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Échelle-dispersion definitions:
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λnom
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λB
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Click Add.
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Click
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Click
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In the Settings window for Parameters, type Parameters 1: Geometry in the Label text field. The geometry parameters will be added when the geometry sequence is inserted below.
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Browse to the model’s Application Libraries folder and double-click the file cross_grating_echelle_spectrograph_parameters.txt.
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In the Settings window for Geometry, type Cross Grating Échelle Spectrograph Geometry Sequence in the Label text field.
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Browse to the model’s Application Libraries folder and double-click the file cross_grating_echelle_spectrograph_geom_sequence.mph.
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From the Wavelength distribution of released rays list, choose Polychromatic, specify vacuum wavelength.
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Locate the Material Properties of Exterior and Unmeshed Domains section. From the Optical dispersion model list, choose Air, Edlen (1953). The collimator lens and camera objective have been optimized for use in air.
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Locate the Additional Variables section. Select the Compute optical path length check box. The optical path length will be used to distinguish rays on the image plane from other rays which also intersect the same plane.
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In the Model Builder window, under Component 1 (comp1)>Geometrical Optics (gop) click Medium Properties 1.
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From the Refractive index of domains list, choose Get dispersion model from material. The materials previously loaded contain the coefficients for the optical dispersions models that are used to compute the wavelength dependent refractive indices.
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From the Release reflected rays list, choose Never. Scattered light is not considered in this model.
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Locate the Grating Orientation 1 section. From the Direction of periodicity 1 list, choose Parallel to reference edge.
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Locate the Reference Edge Selection, Direction 1 section. Click to select the
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Locate the Grating Orientation 2 section. From the Direction of periodicity 2 list, choose Parallel to reference edge.
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Locate the Reference Edge Selection, Direction 2 section. Click to select the
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In the Model Builder window, expand the Cross Grating 1 node, then click Diffraction Order (m = 0, n = 0).
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In the m text field, type m. The echelle order number is computed in the Parameters 2: Model node using the nominal wavelength lam_nom.
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Locate the Wall Condition section. From the Wall condition list, choose Disappear. Note that in this model, the internal aperture stop of the Petzval lens will be ignored.
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Locate the Boundary Selection section. From the Selection list, choose Image Plane. The default Wall condition Freeze will be applied to rays that intersect the image surface.
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In the Nθ text field, type N_hex. The number of hexapolar angles was defined in the Parameters 2: Model node.
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Specify the r vector as
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In the Values text field, type range(lam_min,lam_step,lam_max). These wavelengths span one free spectral range centered on the blaze wavelength. The values are also defined in the Parameters node.
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In the Lengths text field, type 0 450. This path length is sufficient to ensure that all rays make it to the image plane.
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Click
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Click OK.
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In the Model Builder window, under Results>Ray Diagram right-click Ray Trajectories 1 and choose Duplicate.
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In the Results toolbar, click
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Locate the Filters section.
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Select the Filter by additional logical expression check box. In the associated text field, type comp1.gop.L>100[mm]. Because the plane intersecting the image surface also passes through ray trajectories before they reach the image plane, these ray intersections must be removed from the plot.
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Locate the Filters section.
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Select the Filter by additional logical expression check box. In the associated text field, type comp1.gop.L>100[mm].
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In the Expression text field, type at(0,gop.phic). This is the angle from the cone axis at the entrance slit.
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Click
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Browse to the model’s Application Libraries folder and double-click the file cross_grating_echelle_spectrograph_geom_sequence_parameters.txt.
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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>Doublet and Triplet Lenses>spherical_doublet_lens_3d in the tree.
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In the Select Part Variant dialog box, select Contact doublet, 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 Spherical Doublet Lens 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 BFL_doub.
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Click to expand the Domain Selections section. In the table, select the Keep check boxes for Element 1 and Element 2.
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In the Settings window for Work Plane, type Cross Grating Incoming Reference in the Label text field.
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Locate the Selections of Resulting Entities section. Select the Resulting objects selection check box. The grating surface will be defined on this work plane.
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Locate the Distances section. In the table, enter the following settings:
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In the Settings window for Work Plane, type Cross Grating Outgoing Reference in the Label text field.
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Browse to the model’s Application Libraries folder and double-click the file cross_grating_echelle_spectrograph_petzval_lens_geom_sequence.mph.
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Find the Coordinate system to match subsection. From the Work plane list, choose Cross Grating Outgoing Reference (wp5).
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In the Model Builder window, under Component 1 (comp1)>Geometry 1, Ctrl-click to select Group 1 Aperture (pi9), Group 2 Aperture (pi10), and Group 3 Aperture (pi11).
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Right-click and choose Disable. These apertures are not needed in this model.
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