T. Li, L.W. Zhang, H. Li, Q. Wang, X. Song, H.F. Liu, L. Tu
{"title":"月球任务用MEMS重力仪的设计与仿真","authors":"T. Li, L.W. Zhang, H. Li, Q. Wang, X. Song, H.F. Liu, L. Tu","doi":"10.1109/IMCCC.2018.00232","DOIUrl":null,"url":null,"abstract":"Lunar gravity filed determines the optimization design of lunar orbiters and selections for landing sites. Direct gravity measurement by deploying high-resolution gravimeter is the only option for obtaining precise local gravity data rather than the satellite gravity survey. However, there are both light-weight and shock-resistance demands for payloads of lunar landers. Therefore, this paper proposes a Micro-Electromechanical-Systems (MEMS) based gravimeter for lunar gravity survey, taking the advantages of both light and robust. The basis of this MEMS lunar gravimeter is: a silicon-based spring-mass system performs as the gravity-sensitive element. When gravity varies with locations or time, the spring length will change and so the displacement of mass. Using the optical displacement measurement technology, the gravitational acceleration can be worked out. The gravity-sensitive element requires both an extremely low fundamental frequency for a higher sensitivity and lower noise floor and large spurious resonant frequencies for low cross-sensitivities. Shock-resistance structures are required for robustness of the gravimeter. According to the above design rationales, the gravity-sensitive element is designed and the finite element analysis software COMSOL has been used to simulate the vibration modes of the spring-mass system with the beam width varying from 20µm to 30µm. The gravimeter design with a beam width of 24µm has a fundamental frequency of 5Hz. The mechanical thermal noise can be worked out as 0.3µGal/Hz1/2 under the room temperature and atmosphere with a quality factor of 200. The equivalent noise of the optical displacement transducer is 10µGal/Hz1/2. Hence, the overall noise floor of the MEMS lunar gravimeter is 10µGal/Hz1/2, which can meet the requirement of precise measurement of lunar gravity field.","PeriodicalId":328754,"journal":{"name":"2018 Eighth International Conference on Instrumentation & Measurement, Computer, Communication and Control (IMCCC)","volume":"12 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2018-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Design and Simulation of a MEMS Gravimeter for Lunar Missions\",\"authors\":\"T. Li, L.W. Zhang, H. Li, Q. Wang, X. Song, H.F. Liu, L. Tu\",\"doi\":\"10.1109/IMCCC.2018.00232\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Lunar gravity filed determines the optimization design of lunar orbiters and selections for landing sites. Direct gravity measurement by deploying high-resolution gravimeter is the only option for obtaining precise local gravity data rather than the satellite gravity survey. However, there are both light-weight and shock-resistance demands for payloads of lunar landers. Therefore, this paper proposes a Micro-Electromechanical-Systems (MEMS) based gravimeter for lunar gravity survey, taking the advantages of both light and robust. The basis of this MEMS lunar gravimeter is: a silicon-based spring-mass system performs as the gravity-sensitive element. When gravity varies with locations or time, the spring length will change and so the displacement of mass. Using the optical displacement measurement technology, the gravitational acceleration can be worked out. The gravity-sensitive element requires both an extremely low fundamental frequency for a higher sensitivity and lower noise floor and large spurious resonant frequencies for low cross-sensitivities. Shock-resistance structures are required for robustness of the gravimeter. According to the above design rationales, the gravity-sensitive element is designed and the finite element analysis software COMSOL has been used to simulate the vibration modes of the spring-mass system with the beam width varying from 20µm to 30µm. The gravimeter design with a beam width of 24µm has a fundamental frequency of 5Hz. The mechanical thermal noise can be worked out as 0.3µGal/Hz1/2 under the room temperature and atmosphere with a quality factor of 200. The equivalent noise of the optical displacement transducer is 10µGal/Hz1/2. Hence, the overall noise floor of the MEMS lunar gravimeter is 10µGal/Hz1/2, which can meet the requirement of precise measurement of lunar gravity field.\",\"PeriodicalId\":328754,\"journal\":{\"name\":\"2018 Eighth International Conference on Instrumentation & Measurement, Computer, Communication and Control (IMCCC)\",\"volume\":\"12 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2018-07-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2018 Eighth International Conference on Instrumentation & Measurement, Computer, Communication and Control (IMCCC)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/IMCCC.2018.00232\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"2018 Eighth International Conference on Instrumentation & Measurement, Computer, Communication and Control (IMCCC)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/IMCCC.2018.00232","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Design and Simulation of a MEMS Gravimeter for Lunar Missions
Lunar gravity filed determines the optimization design of lunar orbiters and selections for landing sites. Direct gravity measurement by deploying high-resolution gravimeter is the only option for obtaining precise local gravity data rather than the satellite gravity survey. However, there are both light-weight and shock-resistance demands for payloads of lunar landers. Therefore, this paper proposes a Micro-Electromechanical-Systems (MEMS) based gravimeter for lunar gravity survey, taking the advantages of both light and robust. The basis of this MEMS lunar gravimeter is: a silicon-based spring-mass system performs as the gravity-sensitive element. When gravity varies with locations or time, the spring length will change and so the displacement of mass. Using the optical displacement measurement technology, the gravitational acceleration can be worked out. The gravity-sensitive element requires both an extremely low fundamental frequency for a higher sensitivity and lower noise floor and large spurious resonant frequencies for low cross-sensitivities. Shock-resistance structures are required for robustness of the gravimeter. According to the above design rationales, the gravity-sensitive element is designed and the finite element analysis software COMSOL has been used to simulate the vibration modes of the spring-mass system with the beam width varying from 20µm to 30µm. The gravimeter design with a beam width of 24µm has a fundamental frequency of 5Hz. The mechanical thermal noise can be worked out as 0.3µGal/Hz1/2 under the room temperature and atmosphere with a quality factor of 200. The equivalent noise of the optical displacement transducer is 10µGal/Hz1/2. Hence, the overall noise floor of the MEMS lunar gravimeter is 10µGal/Hz1/2, which can meet the requirement of precise measurement of lunar gravity field.