Phase plates for generation of variable amounts of primary spherical aberration
被引:13
作者:
Acosta, Eva
论文数: 0引用数: 0
h-index: 0
机构:
Univ Santiago de Compostela, Fac Fis, Dept Fis Aplicada, Area Opt, Santiago De Compostela 15782, SpainUniv Santiago de Compostela, Fac Fis, Dept Fis Aplicada, Area Opt, Santiago De Compostela 15782, Spain
Acosta, Eva
[1
]
Sasian, Jose
论文数: 0引用数: 0
h-index: 0
机构:
Univ Arizona, Coll Opt Sci, Tucson, AZ 85721 USAUniv Santiago de Compostela, Fac Fis, Dept Fis Aplicada, Area Opt, Santiago De Compostela 15782, Spain
Sasian, Jose
[2
]
机构:
[1] Univ Santiago de Compostela, Fac Fis, Dept Fis Aplicada, Area Opt, Santiago De Compostela 15782, Spain
[2] Univ Arizona, Coll Opt Sci, Tucson, AZ 85721 USA
来源:
OPTICS EXPRESS
|
2011年
/
19卷
/
14期
关键词:
OPTICS;
LENSES;
SYSTEM;
D O I:
10.1364/OE.19.013171
中图分类号:
O43 [光学];
学科分类号:
070207 ;
0803 ;
摘要:
We discuss a set of phase plate-pairs for the generation of variable amounts of primary spherical aberration. The surface descriptions of these optical plates are provided, and their aberration-generating properties are verified with real ray-tracing. These plate-pairs are robust in that they allow large tolerances to spacing as well as errors in the relative displacement of the plates. Both primary spherical aberration (r(4)) and Zernike spherical aberration (6r(4) - 6r(2) + I) can be generated. The amount of spherical aberration is proportional to the plate-pair displacement and in our example it reaches up to 48 waves (similar to 8 waves Zernike) for a clear aperture of 25 mm. (C)2011 Optical Society of America