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 order misalignment aberrations arise for any TMA telescope. One aberration, field constant 3rd order coma is a well known misalignment aberration commonly seen in two-mirror Ritchey Chretien telescopes. The second aberration, field-asymmetric, field-linear, 3rd order astigmatism is a new and unique image orientation dependence with field derived here for the first time using nodal aberration theory. © 2008 Optical Society of America
Q1: Why deploy N wavefront sensors on a three mirror anastigmat (TMA) and not N + 1? Q2: Why measure...
The performance of optical imaging systems relies on control of aberrations that can arise from limi...
<p> Through introducing transformed pupil vector and shifted center of aberration fields vector int...
There is a long list of new ground-based optical telescopes being considered around the world. While...
There is a long list of new ground-based optical telescopes being considered around the world. While...
The alignment of three mirror anastigmatic (TMA) telescopes has been studied since their invention i...
Following the foundation of aberration theory for rotationally symmetric optical systems established...
We present the effects of misalignments on the field dependence of the third-order aberration fields...
We present the effects of misalignments on the field dependence of the third-order aberration fields...
The effects of alignment perturbations on the aberration fields of two mirror astronomical telescope...
In order to improve the efficiency of alignment for a three;mirror;anastigmatic (TMA) telescope with...
Nodal aberration theory (NAT) has revealed that misalignment astigmatism displays a different signat...
Misalignments always occur in real optical systems. These misalignments do not generate new aberrati...
We present the nodal aberration field response of Ritchey-Chretien telescopes to a combination of op...
We present the aberration field response of Ritchey-Chretien telescopes, with the aperture stop on t...
Q1: Why deploy N wavefront sensors on a three mirror anastigmat (TMA) and not N + 1? Q2: Why measure...
The performance of optical imaging systems relies on control of aberrations that can arise from limi...
<p> Through introducing transformed pupil vector and shifted center of aberration fields vector int...
There is a long list of new ground-based optical telescopes being considered around the world. While...
There is a long list of new ground-based optical telescopes being considered around the world. While...
The alignment of three mirror anastigmatic (TMA) telescopes has been studied since their invention i...
Following the foundation of aberration theory for rotationally symmetric optical systems established...
We present the effects of misalignments on the field dependence of the third-order aberration fields...
We present the effects of misalignments on the field dependence of the third-order aberration fields...
The effects of alignment perturbations on the aberration fields of two mirror astronomical telescope...
In order to improve the efficiency of alignment for a three;mirror;anastigmatic (TMA) telescope with...
Nodal aberration theory (NAT) has revealed that misalignment astigmatism displays a different signat...
Misalignments always occur in real optical systems. These misalignments do not generate new aberrati...
We present the nodal aberration field response of Ritchey-Chretien telescopes to a combination of op...
We present the aberration field response of Ritchey-Chretien telescopes, with the aperture stop on t...
Q1: Why deploy N wavefront sensors on a three mirror anastigmat (TMA) and not N + 1? Q2: Why measure...
The performance of optical imaging systems relies on control of aberrations that can arise from limi...
<p> Through introducing transformed pupil vector and shifted center of aberration fields vector int...