You have requested a machine translation of selected content from our databases. This functionality is provided solely for your convenience and is in no way intended to replace human translation. Neither SPIE nor the owners and publishers of the content make, and they explicitly disclaim, any express or implied representations or warranties of any kind, including, without limitation, representations and warranties as to the functionality of the translation feature or the accuracy or completeness of the translations.
Translations are not retained in our system. Your use of this feature and the translations is subject to all use restrictions contained in the Terms and Conditions of Use of the SPIE website.
Access to the requested content is limited to institutions that have purchased or subscribe to SPIE eBooks.
You are receiving this notice because your organization may not have SPIE eBooks access.*
*Shibboleth/Open Athens users─please
sign in
to access your institution's subscriptions.
To obtain this item, you may purchase the complete book in print format on
SPIE.org.
Abstract
8.1 Introduction
A single element that is corrected for spherical aberration for two chosen wavelengths can be advantageous for alignment purposes in the visible spectrum when the application is in the infrared region. We design such an element for the helium-neon and the carbon dioxide lines. The wavelength for a HeNe laser is 0.6328μm, and is 10.6 μm for a CO 2 laser. The design principle is to determine the shape of the lens for the longer wavelength first and then place a diffractive structure on one side of the lens to add the required power for the shorter wavelength to maintain focus position. Since the wavelength ratio is large, 10.6â0.6328â17, the step height of the diffractive structure for the short wavelength is d=λ nâ1 =0.6328 2.5907â1 â 0.4μm.
This is in the domain of surface roughness for the infrared region.
First, we have to pick a material that is fitting for both wavelengths. We choose ZnSe with an index of refraction of n 0.6328 =2.5907andn 10.6 =2.4027. We elect for our design example 100 mm as a focal length and a relative aperture of fâ#=2, and begin with a thin-lens pre-design.
8.2 Basic Lens Shape for the Long Wavelength
Considering that it is much easier to place a diffractive structure on a flat surface when the number of zones is high, which will be the case here; we opt for an aspheric plano-convex shape and aspherize the first surface to eliminate spherical aberration.
The front radius is R 1 =(n 10.6 â1)f CO 2 =(2.4027â1)Ã100=140.27mm. This shape leads to a focal length for the shorter wavelength of f HeNe =R 1 n 0.6328 â1 =140.27 2.59207â1 =88.1054mm.
To maintain a common focal length for both wavelengths, a negative diffractive power has to be added to the flat surface. That diffractive power is determined with Ï D =Ï CO 2 âÏ HeNe .
Online access to SPIE eBooks is limited to subscribing institutions.