Opto-thermal analysis of a lightweighted mirror for solar telescope.

In this paper, an opto-thermal analysis of a moderately heated lightweighted solar telescope mirror is carried out using 3D finite element analysis (FEA). A physically realistic heat transfer model is developed to account for the radiative heating and energy exchange of the mirror with surroundings. The numerical simulations show the non-uniform temperature distribution and associated thermo-elastic distortions of the mirror blank clearly mimicking the underlying discrete geometry of the lightweighted substrate. The computed mechanical deformation data is analyzed with surface polynomials and the optical quality of the mirror is evaluated with the help of a ray-tracing software. The thermal print-through distortions are further shown to contribute to optical figure changes and mid-spatial frequency errors of the mirror surface. A comparative study presented for three commonly used substrate materials, namely, Zerodur, Pyrex and Silicon Carbide (SiC) is relevant to vast area of large optics requirements in ground and space applications.

[1]  Frank-M. Göttsche,et al.  Modelling of diurnal cycles of brightness temperature extracted from METEOSAT data , 2001 .

[2]  Haobo Cheng,et al.  A thermo-optical analysis method for a space optical remote sensor optostructural system , 2004 .

[3]  John M. Tamkin,et al.  A study of image artifacts caused by structured mid-spatial frequency fabrication errors on optical surfaces , 2010 .

[4]  Roberto Gilmozzi Science and technology drivers for future giant telescopes , 2004, SPIE Astronomical Telescopes + Instrumentation.

[5]  Philip R. Goode,et al.  Scientific instrumentation for the 1.6 m New Solar Telescope in Big Bear , 2010 .

[6]  M. Collados,et al.  Current concept for the 4m European Solar Telescope (EST) optical design , 2010, International Optical Design Conference.

[7]  Dirk Soltau,et al.  NLST: India's National Large Solar Telescope , 2010 .

[8]  Eric R. Hansen,et al.  Gemini primary mirror thermal management system , 1994, Astronomical Telescopes and Instrumentation.

[9]  F. Heidecke,et al.  The 1.5 meter solar telescope GREGOR , 2012 .

[10]  Bruce Bohannan,et al.  Thermal control of classical astronomical primary mirrors , 2000, Astronomical Telescopes and Instrumentation.

[11]  Thomas Werner,et al.  Manufacturing of the ZERODUR 1.5-m primary mirror for the solar telescope GREGOR as preparation of light weighting of blanks up to 4-m diameter , 2010, Astronomical Telescopes + Instrumentation.

[12]  Lucy E. Cohan,et al.  Minimizing high spatial frequency residual error in active space telescope mirrors , 2009, Optical Engineering + Applications.

[13]  B. Ravindra,et al.  Thermal characteristics of a classical solar telescope primary mirror , 2011, 1102.0111.

[14]  R. Racine The Historical Growth of Telescope Aperture , 2003 .

[15]  Ryusuke Ogasawara,et al.  Temperature control for the primary mirror of Subaru Telescope using the data from , 2003 .

[16]  R. Volkmer,et al.  GREGOR M1 mirror and cell design: effects of different mirror substrates on the telescope design , 2010, Astronomical Telescopes + Instrumentation.

[17]  R N Youngworth,et al.  Simple Estimates for the Effects of Mid-spatial-Frequency Surface Errors on Image Quality. , 2000, Applied optics.

[18]  C. M. Lowne An investigation of the effects of mirror temperature upon telescope seeing. , 1979 .

[19]  R. Noll Zernike polynomials and atmospheric turbulence , 1976 .

[20]  Thomas R. Rimmele,et al.  Advanced Technology Solar Telescope , 2001 .

[21]  Peter Emde,et al.  Thermal design features of the solar telescope GREGOR , 2004, SPIE Astronomical Telescopes + Instrumentation.

[22]  Edwin J Sarver,et al.  Are all aberrations equal? , 2002, Journal of refractive surgery.

[23]  James H. Burge,et al.  Open-source data analysis and visualization software platform: SAGUARO , 2011, Optical Engineering + Applications.

[24]  Virendra N. Mahajan,et al.  Zernike annular polynomials and optical aberrations of systems with annular pupils. , 1994, Applied optics.

[25]  Giampiero Naletto,et al.  Method for studying the effects of thermal deformations on optical systems for space application. , 2011, Applied optics.