Alignment aberrations of the New Solar Telescope

The New Solar Telescope (NST) is an off-axis Gregorian telescope at Big Bear Solar Observatory (BBSO). This paper presents the expected aberrations due to misalignments of the secondary mirror for a general Gregorian telescope using an optical model of the on-axis "parent" telescope version of NST. The sensitivities of linear astigmatism and constant coma found by perturbing the axisymmetric model are presented and shown to match those predicted by the theory. Then we discuss how the actual aberrations are different due to the off-axis nature of the NST. Finally, we discuss the effect of the misalignments on the pointing of the telescope.

[1]  Tom L. Zobrist,et al.  Use of a commercial laser tracker for optical alignment , 2007, SPIE Optical Engineering + Applications.

[2]  V. Mahajan Optical Imaging and Aberrations , 1998 .

[3]  L. Lundström,et al.  Transformation of Zernike coefficients: scaled, translated, and rotated wavefronts with circular and elliptical pupils. , 2007, Journal of the Optical Society of America. A, Optics, image science, and vision.

[4]  K. Thompson Description of the third-order optical aberrations of near-circular pupil optical systems without symmetry. , 2005, Journal of the Optical Society of America. A, Optics, image science, and vision.

[5]  Matt Johns Progress on the GMT , 2008, Astronomical Telescopes + Instrumentation.

[6]  James H. Burge,et al.  Manufacture of a 1.7m prototype of the GMT primary mirror segments , 2006, SPIE Astronomical Telescopes + Instrumentation.

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

[8]  Philip R. Goode,et al.  Optical design for a new off-axis 1.7-m solar telescope (NST) at Big Bear , 2004, SPIE Optics + Photonics.

[9]  Raymond N. Wilson Reflecting Telescope Optics I , 1996 .

[10]  Raymond N. Wilson,et al.  Reflecting telescope optics I : basic design theory and its historical development , 2007 .