进到融合能源的应用至关重要.
研究的目的:
- 为了将经典的环理论扩展到可压缩的多流体流.
- 为了解释在冲击加速流中观察到的环的形态差异.
主要方法:
- 构建常规环与由冲击突起相互作用产生的环之间的类比.
- 将恒定密度环理论应用于可压缩的多流体动力学.
主要成果:
- 成功地将环理论扩展到可压缩的多流体流.
- 证明了旋环和度,突起面积比增加.
- 提供了对环中观察到的形态变异的解释.
结论:
- 扩展理论准确地描述了环形成和复杂流动模式中的行为.
- 环和是影响流体形态的一个关键因素.
- 这项工作将基本流体动力学与高能量密度物理学中的实际应用联系起来.
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