Schmid Tobias, Rolland Jannick P, Rakich Andrew, Thompson Kevin P
CREOL - The College of Optics and Photonics, University of Central Florida, Orlando, FL 32816, USA.
Opt Express. 2010 Aug 2;18(16):17433-47. doi: 10.1364/OE.18.017433.
We present the nodal aberration field response of Ritchey-Chrétien telescopes to a combination of optical component misalignments and astigmatic figure error on the primary mirror. It is shown that both astigmatic figure error and secondary mirror misalignments lead to binodal astigmatism, but that each type has unique, characteristic locations for the astigmatic nodes. Specifically, the characteristic node locations in the presence of astigmatic figure error (at the pupil) in an otherwise aligned telescope exhibit symmetry with respect to the field center, i.e. the midpoint between the astigmatic nodes remains at the field center. For the case of secondary mirror misalignments, one of the astigmatic nodes remains nearly at the field center (in a coma compensated state) as presented in Optics Express 18, 5282-5288 (2010), while the second astigmatic node moves away from the field center. This distinction leads directly to alignment methods that preserve the dynamic range of the active wavefront compensation component.
我们展示了 Ritchey-Chrétien 望远镜的节点像差场对光学元件失准和主镜像散面形误差组合的响应。结果表明,像散面形误差和副镜失准都会导致双节点像散,但每种类型在像散节点处都有独特的特征位置。具体而言,在其他方面对准的望远镜中,存在像散面形误差(在光瞳处)时的特征节点位置相对于视场中心呈现对称性,即像散节点之间的中点保持在视场中心。对于副镜失准的情况,如《光学快报》18, 5282 - 5288 (2010) 所述,其中一个像散节点几乎保持在视场中心(处于彗差补偿状态),而第二个像散节点则远离视场中心。这种差异直接导致了能够保留有源波前补偿组件动态范围的对准方法。