超低火星密度环境下生物启发拍打翅膀的实验力和变形测量。

Jesse L McCain, Jeremy A Pohly, Madhu K Sridhar, Chang-Kwon Kang, D Brian Landrum, Hikaru Aono
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摘要

火星飞行器可以为地面漫游车提供第三维空间,补充轨道观测站的不足,提供更详细的空中景观,并对火星大气层进行前所未有的勘测。然而,由于火星大气密度非常低,约为地球海平面密度的 1.3%,因此在火星上飞行非常困难。在低雷诺数环境中,传统飞机的效率会受到影响,而受昆虫启发的火星拍翼飞行器或许可以利用与地球上昆虫相同的升力增强效应。本研究调查了在超低密度火星大气中使用受生物启发的拍翼飞行器产生升力的可行性。受先前计算研究的启发,一个四翼原型被放置在大气舱中模拟火星密度。同时记录升力和机翼变形。在地球密度条件下,被动俯仰翼变形随拍打频率单调增加。另一方面,在火星密度环境中,被动俯仰偏转角度非常不稳定。测量到的升力在 16 赫兹时达到峰值,约为 8 克。这些测量结果表明,6 克重的拍翼飞行器可以产生足够的气动力在火星上悬停。此外,通过更好地了解超低火星密度条件下流体与结构的相互作用,有可能提高飞行器的性能。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Experimental Force and Deformation Measurements of Bioinspired Flapping Wings in Ultra-Low Martian Density Environment.

A Mars flight vehicle could provide a third-dimension for ground-based rovers and supplement orbital observation stations, providing a much more detailed aerial view of the landscape as well as unprecedented survey of the atmosphere of Mars. However, flight on Mars is a difficult proposition due to the very low atmospheric density, which is approximately 1.3% of sea level density on Earth. While traditional aircraft efficiency suffers in the low Reynolds number environment, insect inspired flapping wing flyers on Mars might be able to take advantage of the same lift enhancing effects as insects on Earth. The present work investigates the feasibility of using a bioinspired, flapping wing flight vehicle to produce lift in an ultra-low-density Martian atmosphere. A four-wing prototype, inspired by a prior computational study, was placed in an atmospheric chamber to simulate Martian density. Lift and wing deformation were simultaneously recorded. In Earth density conditions, the passive pitch wing deflection increased monotonically with flapping frequency. On the other hand, in the Martian density environment, the passive pitch deflection angles were very erratic. The measured lift peaked at around 8 grams at 16 Hz. These measurements suggest that sufficient aerodynamic forces for hover on Mars can be generated for a 6-gram flapping wing vehicle. Also, the performance can potentially be improved by better understanding the fluid-structure interaction in ultra-low Mars density condition.

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