How to model an off-axis parabolic mirror

The off-axis parabolic mirror is an important design form in the optics industry. This article demonstrates how to model an off-axis parabolic mirror according to some manufacturer specifications. It also demonstrates use of the Chief Ray Solve for centering the resulting image surface on chief ray path.

Authored By Nam-Hyong Kim

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Introduction

An off-axis parabolic mirror has the advantage of not having to obscure the input beam to access the image plane. OpticStudio can easily model any off-axis portion of a surface, parabolic or not. This tutorial will show you how to model an off-axis parabolic mirror. The concept shown here applies to any decentered surface and is not limited to off-axis parabolic mirrors.

Parabolic mirror design specifications

We will model a commercially-available off-axis parabolic mirror. The goal of this exercise is to be able to tilt the mirror about the X axis at any point along the optical axis (Z axis). The specifications for the mirror are as follows.

Off-axis Distance 150mm
Focal Length 1000mm
Component Physical Diameter 203mm


Back surface of the substrate is perpendicular to the optical axis.

Layout showing measurements

If you are unsure about any of the procedures used in this tutorial, please refer to the either "How to design a singlet lens" or "How to tilt and decenter a sequential optical component" before proceeding further.

Entering the basic geometry

To start the parabolic miror design, we will first define the system settings. Make the following adjustments in the System Explorer.

  • Set Aperture...Aperture Type: Entrance Pupil Diameter and Aperture Value: 100
  • Set Units...Lens Units: Millimeters
  • Set Wavelengths...Wavelength 1: 0.550 um

Next, we can begin defining the system geometry. Add one surface to the Lens Data Editor after the STOP surface. Then enter the following parameter values on Surfaces 1-3. Note that the Image surface has a user-defined Semi-Diameter of 30 mm, as indicated in the solve box.

Lens_Data_Editor_1

The "sag" or z-coordinate of the Standard surface is given by:

equation

where c is the curvature (the reciprocal of the radius), r is the radial coordinate in lens units and k is the conic constant. The conic constant is less than -1 for hyperbolas, -1 for parabolas, between -1 and 0 for ellipses, 0 for spheres, and greater than 0 for oblate ellipsoids. To make the mirror surface parabolic, enter Conic: -1.

Because the focal length of a mirror is half the radius of curvature, enter Radius: -2000 mm. The sign of the radius of curvature is negative since the center of curvature is to the left (toward -Z-axis) of the mirror. Additionally, because Surface 1 and the image surface are co-located, we will choose not to draw Surface 1 in the layout so that we can see only the image surface at that location. Set the following property in the Surface Properties dialog.

Surface Properties Do Not Draw

To make the mirror substrate flat and orthogonal to the optical axis, choose the following options in the Surface Properties dialog. We will set Thickness: 40 mm since the manufacturer does not specify the substrate thickness on their website.

Surface Properties Mirror Substrate Thickness

Open the 3D Layout with the following settings.

3D Layout Settings     3D Layout 2

Add the off-axis distance

 In the Tilt/Decenter tab of Surface Properties of Surface 2, specify Decenter Y: -150 mm. 

Surface Decenter

From the manufacturer's specification, the off-axis distance is 150 mm and the physical diameter of the mirror is 203 mm. Specify the correct aperture size and location in the Aperture Tab of the Surface Properties menu.

Aperture Decenter

Open the 3D Layout.

3D_Layout_showing_Image_Surface_location

Note that the rays are moving away from the coordinate system. In order to center the image surface and make it orthogonal to the chief ray, insert a Coordinate Break surface before the image surface and place a Chief Ray solve on the Decenter Y and the Tilt About X parameters. OpticStudio will automatically calculate the amount of decenter and tilt needed to make the chief ray hit at the center of this surface at normal incidence.

Lens_Data_Editor_showing_Chief_Ray_Solves

Chief_Ray_Solve_on_Parameter_2

Update the 3D Layout.

Final_Layout

Perfect!

KA-01345

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