NIAOT OpenIR  > 中国科学院南京天文光学技术研究所  > 会议论文
Integrated thermal disturbance analysis of optical system of astronomical telescope
Dehua Yang; Zibo Jiang; Xinnan Li
2008-07-07
Source PublicationAdvanced Software and Control for Astronomy II
Volume7017
Issue7017
PagesVol.7017 1N-1-1
Conference Date2008-6-23
Conference PlaceMarseille, France
Funding OrganizationThe International Society for Optical Engineering
PublisherSPIE
Abstract
During operation, astronomical telescope will undergo thermal disturbance, especially more serious in solar telescope, which may cause degradation of image quality. As drives careful thermal load investigation and measure applied to assess its effect on final image quality during design phase. Integrated modeling analysis is boosting the process to find comprehensive optimum design scheme by software simulation. In this paper, we focus on the Finite Element Analysis (FEA) software-ANSYS-for thermal disturbance analysis and the optical design software-ZEMAX-for optical system design. The integrated model based on ANSYS and ZEMAX is briefed in the first from an overview of point. Afterwards, we discuss the establishment of thermal model. Complete power series polynomial with spatial coordinates is introduced to present temperature field analytically. We also borrow linear interpolation technique derived from shape function in finite element theory to interface the thermal model and structural model and further to apply the temperatures onto structural model nodes. Thereby, the thermal loads are transferred with as high fidelity as possible. Data interface and communication between the two softwares are discussed mainly on mirror surfaces and hence on the optical figure representation and transformation. We compare and comment the two different methods, Zernike polynomials and power series expansion, for representing and transforming deformed optical surface to ZEMAX. Additionally, these methods applied to surface with non-circular aperture are discussed. At the end, an optical telescope with parabolic primary mirror of 900 mm in diameter is analyzed to illustrate the above discussion. Finite Element Model with most interested parts of the telescope is generated in ANSYS with necessary structural simplification and equivalence. Thermal analysis is performed and the resulted positions and figures of the optics are to be retrieved and transferred to ZEMAX, and thus final image quality is evaluated with thermal disturbance.
KeywordIntegrated Modeling Thermal Disturbance Astronomical Telescope Power Series Zernike Polynomials Figure Representation Finite Element Method Temperature Field
Subject Area天文光学设计 ; 有限元分析
Document Type会议论文
Identifierhttp://ir.niaot.ac.cn/handle/114a32/553
Collection中国科学院南京天文光学技术研究所_会议论文
望远镜新技术研究室_会议论文
Recommended Citation
GB/T 7714
Dehua Yang,Zibo Jiang,Xinnan Li. Integrated thermal disturbance analysis of optical system of astronomical telescope[C]:SPIE,2008:Vol.7017 1N-1-1.
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