Deployment Schemes of Wireless Sensor Node For In-Situ Measurement of Planetary Surface Mars

Nilofar A. Shekh, J. Pabari
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Abstract

To extant the life on Mars, there are investigations assessing the past habitability potential. The evidence of the presence of water on the Mars identified by the detection of some minerals such as hematite and goethite. To study the properties of regolith for planetary surface for in situ measurement, it is necessary to deploy wireless sensor network on MARS surface. There is a challenging task to deploy the sensors on a planet like the MARS and it requires theoretical Perception before applying along any space mission, as it includes large amount of investment. In this paper, we have learned theoretical details involved in the deployment of sensors on the MARS. In this paper, we propose different sensor node deployment strategies for WSN for maximum coverage prediction. Our study also gives sensor fall time, Impact velocity, Number of sensors are used in topology, total pressure, coverage area, etc. Three schemes of deployment topologies have been also compared.
火星行星表面原位测量无线传感器节点部署方案
为了让火星上的生命存活下来,研究人员正在评估火星过去的可居住性。火星上存在水的证据是通过探测到一些矿物,如赤铁矿和针铁矿来确定的。为了研究行星表面风化层的性质并进行原位测量,有必要在火星表面部署无线传感器网络。在像火星这样的星球上部署传感器是一项具有挑战性的任务,在应用于任何太空任务之前,它需要理论感知,因为它需要大量的投资。在本文中,我们学习了在火星上部署传感器所涉及的理论细节。在本文中,我们提出了不同的传感器节点部署策略,以实现最大的覆盖预测。我们的研究还给出了传感器的下落时间、冲击速度、传感器的数量、拓扑结构、总压力、覆盖面积等。对三种部署拓扑方案进行了比较。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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