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Ultrasonic/sonic drilling/coring (USDC) for planetary applications

机译:适用于行星应用的超声波/超声波钻孔/取芯(USDC)

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Future NASA exploration missions are increasingly seeking to conduct sampling, in-situ analysis and possibly return samples to Earth for further tests. Missions to Mars are the more near term projects that are seeking such capabilities. One of the major limitations of sampling on Mars and other low gravity environments is the need for high axial force when using conventional drilling. To address this limitation an ultrasonic/sonic drilling/coring (USDC) mechanism has been developed that employs an ultrasonic horn driven by a piezoelectric stack. The horn drives a free mass that resonates between the horn and drill stem. Tests have shown that the USDC addresses some of the key challenges to the NASA sampling objectives. The USDC is lightweight (450 g), requires low preload (< 5N) and can be driven at low power (5W). The device has been shown to drill rocks with various levels of hardness including granite, diorite, basalt and limestone. The hammering action involved with the coring process can produce cores of various shapes, which need not necessarily be round. Because it is driven by piezoelectric ceramics, the USDC is highly tolerant to changes in its operating environment. These actuation materials can be designed to operate at a wide range of temperatures including those expected on Mars and Venus. Although the drill is driven electrically at 20 kHz, a substantial sub-harmonic acoustic component is found that is crucial to drilling performance. An analytical model has been developed to explain this low frequency coupling in the hom, free mass, drill stem and rock.
机译:未来的NASA探索任务越来越多地寻求进行采样,原位分析,并可能将样品返回地球进行进一步测试。火星任务是寻求此类能力的近期项目。在火星和其他低重力环境下进行采样的主要限制之一是在使用常规钻探时需要较高的轴向力。为了解决该限制,已经开发了采用由压电叠层驱动的超声变幅杆的超声/超声钻孔/取芯(USDC)机构。变幅杆驱动自由质量,在变幅杆和钻杆之间产生共振。测试表明,USDC解决了NASA抽样目标面临的一些关键挑战。 USDC重量很轻(450 g),要求低预载(<5N),并且可以低功率(5W)驱动。该设备已显示出可钻各种硬度等级的岩石,包括花岗岩,闪长岩,玄武岩和石灰石。取芯过程中涉及的锤击动作可产生各种形状的芯,这些芯不必一定是圆形的。由于它是由压电陶瓷驱动的,因此USDC可以高度耐受其工作环境的变化。这些驱动材料可以设计为在很宽的温度范围内运行,包括火星和金星所预期的温度。尽管电钻以20 kHz的频率驱动,但发现对次谐波性能至关重要的次谐波声分量很大。已经开发出一种解析模型来解释这种在hom,自由质量,钻杆和岩石中的低频耦合。

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