The non-null testing methods have the potential to allow measurement of aspheric surfaces with large departures from a reference sphere. In a non-null configuration, the ray will return along a different path and interfere with a different reference ray. This difference in ‘’mapping” between the test and reference rays creates an additional optical path difference (OPD) contribution, which causes test part errors to be mapped to the wrong location. To correct the mapping errors in non-null test of aspheric surface, correction method are proposed by ray trace and wave-front analysis. Experiments are carried out to illustrate the effectiveness of this approach. The methods can work well, despite large deviation between the theoretic value of ...
A method of measuring aberrations in a null-lens including assembly and alignment aberrations. The n...
The optical measurement of primary mirrors for astronomical telescopes has become increasingly chall...
The objectives for high precision astrometry on ELTs will be challenging, with requirements in the r...
The non-null testing methods have the potential to allow measurement of aspheric surfaces with large...
In interferometric testing of surfaces a major task is to avoid the introduction of aberrations due ...
The use of aspheric surfaces in optical designs can allow for improved performance with fewer optica...
Extreme ultraviolet (EUV) projection systems are designed with mild aspheres so that the mirrors can...
Aspheric surface testing would be greatly expedited by eliminating the need for a null condition. To...
Thesis (Ph. D.)--University of Rochester. Institute of Optics, 2001.Aspheric optical surfaces provid...
In order to better facilitate the use of aspheres in optical design, metrology systems must become i...
Aspheric surfaces can provide significant benefits to optical systems, but manufacturing high-precis...
Various interferometric methods can be used for testing aspheric surfaces with high accuracy. Using ...
An optical nulling apparatus for testing an optical surface includes an aspheric mirror having a ref...
Phase shifting interferometry is one of the most promising methods for testing aspheres. However, on...
An analysis of the performance of simple refractive null compensators was done. Two types of correct...
A method of measuring aberrations in a null-lens including assembly and alignment aberrations. The n...
The optical measurement of primary mirrors for astronomical telescopes has become increasingly chall...
The objectives for high precision astrometry on ELTs will be challenging, with requirements in the r...
The non-null testing methods have the potential to allow measurement of aspheric surfaces with large...
In interferometric testing of surfaces a major task is to avoid the introduction of aberrations due ...
The use of aspheric surfaces in optical designs can allow for improved performance with fewer optica...
Extreme ultraviolet (EUV) projection systems are designed with mild aspheres so that the mirrors can...
Aspheric surface testing would be greatly expedited by eliminating the need for a null condition. To...
Thesis (Ph. D.)--University of Rochester. Institute of Optics, 2001.Aspheric optical surfaces provid...
In order to better facilitate the use of aspheres in optical design, metrology systems must become i...
Aspheric surfaces can provide significant benefits to optical systems, but manufacturing high-precis...
Various interferometric methods can be used for testing aspheric surfaces with high accuracy. Using ...
An optical nulling apparatus for testing an optical surface includes an aspheric mirror having a ref...
Phase shifting interferometry is one of the most promising methods for testing aspheres. However, on...
An analysis of the performance of simple refractive null compensators was done. Two types of correct...
A method of measuring aberrations in a null-lens including assembly and alignment aberrations. The n...
The optical measurement of primary mirrors for astronomical telescopes has become increasingly chall...
The objectives for high precision astrometry on ELTs will be challenging, with requirements in the r...