For Raster CXZ and Spiral XYZ toolpaths, all associated settings, rake calcs, measurement corrections, graphics etc have been altered accordingly

STEADY X tool path is now supported for XYZ spiral Pattern for diamond tool turning. STEADY X new working for XYZ spiral pattern

With this new List Order is added (Sorting N then -M) that corresponds to Zernike Code V file format. Now Zernike surface types can be imported through Code V file format. The aberration plot can be updated by calling :meth:`~.` on abr_plt abr_plt.Code V Zernike import: - new Code V list order The :class:`~.opticalmodel.OpticalModel` class is in the :mod:`~.opticalmodel` module in the :mod:`~.optical` subpackage. osp.set_from_list(,, ])Īfter changing the wavelengths, update the optical model using :meth:`~.OpticalModel.update_model` to ensure all of the data is consistent. The wavelenghts can be specified directly in nm or by using spectral line designations, as done here. Use the :class:`~.opticalspec.OpticalSpecs` instance, osp, to modify the :attr:`~._region` in the optical subpackage to add wavelengths in the red and blue. The model in the CODE V seq file only had 1 wavelength defined. abr_plt = plt.figure(FigureClass=RayFanFigure, opt_model=opm, data_type='Ray', This is done using the :mod:`.axisarrayfigure` module. layout_plt = plt.figure(FigureClass=InteractiveLayout, opt_model=opm,ĭo_draw_rays=True, do_paraxial_layout=False).plot()

This is done using the :mod:`.interactivelayout` module.Īll graphics in rayoptics are based on matplotlib. defocus ( :class:`~.opticalspec.FocusRange`)Ī convenience method in :class:`~.ParaxialModel`, :meth:`~._order_data`, can be used to display the first order properties of the model.field_of_view ( :class:`~.opticalspec.FieldSpec`).pupil ( :class:`~.opticalspec.PupilSpec`).spectral_region ( :class:`~.opticalspec.WvlSpec`).Other essential optical specification data is also managed by the :class:`~.opticalspec.OpticalSpecs` class: The calculated first order data is in the :class:`~.firstorder.FirstOrderData` class.Īn instance of :class:`~.FirstOrderData`, :attr:`~._data`, is managed by the :class:`~.opticalspec.OpticalSpecs` class. Setup convenient aliases for using rayoptics functions sm = opmĭisplay first order properties of the model opm = open_model(root_pth/'codev/tests/CODV_q') It returns an instance of :class:`~.opticalmodel.OpticalModel` that contains all of the model data. zmx files, and the native rayoptics JSON files. Use the :func:`~._model` function to read CODE V. Read CODE V seq file for Edmund part 32-327, Achromatic Lens Use the object oriented filesystem interface from Python 3 root_pth = Path(rayoptics._file_).resolve().parent This notebook shows the steps to follow to open a CODE V seq file of a Edmund achromatic doublet.

Zemax file to codev