Thompson Kevin P, Schmid Tobias, Rolland Jannick P
Optical Research Associates, 3280 E. Foothill Blvd, Suite 300, Pasadena, California 91107, USA.
Opt Express. 2008 Dec 8;16(25):20345-53. doi: 10.1364/oe.16.020345.
The next major space-borne observatory, the James Webb Space Telescope, will be a 6.6M field-biased, obscured, three-mirror anastigmat (TMA). Over the used field of view, the performance of TMA telescopes is dominated by 3(rd) order misalignment aberrations. Here it is shown that two dominant 3(rd) order misalignment aberrations arise for any TMA telescope. One aberration, field constant 3(rd) order coma is a well known misalignment aberration commonly seen in two-mirror Ritchey Chretien telescopes. The second aberration, field-asymmetric, field-linear, 3(rd) order astigmatism is a new and unique image orientation dependence with field derived here for the first time using nodal aberration theory.
下一个主要的太空天文台——詹姆斯·韦布空间望远镜,将是一台口径6.6米、具有场偏置、遮光的三镜消像散望远镜(TMA)。在使用的视场内,TMA望远镜的性能主要由三阶失调像差决定。本文表明,任何TMA望远镜都会产生两种主要的三阶失调像差。一种像差,即场常数三阶彗差,是在双镜里奇克莱琴望远镜中常见的一种众所周知的失调像差。第二种像差,即场非对称、场线性三阶像散,是一种新的、独特的与视场有关的像方位依赖性,本文首次使用节点像差理论推导得出。