지원사업
학술연구/단체지원/교육 등 연구자 활동을 지속하도록 DBpia가 지원하고 있어요.
커뮤니티
연구자들이 자신의 연구와 전문성을 널리 알리고, 새로운 협력의 기회를 만들 수 있는 네트워킹 공간이에요.
논문 기본 정보
- 자료유형
- 학술대회자료
- 저자정보
- 발행연도
- 2012.2
- 수록면
- 1,044 - 1,048 (5page)
이용수
초록· 키워드
오류제보하기
The object of this study is a 3-DOF secondary mirror of Giant Magellan Telescope, which is a 3-DOF parallel manipulator. In order to analyze the kinematic characteristics of this mechanism, the forward kinematic equation and inverse kinematic equation are calculated respectively. To verify the performance of the secondary mirror, a series of experiments are carried out, and some relative experimental data about tip-tilt movement is obtained. To observe the tip-tilt movement of 3-DOF secondary mirror using a computer program, instead of conducting real experiment, a dynamic simulation module and a customizable simulation module are developed. Through comparing these two simulation results, the tip-tilt characteristic of 3-DOF secondary mirror can be visualized and supervised obviously, it also lays a solid foundation for kinematic calibration of this mechanism.
목차
ABSTRACT
1. Introduction
2. Inverse kinematic mo del
3. Simulation model
4. Conclusion
References
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UCI(KEPA) : I410-ECN-0101-2015-500-001136712