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Electrical discharges near the surface of Mars: Laboratory experiments and numerical modeling.

机译:火星表面附近的放电:实验室实验和数值模拟。

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摘要

Due to the prevalence of Martian dust devils and dust storms, an understanding of the underlying physics of electrical discharges in Martian dust is critical to future Mars exploratory missions. Mars' low atmospheric pressure and arid, windy climate provide an environment which supports triboelectric charging of dust. The turbulent motions of particles within a dust cloud cause individual dust particles to collide. This contact allows charge to be transferred between the grains. When the grains have identical compositions, the particle with the larger radius in the collision preferentially becomes positively charged. The upwinds within the dust cloud can then carry the lighter, negatively-charged particles to higher altitudes. The stratification of particle sizes causes an electric field to form. When the electric potential within the cloud exceeds the breakdown voltage of the surrounding atmosphere, a discharge occurs.; I have performed two laboratory experiments to examine the creation of electric fields and the subsequent discharges in a low-pressure CO 2 atmosphere. In both experiments, discharges have been visually and electronically detected, and measurements of their frequencies and intensities showed that triboelectric charging is a sufficient mechanism to promote strong electric fields. The range of pressures, horizontal wind speeds, and particle-size distributions required to efficiently produce these discharges have also been examined. These experiments demonstrate that electrical discharges can occur under conditions expected on the Martian surface.; Additionally, I have created a simple theoretical model to constrain the parameters involved in the dust charging experiments. This model supports the ideas developed in the experimental phase of this project.
机译:由于火星沙尘暴和沙尘暴的盛行,对火星尘埃中放电的基本物理学的理解对于未来的火星探索任务至关重要。火星的低气压和干旱多风的气候提供了一个支持粉尘摩擦带电的环境。尘埃云中颗粒的湍流导致单个尘埃颗粒碰撞。这种接触允许电荷在晶粒之间转移。当颗粒具有相同的组成时,在碰撞中具有较大半径的颗粒优先带正电。然后,尘埃云中的逆风可以将较轻的带负电荷的粒子带到更高的高度。粒度分层导致形成电场。当云中的电势超过周围大气的击穿电压时,就会发生放电。我进行了两个实验室实验,以检查电场的产生以及随后在低压CO 2气氛中的放电。在两个实验中,均已通过视觉和电子方式检测到放电,并且对其频率和强度的测量表明,摩擦带电是促进强电场的充分机制。还检查了有效产生这些放电所需的压力范围,水平风速和粒度分布。这些实验表明,在火星表面预期的条件下可能会发生放电。此外,我创建了一个简单的理论模型来约束粉尘装填实验中涉及的参数。该模型支持了该项目实验阶段提出的想法。

著录项

  • 作者

    Krauss, Corinne Evalta.;

  • 作者单位

    University of Colorado at Boulder.;

  • 授予单位 University of Colorado at Boulder.;
  • 学科 Physics Astronomy and Astrophysics.; Physics Electricity and Magnetism.
  • 学位 Ph.D.
  • 年度 2004
  • 页码 143 p.
  • 总页数 143
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 天文学;电磁学、电动力学;
  • 关键词

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