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Click Add.
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Click Study.
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Click Done.
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Browse to the model’s Application Libraries folder and double-click the file hubble_space_telescope_parameters.txt.
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In the Part Libraries window, select Ray Optics Module>3D>Mirrors>conic_mirror_on_axis_3d in the tree.
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In the Select Part Variant dialog box, select Specify clear aperture diameter in the Select part variant list.
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Click OK.
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In the Model Builder window, under Component 1 (comp1)>Geometry 1 click Conic Mirror On Axis 3D 1 (pi1).
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Locate the Position and Orientation of Output section. Find the Displacement subsection. In the zw text field, type Z_prim.
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Click to expand the Boundary Selections section. In the table, select the Keep check box for Mirror surface.
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Click OK.
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Locate the Position and Orientation of Output section. Find the Coordinate system to match subsection. From the Take work plane from list, choose Primary Mirror (pi1).
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Locate the Parameters section. Find the First parameter subsection. In the Minimum text field, type -hw_image.
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In the z text field, type Cp*(s1^2 + s2^2)/(1 + sqrt(1 - Cp^2*(s1^2 + s2^2)))*1[m]. This is the equation of a sphere having a curvature Cp. This is the Petzval curvature defined in the Parameters node.
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Locate the Coordinate System section. From the Take work plane from list, choose Secondary Mirror (pi2).
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Locate the Selections of Resulting Entities section. Select the Resulting objects selection check box.
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In the Part Libraries window, select Ray Optics Module>3D>Apertures and Obstructions>circular_planar_annulus in the tree.
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In the Model Builder window, under Component 1 (comp1)>Geometry 1 click Circular Planar Annulus 1 (pi3).
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Locate the Position and Orientation of Output section. Find the Coordinate system to match subsection. From the Take work plane from list, choose Secondary Mirror (pi2).
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Locate the Ray Release and Propagation section. In the Maximum number of secondary rays text field, type 0.
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Locate the Boundary Selection section. From the Selection list, choose Mirror surface (Primary Mirror).
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Locate the Boundary Selection section. From the Selection list, choose Mirror surface (Secondary Mirror).
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In the Lengths text field, type 0 17. This path length is sufficient to ensure that all rays reach the image plane.
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In the Model Builder window, expand the Results>Ray Diagram>Ray Trajectories 1 node, then click Color Expression 1.
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In the Expression text field, type at('last',gop.rrel). This is the radial coordinate relative to the centroid at the image plane for each release feature.
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Click Define custom colors.
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Click Add to custom colors.
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In the Expression text field, type at(0,gop.rrel). This is the radial coordinate relative to the centroid at the entrance pupil for each ray release.
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