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Regolith Cohesion Measurement via Induced Electrostatic Lofting

机译:通过诱导的静电宽型凝固凝聚力测量

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Electrostatic dust lofting has been hypothesized to occur on airless bodies such as the Moon and asteroids, but in-situ evidence of this phenomenon has yet to be observed. Nonetheless, experiments and numerical models have provided insight into the fundamental physics of electrostatic dust mobilization. Prior to lofting, grains are bound tightly to the surface by cohesion, the dominant force for sub-mm particles. However, the magnitude of cohesion in regolith remains poorly constrained. We introduce the design of the Electrostatic Sample Collection and Cohesion Quantification (E-SACCQ) system, a technology that induces electrostatic dust lofting to measure regolith cohesion. E-SACCQ induces electrostatic lofting of charged regolith grains via a biased attractor plate and simultaneously images their size and trajectory. Since the local gravity is known and the electrostatic force on the regolith grains is controlled by the attractor plate potential, it is possible to solve for the cohesive force on the grains. Furthermore, the ability to induce electrostatic lofting may also provide a new method of dust removal from spacecraft surfaces and for sample collection on rubble pile asteroids, which may not have suitable, powdery surfaces for conventional scoop style collection methods. In this work, we discuss the preliminary design of the instrument. The feedback between the E-SACCQ electrode and the near-surface plasma environment is numerically modeled. Our models predict that solar wind bombardment will be a significant perturbation to the electric field between the surface and the electrode. The system's sensitivity to key design parameters such as attractor plate potential, size, and operating distance above the surface are also assessed. With respect to grain characterization and position tracking, stereo vision is selected as the preferred solution. Additional plasma simulation modeling and experimental demonstration is required to mature this technology.
机译:静电灰尘浮雕已经假设发生在诸如月球和小行星的无气体上,但原位证明这种现象的证据尚未观察到。尽管如此,实验和数值模型已经为静电粉尘动员的基本物理提供了深入了解。在升温之前,通过内聚力紧密地束缚晶粒,亚mm颗粒的主要力。然而,凝升性的内聚力的大小仍然受到严重的限制。我们介绍了静电样品收集和凝聚量化(E-SACCQ)系统的设计,这是一种诱导静电尘埃源的技术来测量凝固凝聚力。 E-SACCQ通过偏置的吸引板诱导带电的极孔晶粒的静电液位,并同时图像尺寸和轨迹。由于已知局部重力并且通过吸引板电位控制极血清晶粒上的静电力,因此可以解决晶粒上的内聚力。此外,诱导静电液位的能力还可以提供从航天器表面的灰尘去除的新方法,以及用于瓦砾桩小行星上的样品收集,这可能没有适合于传统的勺子风格收集方法的粉状表面。在这项工作中,我们讨论了仪器的初步设计。 E-SACCQ电极和近表面等离子体环境之间的反馈在数值上进行了模拟。我们的模型预测,太阳能轰击将是对表面和电极之间的电场的显着扰动。还评估了系统对关键设计参数的敏感性,例如吸引板电位,尺寸和表面上方的工作距离。关于晶粒表征和位置跟踪,选择立体视觉作为优选的溶液。需要额外的等离子体仿真建模和实验示范来成熟这项技术。

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